002282897 001__ 2282897 002282897 005__ 20210825081726.0 002282897 0248_ $$aoai:cds.cern.ch:2282897$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT 002282897 0247_ $$2DOI$$9bibmatch$$a10.1016/j.physletb.2017.12.021 002282897 035__ $$9Inspire$$a1623558 002282897 037__ $$9arXiv$$aarXiv:1709.04723$$cnucl-ex 002282897 037__ $$aCERN-EP-2017-241 002282897 041__ $$aeng 002282897 088__ $$9CERN-EP-DRAFT-ALICE-2017-022 002282897 100__ $$aAcharya, Shreyasi$$iINSPIRE-00570928$$uCalcutta, VECC$$vVariable Energy Cyclotron Centre, Kolkata, India 002282897 110__ $$aThe ALICE collaboration 002282897 245__ $$aConstraining the magnitude of the Chiral Magnetic Effect with Event Shape Engineering in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV 002282897 246__ $$9arXiv$$aConstraining the magnitude of the Chiral Magnetic Effect with Event Shape Engineering in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76$ TeV 002282897 269__ $$aGeneva$$bCERN$$c11 Sep 2017 002282897 260__ $$c2018-02-10 002282897 300__ $$a12 p 002282897 506__ $$dcds-edboard-alice@cern.ch 002282897 506__ $$malice-member [CERN] 002282897 506__ $$mcds-ph-ep-publications-referee [CERN] 002282897 500__ $$9arXiv$$a20 pages, 6 captioned figures, 1 tables, authors from page 15, submitted to PLB, figures at http://aliceinfo.cern.ch/ArtSubmission/node/3829 002282897 520__ $$aIn ultrarelativistic heavy-ion collisions, the event-by-event variation of the elliptic flow $v_2$ reflects fluctuations in the shape of the initial state of the system. This allows to select events with the same centrality but different initial geometry. This selection technique, Event Shape Engineering, has been used in the analysis of charge-dependent two- and three-particle correlations in Pb-Pb collisions at $\sqrt{s_{_{\rm NN}}} =2.76$ TeV. The two-particle correlator $\langle \cos(\varphi_\alpha - \varphi_\beta) \rangle$, calculated for different combinations of charges $\alpha$ and $\beta$, is almost independent of $v_2$ (for a given centrality), while the three-particle correlator $\langle \cos(\varphi_\alpha + \varphi_\beta - 2\psid) \rangle$ scales almost linearly both with the event $v_2$ and charged-particle pseudorapidity density. The charge dependence of the three-particle correlator is often interpreted as evidence for the Chiral Magnetic Effect (CME), a parity violating effect of the strong interaction. However, its measured dependence on $v_2$ points to a large non-CME contribution to the correlator. Comparing the results with Monte Carlo calculations including a magnetic field due to the spectators, the upper limit of the CME signal contribution to the three-particle correlator in the 10-50% centrality interval is found to be 26-33% at 95% confidence level. 002282897 520__ $$9Elsevier$$aIn ultrarelativistic heavy-ion collisions, the event-by-event variation of the elliptic flow v2 reflects fluctuations in the shape of the initial state of the system. This allows to select events with the same centrality but different initial geometry. This selection technique, Event Shape Engineering, has been used in the analysis of charge-dependent two- and three-particle correlations in Pb–Pb collisions at sNN=2.76 TeV. The two-particle correlator 〈cos(φα−φβ)〉 , calculated for different combinations of charges α and β , is almost independent of v2 (for a given centrality), while the three-particle correlator 〈cos(φα+φβ−2Ψ2)〉 scales almost linearly both with the event v2 and charged-particle pseudorapidity density. The charge dependence of the three-particle correlator is often interpreted as evidence for the Chiral Magnetic Effect (CME), a parity violating effect of the strong interaction. However, its measured dependence on v2 points to a large non-CME contribution to the correlator. Comparing the results with Monte Carlo calculations including a magnetic field due to the spectators, the upper limit of the CME signal contribution to the three-particle correlator in the 10–50% centrality interval is found to be 26–33% at 95% confidence level. 002282897 520__ $$9arXiv$$aIn ultrarelativistic heavy-ion collisions, the event-by-event variation of the elliptic flow $v_2$ reflects fluctuations in the shape of the initial state of the system. This allows to select events with the same centrality but different initial geometry. This selection technique, Event Shape Engineering, has been used in the analysis of charge-dependent two- and three-particle correlations in Pb-Pb collisions at $\sqrt{s_{_{\rm NN}}} =2.76$ TeV. The two-particle correlator $\langle \cos(\varphi_\alpha - \varphi_\beta) \rangle$, calculated for different combinations of charges $\alpha$ and $\beta$, is almost independent of $v_2$ (for a given centrality), while the three-particle correlator $\langle \cos(\varphi_\alpha + \varphi_\beta - 2\Psi_2) \rangle$ scales almost linearly both with the event $v_2$ and charged-particle pseudorapidity density. The charge dependence of the three-particle correlator is often interpreted as evidence for the Chiral Magnetic Effect (CME), a parity violating effect of the strong interaction. However, its measured dependence on $v_2$ points to a large non-CME contribution to the correlator. Comparing the results with Monte Carlo calculations including a magnetic field due to the spectators, the upper limit of the CME signal contribution to the three-particle correlator in the 10-50% centrality interval is found to be 26-33% at 95% confidence level. 002282897 540__ $$3Preprint$$aCC-BY-4.0 002282897 542__ $$3Preprint$$dCERN$$g2017 002282897 562__ $$cPublic comments 002282897 595__ $$aCERN EDS 002282897 65017 $$2SzGeCERN$$aNuclear Physics - Experiment 002282897 693__ $$aCERN LHC$$eALICE 002282897 690C_ $$aCERN 002282897 690C_ $$aARTICLE 002282897 700__ $$aAdam, Jaroslav$$iINSPIRE-00360890$$uCreighton U. 002282897 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. Phys. Inst. 002282897 700__ $$aAdolfsson, Jonatan$$iINSPIRE-00571154$$uLund U. 002282897 700__ $$aAggarwal, Madan Mohan$$iINSPIRE-00180711$$uPanjab U. 002282897 700__ $$aAglieri Rinella, Gianluca$$iINSPIRE-00249866$$uCERN 002282897 700__ $$aAgnello, Michelangelo$$iINSPIRE-00360901$$jORCID:0000-0002-0760-5075$$uTurin Polytechnic 002282897 700__ $$aAgrawal, Neelima$$iINSPIRE-00381545$$uIndian Inst. Tech., Mumbai 002282897 700__ $$aAhammed, Zubayer$$iINSPIRE-00180720$$uCalcutta, VECC 002282897 700__ $$aAhmad, Nazeer$$iINSPIRE-00249891$$uAligarh Muslim U. 002282897 700__ $$aAhn, Sang Un$$iINSPIRE-00254695$$uKISTI, Daejeon 002282897 700__ $$aAiola, Salvatore$$iINSPIRE-00381830$$jORCID:0000-0001-6209-7627$$uYale U. 002282897 700__ $$aAkindinov, Alexander$$iINSPIRE-00061314$$uMoscow, ITEP 002282897 700__ $$aAl-turany, Mohammad$$iINSPIRE-00571954$$uDarmstadt, EMMI 002282897 700__ $$aAlam, Sk Noor$$iINSPIRE-00415748$$uCalcutta, VECC 002282897 700__ $$aSilva De Albuquerque, Danilo$$iINSPIRE-00560229$$uCampinas State U. 002282897 700__ $$aAleksandrov, Dmitry$$iINSPIRE-00158344$$uKurchatov Inst., Moscow 002282897 700__ $$aAlessandro, Bruno$$iINSPIRE-00250010$$jORCID:0000-0001-9680-4940$$uINFN, Turin 002282897 700__ $$aAlfaro Molina, Jose Ruben$$iINSPIRE-00249844$$uMexico U. 002282897 700__ $$aAlici, Andrea$$iINSPIRE-00249832$$jORCID:0000-0003-3618-4617$$uBologna U.$$uINFN, Bologna$$uEnrico Fermi Ctr., Rome 002282897 700__ $$aAlkin, Anton$$iINSPIRE-00245838$$uBITP, Kiev 002282897 700__ $$aAlme, Johan$$iINSPIRE-00249819$$uBergen U. 002282897 700__ $$aAlt, Torsten$$iINSPIRE-00249807$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aAltenkamper, Lucas$$iINSPIRE-00639902$$uBergen U. 002282897 700__ $$aAltsybeev, Igor$$iINSPIRE-00307325$$uSt. Petersburg State U. 002282897 700__ $$aAlves Garcia Prado, Caio$$iINSPIRE-00382006$$uSao Paulo U. 002282897 700__ $$aAndrei, Cristian$$iINSPIRE-00249783$$uBucharest, IFIN-HH 002282897 700__ $$aAndreou, Dimitra$$iINSPIRE-00640214$$uCERN 002282897 700__ $$aAndrews, Harry Arthur$$iINSPIRE-00563780$$uBirmingham U. 002282897 700__ $$aAndronic, Anton$$iINSPIRE-00261430$$uDarmstadt, EMMI 002282897 700__ $$aAnguelov, Venelin$$iINSPIRE-00244018$$uHeidelberg U. 002282897 700__ $$aAnson, Christopher Daniel$$iINSPIRE-00240940$$uCreighton U. 002282897 700__ $$aAnticic, Tome$$iINSPIRE-00062373$$uBoskovic Inst., Zagreb 002282897 700__ $$aAntinori, Federico$$iINSPIRE-00175367$$jORCID:0000-0002-7366-8891$$uINFN, Padua 002282897 700__ $$aAntonioli, Pietro$$iINSPIRE-00058331$$jORCID:0000-0001-7516-3726$$uINFN, Bologna 002282897 700__ $$aAnwar, Rafay$$iINSPIRE-00563792$$uHouston U. 002282897 700__ $$aAphecetche, Laurent Bernard$$iINSPIRE-00058998$$uSUBATECH, Nantes 002282897 700__ $$aAppelshaeuser, Harald$$iINSPIRE-00250020$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aArcelli, Silvia$$iINSPIRE-00250042$$jORCID:0000-0001-6367-9215$$uBologna U.$$uINFN, Bologna 002282897 700__ $$aArnaldi, Roberta$$iINSPIRE-00261446$$jORCID:0000-0001-6698-9577$$uINFN, Turin 002282897 700__ $$aArnold, Oliver Werner$$iINSPIRE-00537106$$uTech. U., Munich (main)$$uMunich, Tech. U., Universe 002282897 700__ $$aArsene, Ionut Cristian$$iINSPIRE-00261457$$uOslo U. 002282897 700__ $$aArslandok, Mesut$$iINSPIRE-00245664$$uHeidelberg U. 002282897 700__ $$aAudurier, Benjamin$$iINSPIRE-00522415$$uSUBATECH, Nantes 002282897 700__ $$aAugustinus, Andre$$iINSPIRE-00261469$$uCERN 002282897 700__ $$aAverbeck, Ralf Peter$$iINSPIRE-00063377$$uDarmstadt, EMMI 002282897 700__ $$aAzmi, Mohd Danish$$iINSPIRE-00249731$$uAligarh Muslim U. 002282897 700__ $$aBadala, Angela$$iINSPIRE-00249728$$jORCID:0000-0002-0569-4828$$uINFN, Catania 002282897 700__ $$aBaek, Yong Wook$$iINSPIRE-00249716$$uInha U.$$uKonkuk U. 002282897 700__ $$aBagnasco, Stefano$$iINSPIRE-00028794$$jORCID:0000-0001-6062-6505$$uINFN, Turin 002282897 700__ $$aBailhache, Raphaelle Marie$$iINSPIRE-00247346$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aBala, Renu$$iINSPIRE-00261473$$uJammu U. 002282897 700__ $$aBaldisseri, Alberto$$iINSPIRE-00064101$$uIRFU, Saclay 002282897 700__ $$aBall, Markus$$iINSPIRE-00386117$$uBonn U., HISKP 002282897 700__ $$aBaral, Rama Chandra$$iINSPIRE-00289153$$uBhubaneswar, Inst. Phys.$$uNISER, Jatni 002282897 700__ $$aBarbano, Anastasia Maria$$iINSPIRE-00506685$$uTurin U.$$uINFN, Turin 002282897 700__ $$aBarbera, Roberto$$iINSPIRE-00250052$$jORCID:0000-0001-5971-6415$$uCatania U.$$uINFN, Catania 002282897 700__ $$aBarile, Francesco$$iINSPIRE-00249702$$jORCID:0000-0003-2088-1290$$uINFN, Bari$$uBari U. 002282897 700__ $$aBarioglio, Luca$$iINSPIRE-00575020$$uTurin U.$$uINFN, Turin 002282897 700__ $$aBarnafoldi, Gergely Gabor$$iINSPIRE-00261490$$uWigner RCP, Budapest 002282897 700__ $$aBarnby, Lee Stuart$$iINSPIRE-00064600$$jORCID:0000-0001-7357-9904$$uDaresbury 002282897 700__ $$aRamillien Barret, Valerie$$iINSPIRE-00261503$$uClermont-Ferrand U. 002282897 700__ $$aBartalini, Paolo$$iINSPIRE-00064862$$uHua-Zhong Normal U. 002282897 700__ $$aBarth, Klaus$$iINSPIRE-00522252$$uCERN 002282897 700__ $$aBartsch, Esther$$iINSPIRE-00506794$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aBasile, Maurizio$$iINSPIRE-00172080$$jORCID:0000-0002-1372-8063$$uBologna U.$$uINFN, Bologna 002282897 700__ $$aBastid, Nicole$$iINSPIRE-00065071$$uClermont-Ferrand U. 002282897 700__ $$aBasu, Sumit$$iINSPIRE-00360931$$uWayne State U. 002282897 700__ $$aBatigne, Guillaume$$iINSPIRE-00057450$$uSUBATECH, Nantes 002282897 700__ $$aBatyunya, Boris$$iINSPIRE-00180230$$uDubna, JINR 002282897 700__ $$aBatzing, Paul Christoph$$iINSPIRE-00382071$$uOslo U. 002282897 700__ $$aBazo Alba, Jose Luis$$iINSPIRE-00047770$$uLima, Pont. U. Catolica 002282897 700__ $$aBearden, Ian Gardner$$iINSPIRE-00261515$$jORCID:0000-0003-2784-3094$$uBohr Inst. 002282897 700__ $$aBeck, Hans$$iINSPIRE-00261523$$uHeidelberg U. 002282897 700__ $$aBedda, Cristina$$iINSPIRE-00382119$$uUtrecht U. 002282897 700__ $$aBehera, Nirbhay Kumar$$iINSPIRE-00299673$$uInha U. 002282897 700__ $$aBelikov, Iouri$$iINSPIRE-00250068$$uStrasbourg, IPHC 002282897 700__ $$aBellini, Francesca$$iINSPIRE-00244351$$jORCID:0000-0003-3498-4661$$uBologna U.$$uINFN, Bologna$$uCERN 002282897 700__ $$aBello Martinez, Hector$$iINSPIRE-00506861$$uPuebla U., Mexico 002282897 700__ $$aBellwied, Rene$$iINSPIRE-00180735$$uHouston U. 002282897 700__ $$aEspinoza Beltran, Lucina Gabriela$$iINSPIRE-00563992$$uSinaloa U. 002282897 700__ $$aBelyaev, Vladimir$$iINSPIRE-00386131$$uMoscow Phys. Eng. Inst. 002282897 700__ $$aBencedi, Gyula$$iINSPIRE-00360943$$uWigner RCP, Budapest 002282897 700__ $$aBeole, Stefania$$iINSPIRE-00261543$$jORCID:0000-0003-4673-8038$$uTurin U.$$uINFN, Turin 002282897 700__ $$aBercuci, Alexandru$$iINSPIRE-00261560$$uBucharest, IFIN-HH 002282897 700__ $$aBerdnikov, Yaroslav$$iINSPIRE-00066204$$uSt. Petersburg, INP 002282897 700__ $$aBerenyi, Daniel$$iINSPIRE-00245794$$uWigner RCP, Budapest 002282897 700__ $$aBertens, Redmer Alexander$$iINSPIRE-00382235$$uTennessee U. 002282897 700__ $$aBerzano, Dario$$iINSPIRE-00245123$$uCERN 002282897 700__ $$aBetev, Latchezar$$iINSPIRE-00250085$$uCERN 002282897 700__ $$aBhasin, Anju$$iINSPIRE-00180740$$uJammu U. 002282897 700__ $$aBhat, Inayat Rasool$$iINSPIRE-00415990$$uJammu U. 002282897 700__ $$aBhati, Ashok Kumar$$iINSPIRE-00180755$$uPanjab U. 002282897 700__ $$aBhattacharjee, Buddhadeb$$iINSPIRE-00385476$$uGauhati U. 002282897 700__ $$aBhom, Jihyun$$iINSPIRE-00287624$$uCracow, INP 002282897 700__ $$aBianchi, Antonio$$iINSPIRE-00584065$$uTurin U.$$uINFN, Turin 002282897 700__ $$aBianchi, Livio$$iINSPIRE-00254651$$uHouston U. 002282897 700__ $$aBianchi, Nicola$$iINSPIRE-00139110$$jORCID:0000-0001-6861-2810$$uFrascati 002282897 700__ $$aBianchin, Chiara$$iINSPIRE-00247334$$uWayne State U. 002282897 700__ $$aBielcik, Jaroslav$$iINSPIRE-00180768$$uPrague, Tech. 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Volta' 002282897 700__ $$aBock, Friederike$$iINSPIRE-00246175$$jORCID:0000-0003-4185-2093$$uLBL, Berkeley$$uCERN$$uHeidelberg U. 002282897 700__ $$aBogdanov, Alexey$$iINSPIRE-00261637$$uMoscow Phys. Eng. Inst. 002282897 700__ $$aBoldizsar, Laszlo$$iINSPIRE-00307799$$uWigner RCP, Budapest 002282897 700__ $$aBombara, Marek$$iINSPIRE-00261642$$uKosice U. 002282897 700__ $$aBonomi, Germano$$iINSPIRE-00068097$$jORCID:0000-0003-1618-9648$$uU. Brescia 002282897 700__ $$aBonora, Matthias$$iINSPIRE-00563828$$uCERN 002282897 700__ $$aBook, Julian Heinz$$iINSPIRE-00261651$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aBorel, Herve$$iINSPIRE-00068253$$uIRFU, Saclay 002282897 700__ $$aBorissov, Alexander$$iINSPIRE-00254729$$uHeidelberg U.$$uPusan Natl. U. 002282897 700__ $$aBorri, Marcello$$iINSPIRE-00286268$$uLiverpool U. 002282897 700__ $$aBotta, Elena$$iINSPIRE-00250108$$jORCID:0000-0002-5054-1521$$uTurin U.$$uINFN, Turin 002282897 700__ $$aBourjau, Christian$$iINSPIRE-00537054$$uBohr Inst. 002282897 700__ $$aBratrud, Lars$$iINSPIRE-00246212$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aBraun-munzinger, Peter$$iINSPIRE-00069060$$uDarmstadt, EMMI 002282897 700__ $$aBregant, Marco$$iINSPIRE-00261672$$uSao Paulo U. 002282897 700__ $$aBroker, Theo Alexander$$iINSPIRE-00382350$$uFrankfurt U., Inst. Kernphys. 002282897 700__ $$aBroz, Michal$$iINSPIRE-00246094$$uPrague, Tech. 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Subatomare Phys. 002282897 700__ $$aCarena, Francesco$$iINSPIRE-00289308$$uCERN 002282897 700__ $$aCarena, Wisla$$iINSPIRE-00186542$$uCERN 002282897 700__ $$aCarnesecchi, Francesca$$iINSPIRE-00531272$$jORCID:0000-0001-9981-7536$$uBologna U.$$uINFN, Bologna$$uEnrico Fermi Ctr., Rome 002282897 700__ $$aCastillo Castellanos, Javier Ernesto$$iINSPIRE-00247261$$jORCID:0000-0002-5187-2779$$uIRFU, Saclay 002282897 700__ $$aCastro, Andrew John$$iINSPIRE-00507151$$uTennessee U. 002282897 700__ $$aCasula, Ester Anna Rita$$iINSPIRE-00360992$$jORCID:0000-0003-3599-4570$$uINFN, Cagliari 002282897 700__ $$aCeballos Sanchez, Cesar$$iINSPIRE-00361004$$uHavana, CEADEN 002282897 700__ $$aCerello, Piergiorgio$$iINSPIRE-00071926$$jORCID:0000-0002-2443-5178$$uINFN, Turin 002282897 700__ $$aChandra, Sinjini$$iINSPIRE-00576517$$jORCID:0000-0003-4238-2302$$uCalcutta, VECC 002282897 700__ $$aChang, Beomsu$$iINSPIRE-00241230$$uJyvaskyla U. 002282897 700__ $$aChapeland, Sylvain$$iINSPIRE-00249510$$jORCID:0000-0003-4511-4784$$uCERN 002282897 700__ $$aChartier, Marielle$$iINSPIRE-00385460$$uLiverpool U. 002282897 700__ $$aChattopadhyay, Subhasis$$iINSPIRE-00180920$$uCalcutta, VECC 002282897 700__ $$aChattopadhyay, Sukalyan$$iINSPIRE-00207158$$uSaha Inst. 002282897 700__ $$aChauvin, Alex$$iINSPIRE-00548342$$uMunich, Tech. 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Eng. Inst. 002282897 700__ $$aKar, Somnath$$iINSPIRE-00383167$$uCalcutta, VECC 002282897 700__ $$aKarasu Uysal, Ayben$$iINSPIRE-00245978$$uKaratay U. 002282897 700__ $$aKaravichev, Oleg$$iINSPIRE-00262581$$uMoscow, INR 002282897 700__ $$aKaravicheva, Tatiana$$iINSPIRE-00262593$$uMoscow, INR 002282897 700__ $$aKarayan, Lilit$$iINSPIRE-00522297$$uDarmstadt, EMMI$$uHeidelberg U. 002282897 700__ $$aKarczmarczyk, Przemyslaw$$iINSPIRE-00577574$$uCERN 002282897 700__ $$aKarpechev, Evgeny$$iINSPIRE-00248813$$uMoscow, INR 002282897 700__ $$aKebschull, Udo Wolfgang$$iINSPIRE-00248807$$uGoethe U., Frankfurt, Inst. 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Tech., Mumbai 002282897 700__ $$aNania, Rosario$$iINSPIRE-00172055$$uINFN, Bologna$$uEnrico Fermi Ctr., Rome 002282897 700__ $$aNappi, Eugenio$$iINSPIRE-00110416$$jORCID:0000-0003-2080-9010$$uINFN, Bari 002282897 700__ $$aNarayan, Amrendra$$iINSPIRE-00470117$$jORCID:0000-0003-3814-9559$$uIndian Inst. Tech., Mumbai 002282897 700__ $$aNaru, Muhammad Umair$$iINSPIRE-00507883$$uCOMSATS, Islamabad 002282897 700__ $$aFerreira Natal Da Luz, Pedro Hugo$$iINSPIRE-00511516$$uSao Paulo U. 002282897 700__ $$aNattrass, Christine$$iINSPIRE-00301613$$jORCID:0000-0002-8768-6468$$uTennessee U. 002282897 700__ $$aRosado Navarro, Sebastian$$iINSPIRE-00548422$$uPuebla U., Mexico 002282897 700__ $$aNayak, Kishora$$iINSPIRE-00416777$$uNISER, Jatni 002282897 700__ $$aNayak, Ranjit$$iINSPIRE-00548439$$jORCID:0000-0001-6988-0606$$uIndian Inst. 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Phys. 002282897 700__ $$aZavyalov, Nikolay$$iINSPIRE-00290800$$uRFNC-VNIIEF, Sarov 002282897 700__ $$aZbroszczyk, Hanna Paulina$$iINSPIRE-00183708$$uWarsaw U. of Tech. 002282897 700__ $$aZhalov, Mikhail$$iINSPIRE-00254612$$uSt. Petersburg, INP 002282897 700__ $$aZhang, Haitao$$iINSPIRE-00361703$$uBergen U.$$uHua-Zhong Normal U. 002282897 700__ $$aZhang, Xiaoming$$iINSPIRE-00290818$$uHua-Zhong Normal U. 002282897 700__ $$aZhang, Yonghong$$iINSPIRE-00385253$$uHua-Zhong Normal U. 002282897 700__ $$aChunhui, Zhang$$iINSPIRE-00522436$$uUtrecht U. 002282897 700__ $$aZhang, Zuman$$iINSPIRE-00531444$$uHua-Zhong Normal U.$$uClermont-Ferrand U. 002282897 700__ $$aZhao, Chengxin$$iINSPIRE-00385310$$uOslo U. 002282897 700__ $$aZhigareva, Natalia$$iINSPIRE-00385354$$uMoscow, ITEP 002282897 700__ $$aZhou, Daicui$$iINSPIRE-00290834$$uHua-Zhong Normal U. 002282897 700__ $$aZhou, You$$iINSPIRE-00290856$$jORCID:0000-0002-7868-6706$$uBohr Inst. 002282897 700__ $$aZhou, Zhuo$$iINSPIRE-00417116$$uBergen U. 002282897 700__ $$aZhu, Hongsheng$$iINSPIRE-00361728$$uBergen U. 002282897 700__ $$aZhu, Jianhui$$iINSPIRE-00361715$$uHua-Zhong Normal U. 002282897 700__ $$aZichichi, Antonino$$iINSPIRE-00172134$$uBologna U.$$uINFN, Bologna$$uEnrico Fermi Ctr., Rome 002282897 700__ $$aZimmermann, Alice$$iINSPIRE-00361741$$uHeidelberg U. 002282897 700__ $$aZimmermann, Markus Bernhard$$iINSPIRE-00385420$$uCERN 002282897 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev 002282897 700__ $$aZmeskal, Johann$$iINSPIRE-00564793$$uStefan Meyer Inst. Subatomare Phys. 002282897 700__ $$aZou, Shuguang$$iINSPIRE-00571982$$uHua-Zhong Normal U. 002282897 710__ $$5PH 002282897 710__ $$gALICE 002282897 773__ $$c151-162$$pPhys. Lett. B$$v777$$y2018 002282897 859__ $$fcloizides@lbl.gov 002282897 8564_ $$81348079$$s489156$$uhttps://cds.cern.ch/record/2282897/files/CERN-EP-DRAFT-ALICE-2017-022 - draft.pdf$$yDraft (restricted)$$zStamped by WebSubmit: 12/09/2017 002282897 8564_ $$82207616$$s59319$$uhttps://cds.cern.ch/record/2282897/files/plots_fig3.png$$y00002 (Colour online) Top: Difference between opposite and same charge pair correlations for $\gc$ as a function of $v_2$ for shape selected events together with a linear fit (dashed lines) for various centrality classes. Bottom: Difference between opposite and same charge pair correlations for $\gc$ multiplied by the charged-particle density~\cite{Aamodt:2010cz} as a function of $v_2$ for shape selected events for various centrality classes. The event selection is based on $q_2$ determined in the V0C with the lowest (highest) value corresponding to 0--10\% (90--100\%) $q_2$. Error bars (shaded boxes) represent the statistical (systematic) uncertainties. 002282897 8564_ $$82207617$$s83865$$uhttps://cds.cern.ch/record/2282897/files/plots_fig2.png$$y00001 (Colour online) Top: Centrality dependence of $\gc$ for pairs of particles with same and opposite charge for shape selected and unbiased events. Bottom: Centrality dependence of $\dc$ for pairs of particles with same and opposite charge for shape selected and unbiased events.The event selection is based on $q_2$ determined in the V0C with the lowest (highest) value corresponding to 0--10\% (90--100\%) $q_2$. Points are slightly shifted along the horizontal axis for better visibility in both panels. Error bars (shaded boxes) represent the statistical (systematic) uncertainties. 002282897 8564_ $$82207618$$s31277$$uhttps://cds.cern.ch/record/2282897/files/plots_fig1.png$$y00000 (Colour online) Unidentified charged particle $v_2$ for shape selected and unbiased events as a function of collision centrality. The event selection is based on $q_2$ determined in the V0C with the lowest (highest) value corresponding to 0--10\% (90--100\%) $q_2$. Points are slightly shifted along the horizontal axis for better visibility. Error bars (shaded boxes) represent the statistical (systematic) uncertainties. 002282897 8564_ $$82207619$$s7634$$uhttps://cds.cern.ch/record/2282897/files/plots_fig6.png$$y00005 (Colour online) Centrality dependence of the CME fraction extracted from the slope parameter of fits to data and MC-Glauber~\cite{Miller:2007ri}, MC-KLN CGC~\cite{Drescher:2007ax, ALbacete:2010ad} and EKRT~\cite{Niemi:2015qia} models, respectively (see text for details). The dashed lines indicate the physical parameter space of the CME fraction. Points are slightly shifted along the horizontal axis for better visibility. Only statistical uncertainties are shown. 002282897 8564_ $$82207620$$s10368$$uhttps://cds.cern.ch/record/2282897/files/plots_fig5.png$$y00004 (Colour online) Centrality dependence of the $p_{1}$ parameter from a linear fit to the difference between opposite and same charge pair correlations for $\gc$ and from linear fits to the CME signal expectations from MC-Glauber~\cite{Miller:2007ri}, MC-KLN CGC~\cite{Drescher:2007ax, ALbacete:2010ad} and EKRT~\cite{Niemi:2015qia} models (see text for details). Points from MC simulations are slightly shifted along the horizontal axis for better visibility. Only statistical uncertainties are shown. 002282897 8564_ $$82207621$$s40814$$uhttps://cds.cern.ch/record/2282897/files/plots_fig4.png$$y00003 (Colour online) The expected dependence of the CME signal on $v_2$ for various centrality classes from a MC-Glauber simulation~\cite{Miller:2007ri} (see text for details). No event shape selection is performed in the model, and therefore a large range in $v_2$ is covered. The solid lines depict linear fits based on the $v_2$ variation observed within each centrality interval. 002282897 8564_ $$82207622$$s787669$$uhttps://cds.cern.ch/record/2282897/files/arXiv:1709.04723.pdf 002282897 8564_ $$82207623$$s861072$$uhttps://cds.cern.ch/record/2282897/files/scoap3-fulltext.pdf$$yArticle from SCOAP3 002282897 9031_ $$aApproval requested for number CERN-EP-2017-241$$bCERN-EP-2017-241$$cEPPHAPP$$d2017-09-11 12:15:31$$e2017-09-18 12:15:31$$fcloizides@lbl.gov$$swaiting 002282897 9031_ $$aDocument approved$$bCERN-EP-2017-241$$cEPPHAPP$$d2017-09-12 17:37:16$$froger.forty@cern.ch$$sapproved 002282897 916__ $$sn$$w201737 002282897 980__ $$aALICE_Papers 002282897 980__ $$aARTICLE