Главная страница > CERN Experiments > LHC Experiments > ALICE > ALICE Preprints > Neutral pion and $\eta$ meson production in p-Pb collisions at $\sqrt{s_\mathrm{NN}} = 5.02$ TeV > HTML MARC |
002299472 001__ 2299472 002299472 005__ 20241127050428.0 002299472 0248_ $$aoai:cds.cern.ch:2299472$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT 002299472 0247_ $$2DOI$$9bibmatch$$a10.1140/epjc/s10052-018-6013-8 002299472 037__ $$9arXiv$$aarXiv:1801.07051$$cnucl-ex 002299472 037__ $$aCERN-EP-2018-002 002299472 035__ $$9arXiv$$aoai:arXiv.org:1801.07051 002299472 035__ $$9Inspire$$aoai:inspirehep.net:1649235$$d2024-11-26T15:21:17Z$$h2024-11-27T03:03:01Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d 002299472 035__ $$9Inspire$$a1649235 002299472 041__ $$aeng 002299472 088__ $$9CERN-EP-DRAFT-ALICE-2018-001 002299472 100__ $$aAcharya, Shreyasi$$iINSPIRE-00570928$$tGRID:grid.482273.8$$uCalcutta, VECC$$vVariable Energy Cyclotron Centre - Kolkata - India 002299472 110__ $$aThe ALICE collaboration 002299472 245__ $$9arXiv$$aNeutral pion and $\eta$ meson production in p-Pb collisions at $\sqrt{s_\mathrm{NN}} = 5.02$ TeV 002299472 260__ $$c2018-08-06 002299472 269__ $$aGeneva$$bCERN$$c08 Jan 2018 002299472 300__ $$a34 p 002299472 506__ $$dcds-edboard-alice@cern.ch 002299472 506__ $$malice-member [CERN] 002299472 506__ $$mcds-ph-ep-publications-referee [CERN] 002299472 500__ $$9arXiv$$a34 pages, 11 captioned figures, 5+1 tables, authors from page 29, submitted to EPJC, figures at http://aliceinfo.cern.ch/ArtSubmission/node/4156 002299472 520__ $$9Springer$$aNeutral pion and $\eta $ meson invariant differential yields were measured in non-single diffractive p–Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 5.02 TeV with the ALICE experiment at the CERN LHC. The analysis combines results from three complementary photon measurements, utilizing the PHOS and EMCal calorimeters and the Photon Conversion Method. The invariant differential yields of $\pi ^{0}$ and $\eta $ meson inclusive production are measured near mid-rapidity in a broad transverse momentum range of $0.3< p_{\mathrm{T}} < 20 \hbox { GeV}/c$ and $0.7< p_{\mathrm{T}} < 20\hbox { GeV}/c$ , respectively. The measured $\eta /\pi ^{0}$ ratio increases with $p_{\mathrm{T}}$ and saturates for $p_{\mathrm{T}}$ > 4 $\hbox {GeV}/c$ at $0.483 \pm 0.015_{\mathrm{stat}} \pm 0.015_{\mathrm{sys}}$ . A deviation from $m_{\mathrm{T}}$ scaling is observed for $p_{\mathrm{T}}<$ 2 $\hbox {GeV}/c$ . The measured $\eta /\pi ^{0}$ ratio is consistent with previous measurements from proton-nucleus and pp collisions over the full $p_{\mathrm{T}}$ range. The measured $\eta /\pi ^{0}$ ratio at high $p_{\mathrm{T}}$ also agrees within uncertainties with measurements from nucleus–nucleus collisions. The $\pi ^{0}$ and $\eta $ yields in p–Pb relative to the scaled pp interpolated reference, $R_{{\mathrm{pPb}}}$ , are presented for $0.3 < p_{\mathrm{T}}<$ 20 $\hbox {GeV}/c$ and $0.7 < p_{\mathrm{T}}<$ 20 $\hbox {GeV}/c$ , respectively. The results are compared with theoretical model calculations. The values of $R_{{\mathrm{pPb}}}$ are consistent with unity for transverse momenta above 2 $\hbox {GeV}/c$ . These results support the interpretation that the suppressed yield of neutral mesons measured in Pb–Pb collisions at LHC energies is due to parton energy loss in the hot QCD medium. 002299472 520__ $$9arXiv$$aNeutral pion and $\eta$ meson invariant differential yields were measured in non-single diffractive p-Pb collisions at $\sqrt{s_{\rm NN}} = 5.02$ TeV with the ALICE experiment at the CERN LHC. The analysis combines results from three complementary photon measurements, utilizing the PHOS and EMCal calorimeters and the Photon Conversion Method. The invariant differential yields of $\pi^0$ and $\eta$ meson inclusive production are measured near mid-rapidity in a broad transverse momentum range of $0.3<p_{\rm T}< 20$ GeV/$c$ and $0.7<p_{\rm T}<20$ GeV/$c$, respectively. The measured $\eta$/$\pi^{0}$ ratio increases with $p_{\rm T}$ and saturates for $p_{\rm T} > 4$ GeV/$c$ at $0.483\pm 0.015_{\rm stat}\pm 0.015_{\rm sys}$. A deviation from $m_{\rm T}$ scaling is observed for $p_{\rm T}<2$ GeV/$c$. The measured $\eta$/$\pi^{0}$ ratio is consistent with previous measurements from proton-nucleus and pp collisions over the full $p_{\rm T}$ range. The measured $\eta$/$\pi^{0}$ ratio at high $p_{\rm T}$ also agrees within uncertainties with measurements from nucleus-nucleus collisions. The $\pi^0$ and $\eta$ yields in p-Pb relative to the scaled pp interpolated reference, $R_{\rm pPb}$, are presented for $0.3<p_{\rm T}<20$ GeV/$c$ and $0.7<p_{\rm T}< 20$ GeV/$c$, respectively. The results are compared with theoretical model calculations. The values of $R_{\rm pPb}$ are consistent with unity for transverse momenta above 2 GeV/$c$. These results support the interpretation that the suppressed yield of neutral mesons measured in Pb-Pb collisions at LHC energies is due to parton energy loss in the hot QCD medium. 002299472 540__ $$3Preprint$$aCC-BY-4.0 002299472 540__ $$3publication$$9Springer$$aCC-BY-4.0 002299472 542__ $$3Preprint$$dCERN$$g2018 002299472 562__ $$cPublic comments 002299472 595__ $$aCERN EDS 002299472 65017 $$2SzGeCERN$$aParticle Physics - Experiment 002299472 65017 $$2arXiv$$ahep-ex 002299472 65017 $$2arXiv$$anucl-ex 002299472 65017 $$2SzGeCERN$$aNuclear Physics - Experiment 002299472 6531_ $$9CERN$$arelativistic heavy ion physics 002299472 6531_ $$9CERN$$aparticle and resonance production 002299472 6531_ $$9CERN$$aexperimental results 002299472 693__ $$aCERN LHC$$eALICE 002299472 690C_ $$aCERN 002299472 690C_ $$aARTICLE 002299472 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. Phys. 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Higher Educ. 002299472 700__ $$aHerghelegiu, Andrei Ionut$$iINSPIRE-00248972$$uBucharest, IFIN-HH 002299472 700__ $$aGonzalez Hernandez, Emma$$iINSPIRE-00649608$$uPuebla U., Mexico 002299472 700__ $$aHerrera Corral, Gerardo Antonio$$iINSPIRE-00089895$$uCINVESTAV, IPN 002299472 700__ $$aHerrmann, Florian$$iINSPIRE-00564065$$uMunster U. 002299472 700__ $$aHess, Benjamin Andreas$$iINSPIRE-00361150$$uTubingen U. 002299472 700__ $$aHetland, Kristin Fanebust$$iINSPIRE-00080364$$uBergen Coll. Higher Educ. 002299472 700__ $$aHillemanns, Hartmut$$iINSPIRE-00507591$$uCERN 002299472 700__ $$aHills, Christopher$$iINSPIRE-00575031$$jORCID:0000-0003-4647-4159$$uLiverpool U. 002299472 700__ $$aHippolyte, Boris$$iINSPIRE-00262496$$jORCID:0000-0003-4562-2922$$uStrasbourg, IPHC 002299472 700__ $$aHohlweger, Bernhard$$iINSPIRE-00580270$$uTech. U., Munich (main) 002299472 700__ $$aHorak, David$$iINSPIRE-00548374$$uPrague, Tech. U. 002299472 700__ $$aHornung, Sebastian$$iINSPIRE-00584070$$uDarmstadt, EMMI 002299472 700__ $$aHosokawa, Ritsuya$$iINSPIRE-00522280$$uTsukuba U.$$uLPSC, Grenoble 002299472 700__ $$aHristov, Peter Zahariev$$iINSPIRE-00091290$$uCERN 002299472 700__ $$aHughes, Charles$$iINSPIRE-00564077$$uTennessee U. 002299472 700__ $$aHuhn, Patrick$$uFrankfurt U., Inst. 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Inst. 002299472 700__ $$aIslam, Md Samsul$$iINSPIRE-00564099$$uSaha Inst. 002299472 700__ $$aIvanov, Marian$$iINSPIRE-00262538$$uDarmstadt, EMMI 002299472 700__ $$aIvanov, Vladimir$$iINSPIRE-00262542$$uSt. Petersburg, INP 002299472 700__ $$aIzucheev, Vladimir$$iINSPIRE-00506818$$uSerpukhov, IHEP 002299472 700__ $$aJacak, Barbara$$iINSPIRE-00155696$$uLBL, Berkeley 002299472 700__ $$aJacazio, Nicolo$$iINSPIRE-00548380$$jORCID:0000-0002-3066-855X$$uINFN, Bologna$$uBologna U. 002299472 700__ $$aJacobs, Peter Martin$$iINSPIRE-00181871$$jORCID:0000-0001-9980-5199$$uLBL, Berkeley 002299472 700__ $$aJadhav, Manoj Bhanudas$$iINSPIRE-00531323$$jORCID:0000-0002-5225-2803$$uIndian Inst. Tech., Mumbai 002299472 700__ $$aJadlovska, Slavka$$iINSPIRE-00522452$$uKosice Tech. U. 002299472 700__ $$aJadlovsky, Jan$$iINSPIRE-00537120$$uKosice Tech. U. 002299472 700__ $$aJaelani, Syaefudin$$iINSPIRE-00581977$$uUtrecht U. 002299472 700__ $$aJahnke, Cristiane$$iINSPIRE-00383021$$uMunich, Tech. U., Universe$$uSao Paulo U. 002299472 700__ $$aJakubowska, Monika Joanna$$iINSPIRE-00537133$$uWarsaw U. of Tech. 002299472 700__ $$aJanik, Malgorzata Anna$$iINSPIRE-00244548$$uWarsaw U. of Tech. 002299472 700__ $$aPahula Hewage, Sandun$$iINSPIRE-00246609$$uHouston U. 002299472 700__ $$aJena, Chitrasen$$iINSPIRE-00181905$$uNISER, Jatni 002299472 700__ $$aJercic, Marko$$iINSPIRE-00578879$$uZagreb U. 002299472 700__ $$aJimenez Bustamante, Raul Tonatiuh$$iINSPIRE-00355862$$uDarmstadt, EMMI 002299472 700__ $$aJones, Peter Graham$$iINSPIRE-00181937$$uBirmingham U. 002299472 700__ $$aJusko, Anton$$iINSPIRE-00250331$$uBirmingham U. 002299472 700__ $$aKalinak, Peter$$iINSPIRE-00247100$$jORCID:0000-0002-0559-6697$$uKosice, IEF 002299472 700__ $$aKalweit, Alexander Philipp$$iINSPIRE-00248849$$jORCID:0000-0001-6907-0486$$uCERN 002299472 700__ $$aKang, Ju Hwan$$iINSPIRE-00241999$$uYonsei U. 002299472 700__ $$aKaplin, Vladimir$$iINSPIRE-00248837$$uMoscow Phys. Eng. Inst. 002299472 700__ $$aKar, Somnath$$iINSPIRE-00383167$$uCalcutta, VECC 002299472 700__ $$aKarasu Uysal, Ayben$$iINSPIRE-00245978$$jORCID:0000-0001-6297-2532$$uKaratay U. 002299472 700__ $$aKaravichev, Oleg$$iINSPIRE-00262581$$uMoscow, INR 002299472 700__ $$aKaravicheva, Tatiana$$iINSPIRE-00262593$$jORCID:0000-0002-9355-6379$$uMoscow, INR 002299472 700__ $$aKarayan, Lilit$$iINSPIRE-00522297$$uHeidelberg U.$$uDarmstadt, EMMI 002299472 700__ $$aKarczmarczyk, Przemyslaw$$iINSPIRE-00577574$$jORCID:0000-0002-9057-9719$$uCERN 002299472 700__ $$aKarpechev, Evgeny$$iINSPIRE-00248813$$uMoscow, INR 002299472 700__ $$aKebschull, Udo Wolfgang$$iINSPIRE-00248807$$uGoethe U., Frankfurt, Inst. Inform. 002299472 700__ $$aKeidel, Ralf$$iINSPIRE-00248795$$uFachhochsch., Worms 002299472 700__ $$aKeijdener, Darius Laurens$$iINSPIRE-00416339$$uUtrecht U. 002299472 700__ $$aKeil, Markus$$iINSPIRE-00216636$$uCERN 002299472 700__ $$aKetzer, Bernhard Franz$$iINSPIRE-00095813$$uBonn U., HISKP 002299472 700__ $$aKhabanova, Zhanna$$iINSPIRE-00539181$$uNIKHEF, Amsterdam 002299472 700__ $$aKhan, Shaista$$iINSPIRE-00641195$$uAligarh Muslim U. 002299472 700__ $$aKhan, Shuaib Ahmad$$iINSPIRE-00243963$$uCalcutta, VECC 002299472 700__ $$aKhanzadeev, Alexei$$iINSPIRE-00242036$$uSt. Petersburg, INP 002299472 700__ $$aKharlov, Yury$$iINSPIRE-00095925$$uSerpukhov, IHEP 002299472 700__ $$aKhatun, Anisa$$iINSPIRE-00564120$$uAligarh Muslim U. 002299472 700__ $$aKhuntia, Arvind$$iINSPIRE-00564138$$jORCID:0000-0003-0996-8547$$uIndian Inst. Tech., Indore 002299472 700__ $$aKielbowicz, Miroslaw Marek$$iINSPIRE-00564106$$uCracow, INP 002299472 700__ $$aKileng, Bjarte$$iINSPIRE-00262606$$uBergen Coll. 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Kernphys. 002299472 700__ $$aKlein, Jochen$$iINSPIRE-00262064$$uCERN 002299472 700__ $$aKlein-boesing, Christian$$iINSPIRE-00003561$$jORCID:0000-0002-7285-3411$$uMunster U. 002299472 700__ $$aKlewin, Sebastian$$iINSPIRE-00537149$$uHeidelberg U. 002299472 700__ $$aKluge, Alexander$$iINSPIRE-00250353$$uCERN 002299472 700__ $$aKnichel, Michael Linus$$iINSPIRE-00245547$$jORCID:0000-0003-2471-9688$$uCERN$$uHeidelberg U. 002299472 700__ $$aKnospe, Anders Garritt$$iINSPIRE-00182064$$uHouston U. 002299472 700__ $$aKobdaj, Chinorat$$iINSPIRE-00227795$$jORCID:0000-0001-7296-5248$$uSuranaree U. of Tech. 002299472 700__ $$aVarga-kofarago, Monika$$iINSPIRE-00410392$$uWigner RCP, Budapest 002299472 700__ $$aKohler, Markus Konrad$$iINSPIRE-00244603$$uHeidelberg U. 002299472 700__ $$aKollegger, Thorsten$$iINSPIRE-00182076$$uDarmstadt, EMMI 002299472 700__ $$aKondratev, Valerii$$iINSPIRE-00248784$$jORCID:0000-0002-0031-0741$$uSt. Petersburg State U. 002299472 700__ $$aKondratyeva, Natalia$$iINSPIRE-00262112$$uMoscow Phys. Eng. Inst. 002299472 700__ $$aKondratyuk, Evgeny$$iINSPIRE-00507275$$uSerpukhov, IHEP 002299472 700__ $$aKonevskikh, Artem$$iINSPIRE-00248772$$uMoscow, INR 002299472 700__ $$aKonyushikhin, Maxim$$iINSPIRE-00381357$$uWayne State U. 002299472 700__ $$aKopcik, Michal$$iINSPIRE-00522467$$uKosice Tech. U. 002299472 700__ $$aKouzinopoulos, Charalampos$$iINSPIRE-00507396$$uCERN 002299472 700__ $$aKovalenko, Oleksandr$$iINSPIRE-00507510$$uWarsaw, Inst. Nucl. 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Kernphys. 002299472 700__ $$aKryshen, Evgeny$$iINSPIRE-00262643$$uSt. Petersburg, INP 002299472 700__ $$aKrzewicki, Mikolaj$$iINSPIRE-00248715$$uFrankfurt U., FIAS 002299472 700__ $$aKubera, Andrew Michael$$iINSPIRE-00507630$$jORCID:0000-0002-1851-2739$$uOhio State U. 002299472 700__ $$aKucera, Vit$$iINSPIRE-00383170$$uRez, Nucl. Phys. Inst. 002299472 700__ $$aKuhn, Christian Claude$$iINSPIRE-00244002$$uStrasbourg, IPHC 002299472 700__ $$aKuijer, Paulus Gerardus$$iINSPIRE-00098956$$jORCID:0000-0002-6987-2048$$uNIKHEF, Amsterdam 002299472 700__ $$aKumar, Jitendra$$iINSPIRE-00361265$$uIndian Inst. Tech., Mumbai 002299472 700__ $$aKumar, Lokesh$$iINSPIRE-00182175$$uPanjab U. 002299472 700__ $$aKumar, Shyam$$iINSPIRE-00531331$$uIndian Inst. Tech., Mumbai 002299472 700__ $$aKundu, Sourav$$iINSPIRE-00564145$$uNISER, Jatni 002299472 700__ $$aKurashvili, Podist$$iINSPIRE-00247073$$uWarsaw, Inst. Nucl. Studies 002299472 700__ $$aKurepin, Alexander$$iINSPIRE-00244630$$uMoscow, INR 002299472 700__ $$aKurepin, Alexey$$iINSPIRE-00244643$$jORCID:0000-0002-1851-4136$$uMoscow, INR 002299472 700__ $$aKuryakin, Alexey$$iINSPIRE-00248681$$uRFNC-VNIIEF, Sarov 002299472 700__ $$aKushpil, Svetlana$$iINSPIRE-00262657$$jORCID:0000-0001-9289-2840$$uRez, Nucl. Phys. 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Subatomare Phys. 002299472 700__ $$aLehrbach, Johannes$$iINSPIRE-00567842$$uFrankfurt U., FIAS 002299472 700__ $$aLemmon, Roy Crawford$$iINSPIRE-00385690$$jORCID:0000-0002-1259-979X$$uDaresbury 002299472 700__ $$aLeogrande, Emilia$$iINSPIRE-00416444$$uUtrecht U. 002299472 700__ $$aLeon Monzon, Ildefonso$$iINSPIRE-00248605$$jORCID:0000-0002-7919-2150$$uSinaloa U. 002299472 700__ $$aLevai, Peter$$iINSPIRE-00162508$$uWigner RCP, Budapest 002299472 700__ $$aLi, Xiaomei$$iINSPIRE-00242399$$uBeijing, Inst. Atomic Energy 002299472 700__ $$aLi, Xing Long$$iINSPIRE-00653591$$uHua-Zhong Normal U. 002299472 700__ $$aLien, Jorgen Andre$$iINSPIRE-00101774$$uVestfold U. Coll., Tonsberg 002299472 700__ $$aLietava, Roman$$iINSPIRE-00206588$$uBirmingham U. 002299472 700__ $$aLim, Bong-hwi$$iINSPIRE-00585228$$uPusan Natl. U. 002299472 700__ $$aLindal, Svein$$iINSPIRE-00262704$$uOslo U. 002299472 700__ $$aLindenstruth, Volker$$iINSPIRE-00171460$$uFrankfurt U., FIAS 002299472 700__ $$aLindsay, Scott William$$iINSPIRE-00261912$$uLiverpool U. 002299472 700__ $$aLippmann, Christian$$iINSPIRE-00247046$$uDarmstadt, EMMI 002299472 700__ $$aLisa, Michael Annan$$iINSPIRE-00182345$$uOhio State U. 002299472 700__ $$aLitichevskyi, Vladyslav$$iINSPIRE-00564223$$uHelsinki Inst. of Phys. 002299472 700__ $$aLiu, Alwina$$iINSPIRE-00642235$$uLBL, Berkeley 002299472 700__ $$aLjunggren, Hans Martin$$iINSPIRE-00361314$$uLund U. 002299472 700__ $$aLlope, William$$iINSPIRE-00102341$$uWayne State U. 002299472 700__ $$aLodato, Davide Francesco$$iINSPIRE-00383301$$uUtrecht U. 002299472 700__ $$aLonne, Per-ivar$$iINSPIRE-00262720$$uBergen U. 002299472 700__ $$aLoginov, Vitaly$$iINSPIRE-00262733$$uMoscow Phys. Eng. 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Space Science 002299472 700__ $$aRodriguez Cahuantzi, Mario$$iINSPIRE-00247954$$uPuebla U., Mexico 002299472 700__ $$aRoeed, Ketil$$iINSPIRE-00247948$$uOslo U. 002299472 700__ $$aRogalev, Roman$$iINSPIRE-00574457$$uSerpukhov, IHEP 002299472 700__ $$aRogochaya, Elena$$iINSPIRE-00385804$$jORCID:0000-0002-4278-5999$$uDubna, JINR 002299472 700__ $$aRohr, David Michael$$iINSPIRE-00248142$$uFrankfurt U., FIAS$$uCERN 002299472 700__ $$aRoehrich, Dieter$$iINSPIRE-00250583$$uBergen U. 002299472 700__ $$aRokita, Przemyslaw Stefan$$iINSPIRE-00564661$$uWarsaw U. of Tech. 002299472 700__ $$aRonchetti, Federico$$iINSPIRE-00139171$$jORCID:0000-0001-5245-8441$$uFrascati 002299472 700__ $$aDominguez Rosas, Edgar$$iINSPIRE-00576935$$uMexico U., ICN 002299472 700__ $$aRoslon, Krystian$$iINSPIRE-00639920$$uWarsaw U. of Tech. 002299472 700__ $$aRosnet, Philippe$$iINSPIRE-00121285$$uClermont-Ferrand U. 002299472 700__ $$aRossi, Andrea$$iINSPIRE-00290284$$jORCID:0000-0002-6067-6294$$uINFN, Padua$$uPadua U. 002299472 700__ $$aRotondi, Alberto$$iINSPIRE-00121413$$jORCID:0000-0003-1921-6808$$uPavia U., Dept. 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Space Science 002299472 700__ $$aShabanov, Arseniy$$iINSPIRE-00509394$$uMoscow, INR 002299472 700__ $$aShabetai, Alexandre$$iINSPIRE-00361563$$uSUBATECH, Nantes 002299472 700__ $$aShahoyan, Ruben$$iINSPIRE-00125510$$uCERN 002299472 700__ $$aShaikh, Wadut$$iINSPIRE-00574466$$uSaha Inst. 002299472 700__ $$aShangaraev, Artem$$iINSPIRE-00384482$$uSerpukhov, IHEP 002299472 700__ $$aSharma, Anjali$$iINSPIRE-00564690$$uPanjab U. 002299472 700__ $$aSharma, Ankita$$iINSPIRE-00509560$$uJammu U. 002299472 700__ $$aSharma, Natasha$$iINSPIRE-00291700$$uPanjab U. 002299472 700__ $$aSheikh, Ashik Ikbal$$iINSPIRE-00560398$$uCalcutta, VECC 002299472 700__ $$aShigaki, Kenta$$iINSPIRE-00125910$$uHiroshima U. 002299472 700__ $$aShimomura, Maya$$iINSPIRE-00243055$$uNara Women's U. 002299472 700__ $$aShirinkin, Sergey$$iINSPIRE-00577580$$uMoscow, ITEP 002299472 700__ $$aShou, Qiye$$iINSPIRE-00565745$$uHua-Zhong Normal U. 002299472 700__ $$aShtejer Diaz, Katherin$$iINSPIRE-00247746$$uINFN, Turin$$uTurin U.$$uHavana, CEADEN 002299472 700__ $$aSibiryak, Yury$$iINSPIRE-00250642$$uKurchatov Inst., Moscow 002299472 700__ $$aSiddhanta, Sabyasachi$$iINSPIRE-00245363$$jORCID:0000-0002-0543-9245$$uINFN, Cagliari 002299472 700__ $$aSielewicz, Krzysztof Marek$$iINSPIRE-00509501$$uCERN 002299472 700__ $$aSiemiarczuk, Teodor$$iINSPIRE-00291730$$uWarsaw, Inst. 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Phys. 002299472 700__ $$aSzabo, Alexander$$iINSPIRE-00416943$$uComenius U. 002299472 700__ $$aSzarka, Imrich$$iINSPIRE-00290465$$uComenius U. 002299472 700__ $$aTabassam, Uzma$$iINSPIRE-00531415$$uCOMSATS, Islamabad 002299472 700__ $$aTakahashi, Jun$$iINSPIRE-00183279$$jORCID:0000-0002-4091-1779$$uCampinas State U. 002299472 700__ $$aTambave, Ganesh Jagannath$$iINSPIRE-00529619$$uBergen U. 002299472 700__ $$aTanaka, Naoto$$iINSPIRE-00509743$$uTsukuba U. 002299472 700__ $$aTarhini, Mohamad$$iINSPIRE-00522518$$uOrsay, IPN$$uSUBATECH, Nantes 002299472 700__ $$aTariq, Mohammad$$iINSPIRE-00509805$$jORCID:0000-0002-9419-0102$$uAligarh Muslim U. 002299472 700__ $$aTarzila, Madalina-gabriela$$iINSPIRE-00416999$$uBucharest, IFIN-HH 002299472 700__ $$aTauro, Arturo$$iINSPIRE-00247582$$uCERN 002299472 700__ $$aTejeda Munoz, Guillermo$$iINSPIRE-00247570$$jORCID:0000-0003-2184-3106$$uPuebla U., Mexico 002299472 700__ $$aTelesca, Adriana$$iINSPIRE-00247569$$jORCID:0000-0002-6783-7230$$uCERN 002299472 700__ $$aTerasaki, Kohei$$iINSPIRE-00509855$$uTokyo U. 002299472 700__ $$aTerrevoli, Cristina$$iINSPIRE-00246722$$jORCID:0000-0002-1318-684X$$uINFN, Padua$$uPadua U. 002299472 700__ $$aTeyssier, Boris$$iINSPIRE-00509910$$uLyon, IPN 002299472 700__ $$aThakur, Dhananjaya$$iINSPIRE-00560404$$jORCID:0000-0001-7719-5238$$uIndian Inst. 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U., Universe$$uTech. U., Munich (main) 002299472 700__ $$aVoscek, Dominik$$iINSPIRE-00564764$$uKosice Tech. U. 002299472 700__ $$aVranic, Danilo$$iINSPIRE-00290668$$uCERN$$uDarmstadt, EMMI 002299472 700__ $$aVrlakova, Janka$$iINSPIRE-00244985$$uKosice U. 002299472 700__ $$aWagner, Boris$$iINSPIRE-00244999$$uBergen U. 002299472 700__ $$aWang, Hongkai$$iINSPIRE-00510390$$uUtrecht U. 002299472 700__ $$aWang, Mengliang$$iINSPIRE-00290694$$uHua-Zhong Normal U. 002299472 700__ $$aWatanabe, Yosuke$$iINSPIRE-00412045$$jORCID:0000-0001-5643-3516$$uTsukuba U.$$uTokyo U. 002299472 700__ $$aWeber, Michael$$iINSPIRE-00349115$$jORCID:0000-0001-5742-294X$$uStefan Meyer Inst. Subatomare Phys. 002299472 700__ $$aWeber, Steffen Georg$$iINSPIRE-00510469$$uDarmstadt, EMMI 002299472 700__ $$aWegrzynek, Adam$$iINSPIRE-00572414$$jORCID:0000-0002-3155-0887$$uCERN 002299472 700__ $$aWeiser, Dennis Franz$$iINSPIRE-00537176$$uHeidelberg U. 002299472 700__ $$aWenzel, Sandro Christian$$iINSPIRE-00287872$$uCERN 002299472 700__ $$aWessels, Johannes Peter$$iINSPIRE-00178848$$uMunster U. 002299472 700__ $$aWesterhoff, Uwe$$iINSPIRE-00246123$$uMunster U. 002299472 700__ $$aWhitehead, Andile Mothegi$$iINSPIRE-00537181$$uCape Town U. 002299472 700__ $$aWiechula, Jens$$iINSPIRE-00290727$$uFrankfurt U., Inst. Kernphys. 002299472 700__ $$aWikne, Jon$$iINSPIRE-00250749$$uOslo U. 002299472 700__ $$aWilk, Grzegorz Andrzej$$iINSPIRE-00135952$$uWarsaw, Inst. Nucl. Studies 002299472 700__ $$aWilkinson, Jeremy John$$iINSPIRE-00385005$$jORCID:0000-0003-0689-2858$$uINFN, Bologna 002299472 700__ $$aWillems, Guido Alexander$$iINSPIRE-00564789$$uMunster U.$$uCERN 002299472 700__ $$aWilliams, Crispin$$iINSPIRE-00254855$$jORCID:0000-0003-3589-0181$$uINFN, Bologna 002299472 700__ $$aWillsher, Emily$$iINSPIRE-00574082$$uBirmingham U. 002299472 700__ $$aWindelband, Bernd Stefan$$iINSPIRE-00246650$$uHeidelberg U. 002299472 700__ $$aWitt, William Edward$$iINSPIRE-00564770$$uTennessee U. 002299472 700__ $$aXu, Ran$$iINSPIRE-00651767$$uHua-Zhong Normal U. 002299472 700__ $$aYalcin, Serpil$$iINSPIRE-00412449$$uKaratay U. 002299472 700__ $$aYamakawa, Kosei$$iINSPIRE-00639310$$uHiroshima U. 002299472 700__ $$aYang, Ping$$iINSPIRE-00385084$$uHua-Zhong Normal U. 002299472 700__ $$aYano, Satoshi$$iINSPIRE-00385135$$uHiroshima U. 002299472 700__ $$aYin, Zhongbao$$iINSPIRE-00245030$$jORCID:0000-0003-4532-7544$$uHua-Zhong Normal U. 002299472 700__ $$aYokoyama, Hiroki$$iINSPIRE-00245044$$uTsukuba U.$$uLPSC, Grenoble 002299472 700__ $$aYoo, In-kwon$$iINSPIRE-00183678$$uPusan Natl. U. 002299472 700__ $$aYoon, Jin Hee$$iINSPIRE-00537195$$uInha U. 002299472 700__ $$aYun, Eungyu$$iINSPIRE-00639955$$uPusan Natl. U. 002299472 700__ $$aYurchenko, Volodymyr$$iINSPIRE-00510512$$uBITP, Kiev 002299472 700__ $$aZaccolo, Valentina$$iINSPIRE-00361691$$jORCID:0000-0002-6499-752X$$uINFN, Turin 002299472 700__ $$aZaman, Ali$$iINSPIRE-00385199$$uCOMSATS, Islamabad 002299472 700__ $$aZampolli, Chiara$$iINSPIRE-00247387$$jORCID:0000-0002-2608-4834$$uCERN 002299472 700__ $$aCorrea Zanoli, Henrique Jose$$iINSPIRE-00510636$$uSao Paulo U. 002299472 700__ $$aZardoshti, Nima$$iINSPIRE-00522360$$uBirmingham U. 002299472 700__ $$aZarochentsev, Andrey$$iINSPIRE-00246638$$jORCID:0000-0002-3502-8084$$uSt. Petersburg State U. 002299472 700__ $$aZavada, Petr$$iINSPIRE-00138107$$uPrague, Inst. Phys. 002299472 700__ $$aZavyalov, Nikolay$$iINSPIRE-00290800$$uRFNC-VNIIEF, Sarov 002299472 700__ $$aZbroszczyk, Hanna Paulina$$iINSPIRE-00183708$$uWarsaw U. of Tech. 002299472 700__ $$aZhalov, Mikhail$$iINSPIRE-00254612$$uSt. Petersburg, INP 002299472 700__ $$aZhang, Haitao$$iINSPIRE-00361703$$uHua-Zhong Normal U.$$uBergen U. 002299472 700__ $$aZhang, Xiaoming$$iINSPIRE-00290818$$uHua-Zhong Normal U. 002299472 700__ $$aZhang, Yonghong$$iINSPIRE-00385253$$uHua-Zhong Normal U. 002299472 700__ $$aChunhui, Zhang$$iINSPIRE-00522436$$uUtrecht U. 002299472 700__ $$aZhang, Zuman$$iINSPIRE-00531444$$uClermont-Ferrand U.$$uHua-Zhong Normal U. 002299472 700__ $$aZhao, Chengxin$$iINSPIRE-00385310$$uOslo U. 002299472 700__ $$aZhigareva, Natalia$$iINSPIRE-00385354$$uMoscow, ITEP 002299472 700__ $$aZhou, Daicui$$iINSPIRE-00290834$$uHua-Zhong Normal U. 002299472 700__ $$aZhou, You$$iINSPIRE-00290856$$jORCID:0000-0002-7868-6706$$uBohr Inst. 002299472 700__ $$aZhou, Zhuo$$iINSPIRE-00417116$$uBergen U. 002299472 700__ $$aZhu, Hongsheng$$iINSPIRE-00361728$$uBergen U.$$uHua-Zhong Normal U. 002299472 700__ $$aZhu, Jianhui$$iINSPIRE-00361715$$uHua-Zhong Normal U. 002299472 700__ $$aZhu, Ya$$iINSPIRE-00651777$$uHua-Zhong Normal U. 002299472 700__ $$aZichichi, Antonino$$iINSPIRE-00172134$$uEnrico Fermi Ctr., Rome$$uINFN, Bologna$$uBologna U. 002299472 700__ $$aZimmermann, Markus Bernhard$$iINSPIRE-00385420$$uCERN 002299472 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev 002299472 700__ $$aZmeskal, Johann$$iINSPIRE-00564793$$uStefan Meyer Inst. Subatomare Phys. 002299472 700__ $$aZou, Shuguang$$iINSPIRE-00571982$$uHua-Zhong Normal U. 002299472 710__ $$5PH 002299472 710__ $$gALICE Collaboration 002299472 773__ $$c624$$n8$$pEur. Phys. J. C$$v78$$y2018 002299472 859__ $$fenrico.scomparin@cern.ch 002299472 8564_ $$81377691$$s1172485$$uhttp://cds.cern.ch/record/2299472/files/CERN-EP-DRAFT-ALICE-2018-001 - draft.pdf$$yDraft (restricted)$$zStamped by WebSubmit: 10/01/2018 002299472 8564_ $$81380539$$s13006$$uhttp://cds.cern.ch/record/2299472/files/EtaPi0Ratio2mTScaling.png$$y00005 Left: \e /\pai ratio as function of \pT measured in NSD \pPb collisions at \spPb. The statistical uncertainties are shown as vertical error bars. The systematic uncertainties are represented as boxes. For comparison, also the \e /\pai ratios measured in \unit[7]{TeV} pp collisions with ALICE \cite{Abelev:2012cn}, in d-Au collisions at \sNNR with PHENIX \cite{PhysRevC.75.024909}, and in \pAu and \pBe collisions at \sNNSPS with TAPS/CERES \cite{Agakishiev:1998mw} are shown, as well as the ratio where the \e yield is obtained via \mT scaling from the measured \pPb \pai yield. Right: Ratio of the measured \e /\pai ratio to the one obtained via \mT scaling. 002299472 8564_ $$81380540$$s37843$$uhttp://cds.cern.ch/record/2299472/files/Comb_Pi0_RpA_Models_LogX_V3.png$$y00011 Comparison of different theoretical model calculations to the \pai (left) and \e (right) nuclear modification factors \RpA measured in NSD \pPb collisions at \spPb. The grey band shows a pQCD calculation at NLO using the EPPS16 nPDF~\cite{Eskola:2016oht}, the CT14 PDF~\cite{Dulat:2015mca} and the DSS14 FF~\cite{deFlorian:2014xna} including systematic uncertainties. Color Glass Condensate predictions using the {\ensuremath{k_{\mbox{\tiny T}}}\xspace} factorization method are also shown. NLO calculations using nCTEQ nPDF \cite{Kovarik:2015cma}, and DSS14 FF (\pai) \cite{deFlorian:2014xna} or AESSS FF (\e) \cite{Aidala:2010bn} are also shown. 002299472 8564_ $$81380541$$s25925$$uhttp://cds.cern.ch/record/2299472/files/RatioCombFitIndividualEta.png$$y00003 Ratio between individual \pai (left) and \e (right) invariant differential yield measurements, and Tsallis fit to the combined meson yield. The statistical uncertainties are represented as vertical error bars whereas the systematic uncertainties are shown as boxes. 002299472 8564_ $$81380542$$s1452211$$uhttp://cds.cern.ch/record/2299472/files/arXiv:1801.07051.pdf 002299472 8564_ $$81380543$$s47648$$uhttp://cds.cern.ch/record/2299472/files/MesonYields_And_PPReferences_TCM_NoPoints.png$$y00000 Left: Invariant differential \pai and \e yields produced in NSD \pPb collisions at \spPb. The statistical uncertainties are represented as vertical error bars whereas the systematic uncertainties are shown as boxes. In addition, Tsallis fits to the measured yields are shown. The TCM fit to the $\langle \TpPb \rangle$ scaled \pai and \e pp reference spectra (see \hyperref[sec:RpA]{Sect.~\ref*{sec:RpA}} for details) is shown. Right: Ratios of the measured data to their corresponding Tsallis fits. 002299472 8564_ $$81380544$$s9950$$uhttp://cds.cern.ch/record/2299472/files/Comb_Eta_RpA_WO_Models_LogX_V3.png$$y00007 \pai (left) and \e (right) nuclear modification factors \RpPb measured in NSD \pPb collisions at \spPb. The statistical uncertainties are shown as vertical error bars and the systematic uncertainties are represented as boxes. The overall normalization uncertainty is given as the solid black box around unity. 002299472 8564_ $$81380545$$s38079$$uhttp://cds.cern.ch/record/2299472/files/RatioCombFitIndividualPi0.png$$y00002 Ratio between individual \pai (left) and \e (right) invariant differential yield measurements, and Tsallis fit to the combined meson yield. The statistical uncertainties are represented as vertical error bars whereas the systematic uncertainties are shown as boxes. 002299472 8564_ $$81380546$$s12593$$uhttp://cds.cern.ch/record/2299472/files/MesonYields_WOModels_OnlyRatioLarger.png$$y00001 Left: Invariant differential \pai and \e yields produced in NSD \pPb collisions at \spPb. The statistical uncertainties are represented as vertical error bars whereas the systematic uncertainties are shown as boxes. In addition, Tsallis fits to the measured yields are shown. The TCM fit to the $\langle \TpPb \rangle$ scaled \pai and \e pp reference spectra (see \hyperref[sec:RpA]{Sect.~\ref*{sec:RpA}} for details) is shown. Right: Ratios of the measured data to their corresponding Tsallis fits. 002299472 8564_ $$81380547$$s74785$$uhttp://cds.cern.ch/record/2299472/files/MesonYields_EPOS_OnlyRatioLargerv2.png$$y00009 Comparison of several theoretical calculations to the invariant differential \pai and \e yields produced in NSD \pPb collisions at \spPb from \hyperref[fig:Pi0EtaYieldsModels]{Fig.~\ref*{fig:Pi0EtaYields}}. Theoretical calculations are shown for the EPOS3 model \cite{Werner:2013tya}, CGC model \cite{Lappi:2013zma}, pQCD calculations at NLO \cite{Helenius:2012wd,dEnterria:2013sgr,Jager:2002xm} using EPPS16 nPDF \cite{Eskola:2016oht} with the CT14 PDF \cite{Dulat:2015mca} or using the nCTEQ nPDF \cite{Kovarik:2015cma} and DSS14 FF \cite{deFlorian:2014xna} for the \pai and using nCTEQ nPDF \cite{Kovarik:2015cma} and AESSS FF \cite{Aidala:2010bn} for the \e meson, hydrodynamic framework (labeled as VISHNU) \cite{Shen:2016zpp} using the iEBE-VISHNU code \cite{Shen:2014vra}, DPMJET model \cite{Roesler:2000he}, and HIJING model \cite{Gyulassy:1994ew}. The blue band on the EPOS3 calculation shows the statistical errors of the prediction. The gray band on the pQCD calculation includes the uncertainties on the factorization, renormalization and fragmentation scales, as well as on the nPDF and FF. The ratios of the measured data and several theoretical calculations to the data Tsallis fits (\hyperref[fig:Pi0EtaYieldsModels]{Fig.~\ref*{fig:Pi0EtaYields}}) are shown in the right panel. 002299472 8564_ $$81380548$$s90052$$uhttp://cds.cern.ch/record/2299472/files/MesonYields_EPOSv2.png$$y00008 Comparison of several theoretical calculations to the invariant differential \pai and \e yields produced in NSD \pPb collisions at \spPb from \hyperref[fig:Pi0EtaYieldsModels]{Fig.~\ref*{fig:Pi0EtaYields}}. Theoretical calculations are shown for the EPOS3 model \cite{Werner:2013tya}, CGC model \cite{Lappi:2013zma}, pQCD calculations at NLO \cite{Helenius:2012wd,dEnterria:2013sgr,Jager:2002xm} using EPPS16 nPDF \cite{Eskola:2016oht} with the CT14 PDF \cite{Dulat:2015mca} or using the nCTEQ nPDF \cite{Kovarik:2015cma} and DSS14 FF \cite{deFlorian:2014xna} for the \pai and using nCTEQ nPDF \cite{Kovarik:2015cma} and AESSS FF \cite{Aidala:2010bn} for the \e meson, hydrodynamic framework (labeled as VISHNU) \cite{Shen:2016zpp} using the iEBE-VISHNU code \cite{Shen:2014vra}, DPMJET model \cite{Roesler:2000he}, and HIJING model \cite{Gyulassy:1994ew}. The blue band on the EPOS3 calculation shows the statistical errors of the prediction. The gray band on the pQCD calculation includes the uncertainties on the factorization, renormalization and fragmentation scales, as well as on the nPDF and FF. The ratios of the measured data and several theoretical calculations to the data Tsallis fits (\hyperref[fig:Pi0EtaYieldsModels]{Fig.~\ref*{fig:Pi0EtaYields}}) are shown in the right panel. 002299472 8564_ $$81380549$$s13374$$uhttp://cds.cern.ch/record/2299472/files/Comb_Eta_RpA_Models_LogX_V3.png$$y00012 Comparison of different theoretical model calculations to the \pai (left) and \e (right) nuclear modification factors \RpA measured in NSD \pPb collisions at \spPb. The grey band shows a pQCD calculation at NLO using the EPPS16 nPDF~\cite{Eskola:2016oht}, the CT14 PDF~\cite{Dulat:2015mca} and the DSS14 FF~\cite{deFlorian:2014xna} including systematic uncertainties. Color Glass Condensate predictions using the {\ensuremath{k_{\mbox{\tiny T}}}\xspace} factorization method are also shown. NLO calculations using nCTEQ nPDF \cite{Kovarik:2015cma}, and DSS14 FF (\pai) \cite{deFlorian:2014xna} or AESSS FF (\e) \cite{Aidala:2010bn} are also shown. 002299472 8564_ $$81380550$$s12302$$uhttp://cds.cern.ch/record/2299472/files/Comb_Pi0_RpA_WO_Models_LogX_V3.png$$y00006 \pai (left) and \e (right) nuclear modification factors \RpPb measured in NSD \pPb collisions at \spPb. The statistical uncertainties are shown as vertical error bars and the systematic uncertainties are represented as boxes. The overall normalization uncertainty is given as the solid black box around unity. 002299472 8564_ $$81380551$$s42240$$uhttp://cds.cern.ch/record/2299472/files/EtaPi0Ratio_LogX_EPOS_TAPSv2.png$$y00010 Comparison of different theoretical calculations to the \e /\pai ratio measured in NSD \pPb collisions at \spPb from \hyperref[fig:EtaPi0RatioALICE]{Fig.~\ref*{fig:EtaPi0RatioALICE}}. Theoretical calculations are shown for the EPOS3 model \cite{Werner:2013tya} with statistical errors shown as a band, hydrodynamic framework (VISHNU) \cite{Shen:2016zpp} using the iEBE-VISHNU code \cite{Shen:2014vra}, DPMJET model \cite{Roesler:2000he} and HIJING model \cite{Gyulassy:1994ew}. 002299472 8564_ $$81380552$$s37756$$uhttp://cds.cern.ch/record/2299472/files/EtaPi0Ratio_WO_Models.png$$y00004 Left: \e /\pai ratio as function of \pT measured in NSD \pPb collisions at \spPb. The statistical uncertainties are shown as vertical error bars. The systematic uncertainties are represented as boxes. For comparison, also the \e /\pai ratios measured in \unit[7]{TeV} pp collisions with ALICE \cite{Abelev:2012cn}, in d-Au collisions at \sNNR with PHENIX \cite{PhysRevC.75.024909}, and in \pAu and \pBe collisions at \sNNSPS with TAPS/CERES \cite{Agakishiev:1998mw} are shown, as well as the ratio where the \e yield is obtained via \mT scaling from the measured \pPb \pai yield. Right: Ratio of the measured \e /\pai ratio to the one obtained via \mT scaling. 002299472 8564_ $$81425528$$s2293109$$uhttp://cds.cern.ch/record/2299472/files/scoap3-fulltext.pdf?subformat=pdfa$$xpdfa$$yArticle from SCOAP3 002299472 8564_ $$82334687$$s2293109$$uhttp://cds.cern.ch/record/2299472/files/scoap.pdf$$yArticle from SCOAP3 002299472 9031_ $$aApproval requested for number CERN-EP-2018-002$$bCERN-EP-2018-002$$cEPPHAPP$$d2018-01-08 17:42:00$$e2018-01-15 17:42:00$$fenrico.scomparin@cern.ch$$swaiting 002299472 9031_ $$aDocument approved$$bCERN-EP-2018-002$$cEPPHAPP$$d2018-01-10 11:44:58$$froger.forty@cern.ch$$sapproved 002299472 916__ $$sn$$w201802 002299472 980__ $$aALICE_Papers 002299472 980__ $$aARTICLE