Accueil > CERN Experiments > LHC Experiments > ALICE > ALICE Preprints > Measurement of deuteron spectra and elliptic flow in Pb–Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV at the LHC > HTML MARC |
002274147 001__ 2274147 002274147 005__ 20241127052111.0 002274147 0248_ $$aoai:cds.cern.ch:2274147$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT 002274147 0247_ $$2DOI$$9bibmatch$$a10.1140/epjc/s10052-017-5222-x 002274147 037__ $$9arXiv$$aarXiv:1707.07304$$cnucl-ex 002274147 037__ $$aCERN-EP-2017-176 002274147 035__ $$9arXiv$$aoai:arXiv.org:1707.07304 002274147 035__ $$9Inspire$$aoai:inspirehep.net:1611301$$d2024-11-26T15:21:16Z$$h2024-11-27T03:03:31Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d 002274147 035__ $$9Inspire$$a1611301 002274147 041__ $$aeng 002274147 088__ $$9CERN-EP-DRAFT-ALICE-2017-015 002274147 100__ $$aAcharya, Shreyasi$$iINSPIRE-00570928$$tGRID:grid.482273.8$$uCalcutta, VECC$$vVariable Energy Cyclotron Centre - Kolkata - India 002274147 110__ $$aThe ALICE collaboration 002274147 245__ $$aMeasurement of deuteron spectra and elliptic flow in Pb–Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV at the LHC 002274147 246__ $$9arXiv$$aMeasurement of deuteron spectra and elliptic flow in Pb-Pb collisions at $\mathbf{\sqrt{s_{\rm NN}}}$ = 2.76 TeV at the LHC 002274147 260__ $$c2017-10-04 002274147 269__ $$aGeneva$$bCERN$$c12 Jul 2017 002274147 300__ $$a27 p 002274147 506__ $$dcds-edboard-alice@cern.ch 002274147 506__ $$malice-member [CERN] 002274147 506__ $$mcds-ph-ep-publications-referee [CERN] 002274147 500__ $$9arXiv$$a27 pages, 9 captioned figures, 3 tables, authors from page 22, published version, figures at http://aliceinfo.cern.ch/ArtSubmission/node/3691 002274147 520__ $$9Springer$$aThe transverse momentum ( $p_\mathrm{T} $ ) spectra and elliptic flow coefficient ( $v_{2}$ ) of deuterons and anti-deuterons at mid-rapidity ( $|y|<0.5$ ) are measured with the ALICE detector at the LHC in Pb–Pb collisions at $\sqrt{s_{\mathrm {NN}}}$ = 2.76 TeV. The measurement of the $p_\mathrm{T} $ spectra of (anti-)deuterons is done up to 8 GeV $/c$ in 0–10% centrality class and up to 6 GeV $/c$ in 10–20% and 20–40% centrality classes. The $v_{2}$ is measured in the 0.8 < $p_\mathrm{T} $ $<~$ 5 GeV $/c$ interval and in six different centrality intervals (0–5, 5–10, 10–20, 20–30, 30–40 and 40–50%) using the scalar product technique. Measured $\pi^{\pm }$ , K$^{\pm }$ and p+ $\overline{\mathrm {p}}$ transverse-momentum spectra and $v_{2}$ are used to predict the deuteron $p_\mathrm{T} $ spectra and $v_{2}$ within the Blast-Wave model. The predictions are able to reproduce the $v_{2}$ coefficient in the measured $p_\mathrm{T} $ range and the transverse-momentum spectra for $p_\mathrm{T} $ > 1.8 GeV $/c$ within the experimental uncertainties. The measurement of the coalescence parameter $B_2$ is performed, showing a $p_\mathrm{T} $ dependence in contrast with the simplest coalescence model, which fails to reproduce also the measured $v_{2}$ coefficient. In addition, the coalescence parameter $B_2$ and the elliptic flow coefficient in the 20–40% centrality interval are compared with the AMPT model which is able, in its version without string melting, to reproduce the measured $v_{2}$ ( $p_\mathrm{T} $ ) and the $B_2$ ( $p_\mathrm{T} $ ) trend. 002274147 520__ $$9arXiv$$aThe transverse momentum ($p_{\rm T}$) spectra and elliptic flow coefficient ($v_2$) of deuterons and anti-deuterons at mid-rapidity ($|y|<0.5$) are measured with the ALICE detector at the LHC in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV. The measurement of the $p_{\rm T}$ spectra of (anti-)deuterons is done up to 8 GeV/$c$ in 0-10% centrality class and up to GeV/$c$ in 10-20% and 20-40% centrality classes. The $v_2$ is measured in the $0.8 <p_{\rm T} <5$ GeV/$c$ interval and in six different centrality intervals (0-5%, 5-10%, 10-20%, 20-30%, 30-40% and 40-50%) using the scalar product technique. Measured $\pi^{\pm}$, K$^{\pm}$ and p+$\overline{\mathrm{p}}$ transverse-momentum spectra and $v_2$ are used to predict the deuteron $p_{\rm T}$ spectra and $v_2$ within the Blast-Wave model. The predictions are able to reproduce the $v_2$ coefficient in the measured $p_{\rm T}$ range and the transverse-momentum spectra for $p_{\rm T}>1.8$ GeV/$c$ within the experimental uncertainties. The measurement of the coalescence parameter $B_2$ is performed, showing a $p_{\rm T}$ dependence in contrast with the simplest coalescence model, which fails to reproduce also the measured $v_2$ coefficient. In addition, the coalescence parameter $B_2$ and the elliptic flow coefficient in the 20-40% centrality interval are compared with the AMPT model which is able, in its version without string melting, to reproduce the measured $v_2$($p_{\rm T}$) and the $B_2$($p_{\rm T}$) trend. 002274147 540__ $$3Preprint$$aCC-BY-4.0 002274147 542__ $$3Preprint$$dCERN$$g2017 002274147 562__ $$cPublic comments 002274147 595__ $$aCERN EDS 002274147 65017 $$2SzGeCERN$$aNuclear Physics - Experiment 002274147 65017 $$2arXiv$$ahep-ex 002274147 65017 $$2SzGeCERN$$aParticle Physics - Experiment 002274147 65017 $$2arXiv$$anucl-ex 002274147 693__ $$aCERN LHC$$eALICE 002274147 690C_ $$aCERN 002274147 690C_ $$aARTICLE 002274147 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. Phys. 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U. 002274147 700__ $$aHornung, Sebastian$$iINSPIRE-00584070$$uDarmstadt, EMMI 002274147 700__ $$aHosokawa, Ritsuya$$iINSPIRE-00522280$$uTsukuba U.$$uLPSC, Grenoble 002274147 700__ $$aHristov, Peter Zahariev$$iINSPIRE-00091290$$uCERN 002274147 700__ $$aHughes, Charles$$iINSPIRE-00564077$$uTennessee U. 002274147 700__ $$aHumanic, Thomas$$iINSPIRE-00091603$$uOhio State U. 002274147 700__ $$aHussain, Nur$$iINSPIRE-00416277$$uGauhati U. 002274147 700__ $$aHussain, Tahir$$iINSPIRE-00507708$$jORCID:0000-0002-4951-5756$$uAligarh Muslim U. 002274147 700__ $$aHutter, Dirk$$iINSPIRE-00382970$$jORCID:0000-0002-1488-4009$$uFrankfurt U., FIAS 002274147 700__ $$aHwang, Dae Sung$$iINSPIRE-00091772$$uSejong U. 002274147 700__ $$aIga Buitron, Sergio Arturo$$iINSPIRE-00572756$$uMexico U., ICN 002274147 700__ $$aIlkaev, Radiy$$iINSPIRE-00248935$$uRFNC-VNIIEF, Sarov 002274147 700__ $$aInaba, Motoi$$iINSPIRE-00241821$$uTsukuba U. 002274147 700__ $$aIppolitov, Mikhail$$iINSPIRE-00250300$$uMoscow Phys. Eng. Inst.$$uKurchatov Inst., Moscow 002274147 700__ $$aIrfan, Muhammad$$iINSPIRE-00248911$$uAligarh Muslim U. 002274147 700__ $$aIsakov, Vladimir$$iINSPIRE-00564085$$uMoscow, INR 002274147 700__ $$aIvanov, Marian$$iINSPIRE-00262538$$uDarmstadt, EMMI 002274147 700__ $$aIvanov, Vladimir$$iINSPIRE-00262542$$uSt. Petersburg, INP 002274147 700__ $$aIzucheev, Vladimir$$iINSPIRE-00506818$$uSerpukhov, IHEP 002274147 700__ $$aJacak, Barbara$$iINSPIRE-00155696$$uLBL, Berkeley 002274147 700__ $$aJacazio, Nicolo$$iINSPIRE-00548380$$uBologna U.$$uINFN, Bologna 002274147 700__ $$aJacobs, Peter Martin$$iINSPIRE-00181871$$uLBL, Berkeley 002274147 700__ $$aJadhav, Manoj Bhanudas$$iINSPIRE-00531323$$jORCID:0000-0002-5225-2803$$uIndian Inst. Tech., Mumbai 002274147 700__ $$aJadlovsky, Jan$$iINSPIRE-00537120$$uKosice Tech. U. 002274147 700__ $$aJaelani, Syaefudin$$iINSPIRE-00581977$$uUtrecht U. 002274147 700__ $$aJahnke, Cristiane$$iINSPIRE-00383021$$uMunich, Tech. 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Eng. Inst. 002274147 700__ $$aKar, Somnath$$iINSPIRE-00383167$$uCalcutta, VECC 002274147 700__ $$aKarasu Uysal, Ayben$$iINSPIRE-00245978$$uKaratay U. 002274147 700__ $$aKaravichev, Oleg$$iINSPIRE-00262581$$uMoscow, INR 002274147 700__ $$aKaravicheva, Tatiana$$iINSPIRE-00262593$$uMoscow, INR 002274147 700__ $$aKarayan, Lilit$$iINSPIRE-00522297$$uHeidelberg U.$$uDarmstadt, EMMI 002274147 700__ $$aKarczmarczyk, Przemyslaw$$iINSPIRE-00577574$$uCERN 002274147 700__ $$aKarpechev, Evgeny$$iINSPIRE-00248813$$uMoscow, INR 002274147 700__ $$aKebschull, Udo Wolfgang$$iINSPIRE-00248807$$uGoethe U., Frankfurt, Inst. Inform. 002274147 700__ $$aKeidel, Ralf$$iINSPIRE-00248795$$uFachhochsch., Worms 002274147 700__ $$aKeijdener, Darius Laurens$$iINSPIRE-00416339$$uUtrecht U. 002274147 700__ $$aKeil, Markus$$iINSPIRE-00216636$$uCERN 002274147 700__ $$aKetzer, Bernhard Franz$$iINSPIRE-00095813$$uBonn U., HISKP 002274147 700__ $$aKhabanova, Zhanna$$iINSPIRE-00539181$$uNIKHEF, Amsterdam 002274147 700__ $$aKhan, Palash$$iINSPIRE-00289764$$uSaha Inst. 002274147 700__ $$aKhan, Shuaib Ahmad$$iINSPIRE-00243963$$uCalcutta, VECC 002274147 700__ $$aKhanzadeev, Alexei$$iINSPIRE-00242036$$uSt. Petersburg, INP 002274147 700__ $$aKharlov, Yury$$iINSPIRE-00095925$$uSerpukhov, IHEP 002274147 700__ $$aKhatun, Anisa$$iINSPIRE-00564120$$uAligarh Muslim U. 002274147 700__ $$aKhuntia, Arvind$$iINSPIRE-00564138$$jORCID:0000-0003-0996-8547$$uIndian Inst. Tech., Indore 002274147 700__ $$aKielbowicz, Miroslaw Marek$$iINSPIRE-00564106$$uCracow, INP 002274147 700__ $$aKileng, Bjarte$$iINSPIRE-00262606$$uBergen Coll. 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Kernphys. 002274147 700__ $$aKlein, Jochen$$iINSPIRE-00262064$$uCERN 002274147 700__ $$aKlein-boesing, Christian$$iINSPIRE-00003561$$jORCID:0000-0002-7285-3411$$uMunster U. 002274147 700__ $$aKlewin, Sebastian$$iINSPIRE-00537149$$uHeidelberg U. 002274147 700__ $$aKluge, Alexander$$iINSPIRE-00250353$$uCERN 002274147 700__ $$aKnichel, Michael Linus$$iINSPIRE-00245547$$uHeidelberg U. 002274147 700__ $$aKnospe, Anders Garritt$$iINSPIRE-00182064$$uHouston U. 002274147 700__ $$aKobdaj, Chinorat$$iINSPIRE-00227795$$uSuranaree U. of Tech. 002274147 700__ $$aKofarago, Monika$$iINSPIRE-00410392$$uWigner RCP, Budapest 002274147 700__ $$aKollegger, Thorsten$$iINSPIRE-00182076$$uDarmstadt, EMMI 002274147 700__ $$aKolozhvari, Anatoly$$iINSPIRE-00244610$$uSt. Petersburg State U. 002274147 700__ $$aKondratev, Valerii$$iINSPIRE-00248784$$uSt. Petersburg State U. 002274147 700__ $$aKondratyeva, Natalia$$iINSPIRE-00262112$$uMoscow Phys. Eng. 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Tech., Mumbai 002274147 700__ $$aKralik, Ivan$$iINSPIRE-00098249$$uKosice, IEF 002274147 700__ $$aKravcakova, Adela$$iINSPIRE-00248740$$uKosice U. 002274147 700__ $$aKrivda, Marian$$iINSPIRE-00248727$$uKosice, IEF$$uBirmingham U. 002274147 700__ $$aKrizek, Filip$$iINSPIRE-00262142$$uRez, Nucl. Phys. Inst. 002274147 700__ $$aKryshen, Evgeny$$iINSPIRE-00262643$$uSt. Petersburg, INP 002274147 700__ $$aKrzewicki, Mikolaj$$iINSPIRE-00248715$$uFrankfurt U., FIAS 002274147 700__ $$aKubera, Andrew Michael$$iINSPIRE-00507630$$jORCID:0000-0002-1851-2739$$uOhio State U. 002274147 700__ $$aKucera, Vit$$iINSPIRE-00383170$$uRez, Nucl. Phys. Inst. 002274147 700__ $$aKuhn, Christian Claude$$iINSPIRE-00244002$$uStrasbourg, IPHC 002274147 700__ $$aKuijer, Paulus Gerardus$$iINSPIRE-00098956$$jORCID:0000-0002-6987-2048$$uNIKHEF, Amsterdam 002274147 700__ $$aKumar, Ajay$$iINSPIRE-00522302$$uJammu U. 002274147 700__ $$aKumar, Jitendra$$iINSPIRE-00361265$$uIndian Inst. 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Kernphys. 002274147 700__ $$aLunardon, Marcello$$iINSPIRE-00289820$$jORCID:0000-0002-6027-0024$$uPadua U.$$uINFN, Padua 002274147 700__ $$aLuparello, Grazia$$iINSPIRE-00248554$$jORCID:0000-0002-9901-2014$$uINFN, Trieste$$uTrieste U. 002274147 700__ $$aLupi, Matteo$$iINSPIRE-00564238$$jORCID:0000-0001-9770-6197$$uCERN 002274147 700__ $$aLutz, Tyler Harrison$$iINSPIRE-00548403$$uYale U. 002274147 700__ $$aMaevskaya, Alla$$iINSPIRE-00248542$$uMoscow, INR 002274147 700__ $$aMager, Magnus$$iINSPIRE-00248536$$uCERN 002274147 700__ $$aMahajan, Sanjay$$iINSPIRE-00244673$$uJammu U. 002274147 700__ $$aMahmood, Sohail Musa$$iINSPIRE-00416518$$uOslo U. 002274147 700__ $$aMaire, Antonin$$iINSPIRE-00248522$$jORCID:0000-0002-4831-2367$$uStrasbourg, IPHC 002274147 700__ $$aMajka, Richard Daniel$$iINSPIRE-00182435$$uYale U. 002274147 700__ $$aMalaev, Mikhail$$iINSPIRE-00247010$$uSt. Petersburg, INP 002274147 700__ $$aMalinina, Liudmila$$iINSPIRE-00361332$$uDubna, JINR 002274147 700__ $$aMal'kevich, Dmitry$$iINSPIRE-00289856$$uMoscow, ITEP 002274147 700__ $$aMalzacher, Peter$$iINSPIRE-00248471$$uDarmstadt, EMMI 002274147 700__ $$aMamonov, Alexander$$iINSPIRE-00247009$$uRFNC-VNIIEF, Sarov 002274147 700__ $$aManko, Vladislav$$iINSPIRE-00242429$$uKurchatov Inst., Moscow 002274147 700__ $$aManso, Franck$$iINSPIRE-00250406$$uClermont-Ferrand U. 002274147 700__ $$aManzari, Vito$$iINSPIRE-00104539$$jORCID:0000-0002-3102-1504$$uINFN, Bari 002274147 700__ $$aMao, Yaxian$$iINSPIRE-00261802$$uHua-Zhong Normal U. 002274147 700__ $$aMarchisone, Massimiliano$$iINSPIRE-00245991$$uiThemba LABS$$uWitwatersrand U. 002274147 700__ $$aMares, Jiri$$iINSPIRE-00289864$$uPrague, Inst. 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Inst. 002274147 700__ $$aMenchaca-rocha, Arturo Alejandro$$iINSPIRE-00244703$$uMexico U. 002274147 700__ $$aMeninno, Elisa$$iINSPIRE-00507326$$jORCID:0000-0003-4389-7711$$uSalerno U.$$uINFN, Salerno 002274147 700__ $$aMercado-perez, Jorge$$iINSPIRE-00289899$$uHeidelberg U. 002274147 700__ $$aMeres, Michal$$iINSPIRE-00245096$$uComenius U. 002274147 700__ $$aMhlanga, Sibaliso$$iINSPIRE-00564240$$uCape Town U. 002274147 700__ $$aMiake, Yasuo$$iINSPIRE-00242486$$uTsukuba U. 002274147 700__ $$aMieskolainen, Matti Mikael$$iINSPIRE-00507452$$uHelsinki Inst. of Phys. 002274147 700__ $$aMihaylov, Dimitar$$iINSPIRE-00580281$$uTech. U., Munich (main) 002274147 700__ $$aMihaylov, Dimitar Lubomirov$$uTech. U., Munich (main) 002274147 700__ $$aMikhaylov, Konstantin$$iINSPIRE-00245462$$uMoscow, ITEP$$uDubna, JINR 002274147 700__ $$aMilano, Leonardo$$iINSPIRE-00254899$$uLBL, Berkeley 002274147 700__ $$aMilosevic, Jovan$$iINSPIRE-00191774$$jORCID:0000-0001-8486-4604$$uOslo U. 002274147 700__ $$aMischke, Andre$$iINSPIRE-00182548$$jORCID:0000-0003-0078-4522$$uUtrecht U. 002274147 700__ $$aMishra, Aditya Nath$$iINSPIRE-00361381$$uIndian Inst. Tech., Indore 002274147 700__ $$aMiskowiec, Dariusz Czeslaw$$iINSPIRE-00108019$$uDarmstadt, EMMI 002274147 700__ $$aMitra, Jubin$$iINSPIRE-00416586$$uCalcutta, VECC 002274147 700__ $$aMitu, Ciprian Mihai$$iINSPIRE-00248369$$uBucharest, Inst. 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U. 002274147 700__ $$aMuhlheim, Daniel Michael$$iINSPIRE-00416728$$uMunster U. 002274147 700__ $$aMuhuri, Sanjib$$iINSPIRE-00248321$$uCalcutta, VECC 002274147 700__ $$aMukherjee, Maitreyee$$iINSPIRE-00361435$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002274147 700__ $$aMulligan, James Declan$$iINSPIRE-00507724$$uYale U. 002274147 700__ $$aGameiro Munhoz, Marcelo$$iINSPIRE-00182574$$uSao Paulo U. 002274147 700__ $$aMunning, Konstantin$$iINSPIRE-00564280$$uBonn U., HISKP 002274147 700__ $$aMunzer, Robert Helmut$$iINSPIRE-00531366$$uFrankfurt U., Inst. 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Tech., Mumbai 002274147 700__ $$aNaru, Muhammad Umair$$iINSPIRE-00507883$$uCOMSATS, Islamabad 002274147 700__ $$aFerreira Natal Da Luz, Pedro Hugo$$iINSPIRE-00511516$$uSao Paulo U. 002274147 700__ $$aNattrass, Christine$$iINSPIRE-00301613$$jORCID:0000-0002-8768-6468$$uTennessee U. 002274147 700__ $$aRosado Navarro, Sebastian$$iINSPIRE-00548422$$uPuebla U., Mexico 002274147 700__ $$aNayak, Kishora$$iINSPIRE-00416777$$uNISER, Jatni 002274147 700__ $$aNayak, Ranjit$$iINSPIRE-00548439$$jORCID:0000-0001-6988-0606$$uIndian Inst. Tech., Mumbai 002274147 700__ $$aNayak, Tapan Kumar$$iINSPIRE-00182590$$uCalcutta, VECC 002274147 700__ $$aNazarenko, Sergey$$iINSPIRE-00289965$$uRFNC-VNIIEF, Sarov 002274147 700__ $$aNedosekin, Alexander$$iINSPIRE-00060091$$uMoscow, ITEP 002274147 700__ $$aNegrao De Oliveira, Renato Aparecido$$iINSPIRE-00564311$$uCERN 002274147 700__ $$aNellen, Lukas$$iINSPIRE-00110793$$jORCID:0000-0003-1059-8731$$uMexico U., ICN 002274147 700__ $$aNesbo, Simon Voigt$$iINSPIRE-00564307$$uBergen Coll. Higher Educ. 002274147 700__ $$aNg, Fabian$$iINSPIRE-00507999$$uHouston U. 002274147 700__ $$aNicassio, Maria$$iINSPIRE-00246928$$uDarmstadt, EMMI 002274147 700__ $$aNiculescu, Mihai$$iINSPIRE-00361459$$uBucharest, Inst. 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Tech., Mumbai 002274147 700__ $$aPanebianco, Stefano$$iINSPIRE-00521498$$uIRFU, Saclay 002274147 700__ $$aPapikyan, Vardanush$$iINSPIRE-00246268$$uYerevan Phys. Inst. 002274147 700__ $$aPappalardo, Giuseppe$$iINSPIRE-00178786$$jORCID:0000-0002-5038-2962$$uINFN, Catania 002274147 700__ $$aPareek, Pooja$$iINSPIRE-00383898$$uIndian Inst. 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Inst.$$uKurchatov Inst., Moscow 002274147 700__ $$aPerez Lezama, Edgar$$iINSPIRE-00433111$$uFrankfurt U., Inst. Kernphys. 002274147 700__ $$aPeskov, Vladimir$$iINSPIRE-00115907$$uFrankfurt U., Inst. Kernphys. 002274147 700__ $$aPestov, Yury$$iINSPIRE-00248095$$uNovosibirsk, IYF 002274147 700__ $$aPetracek, Vojtech$$iINSPIRE-00250478$$uPrague, Tech. U. 002274147 700__ $$aPetrov, Viacheslav$$iINSPIRE-00508460$$uSerpukhov, IHEP 002274147 700__ $$aPetrovici, Mihai$$iINSPIRE-00290111$$uBucharest, IFIN-HH 002274147 700__ $$aPetta, Catia$$iINSPIRE-00250481$$jORCID:0000-0002-2055-4196$$uCatania U.$$uINFN, Catania 002274147 700__ $$aPeretti Pezzi, Rafael$$iINSPIRE-00564375$$uRio Grande do Sul U. 002274147 700__ $$aPiano, Stefano$$iINSPIRE-00249971$$jORCID:0000-0003-4903-9865$$uINFN, Trieste 002274147 700__ $$aPikna, Miroslav$$iINSPIRE-00116456$$uComenius U. 002274147 700__ $$aPillot, Philippe$$iINSPIRE-00290120$$uSUBATECH, Nantes 002274147 700__ $$aOzelin De Lima Pimentel, Lais$$iINSPIRE-00548449$$uBohr Inst. 002274147 700__ $$aPinazza, Ombretta$$iINSPIRE-00290138$$jORCID:0000-0001-8923-4003$$uINFN, Bologna$$uCERN 002274147 700__ $$aPinsky, Lawrence$$iINSPIRE-00116547$$uHouston U. 002274147 700__ $$aPiyarathna, Danthasinghe$$iINSPIRE-00246340$$uHouston U. 002274147 700__ $$aPloskon, Mateusz Andrzej$$iINSPIRE-00248071$$uLBL, Berkeley 002274147 700__ $$aPlaninic, Mirko$$iINSPIRE-00182770$$uZagreb U. 002274147 700__ $$aPliquett, Fabian$$iINSPIRE-00584629$$uFrankfurt U., Inst. Kernphys. 002274147 700__ $$aPluta, Jan Marian$$iINSPIRE-00182781$$uWarsaw U. of Tech. 002274147 700__ $$aPochybova, Sona$$iINSPIRE-00248060$$uWigner RCP, Budapest 002274147 700__ $$aPodesta Lerma, Pedro Luis Manuel$$iINSPIRE-00049100$$uSinaloa U. 002274147 700__ $$aPoghosyan, Martin$$iINSPIRE-00249924$$uOak Ridge 002274147 700__ $$aPolishchuk, Boris$$iINSPIRE-00248058$$uSerpukhov, IHEP 002274147 700__ $$aPoljak, Nikola$$iINSPIRE-00182793$$uZagreb U. 002274147 700__ $$aPoonsawat, Wanchaloem$$iINSPIRE-00508526$$uSuranaree U. of Tech. 002274147 700__ $$aPop, Amalia$$iINSPIRE-00290166$$uBucharest, IFIN-HH 002274147 700__ $$aPoppenborg, Hendrik$$iINSPIRE-00564335$$uMunster U. 002274147 700__ $$aPorteboeuf, Sarah Julie$$iINSPIRE-00207321$$uClermont-Ferrand U. 002274147 700__ $$aPorter, R Jefferson$$iINSPIRE-00254707$$jORCID:0000-0002-6265-8794$$uLBL, Berkeley 002274147 700__ $$aPozdniakov, Valeriy$$iINSPIRE-00237200$$uDubna, JINR 002274147 700__ $$aPrasad, Sidharth Kumar$$iINSPIRE-00244190$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002274147 700__ $$aPreghenella, Roberto$$iINSPIRE-00246857$$jORCID:0000-0002-1539-9275$$uINFN, Bologna 002274147 700__ $$aPrino, Francesco$$iINSPIRE-00270661$$uINFN, Turin 002274147 700__ $$aPruneau, Claude Andre$$iINSPIRE-00182834$$uWayne State U. 002274147 700__ $$aPshenichnov, Igor$$iINSPIRE-00117975$$jORCID:0000-0003-1752-4524$$uMoscow, INR 002274147 700__ $$aPuccio, Maximiliano$$iINSPIRE-00508690$$uTurin U.$$uINFN, Turin 002274147 700__ $$aPuddu, Giovanna$$iINSPIRE-00250538$$jORCID:0000-0001-6391-8976$$uCagliari U.$$uINFN, Cagliari 002274147 700__ $$aPujahari, Prabhat Ranjan$$iINSPIRE-00182850$$uWayne State U. 002274147 700__ $$aPunin, Valery$$iINSPIRE-00248029$$uRFNC-VNIIEF, Sarov 002274147 700__ $$aPutschke, Jorn Henning$$iINSPIRE-00001210$$uWayne State U. 002274147 700__ $$aRachevski, Alexandre$$iINSPIRE-00250549$$jORCID:0000-0002-2723-6297$$uINFN, Trieste 002274147 700__ $$aRaha, Sibaji$$iINSPIRE-00360571$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002274147 700__ $$aRajput, Sonia$$iINSPIRE-00508791$$uJammu U. 002274147 700__ $$aRak, Jan$$iINSPIRE-00242842$$uJyvaskyla U. 002274147 700__ $$aRakotozafindrabe, Andry Malala$$iINSPIRE-00030930$$uIRFU, Saclay 002274147 700__ $$aRamello, Luciano$$iINSPIRE-00118788$$jORCID:0000-0003-2325-8680$$uPiemonte Orientale U., Alessandria 002274147 700__ $$aRami, Fouad$$iINSPIRE-00531399$$uStrasbourg, IPHC 002274147 700__ $$aRana, Dhan Bahadur$$iINSPIRE-00564631$$uHouston U. 002274147 700__ $$aRaniwala, Rashmi$$iINSPIRE-00182881$$uRajasthan U. 002274147 700__ $$aRaniwala, Sudhir$$iINSPIRE-00182870$$uRajasthan U. 002274147 700__ $$aRasanen, Sami Sakari$$iINSPIRE-00290180$$uHelsinki Inst. of Phys. 002274147 700__ $$aRascanu, Bogdan Theodor$$iINSPIRE-00361496$$uFrankfurt U., Inst. 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Tech., Indore 002274147 700__ $$aRoy, Christelle Sophie$$iINSPIRE-00182943$$uStrasbourg, IPHC 002274147 700__ $$aRoy, Pradip Kumar$$iINSPIRE-00290300$$uSaha Inst. 002274147 700__ $$aRubio Montero, Antonio Juan$$iINSPIRE-00290319$$uMadrid, CIEMAT 002274147 700__ $$aVazquez Rueda, Omar$$iINSPIRE-00570190$$uMexico U., ICN 002274147 700__ $$aRui, Rinaldo$$iINSPIRE-00121777$$jORCID:0000-0002-6993-0332$$uTrieste U.$$uINFN, Trieste 002274147 700__ $$aRumyantsev, Boris$$iINSPIRE-00578882$$uDubna, JINR 002274147 700__ $$aRustamov, Anar$$iINSPIRE-00227304$$uNNRC, Baku 002274147 700__ $$aRyabinkin, Evgeny$$iINSPIRE-00246815$$uKurchatov Inst., Moscow 002274147 700__ $$aRyabov, Yury$$iINSPIRE-00306193$$uSt. Petersburg, INP 002274147 700__ $$aRybicki, Andrzej$$iINSPIRE-00250603$$uCracow, INP 002274147 700__ $$aSaarinen, Sampo$$iINSPIRE-00560357$$uHelsinki Inst. of Phys. 002274147 700__ $$aSadhu, Samrangy$$iINSPIRE-00560369$$uCalcutta, VECC 002274147 700__ $$aSadovskiy, Sergey$$iINSPIRE-00247897$$uSerpukhov, IHEP 002274147 700__ $$aSafarik, Karel$$iINSPIRE-00290327$$uCERN 002274147 700__ $$aSaha, Sumit Kumar$$iINSPIRE-00568429$$uCalcutta, VECC 002274147 700__ $$aSahlmuller, Baldo$$iINSPIRE-00242967$$uFrankfurt U., Inst. Kernphys. 002274147 700__ $$aSahoo, Baidyanath$$iINSPIRE-00564677$$uIndian Inst. Tech., Mumbai 002274147 700__ $$aSahoo, Pragati$$iINSPIRE-00384329$$uIndian Inst. Tech., Indore 002274147 700__ $$aSahoo, Raghunath$$iINSPIRE-00182966$$uIndian Inst. Tech., Indore 002274147 700__ $$aSahoo, Sarita$$iINSPIRE-00508953$$uBhubaneswar, Inst. Phys. 002274147 700__ $$aSahu, Pradip Kumar$$iINSPIRE-00122421$$uBhubaneswar, Inst. Phys. 002274147 700__ $$aSaini, Jogender$$iINSPIRE-00246803$$uCalcutta, VECC 002274147 700__ $$aSakai, Shingo$$iINSPIRE-00182972$$uTsukuba U.$$uFrascati 002274147 700__ $$aSaleh, Mohammad Ahmad$$iINSPIRE-00509062$$uWayne State U. 002274147 700__ $$aSalzwedel, Jai Samuel Nielsen$$iINSPIRE-00361540$$jORCID:0000-0003-4032-9612$$uOhio State U. 002274147 700__ $$aSambyal, Sanjeev Singh$$iINSPIRE-00247865$$uJammu U. 002274147 700__ $$aSamsonov, Vladimir$$iINSPIRE-00242999$$uSt. Petersburg, INP$$uMoscow Phys. Eng. Inst. 002274147 700__ $$aSandoval, Andres$$iINSPIRE-00123048$$uMexico U. 002274147 700__ $$aSarkar, Debojit$$iINSPIRE-00384381$$uCalcutta, VECC 002274147 700__ $$aSarkar, Nachiketa$$iINSPIRE-00560376$$uCalcutta, VECC 002274147 700__ $$aSarma, Pranjal$$iINSPIRE-00548452$$uGauhati U. 002274147 700__ $$aSas, Mike Henry Petrus$$iINSPIRE-00572407$$uUtrecht U. 002274147 700__ $$aScapparone, Eugenio$$iINSPIRE-00250631$$jORCID:0000-0001-5960-6734$$uINFN, Bologna 002274147 700__ $$aScarlassara, Fernando$$iINSPIRE-00249930$$jORCID:0000-0002-4663-8216$$uPadua U.$$uINFN, Padua 002274147 700__ $$aScharenberg, Rolf Paul$$iINSPIRE-00183017$$uPurdue U. 002274147 700__ $$aScheid, Horst Sebastian$$iINSPIRE-00580969$$uFrankfurt U., Inst. Kernphys. 002274147 700__ $$aSchiaua, Claudiu Cornel$$iINSPIRE-00247838$$uBucharest, IFIN-HH 002274147 700__ $$aSchicker, Rainer Martin$$iINSPIRE-00244227$$uHeidelberg U. 002274147 700__ $$aSchmidt, Christian Joachim$$iINSPIRE-00244248$$uDarmstadt, EMMI 002274147 700__ $$aSchmidt, Hans Rudolf$$iINSPIRE-00290373$$uTubingen U. 002274147 700__ $$aSchmidt, Marten Ole$$iINSPIRE-00571169$$uHeidelberg U. 002274147 700__ $$aSchmidt, Martin$$iINSPIRE-00560380$$uTubingen U. 002274147 700__ $$aSchmidt, Nicolas Vincent$$iINSPIRE-00640513$$uFrankfurt U., Inst. 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Studies 002274147 700__ $$aWilkinson, Jeremy John$$iINSPIRE-00385005$$uHeidelberg U.$$uINFN, Bologna 002274147 700__ $$aWillems, Guido Alexander$$iINSPIRE-00564789$$uMunster U. 002274147 700__ $$aWilliams, Crispin$$iINSPIRE-00254855$$jORCID:0000-0003-3589-0181$$uINFN, Bologna 002274147 700__ $$aWillsher, Emily$$iINSPIRE-00574082$$uBirmingham U. 002274147 700__ $$aWindelband, Bernd Stefan$$iINSPIRE-00246650$$uHeidelberg U. 002274147 700__ $$aWitt, William Edward$$iINSPIRE-00564770$$uTennessee U. 002274147 700__ $$aYalcin, Serpil$$iINSPIRE-00412449$$uKaratay U. 002274147 700__ $$aYamakawa, Kosei$$iINSPIRE-00639310$$uHiroshima U. 002274147 700__ $$aYang, Ping$$iINSPIRE-00385084$$uHua-Zhong Normal U. 002274147 700__ $$aYano, Satoshi$$iINSPIRE-00385135$$uHiroshima U. 002274147 700__ $$aYin, Zhongbao$$iINSPIRE-00245030$$uHua-Zhong Normal U. 002274147 700__ $$aYokoyama, Hiroki$$iINSPIRE-00245044$$uTsukuba U.$$uLPSC, Grenoble 002274147 700__ $$aYoo, In-kwon$$iINSPIRE-00183678$$uCERN$$uPusan Natl. U. 002274147 700__ $$aYoon, Jin Hee$$iINSPIRE-00537195$$uInha U. 002274147 700__ $$aYurchenko, Volodymyr$$iINSPIRE-00510512$$uBITP, Kiev 002274147 700__ $$aZaccolo, Valentina$$iINSPIRE-00361691$$uINFN, Turin$$uBohr Inst. 002274147 700__ $$aZaman, Ali$$iINSPIRE-00385199$$uCOMSATS, Islamabad 002274147 700__ $$aZampolli, Chiara$$iINSPIRE-00247387$$jORCID:0000-0002-2608-4834$$uCERN 002274147 700__ $$aCorrea Zanoli, Henrique Jose$$iINSPIRE-00510636$$uSao Paulo U. 002274147 700__ $$aZardoshti, Nima$$iINSPIRE-00522360$$uBirmingham U. 002274147 700__ $$aZarochentsev, Andrey$$iINSPIRE-00246638$$uSt. Petersburg State U. 002274147 700__ $$aZavada, Petr$$iINSPIRE-00138107$$uPrague, Inst. Phys. 002274147 700__ $$aZavyalov, Nikolay$$iINSPIRE-00290800$$uRFNC-VNIIEF, Sarov 002274147 700__ $$aZbroszczyk, Hanna Paulina$$iINSPIRE-00183708$$uWarsaw U. of Tech. 002274147 700__ $$aZhalov, Mikhail$$iINSPIRE-00254612$$uSt. Petersburg, INP 002274147 700__ $$aZhang, Haitao$$iINSPIRE-00361703$$uBergen U.$$uHua-Zhong Normal U. 002274147 700__ $$aZhang, Xiaoming$$iINSPIRE-00290818$$uHua-Zhong Normal U. 002274147 700__ $$aZhang, Yonghong$$iINSPIRE-00385253$$uHua-Zhong Normal U. 002274147 700__ $$aChunhui, Zhang$$iINSPIRE-00522436$$uUtrecht U. 002274147 700__ $$aZhang, Zuman$$iINSPIRE-00531444$$uHua-Zhong Normal U.$$uClermont-Ferrand U. 002274147 700__ $$aZhao, Chengxin$$iINSPIRE-00385310$$uOslo U. 002274147 700__ $$aZhigareva, Natalia$$iINSPIRE-00385354$$uMoscow, ITEP 002274147 700__ $$aZhou, Daicui$$iINSPIRE-00290834$$uHua-Zhong Normal U. 002274147 700__ $$aZhou, You$$iINSPIRE-00290856$$jORCID:0000-0002-7868-6706$$uBohr Inst. 002274147 700__ $$aZhou, Zhuo$$iINSPIRE-00417116$$uBergen U. 002274147 700__ $$aZhu, Hongsheng$$iINSPIRE-00361728$$uBergen U. 002274147 700__ $$aZhu, Jianhui$$iINSPIRE-00361715$$uHua-Zhong Normal U. 002274147 700__ $$aZhu, Xiangrong$$iINSPIRE-00290864$$uHua-Zhong Normal U. 002274147 700__ $$aZichichi, Antonino$$iINSPIRE-00172134$$uEnrico Fermi Ctr., Rome$$uBologna U.$$uINFN, Bologna 002274147 700__ $$aZimmermann, Alice$$iINSPIRE-00361741$$uHeidelberg U. 002274147 700__ $$aZimmermann, Markus Bernhard$$iINSPIRE-00385420$$uCERN$$uMunster U. 002274147 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev 002274147 700__ $$aZmeskal, Johann$$iINSPIRE-00564793$$uStefan Meyer Inst. Subatomare Phys. 002274147 700__ $$aZou, Shuguang$$iINSPIRE-00571982$$uHua-Zhong Normal U. 002274147 710__ $$5PH 002274147 710__ $$gALICE 002274147 773__ $$c658$$n10$$pEur. Phys. J. C$$v77$$y2017 002274147 859__ $$fcloizides@lbl.gov 002274147 8564_ $$81328432$$s853719$$uhttp://cds.cern.ch/record/2274147/files/CERN-EP-DRAFT-ALICE-2017-015 - draft.pdf$$yDraft (restricted)$$zStamped by WebSubmit: 13/07/2017 002274147 8564_ $$81332874$$s35454$$uhttp://cds.cern.ch/record/2274147/files/v2differenceCentrality.png$$y00006 Measured \vtwo\ as a function of \pt\ for \dbar\ (\pt~$<$~1.4~\gmom) and d+\dbar\ (\pt~$\geq$~1.4~\gmom) for different centrality intervals in \mbox{\PbPb} collisions at \s~=~2.76~TeV. Vertical bars represent statistical errors, while boxes are systematic uncertainties. 002274147 8564_ $$81332875$$s51430$$uhttp://cds.cern.ch/record/2274147/files/CompareOtherParticles2040.png$$y00007 \vtwo\ of $\pi^{\pm}$ (empty circles), p+$\overline{\rm p}$ (filled squares) and d+\dbar\ (filled circles) measured in the 20--40\% centrality interval. A detailed description of each panel can be found in the text. 002274147 8564_ $$81332876$$s47325$$uhttp://cds.cern.ch/record/2274147/files/AMPTflow.png$$y00013 Measured deuteron (filled dots) $B_2$ as a function of the transverse momentum per nucleon (\pt/A) (top left panel) and \vtwo(\pt) parameter (top right panel) compared to those produced with two versions of the AMPT model (dashed and dotted lines). In the bottom panels, the ratios between the measured data and the expectations from the two models are shown. 002274147 8564_ $$81332877$$s25737$$uhttp://cds.cern.ch/record/2274147/files/Efficiency.png$$y00002 Acceptance $\times$ efficiency (A $\times \epsilon$) as a function of transverse momentum for deuterons (filled markers) and anti--deuterons (open markers) in the most 10\% central \PbPb\ collisions at \s\ ~=~2.76 TeV for TPC-TOF and HMPID (multiplied by a scaling factor) analyses. The TPC-TOF points account for tracking, matching efficiency and geometrical acceptance. The dashed and solid curves represent the fits with the function presented in equation~\ref{eq:lineTOF} for deuterons and anti--deuterons respectively (see text for details). The HMPID points take into account tracking efficiency, geometrical acceptance, $\epsilon_\mathrm{{dist}}$ (`` distance correction factor" as explained in the text) and PID efficiency. The lower value with respect to the TPC-TOF is mainly due to the limited geometrical acceptance of the HMPID detector (5\%). 002274147 8564_ $$81332878$$s40984$$uhttp://cds.cern.ch/record/2274147/files/MassTOF.png$$y00004 Left: Distribution of $\Delta \rm{M}$ for d+\dbar\ in the $2.2~\leq$~\pt~$<2.4$~\gmom\ and centrality interval 30-40\% fitted with a Gaussian with an exponential used to reproduce the signal and an exponential to reproduce the background. Right: The \vtwo$^{\rm{Tot}}$ vs $\Delta \rm{M}$ for d+\dbar\ for 2.2~$\leq$~\pt~$<$~2.4~\gmom\ in events with 30-40\% centrality. Points represent the measured $v_2^{\mathrm{Tot}}$, while the curve is the fit performed using equation~\ref{eq:v2tot}. 002274147 8564_ $$81332879$$s15496$$uhttp://cds.cern.ch/record/2274147/files/V2vsMass.png$$y00005 Left: Distribution of $\Delta \rm{M}$ for d+\dbar\ in the $2.2~\leq$~\pt~$<2.4$~\gmom\ and centrality interval 30-40\% fitted with a Gaussian with an exponential used to reproduce the signal and an exponential to reproduce the background. Right: The \vtwo$^{\rm{Tot}}$ vs $\Delta \rm{M}$ for d+\dbar\ for 2.2~$\leq$~\pt~$<$~2.4~\gmom\ in events with 30-40\% centrality. Points represent the measured $v_2^{\mathrm{Tot}}$, while the curve is the fit performed using equation~\ref{eq:v2tot}. 002274147 8564_ $$81332880$$s43874$$uhttp://cds.cern.ch/record/2274147/files/AMPTB2.png$$y00012 Measured deuteron (filled dots) $B_2$ as a function of the transverse momentum per nucleon (\pt/A) (top left panel) and \vtwo(\pt) parameter (top right panel) compared to those produced with two versions of the AMPT model (dashed and dotted lines). In the bottom panels, the ratios between the measured data and the expectations from the two models are shown. 002274147 8564_ $$81332881$$s37597$$uhttp://cds.cern.ch/record/2274147/files/TOF_fit.png$$y00000 The $m^2-m_{\mathrm{PDG}}^2$ distributions obtained using the TOF detector (left) and with the HMPID detector (right) in two different \pt\ intervals ($4.4\leq\pt<5$ \gmom\ and $5\leq\pt<6$ \gmom) for positive tracks in the \mbox{0--10\%} centrality class. Here $m_{\mathrm{PDG}}$ is the nominal mass of deuteron as reported in~\cite{Olive:2016xmw}. Solid lines represent the total fit (signal plus background), dotted lines correspond to background and dashed lines to deuterons signal. 002274147 8564_ $$81332882$$s58072$$uhttp://cds.cern.ch/record/2274147/files/CombinedBWSpectra.png$$y00008 Combined Blast-Wave fit to \pt\ and \vtwo(\pt) distributions using equations \ref{eq:spectrum} and \ref{eq:v2}. The six upper panels show the \pt\ spectra and the ratio between data and fit, while the six panels in the bottom part shows the \vtwo(\pt) and the ratio between data and fit. In each panel, $\pi^\pm$ (empty circles), K$^\pm$ (diamonds), p+$\overline{\rm p}$ (filled squares) and d+\dbar\ (filled circles) are shown. For $\pi^\pm$, K$^\pm$ and p+$\overline{\rm p}$ the long dashed curves represent the combined \pt\ and \vtwo\ Blast-Wave fit. Deuteron curves (dash dotted lines) are predictions from lighter particles Blast-Wave combined fit. Each column shows a different centrality intervals (0-10\% left, 10-20\% middle and 20-40\% right). 002274147 8564_ $$81332883$$s6697$$uhttp://cds.cern.ch/record/2274147/files/B2vsPt.png$$y00010 Left: Coalescence parameter $B_2$ as a function of the transverse momentum per nucleon (\pt/A) for different centrality classes. Right: Measured \vtwo\ of d+\dbar\ compared with the expectations from simple coalescence (equation~\ref{eq:v2coal}) for different centrality intervals as indicated in the legend. 002274147 8564_ $$81332884$$s55208$$uhttp://cds.cern.ch/record/2274147/files/spectraratio.png$$y00003 In the upper panel the deuteron \pt\ spectra are shown for the three centrality intervals extended to high \pt\ with the TOF and HMPID analyses. In the lower panels the ratios of anti-deuterons and deuterons are shown for the 0--10\%, 10--20\% and 20--40\% centrality intervals, from top to bottom. The ratios are consistent with unity over the whole \pt\ range covered by the presented analyses. 002274147 8564_ $$81332885$$s34522$$uhttp://cds.cern.ch/record/2274147/files/deuteroncoalescence.png$$y00011 Left: Coalescence parameter $B_2$ as a function of the transverse momentum per nucleon (\pt/A) for different centrality classes. Right: Measured \vtwo\ of d+\dbar\ compared with the expectations from simple coalescence (equation~\ref{eq:v2coal}) for different centrality intervals as indicated in the legend. 002274147 8564_ $$81332886$$s57902$$uhttp://cds.cern.ch/record/2274147/files/CombinedBWFlow.png$$y00009 Combined Blast-Wave fit to \pt\ and \vtwo(\pt) distributions using equations \ref{eq:spectrum} and \ref{eq:v2}. The six upper panels show the \pt\ spectra and the ratio between data and fit, while the six panels in the bottom part shows the \vtwo(\pt) and the ratio between data and fit. In each panel, $\pi^\pm$ (empty circles), K$^\pm$ (diamonds), p+$\overline{\rm p}$ (filled squares) and d+\dbar\ (filled circles) are shown. For $\pi^\pm$, K$^\pm$ and p+$\overline{\rm p}$ the long dashed curves represent the combined \pt\ and \vtwo\ Blast-Wave fit. Deuteron curves (dash dotted lines) are predictions from lighter particles Blast-Wave combined fit. Each column shows a different centrality intervals (0-10\% left, 10-20\% middle and 20-40\% right). 002274147 8564_ $$81332887$$s33797$$uhttp://cds.cern.ch/record/2274147/files/HMPID_fit_2017_fb.png$$y00001 The $m^2-m_{\mathrm{PDG}}^2$ distributions obtained using the TOF detector (left) and with the HMPID detector (right) in two different \pt\ intervals ($4.4\leq\pt<5$ \gmom\ and $5\leq\pt<6$ \gmom) for positive tracks in the \mbox{0--10\%} centrality class. Here $m_{\mathrm{PDG}}$ is the nominal mass of deuteron as reported in~\cite{Olive:2016xmw}. Solid lines represent the total fit (signal plus background), dotted lines correspond to background and dashed lines to deuterons signal. 002274147 8564_ $$81334052$$s846552$$uhttp://cds.cern.ch/record/2274147/files/arXiv:1707.07304.pdf 002274147 8564_ $$81358992$$s1536076$$uhttp://cds.cern.ch/record/2274147/files/scoap3-fulltext.pdf?subformat=pdfa$$xpdfa$$yArticle from SCOAP3 002274147 8564_ $$82335839$$s1536076$$uhttp://cds.cern.ch/record/2274147/files/scoap.pdf$$yArticle from SCOAP3 002274147 9031_ $$aApproval requested for number CERN-EP-2017-176$$bCERN-EP-2017-176$$cEPPHAPP$$d2017-07-12 18:12:46$$e2017-07-19 18:12:46$$fcloizides@lbl.gov$$swaiting 002274147 9031_ $$aDocument approved$$bCERN-EP-2017-176$$cEPPHAPP$$d2017-07-13 09:33:53$$froger.forty@cern.ch$$sapproved 002274147 916__ $$sn$$w201728 002274147 980__ $$aALICE_Papers 002274147 980__ $$aARTICLE