Hauptseite > CMS Collection > CMS Preprints > Searches for Higgs boson production through decays of heavy resonances > HTML MARC |
002892661 001__ 2892661 002892661 005__ 20240405044710.0 002892661 0248_ $$aoai:cds.cern.ch:2892661$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN 002892661 035__ $$9Inspire$$a2771692 002892661 037__ $$9arXiv$$aarXiv:2403.16926$$chep-ex 002892661 037__ $$9arXiv:reportnumber$$aCMS-B2G-23-002 002892661 037__ $$9arXiv:reportnumber$$aCERN-EP-2024-062 002892661 041__ $$aeng 002892661 088__ $$aCMS-B2G-23-002-003 002892661 100__ $$aHayrapetyan, Aram$$jCCID-838558$$uYerevan Phys. Inst. 002892661 110__ $$aCMS Collaboration 002892661 245__ $$aSearches for Higgs boson production through decays of heavy resonances 002892661 260__ $$c2024 002892661 269__ $$aGeneva$$bCERN$$c24 Mar 2024 002892661 300__ $$a115 p 002892661 500__ $$9arXiv$$aTo be submitted to Physics Reports. All figures and tables can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/B2G-23-002 (CMS Public Pages) 002892661 520__ $$aThe discovery of the Higgs boson has led to new possible signatures for heavy resonance searches at the LHC. Since then, search channels including at least one Higgs boson plus another particle have formed an important part of the program of new physics searches. In this report, the status of these searches by the CMS Collaboration is reviewed. Searches are discussed for resonances decaying to two Higgs bosons, a Higgs and a vector boson, or a Higgs boson and another new resonance, with proton-proton collision data collected at $ \sqrt{s}= $ 13 TeV in the years 2016-2018. A combination of the results of these searches is presented together with constraints on different beyond-the-standard model scenarios, including scenarios with extended Higgs sectors, heavy vector bosons and extra dimensions. Studies are shown for the first time by CMS on the validity of the narrow-width approximation in searches for the resonant production of a pair of Higgs bosons. The potential for a discovery at the High Luminosity LHC is also discussed. 002892661 520__ $$9arXiv$$aThe discovery of the Higgs boson has led to new possible signatures for heavy resonance searches at the LHC. Since then, search channels including at least one Higgs boson plus another particle have formed an important part of the program of new physics searches. In this report, the status of these searches by the CMS Collaboration is reviewed. Searches are discussed for resonances decaying to two Higgs bosons, a Higgs and a vector boson, or a Higgs boson and another new resonance, with proton-proton collision data collected at $\sqrt{s}$ = 13 TeV in the years 2016-2018. A combination of the results of these searches is presented together with constraints on different beyond-the-standard model scenarios, including scenarios with extended Higgs sectors, heavy vector bosons and extra dimensions. Studies are shown for the first time by CMS on the validity of the narrow-width approximation in searches for the resonant production of a pair of Higgs bosons. The potential for a discovery at the High Luminosity LHC is also discussed. 002892661 540__ $$3Preprint$$aCC-BY-4.0 002892661 542__ $$3Preprint$$dCERN$$g2024 002892661 65017 $$2SzGeCERN$$aParticle Physics - Experiment 002892661 6531_ $$9CERN$$aexotics 002892661 693__ $$aCERN LHC$$eCMS 002892661 690C_ $$aCMS_Papers 002892661 690C_ $$aCERN 002892661 690C_ $$aPREPRINT 002892661 700__ $$aTumasyan, Armen$$iINSPIRE-00175052$$jCCID-673689$$jORCID:0009-0000-0684-6742$$uYerevan Phys. 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Res. 002892661 700__ $$aDimitrov, Anton$$iINSPIRE-00174462$$jCCID-582534$$jORCID:0000-0003-2899-701X$$uSofiya U. 002892661 700__ $$aLitov, Leander$$iINSPIRE-00102196$$jCCID-408342$$jORCID:0000-0002-8511-6883$$uSofiya U. 002892661 700__ $$aPavlov, Borislav$$iINSPIRE-00169986$$jCCID-555088$$jORCID:0000-0003-3635-0646$$uSofiya U. 002892661 700__ $$aPetkov, Peicho$$iINSPIRE-00315084$$jCCID-555450$$jORCID:0000-0002-0420-9480$$uSofiya U. 002892661 700__ $$aPetrov, Anton$$iINSPIRE-00679657$$jCCID-785826$$jORCID:0009-0003-8899-1514$$uSofiya U. 002892661 700__ $$aShumka, Elton$$jCCID-838342$$jORCID:0000-0002-0104-2574$$uSofiya U. 002892661 700__ $$aKeshri, Sumit$$iINSPIRE-00414882$$jCCID-759318$$jORCID:0000-0003-3280-2350$$uTarapaca U. 002892661 700__ $$aThakur, Shalini$$iINSPIRE-00444529$$jCCID-764789$$jORCID:0000-0002-1647-0360$$uTarapaca U. 002892661 700__ $$aCheng, Tongguang$$iINSPIRE-00239195$$jCCID-718537$$jORCID:0000-0003-2954-9315$$uBeihang U. 002892661 700__ $$aJavaid, Tahir$$iINSPIRE-00576849$$jCCID-815753$$jORCID:0009-0007-2757-4054$$uBeihang U. 002892661 700__ $$aYuan, Li$$iINSPIRE-00226222$$jCCID-672753$$jORCID:0000-0002-6719-5397$$uBeihang U. 002892661 700__ $$aHu, Zhen$$iINSPIRE-00170070$$jCCID-673885$$jORCID:0000-0001-8209-4343$$uTsinghua U., Beijing 002892661 700__ $$aLiang, Zhengchen$$iINSPIRE-00704889$$jCCID-848682$$uTsinghua U., Beijing 002892661 700__ $$aLiu, Jinfeng$$iINSPIRE-00702593$$jCCID-844718$$uTsinghua U., Beijing 002892661 700__ $$aYi, Kai$$iINSPIRE-00137481$$jCCID-677774$$jORCID:0000-0002-2459-1824$$uTsinghua U., Beijing$$uNanjing Normal U.$$uIowa U. 002892661 700__ $$aChen, Guo-Ming$$iINSPIRE-00147979$$jCCID-381894$$jORCID:0000-0002-2629-5420$$uBeijing, Inst. 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High Energy Phys. 002892661 700__ $$aShahzad, Muhammad Aamir$$iINSPIRE-00655840$$jCCID-825961$$uBeijing, Inst. High Energy Phys.$$uUCAS, Beijing 002892661 700__ $$aSharma, Ramkrishna$$iINSPIRE-00375203$$jCCID-749075$$jORCID:0000-0003-1181-1426$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aSong, Jia-ning$$iINSPIRE-00694015$$jCCID-844501$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aTao, Junquan$$iINSPIRE-00315108$$jCCID-654883$$jORCID:0000-0003-2006-3490$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aWang, Chu$$iINSPIRE-00670842$$jCCID-833028$$uBeijing, Inst. High Energy Phys.$$uUCAS, Beijing 002892661 700__ $$aWang, Jin$$iINSPIRE-00225390$$jCCID-670921$$jORCID:0000-0002-3103-1083$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aWang, Zebing$$iINSPIRE-00671491$$jCCID-833137$$uBeijing, Inst. High Energy Phys.$$uUCAS, Beijing 002892661 700__ $$aZhang, Huaqiao$$iINSPIRE-00227084$$jCCID-645936$$jORCID:0000-0001-8843-5209$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aZhao, Jingzhou$$iINSPIRE-00375220$$jCCID-749066$$jORCID:0000-0001-8365-7726$$uBeijing, Inst. High Energy Phys. 002892661 700__ $$aAgapitos, Antonis$$iINSPIRE-00176251$$jCCID-669162$$jORCID:0000-0002-8953-1232$$uPeking U. 002892661 700__ $$aBan, Yong$$iINSPIRE-00170030$$jCCID-498802$$jORCID:0000-0002-1912-0374$$uPeking U. 002892661 700__ $$aDeng, Sen$$jCCID-826412$$jORCID:0000-0002-2999-1843$$uPeking U. 002892661 700__ $$aGuo, Botao$$jCCID-858212$$uPeking U. 002892661 700__ $$aJiang, Chuqiao$$iINSPIRE-00681892$$jCCID-838503$$jORCID:0009-0008-6986-388X$$uPeking U. 002892661 700__ $$aLevin, Andrew$$iINSPIRE-00285662$$jCCID-724731$$jORCID:0000-0001-9565-4186$$uPeking U. 002892661 700__ $$aLi, Congqiao$$iINSPIRE-00688254$$jCCID-832620$$jORCID:0000-0002-6339-8154$$uPeking U. 002892661 700__ $$aLi, Qiang$$iINSPIRE-00329296$$jCCID-730168$$jORCID:0000-0002-8290-0517$$uPeking U. 002892661 700__ $$aMao, Yajun$$iINSPIRE-00170086$$jCCID-412260$$uPeking U. 002892661 700__ $$aQian, Sitian$$iINSPIRE-00705512$$jCCID-849198$$uPeking U. 002892661 700__ $$aQian, Si-Jin$$iINSPIRE-00311576$$jCCID-403143$$jORCID:0000-0002-0630-481X$$uPeking U. 002892661 700__ $$aQin, Xuelong$$iINSPIRE-00693231$$jCCID-844067$$uPeking U. 002892661 700__ $$aSun, Xiaohu$$iINSPIRE-00226957$$jCCID-676505$$jORCID:0000-0003-4409-4574$$uPeking U. 002892661 700__ $$aWang, Dayong$$iINSPIRE-00164378$$jCCID-664696$$jORCID:0000-0002-9013-1199$$uPeking U. 002892661 700__ $$aYang, Heng$$iINSPIRE-00691417$$jCCID-839502$$uPeking U. 002892661 700__ $$aZhang, Licheng$$iINSPIRE-00691224$$jCCID-843148$$jORCID:0000-0001-7947-9007$$uPeking U. 002892661 700__ $$aZhao, Yuzhe$$jCCID-852060$$uPeking U. 002892661 700__ $$aZhou, Chen$$jCCID-730718$$jORCID:0000-0001-5904-7258$$uPeking U. 002892661 700__ $$aYang, Shuai$$iINSPIRE-00480126$$jCCID-833699$$jORCID:0000-0002-2075-8631$$uSouth China Normal U. 002892661 700__ $$aYou, Zhengyun$$iINSPIRE-00255263$$jCCID-820401$$jORCID:0000-0001-8324-3291$$uSYSU, Guangzhou 002892661 700__ $$aGuo, Zhengliang$$jCCID-869959 002892661 700__ $$aJaffel, Khawla$$iINSPIRE-00679173$$jCCID-830340$$jORCID:0000-0001-7419-4248 002892661 700__ $$aLu, Nan$$iINSPIRE-00378788$$jCCID-738118$$jORCID:0000-0002-2631-6770 002892661 700__ $$aBauer, Gerry$$iINSPIRE-00065190$$jCCID-373242$$uNanjing Normal U. 002892661 700__ $$aLi, Bolin$$iINSPIRE-00691173$$jCCID-843145$$uNanjing Normal U. 002892661 700__ $$aZhang, Jingqing$$iINSPIRE-00703154$$jCCID-847570$$jORCID:0000-0003-3314-2534$$uNanjing Normal U. 002892661 700__ $$aGao, Xuyang$$iINSPIRE-00534435$$jCCID-783508$$jORCID:0000-0001-7205-2318$$uFudan U.$$uBrussels U. 002892661 700__ $$aLin, Zhen$$iINSPIRE-00697016$$jCCID-844849$$jORCID:0000-0003-1812-3474$$uZhejiang U. 002892661 700__ $$aLu, Chenfeng$$iINSPIRE-00687687$$jCCID-841788$$jORCID:0000-0002-7421-0313$$uZhejiang U. 002892661 700__ $$aXiao, Meng$$iINSPIRE-00237895$$jCCID-683454$$jORCID:0000-0001-9628-9336$$uZhejiang U. 002892661 700__ $$aAvila, Carlos$$iINSPIRE-00063395$$jCCID-371667$$jORCID:0000-0002-5610-2693$$uAndes U., Bogota 002892661 700__ $$aBarbosa Trujillo, Diego Andres$$iINSPIRE-00701065$$jCCID-846706$$uAndes U., Bogota 002892661 700__ $$aCabrera, Andrés$$iINSPIRE-00191453$$jCCID-694873$$jORCID:0000-0002-0486-6296$$uAndes U., Bogota 002892661 700__ $$aFlorez, Carlos$$iINSPIRE-00319880$$jCCID-664441$$jORCID:0000-0002-3222-0249$$uAndes U., Bogota 002892661 700__ $$aFraga, Jorge$$iINSPIRE-00671476$$jCCID-833095$$jORCID:0000-0002-5137-8543$$uAndes U., Bogota 002892661 700__ $$aReyes Vega, Jose Antonio$$iINSPIRE-00801244$$jCCID-849816$$uAndes U., Bogota 002892661 700__ $$aRamirez, Felipe$$iINSPIRE-00679870$$jCCID-837083$$jORCID:0000-0002-7178-0484$$uAntioquia U. 002892661 700__ $$aRodriguez, Manuel$$jCCID-838419$$jORCID:0000-0002-9480-213X$$uAntioquia U. 002892661 700__ $$aRuales Barbosa, Anderson Alexis$$jCCID-854294$$jORCID:0000-0003-0826-0803$$uAntioquia U. 002892661 700__ $$aRuiz Alvarez, José David$$iINSPIRE-00355050$$jCCID-723434$$jORCID:0000-0002-3306-0363$$uAntioquia U. 002892661 700__ $$aGiljanovic, Duje$$iINSPIRE-00655821$$jCCID-825904$$jORCID:0009-0005-6792-6881$$uSplit Tech. 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Tbilisi$$uUnlisted 002892661 700__ $$aBotta, Valeria$$iINSPIRE-00535551$$jCCID-735546$$jORCID:0000-0003-1661-9513$$uAachen, Tech. Hochsch. 002892661 700__ $$aFeld, Lutz$$iINSPIRE-00315477$$jCCID-456299$$jORCID:0000-0001-9813-8646$$uAachen, Tech. Hochsch. 002892661 700__ $$aKlein, Katja$$iINSPIRE-00315490$$jCCID-488837$$jORCID:0000-0002-1546-7880$$uAachen, Tech. Hochsch. 002892661 700__ $$aLipinski, Martin$$iINSPIRE-00391791$$jCCID-743604$$jORCID:0000-0002-6839-0063$$uAachen, Tech. Hochsch. 002892661 700__ $$aMeuser, Danilo$$iINSPIRE-00675980$$jCCID-793079$$jORCID:0000-0002-2722-7526$$uAachen, Tech. Hochsch. 002892661 700__ $$aPauls, Alexander$$iINSPIRE-00675994$$jCCID-797501$$jORCID:0000-0002-8117-5376$$uAachen, Tech. Hochsch. 002892661 700__ $$aPérez Adán, Danyer$$iINSPIRE-00648171$$jCCID-822291$$jORCID:0000-0003-3416-0726$$uAachen, Tech. Hochsch. 002892661 700__ $$aRöwert, Nicolas$$iINSPIRE-00701733$$jCCID-798288$$jORCID:0000-0002-4745-5470$$uAachen, Tech. Hochsch. 002892661 700__ $$aTeroerde, Marius$$iINSPIRE-00646496$$jCCID-759515$$jORCID:0000-0002-5892-1377$$uAachen, Tech. Hochsch. 002892661 700__ $$aDiekmann, Svenja$$jCCID-831878$$jORCID:0009-0004-8867-0881$$uAachen, Tech. Hochsch. 002892661 700__ $$aDodonova, Alena$$jCCID-821669$$jORCID:0000-0002-5115-8487$$uAachen, Tech. Hochsch. 002892661 700__ $$aEich, Niclas$$iINSPIRE-00703762$$jCCID-839869$$jORCID:0000-0001-9494-4317$$uAachen, Tech. Hochsch. 002892661 700__ $$aEliseev, Dmitry$$iINSPIRE-00675036$$jCCID-833666$$jORCID:0000-0001-5844-8156$$uAachen, Tech. Hochsch. 002892661 700__ $$aEngelke, Frederic$$jCCID-831887$$jORCID:0000-0002-9288-8144$$uAachen, Tech. Hochsch. 002892661 700__ $$aErdmann, Johannes$$jCCID-674792$$jORCID:0000-0002-8073-2740$$uAachen, Tech. Hochsch. 002892661 700__ $$aErdmann, Martin$$iINSPIRE-00079752$$jCCID-390164$$jORCID:0000-0002-1653-1303$$uAachen, Tech. Hochsch. 002892661 700__ $$aFackeldey, Peter$$iINSPIRE-00745016$$jCCID-796765$$jORCID:0000-0003-4932-7162$$uAachen, Tech. Hochsch. 002892661 700__ $$aFischer, Benjamin$$iINSPIRE-00674378$$jCCID-782998$$jORCID:0000-0002-3900-3482$$uAachen, Tech. Hochsch. 002892661 700__ $$aHebbeker, Thomas$$iINSPIRE-00089340$$jCCID-399614$$jORCID:0000-0002-9736-266X$$uAachen, Tech. Hochsch. 002892661 700__ $$aHoepfner, Kerstin$$iINSPIRE-00090570$$jCCID-400602$$jORCID:0000-0002-2008-8148$$uAachen, Tech. Hochsch. 002892661 700__ $$aIvone, Francesco$$iINSPIRE-00702184$$jCCID-832288$$jORCID:0000-0002-2388-5548$$uAachen, Tech. Hochsch. 002892661 700__ $$aJung, Alexander$$jCCID-858323$$jORCID:0000-0002-2511-1490$$uAachen, Tech. Hochsch. 002892661 700__ $$aLee, Ming-yan$$jCCID-806210$$jORCID:0000-0002-4430-1695$$uAachen, Tech. Hochsch. 002892661 700__ $$aMausolf, Florian$$jCCID-847362$$jORCID:0000-0003-2479-8419$$uAachen, Tech. Hochsch. 002892661 700__ $$aMerschmeyer, Markus$$iINSPIRE-00028349$$jCCID-665143$$jORCID:0000-0003-2081-7141$$uAachen, Tech. Hochsch. 002892661 700__ $$aMeyer, Arnd$$iINSPIRE-00300593$$jCCID-664326$$jORCID:0000-0001-9598-6623$$uAachen, Tech. Hochsch. 002892661 700__ $$aMukherjee, Swagata$$iINSPIRE-00332029$$jCCID-736533$$jORCID:0000-0001-6341-9982$$uAachen, Tech. Hochsch. 002892661 700__ $$aNoll, Dennis$$iINSPIRE-00674419$$jCCID-769882$$jORCID:0000-0002-0176-2360$$uAachen, Tech. Hochsch. 002892661 700__ $$aNowotny, Fabian$$jCCID-831869$$uAachen, Tech. Hochsch. 002892661 700__ $$aPozdnyakov, Andrey$$iINSPIRE-00305303$$jCCID-663712$$jORCID:0000-0003-3478-9081$$uAachen, Tech. Hochsch. 002892661 700__ $$aRath, Yannik$$iINSPIRE-00674447$$jCCID-784173$$uAachen, Tech. Hochsch. 002892661 700__ $$aRedjeb, Wahid$$jCCID-842563$$jORCID:0000-0001-9794-8292$$uAachen, Tech. Hochsch. 002892661 700__ $$aRehm, Florian$$iINSPIRE-00702507$$jCCID-845381$$uAachen, Tech. Hochsch. 002892661 700__ $$aReithler, Hans$$iINSPIRE-00315581$$jCCID-425714$$jORCID:0000-0003-4409-702X$$uAachen, Tech. Hochsch. 002892661 700__ $$aSarkisovi, Valentina$$jCCID-830382$$jORCID:0000-0001-9430-5419$$uAachen, Tech. Hochsch. 002892661 700__ $$aSchmidt, Alexander$$iINSPIRE-00318446$$jCCID-617928$$jORCID:0000-0003-2711-8984$$uAachen, Tech. Hochsch. 002892661 700__ $$aSharma, Archana$$iINSPIRE-00316081$$jCCID-672739$$jORCID:0000-0002-5295-1460$$uAachen, Tech. Hochsch. 002892661 700__ $$aSpah, Jan Lukas$$jCCID-849497$$jORCID:0000-0002-5215-3258$$uAachen, Tech. Hochsch. 002892661 700__ $$aStein, Annika$$jCCID-849618$$jORCID:0000-0003-0713-811X$$uAachen, Tech. Hochsch. 002892661 700__ $$aTorres Da Silva De Araujo, Felipe$$iINSPIRE-00175930$$jCCID-676333$$jORCID:0000-0002-4785-3057$$uAachen, Tech. Hochsch. 002892661 700__ $$aWiedenbeck, Sebastian$$iINSPIRE-00657284$$jCCID-780383$$jORCID:0000-0002-4692-9304$$uAachen, Tech. Hochsch. 002892661 700__ $$aZaleski, Shawn$$iINSPIRE-00441188$$jCCID-764014$$uAachen, Tech. Hochsch. 002892661 700__ $$aDziwok, Christian$$iINSPIRE-00655550$$jCCID-825769$$jORCID:0000-0001-9806-0244$$uAachen, Tech. Hochsch. 002892661 700__ $$aFlügge, Günter$$iINSPIRE-00315605$$jCCID-392243$$jORCID:0000-0003-3681-9272$$uAachen, Tech. Hochsch. 002892661 700__ $$aKress, Thomas$$iINSPIRE-00098530$$jCCID-406448$$jORCID:0000-0002-2702-8201$$uAachen, Tech. Hochsch. 002892661 700__ $$aNowack, Andreas$$iINSPIRE-00009768$$jCCID-483371$$jORCID:0000-0002-3522-5926$$uAachen, Tech. Hochsch. 002892661 700__ $$aPooth, Oliver$$iINSPIRE-00314326$$jCCID-455723$$jORCID:0000-0001-6445-6160$$uAachen, Tech. Hochsch. 002892661 700__ $$aStahl, Achim$$iINSPIRE-00315629$$jCCID-433355$$jORCID:0000-0002-8369-7506$$uAachen, Tech. Hochsch. 002892661 700__ $$aZiemons, Tim$$iINSPIRE-00657838$$jCCID-815538$$jORCID:0000-0003-1697-2130$$uAachen, Tech. Hochsch. 002892661 700__ $$aZotz, Alexander$$iINSPIRE-00673400$$jCCID-748436$$jORCID:0000-0002-1320-1712$$uAachen, Tech. Hochsch. 002892661 700__ $$aAarup Petersen, Henriette$$iINSPIRE-00668039$$jCCID-810921$$jORCID:0009-0005-6482-7466$$uDESY 002892661 700__ $$aAldaya Martin, Maria$$iINSPIRE-00002536$$jCCID-611666$$jORCID:0000-0003-1533-0945$$uDESY 002892661 700__ $$aAlimena, Juliette$$iINSPIRE-00236514$$jCCID-718388$$jORCID:0000-0001-6030-3191$$uDESY 002892661 700__ $$aAmoroso, Simone$$jCCID-676067$$uDESY 002892661 700__ $$aAn, Ying$$iINSPIRE-00658221$$jCCID-826694$$jORCID:0000-0003-1299-1879$$uDESY 002892661 700__ $$aBach, Jorn$$jCCID-861567$$jORCID:0000-0001-9572-6645$$uDESY 002892661 700__ $$aBaxter, Samuel$$iINSPIRE-00639816$$jCCID-782829$$jORCID:0009-0008-4191-6716$$uDESY 002892661 700__ $$aBayatmakou, Maryam$$jCCID-844330$$jORCID:0009-0002-9905-0667$$uDESY 002892661 700__ $$aBecerril Gonzalez, Hugo$$iINSPIRE-00746618$$jCCID-824658$$jORCID:0000-0001-5387-712X$$uDESY 002892661 700__ $$aBehnke, Olaf$$iINSPIRE-00172556$$jCCID-373644$$jORCID:0000-0002-4238-0991$$uDESY 002892661 700__ $$aBelvedere, Alberto$$jCCID-852419$$jORCID:0000-0002-2802-8203$$uDESY 002892661 700__ $$aBhattacharya, Soham$$iINSPIRE-00532247$$jCCID-782693$$jORCID:0000-0002-3197-0048$$uDESY 002892661 700__ $$aBlekman, Freya$$iINSPIRE-00052335$$jCCID-524499$$jORCID:0000-0002-7366-7098$$uDESY$$uHamburg U. 002892661 700__ $$aBorras, Kerstin$$iINSPIRE-00315630$$jCCID-376858$$jORCID:0000-0003-1111-249X$$uDESY$$uAachen, Tech. Hochsch. 002892661 700__ $$aCampbell, Alan$$iINSPIRE-00315642$$jCCID-379810$$jORCID:0000-0003-4439-5748$$uDESY 002892661 700__ $$aCardini, Andrea$$iINSPIRE-00664470$$jCCID-819838$$jORCID:0000-0003-1803-0999$$uDESY 002892661 700__ $$aCheng, Chun$$iINSPIRE-00690246$$jCCID-762859$$uDESY 002892661 700__ $$aColombina, Federica$$jCCID-846271$$jORCID:0009-0008-7130-100X$$uDESY 002892661 700__ $$aConsuegra Rodríguez, Sandra$$iINSPIRE-00648133$$jCCID-822284$$jORCID:0000-0002-1383-1837$$uDESY 002892661 700__ $$aCorreia Silva, Gilson$$iINSPIRE-00569055$$jCCID-804922$$jORCID:0000-0001-6232-3591$$uDESY 002892661 700__ $$aDe Silva, Malinda$$iINSPIRE-00701698$$jCCID-799918$$jORCID:0000-0002-5804-6226$$uDESY 002892661 700__ $$aEckerlin, Guenter$$iINSPIRE-00078894$$jCCID-380485$$uDESY 002892661 700__ $$aEckstein, Doris$$iINSPIRE-00078947$$jCCID-389567$$jORCID:0000-0002-7366-6562$$uDESY 002892661 700__ $$aEstevez Banos, Luis Ignacio$$iINSPIRE-00666814$$jCCID-830663$$jORCID:0000-0001-6195-3102$$uDESY 002892661 700__ $$aFilatov, Oleg$$iINSPIRE-00691573$$jCCID-796439$$jORCID:0000-0001-9850-6170$$uDESY 002892661 700__ $$aGallo, Elisabetta$$iINSPIRE-00083353$$jCCID-393837$$jORCID:0000-0001-7200-5175$$uDESY$$uHamburg U. 002892661 700__ $$aGeiser, Achim$$iINSPIRE-00315672$$jCCID-394752$$jORCID:0000-0003-0355-102X$$uDESY 002892661 700__ $$aGuglielmi, Valentina$$jCCID-849863$$jORCID:0000-0003-3240-7393$$uDESY 002892661 700__ $$aGuthoff, Moritz$$iINSPIRE-00204489$$jCCID-711375$$jORCID:0000-0002-3974-589X$$uDESY 002892661 700__ $$aHinzmann, Andreas$$iINSPIRE-00309577$$jCCID-670944$$jORCID:0000-0002-2633-4696$$uDESY 002892661 700__ $$aJeppe, Laurids$$jCCID-856577$$jORCID:0000-0002-1029-0318$$uDESY 002892661 700__ $$aKaech, Benno$$jCCID-846583$$jORCID:0000-0002-1194-2306$$uDESY 002892661 700__ $$aKasemann, Matthias$$iINSPIRE-00315684$$jCCID-404302$$jORCID:0000-0002-0429-2448$$uDESY 002892661 700__ $$aKleinwort, Claus$$iINSPIRE-00315708$$jCCID-405228$$jORCID:0000-0002-9017-9504$$uDESY 002892661 700__ $$aKogler, Roman$$iINSPIRE-00185267$$jCCID-644006$$jORCID:0000-0002-5336-4399$$uDESY 002892661 700__ $$aKomm, Matthias$$iINSPIRE-00360810$$jCCID-709764$$jORCID:0000-0002-7669-4294$$uDESY 002892661 700__ $$aKrücker, Dirk$$iINSPIRE-00205501$$jCCID-696594$$jORCID:0000-0003-1610-8844$$uDESY 002892661 700__ $$aLange, Wolfgang$$iINSPIRE-00315745$$jCCID-407551$$uDESY 002892661 700__ $$aLeyva Pernia, Daina$$jCCID-850996$$jORCID:0009-0009-8755-3698$$uDESY 002892661 700__ $$aLipka, Katerina$$iINSPIRE-00185340$$jCCID-721143$$jORCID:0000-0002-8427-3748$$uDESY 002892661 700__ $$aLohmann, Wolfgang$$iINSPIRE-00315751$$jCCID-410248$$jORCID:0000-0002-8705-0857$$uDESY$$uBrandenburg Tech. U. 002892661 700__ $$aLorkowski, Florian$$jCCID-859481$$jORCID:0000-0003-2677-3805$$uDESY 002892661 700__ $$aMankel, Rainer$$iINSPIRE-00315763$$jCCID-412107$$jORCID:0000-0003-2375-1563$$uDESY 002892661 700__ $$aMelzer-Pellmann, Isabell-Alissandra$$iINSPIRE-00326872$$jCCID-485425$$jORCID:0000-0001-7707-919X$$uDESY 002892661 700__ $$aMendizabal Morentin, Mikel$$iINSPIRE-00701274$$jCCID-834831$$jORCID:0000-0002-6506-5177$$uDESY 002892661 700__ $$aMeyer, Andreas Bernhard$$iINSPIRE-00160151$$jCCID-665299$$jORCID:0000-0001-8532-2356$$uDESY 002892661 700__ $$aMilella, Gabriele$$jCCID-847999$$jORCID:0000-0002-2047-951X$$uDESY 002892661 700__ $$aMoral Figueroa, Keila$$jCCID-863597$$jORCID:0000-0003-1987-1554$$uDESY 002892661 700__ $$aMussgiller, Andreas$$iINSPIRE-00191569$$jCCID-691481$$jORCID:0000-0002-8331-8166$$uDESY 002892661 700__ $$aNair, Lakshmi Priya$$jCCID-855344$$jORCID:0000-0002-2351-9265$$uDESY 002892661 700__ $$aNiedziela, Jeremi$$iINSPIRE-00508100$$jCCID-734471$$jORCID:0000-0002-9514-0799$$uDESY 002892661 700__ $$aNürnberg, Andreas$$iINSPIRE-00234914$$jCCID-718101$$jORCID:0000-0002-7876-3134$$uDESY 002892661 700__ $$aOtarid, Younes$$iINSPIRE-00697062$$jCCID-829499$$uDESY 002892661 700__ $$aPark, Jiwon$$iINSPIRE-00586827$$jCCID-819550$$jORCID:0000-0002-4683-6669$$uDESY 002892661 700__ $$aRanken, Evan$$iINSPIRE-00714972$$jCCID-821336$$jORCID:0000-0001-7472-5029$$uDESY 002892661 700__ $$aRaspereza, Alexei$$iINSPIRE-00191578$$jCCID-471115$$jORCID:0000-0003-2167-498X$$uDESY 002892661 700__ $$aRastorguev, Daniil$$jCCID-857876$$jORCID:0000-0001-6409-7794$$uDESY 002892661 700__ $$aRübenach, Jonas$$iINSPIRE-00693994$$jCCID-823097$$uDESY 002892661 700__ $$aRygaard, Lovisa$$jCCID-856470$$uDESY 002892661 700__ $$aSaggio, Alessia$$iINSPIRE-00551697$$jCCID-781532$$jORCID:0000-0002-7385-3317$$uDESY 002892661 700__ $$aScham, Moritz$$jCCID-839472$$jORCID:0000-0001-9494-2151$$uDESY$$uIAS, Julich$$uAachen, Tech. Hochsch. 002892661 700__ $$aSchnake, Simon$$iINSPIRE-00689294$$jCCID-829797$$jORCID:0000-0003-3409-6584$$uDESY$$uAachen, Tech. Hochsch. 002892661 700__ $$aSchütze, Paul$$iINSPIRE-00543466$$jCCID-785659$$jORCID:0000-0003-4802-6990$$uDESY 002892661 700__ $$aSchwanenberger, Christian$$iINSPIRE-00124643$$jCCID-430709$$jORCID:0000-0001-6699-6662$$uDESY$$uHamburg U. 002892661 700__ $$aSelivanova, Daria$$iINSPIRE-00693243$$jCCID-843167$$jORCID:0000-0002-7031-9434$$uDESY 002892661 700__ $$aSharko, Konstantin$$jCCID-803598$$jORCID:0000-0002-7614-5236$$uDESY 002892661 700__ $$aShchedrolosiev, Mykyta$$iINSPIRE-00679809$$jCCID-784962$$jORCID:0000-0003-3510-2093$$uDESY 002892661 700__ $$aStafford, Dominic$$iINSPIRE-00691208$$jCCID-843036$$uDESY 002892661 700__ $$aVazzoler, Federico$$iINSPIRE-00658302$$jCCID-760201$$jORCID:0000-0001-8111-9318$$uDESY 002892661 700__ $$aVentura Barroso, Ana$$jCCID-820524$$jORCID:0000-0003-3233-6636$$uDESY 002892661 700__ $$aWalsh, Roberval$$iINSPIRE-00209772$$jCCID-682181$$jORCID:0000-0002-3872-4114$$uDESY 002892661 700__ $$aWang, Di$$iINSPIRE-00702649$$jCCID-842212$$jORCID:0000-0002-0050-612X$$uDESY 002892661 700__ $$aWang, Qun$$iINSPIRE-00399615$$jCCID-754460$$jORCID:0000-0003-1014-8677$$uDESY 002892661 700__ $$aWen, Yiwen$$iINSPIRE-00535631$$jCCID-697662$$jORCID:0000-0002-8724-9604$$uDESY 002892661 700__ $$aWichmann, Katarzyna$$iINSPIRE-00346013$$jCCID-776759$$uDESY 002892661 700__ $$aWiens, Lucas$$iINSPIRE-00702214$$jCCID-822591$$jORCID:0000-0002-4423-4461$$uDESY$$uAachen, Tech. 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Phys. 002892661 700__ $$aNayak, Samarendra$$iINSPIRE-00688727$$jCCID-842106$$uBhubaneswar, NISER 002892661 700__ $$aPal, Kuldeep$$iINSPIRE-00801535$$jCCID-850252$$uBhubaneswar, NISER 002892661 700__ $$aSadangi, Priyanka$$iINSPIRE-00690905$$jCCID-842959$$uBhubaneswar, NISER 002892661 700__ $$aSwain, Sanjay Kumar$$iINSPIRE-00051724$$jCCID-710767$$jORCID:0000-0001-6871-3937$$uBhubaneswar, NISER 002892661 700__ $$aVarghese, Sanu$$iINSPIRE-00800641$$jCCID-849528$$jORCID:0009-0000-1318-8266$$uBhubaneswar, NISER$$uBhubaneswar, Inst. Phys. 002892661 700__ $$aVats, Diwakar$$iINSPIRE-00692218$$jCCID-833227$$jORCID:0009-0007-8224-4664$$uBhubaneswar, NISER$$uBhubaneswar, Inst. 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$$aVischia, Pietro$$iINSPIRE-00011001$$jCCID-697128$$jORCID:0000-0002-7088-8557$$uOviedo U. 002892661 700__ $$aBhowmik, Sandeep$$iINSPIRE-00271849$$jCCID-720826$$jORCID:0000-0003-1260-973X$$uCantabria Inst. of Phys. 002892661 700__ $$aBlanco Fernández, Sergio$$jCCID-850842$$jORCID:0000-0001-7301-0670$$uCantabria Inst. of Phys. 002892661 700__ $$aBrochero Cifuentes, Javier Andres$$iINSPIRE-00010796$$jCCID-700045$$jORCID:0000-0003-2093-7856$$uCantabria Inst. of Phys. 002892661 700__ $$aCabrillo, Iban Jose$$iINSPIRE-00307987$$jCCID-660921$$jORCID:0000-0002-0367-4022$$uCantabria Inst. of Phys. 002892661 700__ $$aCalderon, Alicia$$iINSPIRE-00308000$$jCCID-602442$$jORCID:0000-0002-7205-2040$$uCantabria Inst. of Phys. 002892661 700__ $$aDuarte Campderros, Jordi$$iINSPIRE-00308625$$jCCID-675320$$jORCID:0000-0003-0687-5214$$uCantabria Inst. of Phys. 002892661 700__ $$aFernandez, Marcos$$iINSPIRE-00320449$$jCCID-452999$$jORCID:0000-0002-4824-1087$$uCantabria Inst. of Phys. 002892661 700__ 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U. 002892661 700__ $$aCankocak, Kerem$$iINSPIRE-00070870$$jCCID-379968$$jORCID:0000-0002-3829-3481$$uIstanbul Tech. U. 002892661 700__ $$aDincer, Gizem Gul$$jCCID-856986$$jORCID:0009-0001-1997-2841$$uIstanbul Tech. U. 002892661 700__ $$aKomurcu, Yildiray$$iINSPIRE-00568824$$jCCID-804679$$jORCID:0000-0002-7084-030X$$uIstanbul Tech. U. 002892661 700__ $$aSen, Sercan$$iINSPIRE-00319470$$jCCID-680879$$jORCID:0000-0001-7325-1087$$uIstanbul Tech. U.$$uHacettepe U. 002892661 700__ $$aAydilek, Orhan$$jCCID-850539$$jORCID:0000-0002-2567-6766$$uIstanbul U.$$uErzincan U. 002892661 700__ $$aEpshteyn, Vladimir$$jCCID-390124$$jORCID:0000-0002-8863-6374$$uIstanbul U. 002892661 700__ $$aHacisahinoglu, Burak$$jCCID-850537$$jORCID:0000-0002-2646-1230$$uIstanbul U. 002892661 700__ $$aHos, Ilknur$$iINSPIRE-00309620$$jCCID-677013$$jORCID:0000-0002-7678-1101$$uIstanbul U. 002892661 700__ $$aKaynak, Berkan$$iINSPIRE-00676576$$jCCID-822978$$jORCID:0000-0003-3857-2496$$uIstanbul U. 002892661 700__ $$aOzkorucuklu, Suat$$iINSPIRE-00318653$$jCCID-541562$$jORCID:0000-0001-5153-9266$$uIstanbul U. 002892661 700__ $$aPotok, Onur$$jCCID-856242$$jORCID:0009-0005-1141-6401$$uIstanbul U. 002892661 700__ $$aSert, Hale$$iINSPIRE-00565668$$jCCID-799124$$jORCID:0000-0003-0716-6727$$uIstanbul U. 002892661 700__ $$aSimsek, Cagdas$$jCCID-827965$$jORCID:0000-0002-7359-8635$$uIstanbul U. 002892661 700__ $$aZorbilmez, Caglar$$iINSPIRE-00191896$$jCCID-694558$$jORCID:0000-0002-5199-061X$$uIstanbul U. 002892661 700__ $$aCerci, Salim$$iINSPIRE-00014144$$jCCID-638943$$jORCID:0000-0002-8702-6152$$uYildiz Tech. U.$$uAdiyaman U. 002892661 700__ $$aIsildak, Bora$$iINSPIRE-00309693$$jCCID-676887$$jORCID:0000-0002-0283-5234$$uYildiz Tech. U. 002892661 700__ $$aSunar Cerci, Deniz$$iINSPIRE-00185875$$jCCID-628292$$jORCID:0000-0002-5412-4688$$uYildiz Tech. U. 002892661 700__ $$aYetkin, Taylan$$iINSPIRE-00036263$$jCCID-619761$$jORCID:0000-0003-3277-5612$$uYildiz Tech. U. 002892661 700__ $$aBoyaryntsev, Andriy$$iINSPIRE-00390170$$jCCID-755222$$jORCID:0000-0001-9252-0430$$uInst. Scintill. Mat., Kharkiv 002892661 700__ $$aGrynyov, Boris$$jCCID-479424$$jORCID:0000-0003-1700-0173$$uInst. Scintill. 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Giovanna$$iINSPIRE-00801586$$jCCID-837254$$jORCID:0000-0002-2787-1063$$uRutherford 002892661 700__ $$aSchuh, Thomas$$iINSPIRE-00405225$$jCCID-757584$$uRutherford 002892661 700__ $$aShepherd-Themistocleous, Claire$$iINSPIRE-00300627$$jCCID-431511$$jORCID:0000-0003-0551-6949$$uRutherford 002892661 700__ $$aTomalin, Ian R.$$iINSPIRE-00131746$$jCCID-436145$$jORCID:0000-0003-2419-4439$$uRutherford 002892661 700__ $$aWhalen, Kathleen Charlotte$$jCCID-676064$$jORCID:0000-0002-9383-8763$$uRutherford 002892661 700__ $$aWilliams, Thomas$$iINSPIRE-00226123$$jCCID-691992$$jORCID:0000-0002-8724-4678$$uRutherford 002892661 700__ $$aAndreou, Irene$$jCCID-852667$$jORCID:0000-0002-3031-8728$$uImperial Coll., London 002892661 700__ $$aBainbridge, Robert$$iINSPIRE-00318783$$jCCID-525764$$jORCID:0000-0001-9157-4832$$uImperial Coll., London 002892661 700__ $$aBloch, Philippe$$iINSPIRE-00317838$$jCCID-375780$$jORCID:0000-0001-6716-979X$$uImperial Coll., London 002892661 700__ $$aBrown, Christopher Edward$$iINSPIRE-00699723$$jCCID-846011$$jORCID:0000-0002-7766-6615$$uImperial Coll., London 002892661 700__ $$aBuchmuller, Oliver$$iINSPIRE-00069840$$jCCID-444681$$uImperial Coll., London 002892661 700__ $$aCacchio, Vincenzo$$iINSPIRE-00663109$$jCCID-828747$$uImperial Coll., London 002892661 700__ $$aCarrillo Montoya, Camilo Andres$$iINSPIRE-00310740$$jCCID-657934$$jORCID:0000-0002-6245-6535$$uImperial Coll., London 002892661 700__ $$aChahal, Gurpreet Singh$$iINSPIRE-00227512$$jCCID-715610$$jORCID:0000-0003-0320-4407$$uImperial Coll., London 002892661 700__ $$aColling, David$$iINSPIRE-00074062$$jCCID-383237$$jORCID:0000-0001-9959-4977$$uImperial Coll., London 002892661 700__ $$aDancu, Julia Suzana$$iINSPIRE-00679844$$jCCID-825193$$uImperial Coll., London 002892661 700__ $$aDas, Indranil$$jCCID-659972$$jORCID:0000-0002-5437-2067$$uImperial Coll., London 002892661 700__ $$aDauncey, Paul$$iINSPIRE-00075860$$jCCID-385373$$jORCID:0000-0001-6839-9466$$uImperial Coll., London 002892661 700__ $$aDavies, Gavin$$iINSPIRE-00075967$$jCCID-385463$$jORCID:0000-0001-8668-5001$$uImperial Coll., London 002892661 700__ $$aDavies, Joe$$iINSPIRE-00680600$$jCCID-837615$$uImperial Coll., London 002892661 700__ $$aDella Negra, Michel$$iINSPIRE-00318819$$jCCID-386672$$jORCID:0000-0001-6497-8081$$uImperial Coll., London 002892661 700__ $$aFayer, Simon$$iINSPIRE-00280779$$jCCID-722554$$uImperial Coll., London 002892661 700__ $$aFedi, Giacomo$$iINSPIRE-00270970$$jCCID-683940$$jORCID:0000-0001-9101-2573$$uImperial Coll., London 002892661 700__ $$aHall, Geoffrey$$iINSPIRE-00300982$$jCCID-398789$$jORCID:0000-0002-6299-8385$$uImperial Coll., London 002892661 700__ $$aHassanshahi, Mohammad Hassan$$iINSPIRE-00678884$$jCCID-758526$$jORCID:0000-0001-6634-4517$$uImperial Coll., London 002892661 700__ $$aHoward, Alexander$$iINSPIRE-00091246$$jCCID-401174$$uImperial Coll., London 002892661 700__ $$aIles, Gregory$$iINSPIRE-00314080$$jCCID-444630$$jORCID:0000-0002-1219-5859$$uImperial Coll., London 002892661 700__ $$aKnight, Charlotte Rose$$jCCID-846741$$jORCID:0009-0008-1167-4816$$uImperial Coll., London 002892661 700__ $$aLangford, Jonathon$$iINSPIRE-00660610$$jCCID-797720$$jORCID:0000-0002-3931-4379$$uImperial Coll., London 002892661 700__ $$aLeón Holgado, Jaime$$iINSPIRE-00682593$$jCCID-838752$$jORCID:0000-0002-4156-6460$$uImperial Coll., London 002892661 700__ $$aLyons, Louis$$iINSPIRE-00103348$$jCCID-411137$$jORCID:0000-0001-7945-9188$$uImperial Coll., London 002892661 700__ $$aMagnan, Anne-Marie$$iINSPIRE-00049087$$jCCID-645372$$jORCID:0000-0002-4266-1646$$uImperial Coll., London 002892661 700__ $$aMallios, Stavros$$iINSPIRE-00508833$$jCCID-766931$$uImperial Coll., London 002892661 700__ $$aMieskolainen, Mikael$$iINSPIRE-00507452$$jCCID-726052$$jORCID:0000-0001-8893-7401$$uImperial Coll., London 002892661 700__ $$aNash, Jordan$$iINSPIRE-00030092$$jCCID-388020$$jORCID:0000-0003-0607-6519$$uImperial Coll., London$$uMonash U. 002892661 700__ $$aPesaresi, Mark$$iINSPIRE-00311333$$jCCID-659283$$jORCID:0000-0002-9759-1083$$uImperial Coll., London 002892661 700__ $$aPradeep, Prijith Babu$$jCCID-861189$$uImperial Coll., London 002892661 700__ $$aRadburn-Smith, Benjamin Charles$$iINSPIRE-00191917$$jCCID-693367$$jORCID:0000-0003-1488-9675$$uImperial Coll., London 002892661 700__ $$aRichards, Alexander$$iINSPIRE-00222470$$jCCID-666054$$uImperial Coll., London 002892661 700__ $$aRose, Andrew$$iINSPIRE-00016273$$jCCID-663940$$jORCID:0000-0002-9773-550X$$uImperial Coll., London 002892661 700__ $$aSavva, Klitos$$jCCID-852631$$jORCID:0009-0000-7646-3376$$uImperial Coll., London 002892661 700__ $$aSeez, Christopher$$iINSPIRE-00318860$$jCCID-430911$$jORCID:0000-0002-1637-5494$$uImperial Coll., London 002892661 700__ $$aShukla, Raghunandan$$iINSPIRE-00399483$$jCCID-756503$$jORCID:0000-0001-5670-5497$$uImperial Coll., London 002892661 700__ $$aTapper, Alexander$$iINSPIRE-00318872$$jCCID-659680$$jORCID:0000-0003-4543-864X$$uImperial Coll., London 002892661 700__ $$aUchida, Kirika$$iINSPIRE-00170836$$jCCID-675376$$jORCID:0000-0003-0742-2276$$uImperial Coll., London 002892661 700__ $$aUttley, George Peter$$iINSPIRE-00700612$$jCCID-846010$$jORCID:0009-0002-6248-6467$$uImperial Coll., London 002892661 700__ $$aVage, Liv Helen$$iINSPIRE-00699928$$jCCID-832622$$uImperial Coll., London 002892661 700__ $$aVirdee, Tejinder$$iINSPIRE-00318884$$jCCID-439393$$jORCID:0000-0001-7429-2198$$uImperial Coll., London$$uCERN 002892661 700__ $$aVojinovic, Milos$$iINSPIRE-01858298$$jCCID-840367$$jORCID:0000-0001-8665-2808$$uImperial Coll., London 002892661 700__ $$aWardle, Nicholas$$iINSPIRE-00208921$$jCCID-704437$$jORCID:0000-0003-1344-3356$$uImperial Coll., London 002892661 700__ $$aWinterbottom, Daniel$$iINSPIRE-00544977$$jCCID-763953$$jORCID:0000-0003-4582-150X$$uImperial Coll., London 002892661 700__ $$aColdham, Kathryn$$iINSPIRE-00676554$$jCCID-748993$$uBrunel U. 002892661 700__ $$aCole, Joanne$$iINSPIRE-00318908$$jCCID-577588$$jORCID:0000-0001-5638-7599$$uBrunel U. 002892661 700__ $$aKhan, Akram$$iINSPIRE-00095864$$jCCID-404741$$uBrunel U. 002892661 700__ $$aKyberd, Paul$$iINSPIRE-00099432$$jCCID-406952$$jORCID:0000-0002-7353-7090$$uBrunel U. 002892661 700__ $$aReid, Ivan$$iINSPIRE-00311679$$jCCID-609788$$jORCID:0000-0002-9235-779X$$uBrunel U. 002892661 700__ $$aAbdullin, Salavat$$iINSPIRE-00060681$$jCCID-369064$$jORCID:0000-0003-4885-6935$$uBaylor U. 002892661 700__ $$aBrinkerhoff, Andrew$$iINSPIRE-00202930$$jCCID-706972$$jORCID:0000-0002-4819-7995$$uBaylor U. 002892661 700__ $$aCaraway, Bryan$$iINSPIRE-00654169$$jCCID-825055$$jORCID:0000-0002-6088-2020$$uBaylor U. 002892661 700__ $$aCollins, Evan$$jCCID-860848$$jORCID:0009-0008-1661-3537$$uBaylor U. 002892661 700__ $$aDittmann, Jay$$iINSPIRE-00077316$$jCCID-702770$$jORCID:0000-0002-1911-3158$$uBaylor U. 002892661 700__ $$aHatakeyama, Kenichi$$iINSPIRE-00054461$$jCCID-661802$$jORCID:0000-0002-6012-2451$$uBaylor U. 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Inst. 002892661 700__ $$aObraztsov, Stepan$$iINSPIRE-00191763$$jCCID-419057$$jORCID:0009-0001-1152-2758$$uUnlisted 002892661 700__ $$aOreshkin, Vadim$$iINSPIRE-00010613$$jCCID-696983$$jORCID:0000-0003-4749-4995$$uUnlisted 002892661 700__ $$aPalichik, Vladimir$$iINSPIRE-00317375$$jCCID-444992$$jORCID:0009-0008-0356-1061$$uUnlisted 002892661 700__ $$aPerelygin, Victor$$iINSPIRE-00311280$$jCCID-421526$$jORCID:0009-0005-5039-4874$$uUnlisted 002892661 700__ $$aPetrushanko, Sergey$$iINSPIRE-00037084$$jCCID-501302$$jORCID:0000-0003-0210-9061$$uUnlisted 002892661 700__ $$aPolikarpov, Sergey$$iINSPIRE-00529689$$jCCID-732717$$jORCID:0000-0001-6839-928X$$uUnlisted 002892661 700__ $$aPopov, Vladimir$$iINSPIRE-00209688$$jCCID-633720$$jORCID:0000-0001-8049-2583$$uUnlisted 002892661 700__ $$aRadchenko, Olesia$$iINSPIRE-00674727$$jCCID-834843$$jORCID:0000-0001-7116-9469$$uUnlisted 002892661 700__ $$aSavina, Maria$$iINSPIRE-00207880$$jCCID-520117$$jORCID:0000-0002-9020-7384$$uUnlisted 002892661 700__ $$aSavrin, Viktor$$iINSPIRE-00317557$$jCCID-477961$$jORCID:0009-0000-3973-2485$$uUnlisted 002892661 700__ $$aShalaev, Vladislav$$iINSPIRE-00671767$$jCCID-817405$$jORCID:0000-0002-2893-6922$$uUnlisted 002892661 700__ $$aShmatov, Sergey$$iINSPIRE-00317387$$jCCID-513929$$jORCID:0000-0001-5354-8350$$uUnlisted 002892661 700__ $$aShulha, Siarhei$$iINSPIRE-00231309$$jCCID-579032$$jORCID:0000-0002-4265-928X$$uUnlisted 002892661 700__ $$aSkovpen, Yuri$$iINSPIRE-00042992$$jCCID-768842$$jORCID:0000-0002-3316-0604$$uUnlisted 002892661 700__ $$aSlabospitskii, Sergei$$iINSPIRE-00127022$$jCCID-479363$$jORCID:0000-0001-8178-2494$$uUnlisted 002892661 700__ $$aSmirnov, Vitaly$$iINSPIRE-00176404$$jCCID-432414$$jORCID:0000-0002-9049-9196$$uUnlisted 002892661 700__ $$aSnigirev, Alexander$$iINSPIRE-00317569$$jCCID-470468$$jORCID:0000-0003-2952-6156$$uUnlisted 002892661 700__ $$aSosnov, Dmitry$$iINSPIRE-00540151$$jCCID-784833$$jORCID:0000-0002-7452-8380$$uUnlisted 002892661 700__ $$aSulimov, Valentin$$iINSPIRE-00312301$$jCCID-433007$$jORCID:0009-0009-8645-6685$$uUnlisted 002892661 700__ $$aTcherniaev, Evgueni$$iINSPIRE-00563506$$jCCID-435124$$jORCID:0000-0002-3685-0635$$uUnlisted 002892661 700__ $$aTerkulov, Adel$$iINSPIRE-00208530$$jCCID-456374$$jORCID:0000-0003-4985-3226$$uUnlisted 002892661 700__ $$aTeryaev, Oleg$$iINSPIRE-00208541$$jCCID-644823$$jORCID:0000-0001-7002-9093$$uUnlisted 002892661 700__ $$aTlisova, Irina$$iINSPIRE-00654576$$jCCID-824692$$jORCID:0000-0003-1552-2015$$uUnlisted 002892661 700__ $$aToropin, Alexander$$iINSPIRE-00317480$$jCCID-436310$$jORCID:0000-0002-2106-4041$$uUnlisted 002892661 700__ $$aUvarov, Lev$$iINSPIRE-00021932$$jCCID-610284$$jORCID:0000-0002-7602-2527$$uUnlisted 002892661 700__ $$aUzunian, Andrey$$iINSPIRE-00018369$$jCCID-419857$$jORCID:0000-0002-7007-9020$$uUnlisted 002892661 700__ $$aVorobyev, Alexey$$iINSPIRE-00312898$$jCCID-439817$$uUnlisted 002892661 700__ $$aVoytishin, Nikolay$$iINSPIRE-00523315$$jCCID-737873$$jORCID:0000-0001-6590-6266$$uUnlisted 002892661 700__ $$aYuldashev, Bekhzod S.$$iINSPIRE-00209079$$jCCID-442270$$uUnlisted$$uTashkent, IYF 002892661 700__ $$aZarubin, Anatoli$$iINSPIRE-00317400$$jCCID-369703$$jORCID:0000-0002-1964-6106$$uUnlisted 002892661 700__ $$aZhizhin, Ilia$$iINSPIRE-00671892$$jCCID-817403$$jORCID:0000-0001-6171-9682$$uUnlisted 002892661 700__ $$aZhokin, Alexander$$iINSPIRE-00317515$$jCCID-626383$$jORCID:0000-0001-7178-5907$$uUnlisted 002892661 710__ $$gCMS Collaboration 002892661 710__ $$5PH-EP 002892661 859__ $$fcms-publication-committee-chair@cern.ch 002892661 8564_ $$uhttp://cms.cern.ch/iCMS/analysisadmin/cadi?ancode=B2G-23-002$$yAdditional information for the analysis 002892661 8564_ $$uhttp://cms.cern.ch/iCMS/analysisadmin/authorinfo?ancode=B2G-23-002$$yCMS AuthorList 002892661 8564_ $$82520130$$s9116147$$uhttp://cds.cern.ch/record/2892661/files/CMS-B2G-23-002-arXiv.pdf$$yFulltext 002892661 8564_ $$uhttps://www.hepdata.net/record/146897$$yCMS HEPData 002892661 8564_ $$82522104$$s738333$$uhttp://cds.cern.ch/record/2892661/files/Figure_041.png$$y00094 Contours of the variable \Rint as defined in Eq.~(\ref{eq:Rint}) and discussed in the text, in the ($\sin\alpha$, \couplingLambda) plane for the singlet model with $\kappaLambda = 1$ and different resonance masses \mX between (upper \cmsLeft) 280 and (lower \cmsRight) 800\GeV. Contours are shown for \Rint values of (dashed blue) $-0.2$, (solid blue) $-0.1$, (solid green) $+0.1$, and (dashed green) $+0.2$. Regions that are excluded, at 95\%~\CL, from the combined likelihood analysis of the \HH analyses presented in this report are indicated by red filled areas. Dashed black lines indicate constant relative widths of 5, 10, and 20\%. 002892661 8564_ $$82522105$$s46206$$uhttp://cds.cern.ch/record/2892661/files/Figure_028-a.png$$y00059 Search for $\PX\to\PH\PH$/$\PG\to\PH\PH$: Observed and expected 95\%~\CL upper limits on the product of the cross section $\sigma$ for the production of a (\cmsLeft) spin-0 resonance \PX and (\cmsRight) a spin-2 resonance \PG, via gluon-gluon fusion, and the branching fraction \BR for the corresponding \HH decay, as obtained from the combined likelihood analysis of all contributing individual analyses presented in this report and shown in Fig.~\ref{fig:Limits_on_HH}. In addition to the limit from the combined likelihood analysis the 68 and 95\% central intervals for the expected upper limits in the absence of a signal are shown as coloured bands. 002892661 8564_ $$82522106$$s23847$$uhttp://cds.cern.ch/record/2892661/files/Figure_028-b.png$$y00060 Search for $\PX\to\PH\PH$/$\PG\to\PH\PH$: Observed and expected 95\%~\CL upper limits on the product of the cross section $\sigma$ for the production of a (\cmsLeft) spin-0 resonance \PX and (\cmsRight) a spin-2 resonance \PG, via gluon-gluon fusion, and the branching fraction \BR for the corresponding \HH decay, as obtained from the combined likelihood analysis of all contributing individual analyses presented in this report and shown in Fig.~\ref{fig:Limits_on_HH}. In addition to the limit from the combined likelihood analysis the 68 and 95\% central intervals for the expected upper limits in the absence of a signal are shown as coloured bands. 002892661 8564_ $$82522107$$s21339$$uhttp://cds.cern.ch/record/2892661/files/Figure_053-b.png$$y00119 Interpretation of the upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, obtained from the projections to an integrated luminosity of 3000\fbinv of the (upper \cmsLeft) $\PY(\bb)\PH(\gamma\gamma)$~\cite{CMS:2023boe}, (upper \cmsRight) $\PY(\bb)\PH(\tautau)$~\cite{CMS:2021yci}, and (lower row) $\PY(\bb)\PH(\bb)$~\cite{CMS:2022suh} analyses, assuming the S2 systematic uncertainty scenario. The projected limits are mapped onto the (\MX, \MY) plane, and compared with the maximally allowed cross sections of the NMSSM (\cmsLeft and upper \cmsRight), and TRSM models (lower \cmsRight) discussed in Section~\ref{Subsubsec:Interpretations_NMSSM_TRSM}. The points indicate the available theory predictions. The mass dependences of both the projected experimental limits and the maximally allowed theory cross sections have been interpolated to obtain approximate exclusion contours. The NMSSM predictions based on \textsc{NMSSMTools} version 5.6.2 are adapted from Ref.~\cite{Ellwanger:2022jtd}, whereas the TRSM is described in Ref.~\cite{Robens:2019kga}. In both cases, the model predictions have been scaled to $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522108$$s18507$$uhttp://cds.cern.ch/record/2892661/files/Figure_053-c.png$$y00120 Interpretation of the upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, obtained from the projections to an integrated luminosity of 3000\fbinv of the (upper \cmsLeft) $\PY(\bb)\PH(\gamma\gamma)$~\cite{CMS:2023boe}, (upper \cmsRight) $\PY(\bb)\PH(\tautau)$~\cite{CMS:2021yci}, and (lower row) $\PY(\bb)\PH(\bb)$~\cite{CMS:2022suh} analyses, assuming the S2 systematic uncertainty scenario. The projected limits are mapped onto the (\MX, \MY) plane, and compared with the maximally allowed cross sections of the NMSSM (\cmsLeft and upper \cmsRight), and TRSM models (lower \cmsRight) discussed in Section~\ref{Subsubsec:Interpretations_NMSSM_TRSM}. The points indicate the available theory predictions. The mass dependences of both the projected experimental limits and the maximally allowed theory cross sections have been interpolated to obtain approximate exclusion contours. The NMSSM predictions based on \textsc{NMSSMTools} version 5.6.2 are adapted from Ref.~\cite{Ellwanger:2022jtd}, whereas the TRSM is described in Ref.~\cite{Robens:2019kga}. In both cases, the model predictions have been scaled to $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522109$$s876751$$uhttp://cds.cern.ch/record/2892661/files/Figure_049.png$$y00112 Exclusion contours at 95\%~\CL, in the ($\sin\alpha$, \couplingLambda) plane for $\kappaLambda = 1$ in the real-singlet model. These contours are obtained from the combined likelihood analysis of the \HH searches discussed in Section~\ref{Sec:Interp_in_Extended_Higgs_sector} for (upper \cmsLeft to lower \cmsRight) $\mX = 280$, 400, 500, 600, 700, and 1000\GeV. The expected limits from the Run~2 dataset have been projected to integrated luminosities of 300, 1000, and 3000\fbinv. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522110$$s64839$$uhttp://cds.cern.ch/record/2892661/files/Figure_048.png$$y00111 Expected lower limit at 95\%~\CL, on \LambdaR in the warped extra dimensions bulk scenario for the production of a radion \PR, as a function of $m_{\PR}$. The limits are derived from the combined likelihood analysis of the \HH searches discussed in Section~\ref{Sec:Interp_in_Warped_Extra_Dimensions} and shown in Fig.~\ref{fig:Int_WED}, for different values of the integrated luminosity. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522111$$s20850$$uhttp://cds.cern.ch/record/2892661/files/Figure_053-d.png$$y00121 Interpretation of the upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, obtained from the projections to an integrated luminosity of 3000\fbinv of the (upper \cmsLeft) $\PY(\bb)\PH(\gamma\gamma)$~\cite{CMS:2023boe}, (upper \cmsRight) $\PY(\bb)\PH(\tautau)$~\cite{CMS:2021yci}, and (lower row) $\PY(\bb)\PH(\bb)$~\cite{CMS:2022suh} analyses, assuming the S2 systematic uncertainty scenario. The projected limits are mapped onto the (\MX, \MY) plane, and compared with the maximally allowed cross sections of the NMSSM (\cmsLeft and upper \cmsRight), and TRSM models (lower \cmsRight) discussed in Section~\ref{Subsubsec:Interpretations_NMSSM_TRSM}. The points indicate the available theory predictions. The mass dependences of both the projected experimental limits and the maximally allowed theory cross sections have been interpolated to obtain approximate exclusion contours. The NMSSM predictions based on \textsc{NMSSMTools} version 5.6.2 are adapted from Ref.~\cite{Ellwanger:2022jtd}, whereas the TRSM is described in Ref.~\cite{Robens:2019kga}. In both cases, the model predictions have been scaled to $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522112$$s43151$$uhttp://cds.cern.ch/record/2892661/files/Figure_012-b.png$$y00028 (\cmsLeft) Branching fraction for the decay $\PZpr\to\PZ\PH$, and (\cmsRight) total width of the \PZpr boson, for a resonance with 2\TeV mass, for different values of the parameter \gF. Calculations are based the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522113$$s47688$$uhttp://cds.cern.ch/record/2892661/files/Figure_012-a.png$$y00027 (\cmsLeft) Branching fraction for the decay $\PZpr\to\PZ\PH$, and (\cmsRight) total width of the \PZpr boson, for a resonance with 2\TeV mass, for different values of the parameter \gF. Calculations are based the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522114$$s16621$$uhttp://cds.cern.ch/record/2892661/files/Figure_046.png$$y00108 Expected discovery significance for a spin-0 resonance \PX with $\mX=1\TeV$ and cross sections of 1 and 10\unit{fb}, obtained for the combined likelihood analysis of the resonant \HH searches as discussed in Section~\ref{Sec:DiscoveryPotential} and shown in Figs.~\ref{fig:XHH_projections_bychannel} and~\ref{fig:XHHcomb_projections}, shown as function of the integrated luminosity. 002892661 8564_ $$82522115$$s11072$$uhttp://cds.cern.ch/record/2892661/files/Figure_009-b.png$$y00020 Feynman diagrams for the production of \PZpr and \PWpr bosons produced through the (\cmsLeft) Drell--Yan and (\cmsRight) vector boson fusion process. The \PZpr (resp. \PWpr) boson subsequently decays into \ZH and \WH, respectively. 002892661 8564_ $$82522116$$s9668$$uhttp://cds.cern.ch/record/2892661/files/Figure_009-a.png$$y00019 Feynman diagrams for the production of \PZpr and \PWpr bosons produced through the (\cmsLeft) Drell--Yan and (\cmsRight) vector boson fusion process. The \PZpr (resp. \PWpr) boson subsequently decays into \ZH and \WH, respectively. 002892661 8564_ $$82522117$$s22151$$uhttp://cds.cern.ch/record/2892661/files/Figure_044-b.png$$y00104 Expected upper limits at 95\%~\CL, on the product of the cross section for the production of a spin-0 resonance \PX and the branching fraction $\BR(\PX \to\PH\PH)$, as functions of \MX from the (upper \cmsLeft) \bbtt~\cite{CMS:2021yci}, (upper \cmsRight) \bbgg~\cite{CMS:2023boe}, and (lower) \bbbb with two merged \bb jets~\cite{CMS:2022suh} analyses discussed in this report, projected to an integrated luminosity of 3000\fbinv under the assumption of different systematic uncertainty scenarios, as discussed in the text. All estimates include the anticipated statistical uncertainties. 002892661 8564_ $$82522118$$s39331$$uhttp://cds.cern.ch/record/2892661/files/Figure_011-a.png$$y00023 Branching fractions for heavy vector triplet (HVT) bosons with masses of (upper) 1 and (lower) 2\TeV for values of the parameter \gF corresponding to models (\cmsLeft) A and (\cmsRight) B. The exact branching fractions of each model are indicated by the crossing points of the individual curves with the dashed vertical lines. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522119$$s68453$$uhttp://cds.cern.ch/record/2892661/files/Figure_027-a.png$$y00057 Search for $\PX\to\PH\PH$/$\PG\to\PH\PH$: Observed and expected 95\%~\CL upper limits on the product of the cross section $\sigma$ for the production of a (\cmsLeft) spin-0 resonance \PX and (\cmsRight) a spin-2 resonance \PG, via gluon-gluon fusion and the branching fraction \BR for the corresponding \HH decay. The results of the individual analyses presented in this report and the result of their combined likelihood analysis are shown. The observed limits are indicated by markers connected with solid lines and the expected limits by dashed lines. 002892661 8564_ $$82522120$$s38093$$uhttp://cds.cern.ch/record/2892661/files/Figure_011-c.png$$y00025 Branching fractions for heavy vector triplet (HVT) bosons with masses of (upper) 1 and (lower) 2\TeV for values of the parameter \gF corresponding to models (\cmsLeft) A and (\cmsRight) B. The exact branching fractions of each model are indicated by the crossing points of the individual curves with the dashed vertical lines. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522121$$s44952$$uhttp://cds.cern.ch/record/2892661/files/Figure_011-d.png$$y00026 Branching fractions for heavy vector triplet (HVT) bosons with masses of (upper) 1 and (lower) 2\TeV for values of the parameter \gF corresponding to models (\cmsLeft) A and (\cmsRight) B. The exact branching fractions of each model are indicated by the crossing points of the individual curves with the dashed vertical lines. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522122$$s20439$$uhttp://cds.cern.ch/record/2892661/files/Figure_047-a.png$$y00109 Expected exclusion contours at 95\%~\CL, in the (\tanb, \mA) plane of the (\cmsLeft) hMSSM and (\cmsRight) \MhEFTScen scenarios obtained from the combined likelihood analysis of the \HH searches discussed in Section~\ref{Sec:Interp_in_Extended_Higgs_sector} and shown in Figs.~\ref{fig:hMSSM} and~\ref{fig:MSSM_mh125}, for different integrated luminosities and compared to the Run 2 result obtained at $\sqrt{s}=13\TeV$. The projections assume $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522123$$s54357$$uhttp://cds.cern.ch/record/2892661/files/Figure_016-d.png$$y00037 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\text{j}\PH}$, and (\cmsRight) the mass or transverse mass of the X resonance candidate, labeled \MX and $m_{\PX}^{\mathrm{T}}$, respectively, in the $\Zll\PH(\bb)$ (upper) and $\Znn\PH(\bb)$ channels (lower). The shaded area depicts a veto region excluded from the analysis to minimize the event overlap with dedicated searches in the \VV decay channel. Figures from Ref.~\cite{CMS:2021fyk}. 002892661 8564_ $$82522124$$s59452$$uhttp://cds.cern.ch/record/2892661/files/Figure_016-c.png$$y00036 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\text{j}\PH}$, and (\cmsRight) the mass or transverse mass of the X resonance candidate, labeled \MX and $m_{\PX}^{\mathrm{T}}$, respectively, in the $\Zll\PH(\bb)$ (upper) and $\Znn\PH(\bb)$ channels (lower). The shaded area depicts a veto region excluded from the analysis to minimize the event overlap with dedicated searches in the \VV decay channel. Figures from Ref.~\cite{CMS:2021fyk}. 002892661 8564_ $$82522125$$s49248$$uhttp://cds.cern.ch/record/2892661/files/Figure_016-b.png$$y00035 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\text{j}\PH}$, and (\cmsRight) the mass or transverse mass of the X resonance candidate, labeled \MX and $m_{\PX}^{\mathrm{T}}$, respectively, in the $\Zll\PH(\bb)$ (upper) and $\Znn\PH(\bb)$ channels (lower). The shaded area depicts a veto region excluded from the analysis to minimize the event overlap with dedicated searches in the \VV decay channel. Figures from Ref.~\cite{CMS:2021fyk}. 002892661 8564_ $$82522126$$s53949$$uhttp://cds.cern.ch/record/2892661/files/Figure_016-a.png$$y00034 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\text{j}\PH}$, and (\cmsRight) the mass or transverse mass of the X resonance candidate, labeled \MX and $m_{\PX}^{\mathrm{T}}$, respectively, in the $\Zll\PH(\bb)$ (upper) and $\Znn\PH(\bb)$ channels (lower). The shaded area depicts a veto region excluded from the analysis to minimize the event overlap with dedicated searches in the \VV decay channel. Figures from Ref.~\cite{CMS:2021fyk}. 002892661 8564_ $$82522127$$s53488$$uhttp://cds.cern.ch/record/2892661/files/Figure_023-b.png$$y00051 Search for $\PX\to\PY(\bb)\PH(\bb)$: Distributions of the (\cmsLeft) soft-drop mass of the boosted \PY candidate, labeled $M^\PY_\text{J}$, and (\cmsRight) the dijet mass of the \PY and \PH candidates, $M_\text{JJ}$, in the high-purity SR of the $\PY(\bb)\PH(\bb)$ analysis with two merged \bb jets~\cite{CMS:2022suh}. The distributions as expected for signals with three different values of \mX and \mY (labeled $M^\PX$ and $M^\PY$) are also shown. In the lower panels the statistical pull in each bin is displayed. Figure from Ref.~\cite{CMS:2022suh}. 002892661 8564_ $$82522128$$s20176$$uhttp://cds.cern.ch/record/2892661/files/Figure_053-a.png$$y00118 Interpretation of the upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, obtained from the projections to an integrated luminosity of 3000\fbinv of the (upper \cmsLeft) $\PY(\bb)\PH(\gamma\gamma)$~\cite{CMS:2023boe}, (upper \cmsRight) $\PY(\bb)\PH(\tautau)$~\cite{CMS:2021yci}, and (lower row) $\PY(\bb)\PH(\bb)$~\cite{CMS:2022suh} analyses, assuming the S2 systematic uncertainty scenario. The projected limits are mapped onto the (\MX, \MY) plane, and compared with the maximally allowed cross sections of the NMSSM (\cmsLeft and upper \cmsRight), and TRSM models (lower \cmsRight) discussed in Section~\ref{Subsubsec:Interpretations_NMSSM_TRSM}. The points indicate the available theory predictions. The mass dependences of both the projected experimental limits and the maximally allowed theory cross sections have been interpolated to obtain approximate exclusion contours. The NMSSM predictions based on \textsc{NMSSMTools} version 5.6.2 are adapted from Ref.~\cite{Ellwanger:2022jtd}, whereas the TRSM is described in Ref.~\cite{Robens:2019kga}. In both cases, the model predictions have been scaled to $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522129$$s60877$$uhttp://cds.cern.ch/record/2892661/files/Figure_023-a.png$$y00050 Search for $\PX\to\PY(\bb)\PH(\bb)$: Distributions of the (\cmsLeft) soft-drop mass of the boosted \PY candidate, labeled $M^\PY_\text{J}$, and (\cmsRight) the dijet mass of the \PY and \PH candidates, $M_\text{JJ}$, in the high-purity SR of the $\PY(\bb)\PH(\bb)$ analysis with two merged \bb jets~\cite{CMS:2022suh}. The distributions as expected for signals with three different values of \mX and \mY (labeled $M^\PX$ and $M^\PY$) are also shown. In the lower panels the statistical pull in each bin is displayed. Figure from Ref.~\cite{CMS:2022suh}. 002892661 8564_ $$82522130$$s76340$$uhttp://cds.cern.ch/record/2892661/files/Figure_030.png$$y00062 Search for $\PX\to\PY\PH$: Observed and expected upper limits, at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb) \PH$ decay. For the branching fractions of the $\PH\to\tautau$ and $\PH\to\bb$ decays, the SM values are assumed. The results derived from the individual analyses presented in this report and the result of their combined likelihood analysis are shown as functions of \mY and \mX for $\mX\ge1.2\TeV$. Observed limits are indicated by markers connected with solid lines, expected limits by dashed lines. For presentation purposes, the limits have been scaled in successive steps by four orders of magnitude, each. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522131$$s94229$$uhttp://cds.cern.ch/record/2892661/files/Figure_042-d.png$$y00098 Expected differential cross sections for \HH production, as a function of \mHH, for the real-singlet model with $\mX = 280\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522132$$s46076$$uhttp://cds.cern.ch/record/2892661/files/Figure_034-c.png$$y00073 (Upper \cmsLeft) Observed and (upper \cmsRight) expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as obtained from a combined likelihood analysis of the individual analyses presented in this report and shown in Fig.~\ref{fig:XYH_combination}. The results are presented in a plane defined by \mX and \mY. The limits have been evaluated in discrete steps corresponding to the centers of the boxes. The numbers in the boxes are given in~\unit{fb}. The corresponding maximally allowed values of $\sigma\BR$ in the NMSSM are also shown for comparison (lower plot), as adapted from Ref.~\cite{Ellwanger:2022jtd}. 002892661 8564_ $$82522133$$s47650$$uhttp://cds.cern.ch/record/2892661/files/Figure_034-b.png$$y00072 (Upper \cmsLeft) Observed and (upper \cmsRight) expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as obtained from a combined likelihood analysis of the individual analyses presented in this report and shown in Fig.~\ref{fig:XYH_combination}. The results are presented in a plane defined by \mX and \mY. The limits have been evaluated in discrete steps corresponding to the centers of the boxes. The numbers in the boxes are given in~\unit{fb}. The corresponding maximally allowed values of $\sigma\BR$ in the NMSSM are also shown for comparison (lower plot), as adapted from Ref.~\cite{Ellwanger:2022jtd}. 002892661 8564_ $$82522134$$s46945$$uhttp://cds.cern.ch/record/2892661/files/Figure_034-a.png$$y00071 (Upper \cmsLeft) Observed and (upper \cmsRight) expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as obtained from a combined likelihood analysis of the individual analyses presented in this report and shown in Fig.~\ref{fig:XYH_combination}. The results are presented in a plane defined by \mX and \mY. The limits have been evaluated in discrete steps corresponding to the centers of the boxes. The numbers in the boxes are given in~\unit{fb}. The corresponding maximally allowed values of $\sigma\BR$ in the NMSSM are also shown for comparison (lower plot), as adapted from Ref.~\cite{Ellwanger:2022jtd}. 002892661 8564_ $$82522135$$s15951$$uhttp://cds.cern.ch/record/2892661/files/Figure_002-a.png$$y00002 Signal strength parameters extracted for various production modes $\mu_i$, assuming the branching fractions $\BR^f = \BR^\text{f}_\text{SM}$ (\cmsLeft), and decay channels $\mu^\text{f}$, assuming the production cross sections as predicted by the SM (\cmsRight). The thick and thin black lines indicate the one and two \SD confidence intervals (labelled by SD in the figures), with the systematic and statistical components of the former indicated by the red and blue bands, respectively. The vertical dashed line at unity represents the values of $\mu_i$ (resp. $\mu^\text{f}$) in the SM. Taken from Ref~\cite{CMS:2022dwd}. 002892661 8564_ $$82522136$$s32577$$uhttp://cds.cern.ch/record/2892661/files/Figure_002-b.png$$y00003 Signal strength parameters extracted for various production modes $\mu_i$, assuming the branching fractions $\BR^f = \BR^\text{f}_\text{SM}$ (\cmsLeft), and decay channels $\mu^\text{f}$, assuming the production cross sections as predicted by the SM (\cmsRight). The thick and thin black lines indicate the one and two \SD confidence intervals (labelled by SD in the figures), with the systematic and statistical components of the former indicated by the red and blue bands, respectively. The vertical dashed line at unity represents the values of $\mu_i$ (resp. $\mu^\text{f}$) in the SM. Taken from Ref~\cite{CMS:2022dwd}. 002892661 8564_ $$82522137$$s57693$$uhttp://cds.cern.ch/record/2892661/files/Figure_019-a.png$$y00042 Search for $\PX\to\PH(\bb)\PH(\PW\PW)$: Distributions of the \mHH variable, in the (\cmsLeft) SL and (\cmsRight) DL categories of the $\PH(\bb)\PH(\PW\PW)$ analysis with merged jets~\cite{CMS:2021roc}. Expected signal distributions from a spin-0 resonance with a mass of 1 or 3\TeV are also shown, by the open green and blue histograms. Figure from Ref.~\cite{CMS:2021roc}. 002892661 8564_ $$82522138$$s63770$$uhttp://cds.cern.ch/record/2892661/files/Figure_019-b.png$$y00043 Search for $\PX\to\PH(\bb)\PH(\PW\PW)$: Distributions of the \mHH variable, in the (\cmsLeft) SL and (\cmsRight) DL categories of the $\PH(\bb)\PH(\PW\PW)$ analysis with merged jets~\cite{CMS:2021roc}. Expected signal distributions from a spin-0 resonance with a mass of 1 or 3\TeV are also shown, by the open green and blue histograms. Figure from Ref.~\cite{CMS:2021roc}. 002892661 8564_ $$82522139$$s60234$$uhttp://cds.cern.ch/record/2892661/files/Figure_024.png$$y00052 Search for $\PX\to\PZ\PH$: Observed and expected 95\% \CL upper limits on the product of the cross section $\sigma$ for the production of an \PA boson, via gluon-gluon fusion and the branching fraction \BR for the $\PA\to\PZ\PH$ decay. The limits are given in \unit{pb} as functions of \mA. The markers connected with solid lines (dashed lines) indicate the observed (expected) limits. The green (magenta) lines refer to the $\PZ(\lep+\nn)\PH(\bb)$~\cite{CMS:2019qcx} ($\PZ(\lep)\PH(\tautau )$~\cite{CMS:2019kca}) analysis. The red and blue solid lines indicate the product $\sigma\BR$ as expected by the 2HDM Type~I and Type~II models, respectively, for the parameters $\tan\beta=3$ and $\cosba=0.1$. The shaded areas associated with these predictions indicate the corresponding model uncertainties. The results and model predictions have been adapted from Refs.~\cite{CMS:2019qcx, CMS:2019kca}. 002892661 8564_ $$82522140$$s66871$$uhttp://cds.cern.ch/record/2892661/files/Figure_039-b.png$$y00089 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report and the $\PV\PV$ channels of Refs.~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt} and $\Pell\PGn$~\cite{CMS:2022krd} final states. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522141$$s65973$$uhttp://cds.cern.ch/record/2892661/files/Figure_039-c.png$$y00090 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report and the $\PV\PV$ channels of Refs.~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt} and $\Pell\PGn$~\cite{CMS:2022krd} final states. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522142$$s66573$$uhttp://cds.cern.ch/record/2892661/files/Figure_039-a.png$$y00088 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report and the $\PV\PV$ channels of Refs.~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt} and $\Pell\PGn$~\cite{CMS:2022krd} final states. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522143$$s79285$$uhttp://cds.cern.ch/record/2892661/files/Figure_029.png$$y00061 Search for $\PX\to\PY\PH$: Observed and expected upper limits, at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb) \PH$ decay. For the branching fractions of the $\PH\to\tautau$, $\PH\to\gamma\gamma$ and $\PH\to\bb$ decays, the SM values are assumed. The results derived from the individual analyses presented in this report and the result of their combined likelihood analysis are shown as functions of \mY and \mX for $\mX\le1\TeV$. Observed limits are indicated by markers connected with solid lines, expected limits by dashed lines. For presentation purposes, the limits have been scaled in successive steps by two orders of magnitude, each. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522144$$s69439$$uhttp://cds.cern.ch/record/2892661/files/Figure_039-d.png$$y00091 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report and the $\PV\PV$ channels of Refs.~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt} and $\Pell\PGn$~\cite{CMS:2022krd} final states. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522145$$s49678$$uhttp://cds.cern.ch/record/2892661/files/Figure_040-a.png$$y00092 Obseved upper limits, at 95\% \CL, on the coupling \gH within the heavy vector triplet model, as a function of the \PVpr mass. The limits are shown for the vecotr boson fusion production mode in the context of model C, in which $\gF = 0$. The results are shown (\cmsLeft) for the \WH and \ZH analyses of Refs.~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv}, individually, and for a combination with the \WZ final states of Refs.~\cite{CMS:2021itu, CMS:2022pjv,CMS:2021klu} (\cmsRight), where the \WH and \ZH results from all-hadronic final states have been combined with the corresponding $\PV\PV$ channels. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying the narrow width approximation no longer applies. 002892661 8564_ $$82522146$$s47705$$uhttp://cds.cern.ch/record/2892661/files/Figure_018-a.png$$y00040 Search for $\PX\to\PH(\bb)\PH(\PW\PW)$: Distributions of the DNN output for events in the signal nodes of the (upper) SL and (lower) DL categories of the $\PH(\bb)\PH(\PW \PW)$ analysis based on merged and resolved jets~\cite{CMS:2024rgy}. The distributions for a signal of a resonant radion with a mass of 400\GeV is also shown, by an open red histogram. Figure from Ref.~\cite{CMS:2024rgy}. 002892661 8564_ $$82522147$$s55444$$uhttp://cds.cern.ch/record/2892661/files/Figure_018-b.png$$y00041 Search for $\PX\to\PH(\bb)\PH(\PW\PW)$: Distributions of the DNN output for events in the signal nodes of the (upper) SL and (lower) DL categories of the $\PH(\bb)\PH(\PW \PW)$ analysis based on merged and resolved jets~\cite{CMS:2024rgy}. The distributions for a signal of a resonant radion with a mass of 400\GeV is also shown, by an open red histogram. Figure from Ref.~\cite{CMS:2024rgy}. 002892661 8564_ $$82522148$$s49823$$uhttp://cds.cern.ch/record/2892661/files/Figure_022-b.png$$y00049 Search for $\PX\to\PY(\text{bb})\PH(\gamma\gamma)$: Marginal distributions of the (\cmsLeft) \mgg and (\cmsRight) \mjj variables, in the high-purity SR (labeled ``CAT 0'') of the $\PY(\bb)\PH(\GamGam)$ analysis~\cite{CMS:2023boe}. The figure is shown, for a hypothesis of $\mX= 650\GeV$ and $\mY=90\GeV$, for which the largest excess of events over the background model is observed. In the lower panels, the numbers of background-subtracted events are shown after the fit of the background model to the data. Figure from Ref.~\cite{CMS:2023boe}. 002892661 8564_ $$82522149$$s98146$$uhttp://cds.cern.ch/record/2892661/files/Figure_043-d.png$$y00102 Expected differential cross sections for \HH production, as a function of \mHH for the real-singlet model with $\mX = 500\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522150$$s48304$$uhttp://cds.cern.ch/record/2892661/files/Figure_022-a.png$$y00048 Search for $\PX\to\PY(\text{bb})\PH(\gamma\gamma)$: Marginal distributions of the (\cmsLeft) \mgg and (\cmsRight) \mjj variables, in the high-purity SR (labeled ``CAT 0'') of the $\PY(\bb)\PH(\GamGam)$ analysis~\cite{CMS:2023boe}. The figure is shown, for a hypothesis of $\mX= 650\GeV$ and $\mY=90\GeV$, for which the largest excess of events over the background model is observed. In the lower panels, the numbers of background-subtracted events are shown after the fit of the background model to the data. Figure from Ref.~\cite{CMS:2023boe}. 002892661 8564_ $$82522151$$s92254$$uhttp://cds.cern.ch/record/2892661/files/Figure_043-a.png$$y00099 Expected differential cross sections for \HH production, as a function of \mHH for the real-singlet model with $\mX = 500\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522152$$s98832$$uhttp://cds.cern.ch/record/2892661/files/Figure_043-c.png$$y00101 Expected differential cross sections for \HH production, as a function of \mHH for the real-singlet model with $\mX = 500\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522153$$s94172$$uhttp://cds.cern.ch/record/2892661/files/Figure_043-b.png$$y00100 Expected differential cross sections for \HH production, as a function of \mHH for the real-singlet model with $\mX = 500\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522154$$s41927$$uhttp://cds.cern.ch/record/2892661/files/Figure_021-a.png$$y00046 Search for $\PX\to\PY(\bb)\PH(\tautau)$: Distributions of the NN output scores $y_{i}$, in different event categories after NN classification, based on a training for a resonance \PX with $\mX= 500\GeV$ and a resonance \PY with $100\leq\mY<150\GeV$ in the $\etauh$ final state of the $\PH(\tautau)\PY(\bb)$ analysis~\cite{CMS:2021yci}. Shown are the (\cmsLeft) \tautau and (\cmsRight) signal categories. For these figures, the data of all years have been combined. The uncertainty bands correspond to the combination of statistical and systematic uncertainties after the fit of the signal plus background hypothesis for $\mX=500\GeV$ and $\mY=110\GeV$ to the data. In the lower panels of the figures the (\cmsLeft) purity and (\cmsRight) fraction of the expected signal over background yields for a signal with a cross section of $200\unit{fb}$, as well as the ratio of the obtained yields in data over the expectation based on only the background model, are shown. Figure from Ref.~\cite{CMS:2021yci}. 002892661 8564_ $$82522155$$s48675$$uhttp://cds.cern.ch/record/2892661/files/Figure_021-b.png$$y00047 Search for $\PX\to\PY(\bb)\PH(\tautau)$: Distributions of the NN output scores $y_{i}$, in different event categories after NN classification, based on a training for a resonance \PX with $\mX= 500\GeV$ and a resonance \PY with $100\leq\mY<150\GeV$ in the $\etauh$ final state of the $\PH(\tautau)\PY(\bb)$ analysis~\cite{CMS:2021yci}. Shown are the (\cmsLeft) \tautau and (\cmsRight) signal categories. For these figures, the data of all years have been combined. The uncertainty bands correspond to the combination of statistical and systematic uncertainties after the fit of the signal plus background hypothesis for $\mX=500\GeV$ and $\mY=110\GeV$ to the data. In the lower panels of the figures the (\cmsLeft) purity and (\cmsRight) fraction of the expected signal over background yields for a signal with a cross section of $200\unit{fb}$, as well as the ratio of the obtained yields in data over the expectation based on only the background model, are shown. Figure from Ref.~\cite{CMS:2021yci}. 002892661 8564_ $$82522156$$s66195$$uhttp://cds.cern.ch/record/2892661/files/Figure_050-a.png$$y00113 Expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as functions of \MY, for $\MX\leq 1\TeV$. For the branching fractions of the $\PH\to\tautau$, $\PH\to\gamma\gamma$ and $\PH\to\bb$ decays, the SM values are assumed. The limits are obtained from the combined likelihood analysis of all analyses discussed in Section~\ref{Sec:Results_X_to_YH} and shown in Fig.~\ref{fig:XYH_combination}, projected to an integrated luminosity of 3000\fbinv. Shown are the projections for the combined likelihood analysis for different systematic uncertainty scenarios (\cmsLeft), and the projections for the combined likelihood analysis and the individual contributing analyses assuming the S2 scenario (\cmsRight). For presentation purposes, the limits have been scaled in successive steps by two orders of magnitude. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522157$$s68648$$uhttp://cds.cern.ch/record/2892661/files/Figure_050-b.png$$y00114 Expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as functions of \MY, for $\MX\leq 1\TeV$. For the branching fractions of the $\PH\to\tautau$, $\PH\to\gamma\gamma$ and $\PH\to\bb$ decays, the SM values are assumed. The limits are obtained from the combined likelihood analysis of all analyses discussed in Section~\ref{Sec:Results_X_to_YH} and shown in Fig.~\ref{fig:XYH_combination}, projected to an integrated luminosity of 3000\fbinv. Shown are the projections for the combined likelihood analysis for different systematic uncertainty scenarios (\cmsLeft), and the projections for the combined likelihood analysis and the individual contributing analyses assuming the S2 scenario (\cmsRight). For presentation purposes, the limits have been scaled in successive steps by two orders of magnitude. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522158$$s45758$$uhttp://cds.cern.ch/record/2892661/files/Figure_052.png$$y00117 Expected upper limits at 95~\%~\CL on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as obtained from the combined likelihood analysis of the individual analyses presented in Section~\ref{Sec:Results_X_to_YH} and Figure~\ref{fig:XYH_combination}. The results are shown in the plane spanned by \mY and \mX for $\mX\le1\TeV$, and projected to an integrated luminosity of 3000\fbinv, assuming the S2 systematic uncertainty scenario. The numbers in the boxes are given in~\unit{fb}. 002892661 8564_ $$82522159$$s59154$$uhttp://cds.cern.ch/record/2892661/files/Figure_005-c.png$$y00010 Branching fractions of $\PX\to\HH$ decays in 2HDMs of Type~I (upper) and Type~II (lower) in the $\cos(\beta - \alpha)$--$\tan\beta$ plane for $\mX = 500\GeV$ (\cmsLeft) and in the \mX--$\tan\beta$ plane for $\cos(\beta - \alpha) = 0.02$ (\cmsRight). The masses of all non-SM-like Higgs bosons are set to be the same, $\mX = \mA$, and $m_{12}^2 = \mA^2 \tan\beta/(1 + \tan^2\beta)$. The branching fractions have been calculated with 2HDMC~v1.8.0~\cite{Eriksson:2009ws,Harlander:2013qxa}. 002892661 8564_ $$82522160$$s59350$$uhttp://cds.cern.ch/record/2892661/files/Figure_005-b.png$$y00009 Branching fractions of $\PX\to\HH$ decays in 2HDMs of Type~I (upper) and Type~II (lower) in the $\cos(\beta - \alpha)$--$\tan\beta$ plane for $\mX = 500\GeV$ (\cmsLeft) and in the \mX--$\tan\beta$ plane for $\cos(\beta - \alpha) = 0.02$ (\cmsRight). The masses of all non-SM-like Higgs bosons are set to be the same, $\mX = \mA$, and $m_{12}^2 = \mA^2 \tan\beta/(1 + \tan^2\beta)$. The branching fractions have been calculated with 2HDMC~v1.8.0~\cite{Eriksson:2009ws,Harlander:2013qxa}. 002892661 8564_ $$82522161$$s58908$$uhttp://cds.cern.ch/record/2892661/files/Figure_005-a.png$$y00008 Branching fractions of $\PX\to\HH$ decays in 2HDMs of Type~I (upper) and Type~II (lower) in the $\cos(\beta - \alpha)$--$\tan\beta$ plane for $\mX = 500\GeV$ (\cmsLeft) and in the \mX--$\tan\beta$ plane for $\cos(\beta - \alpha) = 0.02$ (\cmsRight). The masses of all non-SM-like Higgs bosons are set to be the same, $\mX = \mA$, and $m_{12}^2 = \mA^2 \tan\beta/(1 + \tan^2\beta)$. The branching fractions have been calculated with 2HDMC~v1.8.0~\cite{Eriksson:2009ws,Harlander:2013qxa}. 002892661 8564_ $$82522162$$s9116694$$uhttp://cds.cern.ch/record/2892661/files/2403.16926.pdf$$yFulltext 002892661 8564_ $$82522163$$s55984$$uhttp://cds.cern.ch/record/2892661/files/Figure_005-d.png$$y00011 Branching fractions of $\PX\to\HH$ decays in 2HDMs of Type~I (upper) and Type~II (lower) in the $\cos(\beta - \alpha)$--$\tan\beta$ plane for $\mX = 500\GeV$ (\cmsLeft) and in the \mX--$\tan\beta$ plane for $\cos(\beta - \alpha) = 0.02$ (\cmsRight). The masses of all non-SM-like Higgs bosons are set to be the same, $\mX = \mA$, and $m_{12}^2 = \mA^2 \tan\beta/(1 + \tan^2\beta)$. The branching fractions have been calculated with 2HDMC~v1.8.0~\cite{Eriksson:2009ws,Harlander:2013qxa}. 002892661 8564_ $$82522164$$s63330$$uhttp://cds.cern.ch/record/2892661/files/Figure_031-b.png$$y00064 Interpretation of the results from the searches for the $\PX\to\HH$ decay, in the hMSSM model. In the upper part of the figure, the observed and expected exclusion contours at 95\%~\CL, in the (\mA, \tanb) plane, from the individual \HH analyses presented in this report and their combined likelihood analysis are shown. In the lower part of the figure, a comparison of the region excluded by the combined likelihood analysis shown in the upper part of the figure with selected results from other searches for the production of heavy scalar bosons in the hMSSM, in \tautau~\cite{CMS:2022goy}, \ttbar~\cite{CMS:2019pzc} and $\PW\PW$~\cite{CMS:2019bnu} decays is shown. Also shown, are the results from one representative search for $\PA\to\ZH $~\cite{CMS:2019kca} and indirect constraints obtained from measurements of the coupling strength of the observed \PH boson~\cite{CMS:2018uag}. Results not marked by a club symbol are based on an integrated luminosity of $35.9 \fbinv$. 002892661 8564_ $$82522165$$s48610$$uhttp://cds.cern.ch/record/2892661/files/Figure_006-a.png$$y00012 Branching fraction of $\PX\to\HH$ decays in the MSSM, for the hMSSM~\cite{Djouadi:2013vqa,Djouadi:2013uqa,Djouadi:2015jea} (\cmsLeft) and the \MhEFTScen~\cite{Bahl:2019ago} benchmarks, in the $\mA$--$\tan \beta$ plane. The branching fractions are taken from benchmark files produced by the MSSM subgroup of the LHC Higgs Working Group~\cite{Bagnaschi:2791954,lhc_higgs_working_group_mssm_subgroup_2022_6793918}. 002892661 8564_ $$82522166$$s41923$$uhttp://cds.cern.ch/record/2892661/files/Figure_006-b.png$$y00013 Branching fraction of $\PX\to\HH$ decays in the MSSM, for the hMSSM~\cite{Djouadi:2013vqa,Djouadi:2013uqa,Djouadi:2015jea} (\cmsLeft) and the \MhEFTScen~\cite{Bahl:2019ago} benchmarks, in the $\mA$--$\tan \beta$ plane. The branching fractions are taken from benchmark files produced by the MSSM subgroup of the LHC Higgs Working Group~\cite{Bagnaschi:2791954,lhc_higgs_working_group_mssm_subgroup_2022_6793918}. 002892661 8564_ $$82522167$$s53837$$uhttp://cds.cern.ch/record/2892661/files/Figure_031-a.png$$y00063 Interpretation of the results from the searches for the $\PX\to\HH$ decay, in the hMSSM model. In the upper part of the figure, the observed and expected exclusion contours at 95\%~\CL, in the (\mA, \tanb) plane, from the individual \HH analyses presented in this report and their combined likelihood analysis are shown. In the lower part of the figure, a comparison of the region excluded by the combined likelihood analysis shown in the upper part of the figure with selected results from other searches for the production of heavy scalar bosons in the hMSSM, in \tautau~\cite{CMS:2022goy}, \ttbar~\cite{CMS:2019pzc} and $\PW\PW$~\cite{CMS:2019bnu} decays is shown. Also shown, are the results from one representative search for $\PA\to\ZH $~\cite{CMS:2019kca} and indirect constraints obtained from measurements of the coupling strength of the observed \PH boson~\cite{CMS:2018uag}. Results not marked by a club symbol are based on an integrated luminosity of $35.9 \fbinv$. 002892661 8564_ $$82522168$$s53396$$uhttp://cds.cern.ch/record/2892661/files/Figure_032-a.png$$y00065 Interpretation of the results from the searches for the $\PX\to\HH$ decay, in the \MhEFTScen benchmark scenario. In the upper part of the figure, the observed and expected exclusion contours at 95\%~\CL are shown, in the (\mA, \tanb) plane from the individual \HH analyses presented in this report and their combined likelihood analysis. In the lower part of the figure, a comparison of the region excluded by the combined likelihood analysis shown in the upper part of the figure with selected results from other searches for the production of heavy scalar bosons in the \MhEFTScen scenario, in \tautau~\cite{CMS:2022goy}, \ttbar~\cite{CMS:2019pzc} and $\PW\PW$~\cite{ CMS:2019bnu} decays is shown. Also shown, are the results from one representative search for $\PA\to\ZH$~\cite{CMS:2019kca}. The parameter region in which the mass of the lightest MSSM Higgs boson does not coincide with 125\GeV within a 3\GeV margin is indicated by the dark hatched area. Results not marked by a club symbol are based on an integrated luminosity of $35.9\fbinv$. 002892661 8564_ $$82522169$$s62869$$uhttp://cds.cern.ch/record/2892661/files/Figure_032-b.png$$y00066 Interpretation of the results from the searches for the $\PX\to\HH$ decay, in the \MhEFTScen benchmark scenario. In the upper part of the figure, the observed and expected exclusion contours at 95\%~\CL are shown, in the (\mA, \tanb) plane from the individual \HH analyses presented in this report and their combined likelihood analysis. In the lower part of the figure, a comparison of the region excluded by the combined likelihood analysis shown in the upper part of the figure with selected results from other searches for the production of heavy scalar bosons in the \MhEFTScen scenario, in \tautau~\cite{CMS:2022goy}, \ttbar~\cite{CMS:2019pzc} and $\PW\PW$~\cite{ CMS:2019bnu} decays is shown. Also shown, are the results from one representative search for $\PA\to\ZH$~\cite{CMS:2019kca}. The parameter region in which the mass of the lightest MSSM Higgs boson does not coincide with 125\GeV within a 3\GeV margin is indicated by the dark hatched area. Results not marked by a club symbol are based on an integrated luminosity of $35.9\fbinv$. 002892661 8564_ $$82522170$$s28594$$uhttp://cds.cern.ch/record/2892661/files/Figure_001-b.png$$y00001 Higgs boson production cross sections in the SM as a function of the collider centre-of-mass energy (\cmsLeft), and Higgs boson branching fractions in the SM as a function of the Higgs boson mass (\cmsRight). Both figures are taken from Ref.~\cite{deFlorian:2016spz}. 002892661 8564_ $$82522171$$s61523$$uhttp://cds.cern.ch/record/2892661/files/Figure_001-a.png$$y00000 Higgs boson production cross sections in the SM as a function of the collider centre-of-mass energy (\cmsLeft), and Higgs boson branching fractions in the SM as a function of the Higgs boson mass (\cmsRight). Both figures are taken from Ref.~\cite{deFlorian:2016spz}. 002892661 8564_ $$82522172$$s42091$$uhttp://cds.cern.ch/record/2892661/files/Figure_044-c.png$$y00105 Expected upper limits at 95\%~\CL, on the product of the cross section for the production of a spin-0 resonance \PX and the branching fraction $\BR(\PX \to\PH\PH)$, as functions of \MX from the (upper \cmsLeft) \bbtt~\cite{CMS:2021yci}, (upper \cmsRight) \bbgg~\cite{CMS:2023boe}, and (lower) \bbbb with two merged \bb jets~\cite{CMS:2022suh} analyses discussed in this report, projected to an integrated luminosity of 3000\fbinv under the assumption of different systematic uncertainty scenarios, as discussed in the text. All estimates include the anticipated statistical uncertainties. 002892661 8564_ $$82522173$$s94561$$uhttp://cds.cern.ch/record/2892661/files/Figure_042-a.png$$y00095 Expected differential cross sections for \HH production, as a function of \mHH, for the real-singlet model with $\mX = 280\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522174$$s91913$$uhttp://cds.cern.ch/record/2892661/files/Figure_042-b.png$$y00096 Expected differential cross sections for \HH production, as a function of \mHH, for the real-singlet model with $\mX = 280\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522175$$s94779$$uhttp://cds.cern.ch/record/2892661/files/Figure_042-c.png$$y00097 Expected differential cross sections for \HH production, as a function of \mHH, for the real-singlet model with $\mX = 280\GeV$ and $\widthRatio = 5\%$. The parameters $\sin\alpha$ and \couplingLambda have been chosen such that (upper row) $\Rint=\pm 10\%$ and (lower row) $\Rint=\pm 20\%$, for (\cmsLeft) negative and (\cmsRight) positive values of \Rint. The total cross section for \HH production $\sigma^{\text{full}}$ (red line, labelled as $\sigma_{\text{full}}$) is compared to the cross sections $\sigma^{\text{ resonant-only}}$ (blue line, labelled as $\sigma_{\text{res}}$) and $\sigma^{ \text{nonresonant}}$ (green line, labelled as $\sigma_{\text{nores}}$) considering only resonant and nonresonant production. In the lower panels the ratio of $\sigma^{\text{full}}$ over $(\sigma^{\text{resonant-only}}+\sigma^{ \text{nonresonant}})$ is shown. 002892661 8564_ $$82522176$$s54160$$uhttp://cds.cern.ch/record/2892661/files/Figure_026-b.png$$y00056 Search for $\PX\to\PZ\PH$: Observed and expected 95\% \CL upper limits on the product of the cross section $\sigma$ for the production of a \PZpr spin-1 resonance, via (\cmsLeft) DY production or (\cmsRight) vector boson fusion and the branching fraction \BR for the $\PZpr\to\PZ\PH$ decay. The solid lines represent the observed and the dotted lines the expected limits. The theory predictions from the heavy vector triplet models A, B and C are also shown. 002892661 8564_ $$82522177$$s62795$$uhttp://cds.cern.ch/record/2892661/files/Figure_026-a.png$$y00055 Search for $\PX\to\PZ\PH$: Observed and expected 95\% \CL upper limits on the product of the cross section $\sigma$ for the production of a \PZpr spin-1 resonance, via (\cmsLeft) DY production or (\cmsRight) vector boson fusion and the branching fraction \BR for the $\PZpr\to\PZ\PH$ decay. The solid lines represent the observed and the dotted lines the expected limits. The theory predictions from the heavy vector triplet models A, B and C are also shown. 002892661 8564_ $$82522178$$s60376$$uhttp://cds.cern.ch/record/2892661/files/Figure_013-b.png$$y00030 Search for $\PX\to\PV\PH(\bb)$: Distributions of the \mtZH and \mZH variables, as introduced in the text, in the (\cmsLeft) $0\Pell$ and (\cmsRight) $2\Pell$ categories, in the 2 \PQb tag signal region of the $\Aboson\to\PZ\PH(\Pb\Pb)$ analysis~\cite{CMS:2019qcx}. In the $2\Pell$ categories, the contributions of the $2\Pe$ and $2\PGm$ channels have been summed. The gray dotted line represents the sum of all background processes before the fit to data; the shaded area represents the post-fit uncertainty. The hatched red histograms represent signal hypotheses for \PQb quark associated \PX production corresponding to $\sigma_{\Aboson}\BR(\Aboson\to\PZ\PH) \BR(\PH\to\Pb\Pb)=0.1\unit{pb}$. The lower panels depict $(N^\text{ data}-N^\text{bkg})/\sigma$ in each bin, where $\sigma$ refers to the statistical uncertainty in the given bin. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 8564_ $$82522179$$s48821$$uhttp://cds.cern.ch/record/2892661/files/Figure_013-a.png$$y00029 Search for $\PX\to\PV\PH(\bb)$: Distributions of the \mtZH and \mZH variables, as introduced in the text, in the (\cmsLeft) $0\Pell$ and (\cmsRight) $2\Pell$ categories, in the 2 \PQb tag signal region of the $\Aboson\to\PZ\PH(\Pb\Pb)$ analysis~\cite{CMS:2019qcx}. In the $2\Pell$ categories, the contributions of the $2\Pe$ and $2\PGm$ channels have been summed. The gray dotted line represents the sum of all background processes before the fit to data; the shaded area represents the post-fit uncertainty. The hatched red histograms represent signal hypotheses for \PQb quark associated \PX production corresponding to $\sigma_{\Aboson}\BR(\Aboson\to\PZ\PH) \BR(\PH\to\Pb\Pb)=0.1\unit{pb}$. The lower panels depict $(N^\text{ data}-N^\text{bkg})/\sigma$ in each bin, where $\sigma$ refers to the statistical uncertainty in the given bin. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 8564_ $$82522180$$s49781$$uhttp://cds.cern.ch/record/2892661/files/Figure_010-a.png$$y00021 Cross sections for (\cmsLeft) Drell--Yan production ($\hat{\sigma}_{\mathrm{DY}}$) and (\cmsRight) production through vector boson fusion ($\hat{\sigma}_{\mathrm{ VBF}}$), as defined in Eqs.~\eqref{eq:DY_HVT} and~\eqref{eq:VBF_HVT}, for \PZpr and \PWpr bosons in the heavy vector triplet (HVT) model B at $\sqrt{s} = 13\TeV$. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522181$$s22990$$uhttp://cds.cern.ch/record/2892661/files/Figure_010-b.png$$y00022 Cross sections for (\cmsLeft) Drell--Yan production ($\hat{\sigma}_{\mathrm{DY}}$) and (\cmsRight) production through vector boson fusion ($\hat{\sigma}_{\mathrm{ VBF}}$), as defined in Eqs.~\eqref{eq:DY_HVT} and~\eqref{eq:VBF_HVT}, for \PZpr and \PWpr bosons in the heavy vector triplet (HVT) model B at $\sqrt{s} = 13\TeV$. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522182$$s11671$$uhttp://cds.cern.ch/record/2892661/files/Figure_008-b.png$$y00017 The decay branching fractions of an RS1 graviton (top \cmsLeft), bulk graviton (upper \cmsRight), and radion (lower). Solid lines assume a fully elementary top quark, while the dashed lines ignore the coupling of the graviton to top quarks. Adapted from Ref.~\cite{Oliveira:2014kla}. 002892661 8564_ $$82522183$$s21107$$uhttp://cds.cern.ch/record/2892661/files/Figure_008-c.png$$y00018 The decay branching fractions of an RS1 graviton (top \cmsLeft), bulk graviton (upper \cmsRight), and radion (lower). Solid lines assume a fully elementary top quark, while the dashed lines ignore the coupling of the graviton to top quarks. Adapted from Ref.~\cite{Oliveira:2014kla}. 002892661 8564_ $$82522184$$s6217$$uhttp://cds.cern.ch/record/2892661/files/Figure_008-a.png$$y00016 The decay branching fractions of an RS1 graviton (top \cmsLeft), bulk graviton (upper \cmsRight), and radion (lower). Solid lines assume a fully elementary top quark, while the dashed lines ignore the coupling of the graviton to top quarks. Adapted from Ref.~\cite{Oliveira:2014kla}. 002892661 8564_ $$82522185$$s60923$$uhttp://cds.cern.ch/record/2892661/files/Figure_027-b.png$$y00058 Search for $\PX\to\PH\PH$/$\PG\to\PH\PH$: Observed and expected 95\%~\CL upper limits on the product of the cross section $\sigma$ for the production of a (\cmsLeft) spin-0 resonance \PX and (\cmsRight) a spin-2 resonance \PG, via gluon-gluon fusion and the branching fraction \BR for the corresponding \HH decay. The results of the individual analyses presented in this report and the result of their combined likelihood analysis are shown. The observed limits are indicated by markers connected with solid lines and the expected limits by dashed lines. 002892661 8564_ $$82522186$$s48267$$uhttp://cds.cern.ch/record/2892661/files/Figure_011-b.png$$y00024 Branching fractions for heavy vector triplet (HVT) bosons with masses of (upper) 1 and (lower) 2\TeV for values of the parameter \gF corresponding to models (\cmsLeft) A and (\cmsRight) B. The exact branching fractions of each model are indicated by the crossing points of the individual curves with the dashed vertical lines. Calculations are based on the work of Ref.~\cite{Pappadopulo:2014qza}. 002892661 8564_ $$82522187$$s41531$$uhttp://cds.cern.ch/record/2892661/files/Figure_044-a.png$$y00103 Expected upper limits at 95\%~\CL, on the product of the cross section for the production of a spin-0 resonance \PX and the branching fraction $\BR(\PX \to\PH\PH)$, as functions of \MX from the (upper \cmsLeft) \bbtt~\cite{CMS:2021yci}, (upper \cmsRight) \bbgg~\cite{CMS:2023boe}, and (lower) \bbbb with two merged \bb jets~\cite{CMS:2022suh} analyses discussed in this report, projected to an integrated luminosity of 3000\fbinv under the assumption of different systematic uncertainty scenarios, as discussed in the text. All estimates include the anticipated statistical uncertainties. 002892661 8564_ $$82522188$$s65664$$uhttp://cds.cern.ch/record/2892661/files/Figure_025-a.png$$y00053 Search for $\PX\to\PW\PH$: Observed and expected 95\% \CL upper limits on the product of the cross section $\sigma$ for the production of a \PWpr spin-1 resonance, via (\cmsLeft) DY production or (\cmsRight) vector boson fusion and the branching fraction \BR for the $\PWpr\to\PW\PH$ decay. The solid lines represent the observed and the dotted lines the expected limits. The theory predictions from the heavy vector triplet models A, B, and C are also shown. 002892661 8564_ $$82522189$$s45528$$uhttp://cds.cern.ch/record/2892661/files/Figure_045-b.png$$y00107 Expected upper limits at 95\%~\CL, on the product of the cross section for the production of a spin-0 resonance \PX and the branching fraction $\BR(\PX \to\PH\PH)$, as a function of \MX, for an integrated luminosity of 3000\fbinv and the combination of the three analyses shown in Fig.~\ref{fig:XHH_projections_bychannel}. Shown are the effects of the different systematic uncertainty scenarios (\cmsLeft), and the reach of the individual analyses for the S2 systematic scenario (\cmsRight). All estimates include the anticipated statistical uncertainties. 002892661 8564_ $$82522190$$s44742$$uhttp://cds.cern.ch/record/2892661/files/Figure_045-a.png$$y00106 Expected upper limits at 95\%~\CL, on the product of the cross section for the production of a spin-0 resonance \PX and the branching fraction $\BR(\PX \to\PH\PH)$, as a function of \MX, for an integrated luminosity of 3000\fbinv and the combination of the three analyses shown in Fig.~\ref{fig:XHH_projections_bychannel}. Shown are the effects of the different systematic uncertainty scenarios (\cmsLeft), and the reach of the individual analyses for the S2 systematic scenario (\cmsRight). All estimates include the anticipated statistical uncertainties. 002892661 8564_ $$82522191$$s46916$$uhttp://cds.cern.ch/record/2892661/files/Figure_025-b.png$$y00054 Search for $\PX\to\PW\PH$: Observed and expected 95\% \CL upper limits on the product of the cross section $\sigma$ for the production of a \PWpr spin-1 resonance, via (\cmsLeft) DY production or (\cmsRight) vector boson fusion and the branching fraction \BR for the $\PWpr\to\PW\PH$ decay. The solid lines represent the observed and the dotted lines the expected limits. The theory predictions from the heavy vector triplet models A, B, and C are also shown. 002892661 8564_ $$82522192$$s58516$$uhttp://cds.cern.ch/record/2892661/files/Figure_017-b.png$$y00039 Search for $\PX\to\PV(\text{qq})\PH(\bb)$: Distributions of (\cmsLeft) the soft drop mass \mj variable, labelled as $m_{\text{jet1}}^{\text{AK8}}$, and (\cmsRight) the dijet mass \mjjAKEight in the $\Vqq\PH(\bb)$ channel~\cite{CMS:2022pjv}. The individual contributions of the background model are shown by open histograms with different colours and line styles. The signal of a \PZpr boson with a mass of 3\TeV decaying via $\PZ\to\text{qq}$ and $\PH\to\bb$ is also shown, by a green filled histogram. Figure from Ref.~\cite{CMS:2022pjv}. 002892661 8564_ $$82522193$$s56432$$uhttp://cds.cern.ch/record/2892661/files/Figure_017-a.png$$y00038 Search for $\PX\to\PV(\text{qq})\PH(\bb)$: Distributions of (\cmsLeft) the soft drop mass \mj variable, labelled as $m_{\text{jet1}}^{\text{AK8}}$, and (\cmsRight) the dijet mass \mjjAKEight in the $\Vqq\PH(\bb)$ channel~\cite{CMS:2022pjv}. The individual contributions of the background model are shown by open histograms with different colours and line styles. The signal of a \PZpr boson with a mass of 3\TeV decaying via $\PZ\to\text{qq}$ and $\PH\to\bb$ is also shown, by a green filled histogram. Figure from Ref.~\cite{CMS:2022pjv}. 002892661 8564_ $$82522194$$s46076$$uhttp://cds.cern.ch/record/2892661/files/Figure_014.png$$y00031 Search for $\PX\to\PV\PH(\tautau)$: Distribution of the $\mlltt^{\mathrm{c}}$ variable, as introduced in the text, of the $\Aboson\to\PZ\PH(\tautau)$ analysis~\cite{CMS:2019kca}, after a fit of the background-only hypothesis in all eight final states. While the fit is based on corresponding distributions, for each final state individually, these have been combined into a single distribution, for visualization purposes for this figure. Uncertainties include both statistical and systematic components. The expected contribution from the $\PA\to\PZ\PH$ signal process is shown for a pseudoscalar Higgs boson with $\mA = 300\GeV$ with the product of the cross section and branching fraction of 20\unit{fb}. Figure from Ref.~\cite{CMS:2019kca}. 002892661 8564_ $$82522195$$s55242$$uhttp://cds.cern.ch/record/2892661/files/Figure_040-b.png$$y00093 Obseved upper limits, at 95\% \CL, on the coupling \gH within the heavy vector triplet model, as a function of the \PVpr mass. The limits are shown for the vecotr boson fusion production mode in the context of model C, in which $\gF = 0$. The results are shown (\cmsLeft) for the \WH and \ZH analyses of Refs.~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv}, individually, and for a combination with the \WZ final states of Refs.~\cite{CMS:2021itu, CMS:2022pjv,CMS:2021klu} (\cmsRight), where the \WH and \ZH results from all-hadronic final states have been combined with the corresponding $\PV\PV$ channels. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr}/\MVpr$, exceeds 4 and 10\%, respectively, implying the narrow width approximation no longer applies. 002892661 8564_ $$82522196$$s80019$$uhttp://cds.cern.ch/record/2892661/files/Figure_035-b.png$$y00075 Observed and expected limits, at 95\%~\CL, on the parameters of models with warped extra dimensions, as obtained from the $\PX\to\PH\PH$ analyses presented in this report and their combined likelihood analysis. Shown are lower limits (\cmsLeft) on the bulk radion ultraviolet cutoff parameter \LambdaR, as a function of the radion mass $m_{\PR}$, and upper limits (\cmsRight) on the parameter $\tilde{k}$ of the spin-2 bulk graviton \PG, as a function of $m_{\PG}$. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522197$$s92190$$uhttp://cds.cern.ch/record/2892661/files/Figure_035-a.png$$y00074 Observed and expected limits, at 95\%~\CL, on the parameters of models with warped extra dimensions, as obtained from the $\PX\to\PH\PH$ analyses presented in this report and their combined likelihood analysis. Shown are lower limits (\cmsLeft) on the bulk radion ultraviolet cutoff parameter \LambdaR, as a function of the radion mass $m_{\PR}$, and upper limits (\cmsRight) on the parameter $\tilde{k}$ of the spin-2 bulk graviton \PG, as a function of $m_{\PG}$. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522198$$s20654$$uhttp://cds.cern.ch/record/2892661/files/Figure_047-b.png$$y00110 Expected exclusion contours at 95\%~\CL, in the (\tanb, \mA) plane of the (\cmsLeft) hMSSM and (\cmsRight) \MhEFTScen scenarios obtained from the combined likelihood analysis of the \HH searches discussed in Section~\ref{Sec:Interp_in_Extended_Higgs_sector} and shown in Figs.~\ref{fig:hMSSM} and~\ref{fig:MSSM_mh125}, for different integrated luminosities and compared to the Run 2 result obtained at $\sqrt{s}=13\TeV$. The projections assume $\sqrt{s}=14\TeV$. 002892661 8564_ $$82522199$$s90341$$uhttp://cds.cern.ch/record/2892661/files/Figure_036-a.png$$y00076 Observed and expected limits, at 95\%~\CL, on the parameters of models with warped extra dimensions, as obtained from the combined likelihood analysis of the individual $\PX\to\PH\PH$ analyses presented in this report and shown in Fig.~\ref{fig:Int_WED}. The exclusion contours obtained from the combined likelihood analysis are compared to similar exclusions obtained from individual searches in the decays $\PZ(\lep)\PZ(\qq/\PGn\PGn/\lep)$~\cite{CMS:2018amk}, $\PW(\Pell\PGn)\PW(\Pell\PGn/\qq)$~\cite{CMS:2019bnu}, $\PW(\Pell\PGn)\PW(\qq)$~\cite{CMS:2021klu}, $\PV(\qq)\PV(\qq)$~\cite{CMS:2022pjv}, and $\PZ(\PGn\PGn)\PZ(\qq)$~\cite{CMS:2021itu}, in case of the radion interpretation, and from individual searches in the decays $\PZ(\qq)\PZ(\lep)$~\cite{CMS:2021xor}, $\PV(\qq)\PV(\qq)$~\cite{CMS:2022pjv}, $\PZ(\PGn\PGn)\PZ(\qq)$~\cite{CMS:2021itu}, and $\PW(\Pell\PGn)\PW(\qq)$~\cite{CMS:2021klu}, in the case of the graviton interpretation. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522200$$s73096$$uhttp://cds.cern.ch/record/2892661/files/Figure_036-b.png$$y00077 Observed and expected limits, at 95\%~\CL, on the parameters of models with warped extra dimensions, as obtained from the combined likelihood analysis of the individual $\PX\to\PH\PH$ analyses presented in this report and shown in Fig.~\ref{fig:Int_WED}. The exclusion contours obtained from the combined likelihood analysis are compared to similar exclusions obtained from individual searches in the decays $\PZ(\lep)\PZ(\qq/\PGn\PGn/\lep)$~\cite{CMS:2018amk}, $\PW(\Pell\PGn)\PW(\Pell\PGn/\qq)$~\cite{CMS:2019bnu}, $\PW(\Pell\PGn)\PW(\qq)$~\cite{CMS:2021klu}, $\PV(\qq)\PV(\qq)$~\cite{CMS:2022pjv}, and $\PZ(\PGn\PGn)\PZ(\qq)$~\cite{CMS:2021itu}, in case of the radion interpretation, and from individual searches in the decays $\PZ(\qq)\PZ(\lep)$~\cite{CMS:2021xor}, $\PV(\qq)\PV(\qq)$~\cite{CMS:2022pjv}, $\PZ(\PGn\PGn)\PZ(\qq)$~\cite{CMS:2021itu}, and $\PW(\Pell\PGn)\PW(\qq)$~\cite{CMS:2021klu}, in the case of the graviton interpretation. Excluded areas are indicated by the direction of the hatching along the exclusion contours. 002892661 8564_ $$82522201$$s47282$$uhttp://cds.cern.ch/record/2892661/files/Figure_003.png$$y00004 Measurements of the coupling modifiers $\kappa_{i}$, allowing both invisible and undetected decay modes, with the SM value used as an upper bound on both $\kappa_\PW$ and $\kappa_\PZ$. The thick and thin black lines indicate the $\pm1$ and $\pm2$ \SD confidence intervals, respectively, with the systematic and statistical components of the $\pm1$~\SD interval indicated by the red and blue bands. The resulting branching fractions for invisible and undetected decay modes are also displayed. Taken from Ref.~\cite{CMS:2022dwd}. 002892661 8564_ $$82522202$$s52899$$uhttp://cds.cern.ch/record/2892661/files/Figure_038-d.png$$y00087 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr} /\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522203$$s49047$$uhttp://cds.cern.ch/record/2892661/files/Figure_038-c.png$$y00086 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr} /\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522204$$s49094$$uhttp://cds.cern.ch/record/2892661/files/Figure_038-b.png$$y00085 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr} /\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522205$$s42050$$uhttp://cds.cern.ch/record/2892661/files/Figure_038-a.png$$y00084 Observed upper limits, at 95\% \CL, on the \PVpr couplings \gF and \gH within the HVT model for \PVpr masses of (upper \cmsLeft) 1, (upper \cmsRight) 2, (lower \cmsLeft) 3, and (lower \cmsRight) 4\TeV, from DY production, derived from \VH channels of Refs.~\cite{CMS:2021klu,CMS:2021fyk, CMS:2022pjv} discussed in this report. Excluded areas are indicated by the direction of the shading along the exclusion contours. The dotted lines denote coupling values above which the relative width of the resonance, $\Gamma_{\PVpr} /\MVpr$, exceeds 4 and 10\%, respectively, implying that the narrow width approximation no longer applies. The couplings corresponding to the heavy vector triplet models A and B are indicated by cross markers. 002892661 8564_ $$82522206$$s56620$$uhttp://cds.cern.ch/record/2892661/files/Figure_020-a.png$$y00044 Search for $\PX\to\PH\PH$ in multi-lepton final states: Distributions of the BDT classifier output for events in the (\cmsLeft) $2\ellss$ and (\cmsRight) $3\Pell$ categories of the $\PH(\PW\PW+\tautau)\PH(\PW\PW+\tautau)$ analysis in multilepton final states~\cite{CMS:2022kdx}. The expected signal for a spin-2 resonance with a mass of 750\GeV resonant \HH signal is shown, by the open dashed histogram. The signal is normalized to a a cross section of 1\unit{pb}. The distributions of the estimated background processes and corresponding uncertainties are shown after a fit of the signal plus background hypothesis to the data. Figure from Ref.~\cite{CMS:2022kdx}. 002892661 8564_ $$82522207$$s49313$$uhttp://cds.cern.ch/record/2892661/files/Figure_020-b.png$$y00045 Search for $\PX\to\PH\PH$ in multi-lepton final states: Distributions of the BDT classifier output for events in the (\cmsLeft) $2\ellss$ and (\cmsRight) $3\Pell$ categories of the $\PH(\PW\PW+\tautau)\PH(\PW\PW+\tautau)$ analysis in multilepton final states~\cite{CMS:2022kdx}. The expected signal for a spin-2 resonance with a mass of 750\GeV resonant \HH signal is shown, by the open dashed histogram. The signal is normalized to a a cross section of 1\unit{pb}. The distributions of the estimated background processes and corresponding uncertainties are shown after a fit of the signal plus background hypothesis to the data. Figure from Ref.~\cite{CMS:2022kdx}. 002892661 8564_ $$82522208$$s34722$$uhttp://cds.cern.ch/record/2892661/files/Figure_015-a.png$$y00032 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\mathrm{jet}}$, and (\cmsRight) the mass of the \PX resonance candidate, labeled $m_{\mathrm{WV}}$ in the $\Wln\PH(\bb)$ channel. The notation $m_{\mathrm{WV}}$ is used as a shorthand since the analysis also searches for resonances in the $\PW\PW$ and $\PW\PZ$ final states. Figures from Ref.~\cite{CMS:2021klu}. 002892661 8564_ $$82522209$$s15508$$uhttp://cds.cern.ch/record/2892661/files/Figure_015-b.png$$y00033 Search for $\PX\to\PV\PH(\bb)$: Distributions of (\cmsLeft) the jet soft drop mass of a boosted Higgs boson candidate, labeled $m_{\mathrm{jet}}$, and (\cmsRight) the mass of the \PX resonance candidate, labeled $m_{\mathrm{WV}}$ in the $\Wln\PH(\bb)$ channel. The notation $m_{\mathrm{WV}}$ is used as a shorthand since the analysis also searches for resonances in the $\PW\PW$ and $\PW\PZ$ final states. Figures from Ref.~\cite{CMS:2021klu}. 002892661 8564_ $$82522210$$s72658$$uhttp://cds.cern.ch/record/2892661/files/Figure_051-a.png$$y00115 Expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as functions of \MY, for $\MX\geq 1.2\TeV$. For the branching fractions of the $\PH\to\tautau$ and $\PH\to\bb$ decays, the SM values are assumed. The limits are obtained from the combined likelihood analysis of all analyses discussed in Section~\ref{Sec:Results_X_to_YH} and shown in Fig.~\ref{fig:XYH_combination_2}, projected to an integrated luminosity of 3000\fbinv. Shown are the projections for the combined likelihood analysis for different systematic uncertainty scenarios (\cmsLeft), and the projections for the combined likelihood analysis and the individual contributing analyses assuming the S2 scenario (\cmsRight). For presentation purposes, the limits have been scaled in successive steps by four orders of magnitude. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522211$$s69229$$uhttp://cds.cern.ch/record/2892661/files/Figure_051-b.png$$y00116 Expected upper limits at 95\%~\CL, on the product of the cross section $\sigma$ for the production of a resonance \PX via gluon-gluon fusion and the branching fraction \BR for the $\PX\to\PY(\bb)\PH$ decay, as functions of \MY, for $\MX\geq 1.2\TeV$. For the branching fractions of the $\PH\to\tautau$ and $\PH\to\bb$ decays, the SM values are assumed. The limits are obtained from the combined likelihood analysis of all analyses discussed in Section~\ref{Sec:Results_X_to_YH} and shown in Fig.~\ref{fig:XYH_combination_2}, projected to an integrated luminosity of 3000\fbinv. Shown are the projections for the combined likelihood analysis for different systematic uncertainty scenarios (\cmsLeft), and the projections for the combined likelihood analysis and the individual contributing analyses assuming the S2 scenario (\cmsRight). For presentation purposes, the limits have been scaled in successive steps by four orders of magnitude. For each set of graphs, a black arrow points to the \MX related legend. 002892661 8564_ $$82522212$$s59987$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-a.png$$y00078 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522213$$s55347$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-b.png$$y00079 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522214$$s55099$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-c.png$$y00080 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522215$$s53938$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-d.png$$y00081 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522216$$s49082$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-e.png$$y00082 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522217$$s48615$$uhttp://cds.cern.ch/record/2892661/files/Figure_037-f.png$$y00083 Observed upper limits, at 95\%~\CL, on the Drell--Yan production cross section of (upper) \PWpr, (middle) \PZpr, and (lower) combined \PVpr spin-1 resonances assuming branching fractions of the heavy vector triplet models (\cmsLeft) A and (\cmsRight) B. The theory predictions from these models are also shown. Results from the $\PV\PH$~\cite{CMS:2021klu,CMS:2021fyk,CMS:2022pjv} and $\PV\PV$ channels~\cite{CMS:2021klu,CMS:2022pjv,CMS:2021xor,CMS:2021itu}, as well as results from dijet~\cite{CMS:2019gwf}, $\PQt\PQb$~\cite{CMS:2021mux}, \lep~\cite{CMS:2021ctt}, and $\Pell\PGn$~\cite{CMS:2022krd} final states are also shown, for comparison. 002892661 8564_ $$82522218$$s4059$$uhttp://cds.cern.ch/record/2892661/files/Figure_004-b.png$$y00006 Leading order Feynman diagrams of Higgs boson pair production via gluon fusion. The left and middle parts of the figure show the ``triangle'' and ``box'' diagrams, respectively for nonresonant \PH production, as expected from the SM. The right part of the figure shows a diagram for \PH boson production through a new resonance of labeled as \PX. 002892661 8564_ $$82522219$$s3956$$uhttp://cds.cern.ch/record/2892661/files/Figure_004-c.png$$y00007 Leading order Feynman diagrams of Higgs boson pair production via gluon fusion. The left and middle parts of the figure show the ``triangle'' and ``box'' diagrams, respectively for nonresonant \PH production, as expected from the SM. The right part of the figure shows a diagram for \PH boson production through a new resonance of labeled as \PX. 002892661 8564_ $$82522220$$s4035$$uhttp://cds.cern.ch/record/2892661/files/Figure_004-a.png$$y00005 Leading order Feynman diagrams of Higgs boson pair production via gluon fusion. The left and middle parts of the figure show the ``triangle'' and ``box'' diagrams, respectively for nonresonant \PH production, as expected from the SM. The right part of the figure shows a diagram for \PH boson production through a new resonance of labeled as \PX. 002892661 8564_ $$82522221$$s4472$$uhttp://cds.cern.ch/record/2892661/files/Figure_007-a.png$$y00014 Localization of fields on the branes, in different types of the Randall-Sundrum (RS) model: RS1 (\cmsLeft) and bulk-RS (\cmsRight). The $x$-axis represents the 5th dimension with the Planck brane on the left and the \TeV brane on the right. The $y$-axis is the probability density. Adapted from Ref.~\cite{Oliveira:2014kla}. 002892661 8564_ $$82522222$$s5341$$uhttp://cds.cern.ch/record/2892661/files/Figure_007-b.png$$y00015 Localization of fields on the branes, in different types of the Randall-Sundrum (RS) model: RS1 (\cmsLeft) and bulk-RS (\cmsRight). The $x$-axis represents the 5th dimension with the Planck brane on the left and the \TeV brane on the right. The $y$-axis is the probability density. Adapted from Ref.~\cite{Oliveira:2014kla}. 002892661 8564_ $$82522223$$s47297$$uhttp://cds.cern.ch/record/2892661/files/Figure_033-d.png$$y00070 Interpretation of the results of the $\PA\to\PZ\PH(\bb)$ analysis~\cite{CMS:2019qcx}, in the (upper \cmsLeft) Type~I, (upper \cmsRight) Type~II, (lower \cmsLeft) flipped, and (lower \cmsRight) lepton-specific 2HDM models. In each case observed and expected exclusion contours at 95\%~\CL, in the plane defined by \cosba and \tanb, are shown. The excluded regions are represented by the shaded gray areas. The 68 and 95\% central intervals of the expected exclusion contours in the absence of a signal are indicated by the green and yellow bands. Contours are derived from the projection on the corresponding 2HDM parameter space for $\mA = 300\GeV$. The regions of parameter space where the natural width of the \PA boson $\Gamma_\PA$ is comparable to or larger than the experimental resolution and thus the narrow-width approximation is not valid are represented by hatched gray areas. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 8564_ $$82522224$$s38500$$uhttp://cds.cern.ch/record/2892661/files/Figure_033-a.png$$y00067 Interpretation of the results of the $\PA\to\PZ\PH(\bb)$ analysis~\cite{CMS:2019qcx}, in the (upper \cmsLeft) Type~I, (upper \cmsRight) Type~II, (lower \cmsLeft) flipped, and (lower \cmsRight) lepton-specific 2HDM models. In each case observed and expected exclusion contours at 95\%~\CL, in the plane defined by \cosba and \tanb, are shown. The excluded regions are represented by the shaded gray areas. The 68 and 95\% central intervals of the expected exclusion contours in the absence of a signal are indicated by the green and yellow bands. Contours are derived from the projection on the corresponding 2HDM parameter space for $\mA = 300\GeV$. The regions of parameter space where the natural width of the \PA boson $\Gamma_\PA$ is comparable to or larger than the experimental resolution and thus the narrow-width approximation is not valid are represented by hatched gray areas. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 8564_ $$82522225$$s52868$$uhttp://cds.cern.ch/record/2892661/files/Figure_033-b.png$$y00068 Interpretation of the results of the $\PA\to\PZ\PH(\bb)$ analysis~\cite{CMS:2019qcx}, in the (upper \cmsLeft) Type~I, (upper \cmsRight) Type~II, (lower \cmsLeft) flipped, and (lower \cmsRight) lepton-specific 2HDM models. In each case observed and expected exclusion contours at 95\%~\CL, in the plane defined by \cosba and \tanb, are shown. The excluded regions are represented by the shaded gray areas. The 68 and 95\% central intervals of the expected exclusion contours in the absence of a signal are indicated by the green and yellow bands. Contours are derived from the projection on the corresponding 2HDM parameter space for $\mA = 300\GeV$. The regions of parameter space where the natural width of the \PA boson $\Gamma_\PA$ is comparable to or larger than the experimental resolution and thus the narrow-width approximation is not valid are represented by hatched gray areas. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 8564_ $$82522226$$s53408$$uhttp://cds.cern.ch/record/2892661/files/Figure_033-c.png$$y00069 Interpretation of the results of the $\PA\to\PZ\PH(\bb)$ analysis~\cite{CMS:2019qcx}, in the (upper \cmsLeft) Type~I, (upper \cmsRight) Type~II, (lower \cmsLeft) flipped, and (lower \cmsRight) lepton-specific 2HDM models. In each case observed and expected exclusion contours at 95\%~\CL, in the plane defined by \cosba and \tanb, are shown. The excluded regions are represented by the shaded gray areas. The 68 and 95\% central intervals of the expected exclusion contours in the absence of a signal are indicated by the green and yellow bands. Contours are derived from the projection on the corresponding 2HDM parameter space for $\mA = 300\GeV$. The regions of parameter space where the natural width of the \PA boson $\Gamma_\PA$ is comparable to or larger than the experimental resolution and thus the narrow-width approximation is not valid are represented by hatched gray areas. Figure from Ref.~\cite{CMS:2019qcx}. 002892661 916__ $$sn$$w202412 002892661 925__ $$b25 Mar 2024 002892661 960__ $$a11 002892661 980__ $$aCMS_Papers 002892661 980__ $$aPREPRINT 002892661 980__ $$aCMSPUBDRAFTFINAL