002244366 001__ 2244366 002244366 005__ 20241127052605.0 002244366 0248_ $$aoai:cds.cern.ch:2244366$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT 002244366 0247_ $$2DOI$$9bibmatch$$a10.1103/PhysRevC.95.064606 002244366 037__ $$9arXiv$$aarXiv:1702.00555$$cnucl-ex 002244366 037__ $$aCERN-EP-2017-010 002244366 035__ $$9arXiv$$aoai:arXiv.org:1702.00555 002244366 035__ $$9Inspire$$aoai:inspirehep.net:1511864$$d2024-11-26T15:21:54Z$$h2024-11-27T03:03:39Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d 002244366 035__ $$9Inspire$$a1511864 002244366 041__ $$aeng 002244366 088__ $$9CERN-EP-DRAFT-ALICE-2017-001 002244366 100__ $$aAdam, Jaroslav$$iINSPIRE-00360890$$uPrague, Tech. U.$$vFaculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague , Prague, Czech Republic 002244366 245__ $$9arXiv$$aK$^{*}(892)^{0}$ and $\phi(1020)$ meson production at high transverse momentum in pp and Pb-Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV 002244366 269__ $$c2017-02-02 002244366 269__ $$aGeneva$$bCERN$$c18 Jan 2017 002244366 260__ $$c2017-06-12 002244366 300__ $$a18 p 002244366 506__ [email protected] 002244366 506__ $$malice-member [CERN] 002244366 506__ $$mcds-ph-ep-publications-referee [CERN] 002244366 500__ $$9arXiv$$a26 pages, 10 captioned figures, 3 tables, authors from page 21, published version, figures at http://aliceinfo.cern.ch/ArtSubmission/node/3363 002244366 520__ $$9APS$$aThe production of K*(892)0 and ϕ(1020) mesons in proton-proton (pp) and lead-lead (Pb-Pb) collisions at sNN=2.76TeV has been analyzed using a high luminosity data sample accumulated in 2011 with the ALICE detector at the Large Hadron Collider (LHC). Transverse momentum (pT) spectra have been measured for K*(892)0 and ϕ(1020) mesons via their hadronic decay channels for pT up to 20GeV/c. The measurements in pp collisions have been compared to model calculations and used to determine the nuclear modification factor and particle ratios. The K*(892)0/K ratio exhibits significant reduction from pp to central Pb-Pb collisions, consistent with the suppression of the K*(892)0 yield at low pT due to rescattering of its decay products in the hadronic phase. In central Pb-Pb collisions the pT dependent ϕ(1020)/π and K*(892)0/π ratios show an enhancement over pp collisions for pT≈3GeV/c, consistent with previous observations of strong radial flow. At high pT, particle ratios in Pb-Pb collisions are similar to those measured in pp collisions. In central Pb-Pb collisions, the production of K*(892)0 and ϕ(1020) mesons is suppressed for pT>8GeV/c. This suppression is similar to that of charged pions, kaons, and protons, indicating that the suppression does not depend on particle mass or flavor in the light quark sector. 002244366 520__ $$9arXiv$$aThe production of K$^{*}(892)^{0}$ and $\phi(1020)$ mesons in proton-proton (pp) and lead-lead (Pb-Pb) collisions at $\sqrt{s_\mathrm{NN}} =$ 2.76 TeV has been analyzed using a high luminosity data sample accumulated in 2011 with the ALICE detector at the Large Hadron Collider (LHC). Transverse momentum ($p_{\mathrm{T}}$) spectra have been measured for K$^{*}(892)^{0}$ and $\phi(1020)$ mesons via their hadronic decay channels for $p_{\mathrm{T}}$ up to 20 GeV/$c$. The measurements in pp collisions have been compared to model calculations and used to determine the nuclear modification factor and particle ratios. The K$^{*}(892)^{0}$/K ratio exhibits significant reduction from pp to central Pb-Pb collisions, consistent with the suppression of the K$^{*}(892)^{0}$ yield at low $p_{\mathrm{T}}$ due to rescattering of its decay products in the hadronic phase. In central Pb-Pb collisions the $p_{\mathrm{T}}$ dependent $\phi(1020)/\pi$ and K$^{*}(892)^{0}$/$\pi$ ratios show an enhancement over pp collisions for $p_{\mathrm{T}}$ $\sim$3 GeV/$c$, consistent with previous observations of strong radial flow. At high $p_{\mathrm{T}}$, particle ratios in Pb-Pb collisions are similar to those measured in pp collisions. In central Pb-Pb collisions, the production of K$^{*}(892)^{0}$ and $\phi(1020)$ mesons is suppressed for $p_{\mathrm{T}}> 8$ GeV/$c$. This suppression is similar to that of charged pions, kaons and protons, indicating that the suppression does not depend on particle mass or flavor in the light quark sector. 002244366 540__ $$3Preprint$$aCC-BY-4.0 002244366 542__ $$3Publication$$dCERN$$g2017 002244366 562__ $$cComments submitted after 18-01-2017 10:08 002244366 595__ $$aCERN EDS 002244366 595__ $$aCERN-EP 002244366 65017 $$2arXiv$$ahep-ex 002244366 65017 $$2SzGeCERN$$aParticle Physics - Experiment 002244366 65017 $$2arXiv$$anucl-ex 002244366 65017 $$2SzGeCERN$$aNuclear Physics - Experiment 002244366 6531_ $$9CERN$$aQCD 002244366 6531_ $$9CERN$$aquark gluon plasma 002244366 6531_ $$9CERN$$aparticle and resonance production 002244366 6531_ $$9CERN$$aexperimental results 002244366 693__ $$aCERN LHC$$eALICE 002244366 690C_ $$aCERN 002244366 690C_ $$aARTICLE 002244366 690C_ $$aALICE_Papers 002244366 695__ $$2INSPIRE$$9bibclassify$$aK: production 002244366 695__ $$2INSPIRE$$9bibclassify$$aheavy ion: scattering 002244366 695__ $$2INSPIRE$$9bibclassify$$ameson: production 002244366 695__ $$2INSPIRE$$9bibclassify$$atransverse momentum: high 002244366 695__ $$2INSPIRE$$9bibclassify$$aluminosity: high 002244366 695__ $$2INSPIRE$$9bibclassify$$ap p: scattering 002244366 695__ $$2INSPIRE$$9bibclassify$$asuppression 002244366 695__ $$2INSPIRE$$9bibclassify$$aCERN LHC Coll 002244366 695__ $$2INSPIRE$$9bibclassify$$ahadronic decay 002244366 695__ $$2INSPIRE$$9bibclassify$$aenhancement 002244366 695__ $$2INSPIRE$$9bibclassify$$anucleus 002244366 695__ $$2INSPIRE$$9bibclassify$$aflavor 002244366 695__ $$2INSPIRE$$9bibclassify$$aALICE 002244366 695__ $$2INSPIRE$$9bibclassify$$aquark 002244366 695__ $$2INSPIRE$$9bibclassify$$aflow 002244366 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. 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Tech., Mumbai 002244366 700__ $$aAhammed, Zubayer$$iINSPIRE-00180720$$uCalcutta, VECC 002244366 700__ $$aAhmad, Shakeel$$iINSPIRE-00560210$$uAligarh Muslim U. 002244366 700__ $$aAhn, Sang Un$$iINSPIRE-00254695$$uKISTI, Daejeon 002244366 700__ $$aAiola, Salvatore$$iINSPIRE-00381830$$uYale U. 002244366 700__ $$aAkindinov, Alexander$$iINSPIRE-00061314$$uMoscow, ITEP 002244366 700__ $$aAlam, Sk Noor$$iINSPIRE-00415748$$uCalcutta, VECC 002244366 700__ $$aSilva De Albuquerque, Danilo$$iINSPIRE-00560229$$uCampinas State U. 002244366 700__ $$aAleksandrov, Dmitry$$iINSPIRE-00158344$$uKurchatov Inst., Moscow 002244366 700__ $$aAlessandro, Bruno$$iINSPIRE-00250010$$uINFN, Turin 002244366 700__ $$aAlexandre, Didier$$iINSPIRE-00381902$$uBirmingham U. 002244366 700__ $$aAlfaro Molina, Jose Ruben$$iINSPIRE-00249844$$uMexico U. 002244366 700__ $$aAlici, Andrea$$iINSPIRE-00249832$$uEnrico Fermi Ctr., Rome$$uINFN, Bologna 002244366 700__ $$aAlkin, Anton$$iINSPIRE-00245838$$uBITP, Kiev 002244366 700__ $$aAlme, Johan$$iINSPIRE-00249819$$uBergen U.$$uBergen Coll. 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U. 002244366 700__ $$aChojnacki, Marek$$iINSPIRE-00244445$$uBohr Inst. 002244366 700__ $$aChoudhury, Subikash$$iINSPIRE-00361022$$uCalcutta, VECC 002244366 700__ $$aChristakoglou, Panagiotis$$iINSPIRE-00261752$$uNIKHEF, Amsterdam 002244366 700__ $$aChristensen, Christian Holm$$iINSPIRE-00228862$$uBohr Inst. 002244366 700__ $$aChristiansen, Peter$$iINSPIRE-00254597$$uLund U. 002244366 700__ $$aChujo, Tatsuya$$iINSPIRE-00073415$$uTsukuba U. 002244366 700__ $$aChung, Suh-urk$$iINSPIRE-00073470$$uPusan Natl. U. 002244366 700__ $$aCicalo, Corrado$$iINSPIRE-00289316$$uINFN, Cagliari 002244366 700__ $$aCifarelli, Luisa$$iINSPIRE-00172106$$uEnrico Fermi Ctr., Rome$$uBologna U.$$uINFN, Bologna 002244366 700__ $$aCindolo, Federico$$iINSPIRE-00073552$$uINFN, Bologna 002244366 700__ $$aCleymans, Jean Willy Andre$$iINSPIRE-00073783$$uCape Town U. 002244366 700__ $$aColamaria, Fabio Filippo$$iINSPIRE-00246108$$uBari U.$$uINFN, Bari 002244366 700__ $$aColella, Domenico$$iINSPIRE-00361034$$uKosice, IEF$$uCERN 002244366 700__ $$aCollu, Alberto$$iINSPIRE-00361046$$uLBL, Berkeley 002244366 700__ $$aColocci, Manuel$$iINSPIRE-00382468$$uBologna U.$$uINFN, Bologna 002244366 700__ $$aConesa Balbastre, Gustavo$$iINSPIRE-00247256$$uLPSC, Grenoble 002244366 700__ $$aConesa Del Valle, Zaida$$iINSPIRE-00026575$$uOrsay, IPN 002244366 700__ $$aConnors, Megan Elizabeth$$iINSPIRE-00255007$$uYale U. 002244366 700__ $$aContreras Nuno, Jesus Guillermo$$iINSPIRE-00240060$$uPrague, Tech. U. 002244366 700__ $$aCormier, Thomas Michael$$iINSPIRE-00261783$$uOak Ridge 002244366 700__ $$aCorrales Morales, Yasser$$iINSPIRE-00261791$$uINFN, Turin 002244366 700__ $$aCortes Maldonado, Ismael$$iINSPIRE-00210299$$uPuebla U., Mexico 002244366 700__ $$aCortese, Pietro$$iINSPIRE-00037929$$uPiemonte Orientale U., Alessandria 002244366 700__ $$aCosentino, Mauro Rogerio$$iINSPIRE-00289338$$uABC Federal U. 002244366 700__ $$aCosta, Filippo$$iINSPIRE-00289393$$uCERN 002244366 700__ $$aCostanza, Susanna$$iINSPIRE-00563963$$uPavia U., Dept. Fis. 'A. Volta' 002244366 700__ $$aCrkovska, Jana$$iINSPIRE-00538124$$uOrsay, IPN 002244366 700__ $$aCrochet, Philippe$$iINSPIRE-00250128$$uClermont-Ferrand U. 002244366 700__ $$aCruz Albino, Rigoberto$$iINSPIRE-00382506$$uCINVESTAV, IPN 002244366 700__ $$aCuautle Flores, Eleazar$$iINSPIRE-00075170$$uMexico U., ICN 002244366 700__ $$aCunqueiro Mendez, Leticia$$iINSPIRE-00289410$$uMunster U. 002244366 700__ $$aDahms, Torsten$$iINSPIRE-00039260$$uMunich, Tech. U., Universe$$uTech. U., Munich (main) 002244366 700__ $$aDainese, Andrea$$iINSPIRE-00250006$$uINFN, Padua 002244366 700__ $$aDanisch, Meike Charlotte$$iINSPIRE-00560270$$uHeidelberg U. 002244366 700__ $$aDanu, Andrea$$iINSPIRE-00249445$$uBucharest, Inst. Space Science 002244366 700__ $$aDas, Debasish$$iINSPIRE-00289436$$uSaha Inst. 002244366 700__ $$aDas, Indranil$$iINSPIRE-00249433$$uSaha Inst. 002244366 700__ $$aDas, Supriya$$iINSPIRE-00058401$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002244366 700__ $$aDash, Ajay Kumar$$iINSPIRE-00249421$$uBhubaneswar, NISER 002244366 700__ $$aDash, Sadhana$$iINSPIRE-00181086$$uIndian Inst. Tech., Mumbai 002244366 700__ $$aDe, Sudipan$$iINSPIRE-00289444$$uIndian Inst. Tech., Indore$$uSao Paulo U. 002244366 700__ $$aDe Caro, Annalisa$$iINSPIRE-00249410$$uSalerno U.$$uINFN, Salerno 002244366 700__ $$aDe Cataldo, Giacinto$$iINSPIRE-00289454$$uINFN, Bari 002244366 700__ $$aDe Conti, Camila$$iINSPIRE-00537075$$uSao Paulo U. 002244366 700__ $$aDe Cuveland, Jan$$iINSPIRE-00249403$$uFrankfurt U., FIAS 002244366 700__ $$aDe Falco, Alessandro$$iINSPIRE-00080339$$uCagliari U.$$uINFN, Cagliari 002244366 700__ $$aDe Gruttola, Daniele$$iINSPIRE-00249391$$uEnrico Fermi Ctr., Rome$$uSalerno U.$$uINFN, Salerno 002244366 700__ $$aDe Marco, Nora$$iINSPIRE-00254814$$uINFN, Turin 002244366 700__ $$aDe Pasquale, Salvatore$$iINSPIRE-00114896$$uSalerno U.$$uINFN, Salerno 002244366 700__ $$aDerradi De Souza, Rafael$$iINSPIRE-00181156$$uCampinas State U. 002244366 700__ $$aFranz Degenhardt, Hermann$$iINSPIRE-00564005$$uSao Paulo U. 002244366 700__ $$aDeisting, Alexander$$iINSPIRE-00507268$$uDarmstadt, EMMI$$uHeidelberg U. 002244366 700__ $$aDeloff, Andrzej$$iINSPIRE-00189124$$uWarsaw, Inst. Nucl. Studies 002244366 700__ $$aDeplano, Caterina$$iINSPIRE-00258120$$uNIKHEF, Amsterdam 002244366 700__ $$aDhankher, Preeti$$iINSPIRE-00531295$$uIndian Inst. Tech., Mumbai 002244366 700__ $$aDi Bari, Domenico$$iINSPIRE-00064510$$uBari U.$$uINFN, Bari 002244366 700__ $$aDi Mauro, Antonio$$iINSPIRE-00105894$$uCERN 002244366 700__ $$aDi Nezza, Pasquale$$iINSPIRE-00139137$$uFrascati 002244366 700__ $$aDi Ruzza, Benedetto$$iINSPIRE-00030649$$uINFN, Padua 002244366 700__ $$aDiaz Corchero, Miguel Angel$$iINSPIRE-00361060$$uMadrid, CIEMAT 002244366 700__ $$aDietel, Thomas$$iINSPIRE-00262178$$uCape Town U. 002244366 700__ $$aDillenseger, Pascal$$iINSPIRE-00416124$$uFrankfurt U., Inst. Kernphys. 002244366 700__ $$aDivia, Roberto$$iINSPIRE-00262189$$uCERN 002244366 700__ $$aDjuvsland, Oeystein$$iINSPIRE-00249457$$uBergen U. 002244366 700__ $$aDobrin, Alexandru Florin$$iINSPIRE-00247195$$uBucharest, Inst. Space Science$$uCERN 002244366 700__ $$aDomenicis Gimenez, Diogenes$$iINSPIRE-00382641$$uSao Paulo U. 002244366 700__ $$aDonigus, Benjamin$$iINSPIRE-00249342$$uFrankfurt U., Inst. Kernphys. 002244366 700__ $$aDordic, Olja$$iINSPIRE-00249337$$uOslo U. 002244366 700__ $$aDrozhzhova, Tatiana$$iINSPIRE-00364225$$uFrankfurt U., Inst. Kernphys. 002244366 700__ $$aDubey, Anand Kumar$$iINSPIRE-00241469$$uCalcutta, VECC 002244366 700__ $$aDubla, Andrea$$iINSPIRE-00361083$$uDarmstadt, EMMI 002244366 700__ $$aDucroux, Laurent$$iINSPIRE-00262200$$uLyon, IPN 002244366 700__ $$aDuggal, Ashpreet Kaur$$iINSPIRE-00563985$$uPanjab U. 002244366 700__ $$aDupieux, Pascal$$iINSPIRE-00078560$$uClermont-Ferrand U. 002244366 700__ $$aEhlers Iii, Raymond James$$iINSPIRE-00382746$$uYale U. 002244366 700__ $$aElia, Domenico$$iINSPIRE-00079305$$uINFN, Bari 002244366 700__ $$aEndress, Eric$$iINSPIRE-00527308$$uLima, Pont. U. Catolica 002244366 700__ $$aEngel, Heiko$$iINSPIRE-00246250$$uGoethe U., Frankfurt, Inst. Inform. 002244366 700__ $$aEpple, Eliane$$iINSPIRE-00476843$$uYale U. 002244366 700__ $$aErazmus, Barbara Ewa$$iINSPIRE-00183847$$uSUBATECH, Nantes 002244366 700__ $$aErhardt, Filip$$iINSPIRE-00507377$$uZagreb U. 002244366 700__ $$aEspagnon, Bruno$$iINSPIRE-00262220$$uOrsay, IPN 002244366 700__ $$aEsumi, Shinichi$$iINSPIRE-00241535$$uTsukuba U. 002244366 700__ $$aEulisse, Giulio$$iINSPIRE-00006913$$uCERN 002244366 700__ $$aEum, Jongsik$$iINSPIRE-00507489$$uPusan Natl. U. 002244366 700__ $$aEvans, David$$iINSPIRE-00162820$$uBirmingham U. 002244366 700__ $$aEvdokimov, Sergey$$iINSPIRE-00382834$$uSerpukhov, IHEP 002244366 700__ $$aFabbietti, Laura$$iINSPIRE-00164656$$uMunich, Tech. U., Universe$$uTech. U., Munich (main) 002244366 700__ $$aFabris, Daniela$$iINSPIRE-00262240$$uINFN, Padua 002244366 700__ $$aFaivre, Julien$$iINSPIRE-00243836$$uLPSC, Grenoble 002244366 700__ $$aFantoni, Alessandra$$iINSPIRE-00139125$$uFrascati 002244366 700__ $$aFasel, Markus$$iINSPIRE-00249303$$uOak Ridge$$uLBL, Berkeley 002244366 700__ $$aFeldkamp, Linus$$iINSPIRE-00361095$$uMunster U. 002244366 700__ $$aFeliciello, Alessandro$$iINSPIRE-00080709$$uINFN, Turin 002244366 700__ $$aFeofilov, Grigorii$$iINSPIRE-00243848$$uSt. Petersburg State U. 002244366 700__ $$aFerencei, Jozef$$iINSPIRE-00185039$$uRez, Nucl. Phys. 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U. Catolica 002244366 700__ $$aGajdosova, Katarina$$iINSPIRE-00538159$$uBohr Inst. 002244366 700__ $$aGallio, Mauro$$iINSPIRE-00250190$$uTurin U.$$uINFN, Turin 002244366 700__ $$aDuarte Galvan, Carlos$$iINSPIRE-00563971$$uSinaloa U. 002244366 700__ $$aGangadharan, Dhevan Raja$$iINSPIRE-00181636$$uLBL, Berkeley 002244366 700__ $$aGanoti, Paraskevi$$iINSPIRE-00249171$$uAthens U. 002244366 700__ $$aGao, Chaosong$$iINSPIRE-00419488$$uHua-Zhong Normal U. 002244366 700__ $$aGarabatos Cuadrado, Jose$$iINSPIRE-00247140$$uDarmstadt, EMMI 002244366 700__ $$aGarcia-solis, Edmundo Javier$$iINSPIRE-00319408$$uChicago State U. 002244366 700__ $$aGarg, Kunal$$iINSPIRE-00564023$$uCatania U.$$uINFN, Catania 002244366 700__ $$aGarg, Prakhar$$iINSPIRE-00362221$$uIndian Inst. Tech., Indore 002244366 700__ $$aGargiulo, Corrado$$iINSPIRE-00304950$$uCERN 002244366 700__ $$aGasik, Piotr Jan$$iINSPIRE-00386209$$uMunich, Tech. U., Universe$$uTech. U., Munich (main) 002244366 700__ $$aGauger, Erin Frances$$iINSPIRE-00531301$$uTexas U. 002244366 700__ $$aDe Leone Gay, Maria Beatriz$$iINSPIRE-00227970$$uRio Grande do Sul U. 002244366 700__ $$aGermain, Marie$$iINSPIRE-00046404$$uSUBATECH, Nantes 002244366 700__ $$aGhosh, Premomoy$$iINSPIRE-00181669$$uCalcutta, VECC 002244366 700__ $$aGhosh, Sanjay Kumar$$iINSPIRE-00385559$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002244366 700__ $$aGianotti, Paola$$iINSPIRE-00084690$$uFrascati 002244366 700__ $$aGiubellino, Paolo$$iINSPIRE-00085080$$uCERN$$uINFN, Turin 002244366 700__ $$aGiubilato, Piero$$iINSPIRE-00017284$$uPadua U.$$uINFN, Padua 002244366 700__ $$aGladysz-dziadus, Ewa$$iINSPIRE-00250209$$uCracow, INP 002244366 700__ $$aGlassel, Peter$$iINSPIRE-00262357$$uHeidelberg U. 002244366 700__ $$aGomez Coral, Diego Mauricio$$iINSPIRE-00531313$$uMexico U. 002244366 700__ $$aGomez Ramirez, Andres$$iINSPIRE-00416173$$uGoethe U., Frankfurt, Inst. Inform. 002244366 700__ $$aSanchez Gonzalez, Andres$$iINSPIRE-00560286$$uCERN 002244366 700__ $$aGonzalez, Victor$$iINSPIRE-00537090$$uMadrid, CIEMAT 002244366 700__ $$aGonzalez Zamora, Pedro$$iINSPIRE-00249119$$uMadrid, CIEMAT 002244366 700__ $$aGorbunov, Sergey$$iINSPIRE-00262379$$uFrankfurt U., FIAS 002244366 700__ $$aGorlich, Lidia Maria$$iINSPIRE-00185075$$uCracow, INP 002244366 700__ $$aGotovac, Sven$$iINSPIRE-00249102$$uSplit Tech. U. 002244366 700__ $$aGrabski, Varlen$$iINSPIRE-00086274$$uMexico U. 002244366 700__ $$aGraczykowski, Lukasz Kamil$$iINSPIRE-00245450$$uWarsaw U. of Tech. 002244366 700__ $$aGraham, Katie Leanne$$iINSPIRE-00522271$$uBirmingham U. 002244366 700__ $$aGreiner, Leo Clifford$$iINSPIRE-00544164$$uLBL, Berkeley 002244366 700__ $$aGrelli, Alessandro$$iINSPIRE-00247138$$uUtrecht U. 002244366 700__ $$aGrigoras, Costin$$iINSPIRE-00249065$$uCERN 002244366 700__ $$aGrigoryev, Vladislav$$iINSPIRE-00262389$$uMoscow Phys. Eng. 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Sci.$$uTokyo U. 002244366 700__ $$aHamar, Gergoe$$iINSPIRE-00262460$$uWigner RCP, Budapest 002244366 700__ $$aHamon, Julien Charles$$iINSPIRE-00548368$$uStrasbourg, IPHC 002244366 700__ $$aHarris, John William$$iINSPIRE-00301628$$uYale U. 002244366 700__ $$aHarton, Austin Vincent$$iINSPIRE-00245718$$uChicago State U. 002244366 700__ $$aHatzifotiadou, Despina$$iINSPIRE-00244493$$uINFN, Bologna 002244366 700__ $$aHayashi, Shinichi$$iINSPIRE-00361149$$uTokyo U. 002244366 700__ $$aHeckel, Stefan Thomas$$iINSPIRE-00245584$$uFrankfurt U., Inst. Kernphys. 002244366 700__ $$aHellbar, Ernst$$iINSPIRE-00560290$$uFrankfurt U., Inst. Kernphys. 002244366 700__ $$aHelstrup, Haavard$$iINSPIRE-00089682$$uBergen Coll. 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Subatomare Phys. 002244366 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev 002244366 700__ $$aZmeskal, Johann$$iINSPIRE-00564793$$uStefan Meyer Inst. Subatomare Phys. 002244366 710__ $$gALICE Collaboration 002244366 710__ $$5PH 002244366 773__ $$c064606$$n6$$pPhys. Rev. C$$v95$$y2017 002244366 859__ [email protected] 002244366 8564_ $$82206970$$s49063$$uhttps://cds.cern.ch/record/2244366/files/Fig1_Invmass_Kstar_pp_PbPb_2760GeV-eps-converted-to.png$$y00000 (Color online) Invariant-mass distributions of $\pi$K pairs for pp and the 0--5$\%$ most central Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 2.76 TeV for the momentum ranges 0.6 $\textless$ $p_{\mathrm{T}}$ $\textless$ 0.9 GeV/$c$ (upper panel) and 10 $\textless$ $p_{\mathrm{T}}$ $\textless$ 15 GeV/$c$ (lower panel), respectively. Panels (a) and (c) show the unlike charge $\pi$K invariant-mass distribution from the same event and normalized mixed event background. Panels (b) and (d) report the invariant-mass distribution after subtraction of the combinatorial background for K$^{*0}$. The statistical uncertainties are shown by bars. The solid curves represent fits to the distributions and the red dashed curves are the components of those fits that describe the residual background. 002244366 8564_ $$82206971$$s47108$$uhttps://cds.cern.ch/record/2244366/files/Fig5b_Spectra_Phi_PbPb_2760GeV_v3-eps-converted-to.png$$y00007 (Color online) Invariant yields of (a) K$^{*0}$ and (b) $\phi$ mesons in various centrality classes in Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The normalization uncertainty is not shown here, but is given in Table~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206972$$s56078$$uhttps://cds.cern.ch/record/2244366/files/Fig4a_InvYield_Kstar_pp2760GeV_v3-eps-converted-to.png$$y00004 (Color online) Invariant yields for (a) K$^{*0}$ and (b) $\phi$ mesons normalized to the number of inelastic pp collisions at $\sqrt{s}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical uncertainties on the data are shown by bars and the systematic uncertainties by boxes. The results are compared with model calculations from PYTHIA 8.14~\cite{Sjostrand:2007gs}, PHOJET~\cite{Engel:1994vs, Engel:1995yda}, PYTHIA D6T~\cite{Field:2008zz}, PYTHIA ATLAS-CSC~\cite{Buttar:2004iy} and PYTHIA PERUGIA~\cite{Skands:2010ak} as shown by different dashed lines. The lower panel for both K$^{*0}$ and $\phi$ shows the model to data ratio. 002244366 8564_ $$82206973$$s43119$$uhttps://cds.cern.ch/record/2244366/files/Fig6_Kstar2Km_phi2Km_mult3-eps-converted-to.png$$y00008 (Color online) K$^{*0}$/K$^{-}$ and $\phi$/K$^{-}$ ratios as a function of $\langle\mathrm{d}N_{\mathrm{ch}}/\mathrm{d}\eta\rangle^{1/3}$ measured at mid-rapidity~\cite{Aamodt:2011mr} in pp collisions at $\sqrt{s}$ = 2.76 TeV and 7 TeV~\cite{Abelev:2012hy}, and Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. For Pb--Pb collisions, the $\phi$/K$^{-}$ values are exclusively from~\cite{Abelev:2014uua}; the previously published K$^{*0}$/K$^{-}$ measurements are compared to new measurements in finer centrality classes. Bars represent the statistical uncertainties, empty boxes represent the total systematic uncertainties, and shaded boxes represent the systematic uncertainties that are uncorrelated between centrality classes. The expectations from a thermal model calculation with chemical freeze-out temperature of 156 MeV for the most central collisions~\cite{Stachel:2013zma} are shown. The EPOS3 calculation of the K$^{*0}$/K and $\phi$/K ratios are also shown as a violet band for different centrality intervals~\cite{Knospe:2015nva}. 002244366 8564_ $$82206974$$s41403$$uhttps://cds.cern.ch/record/2244366/files/Fig5a_Spectra_Kstar_PbPb_2760GeV.png$$y00006 (Color online) Invariant yields of (a) K$^{*0}$ and (b) $\phi$ mesons in various centrality classes in Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The normalization uncertainty is not shown here, but is given in Tab.~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206975$$s23632$$uhttps://cds.cern.ch/record/2244366/files/Fig8_Ratio_Proton_to_Kstar_Phi.png$$y00010 (Color online) Ratios of particle yields p/K$^{*0}$ in panel (a) and p/$\phi$ in panel (b) as a function of $p_{\mathrm{T}}$ in central and peripheral Pb--Pb collisions and pp collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. The p/$\phi$ ratio for $p_{\mathrm{T}}$ $\textless$ 4 GeV/$c$ is from~\cite{Abelev:2014uua}. The statistical and systematic uncertainties are shown as bars and boxes respectively. 002244366 8564_ $$82206976$$s43531$$uhttps://cds.cern.ch/record/2244366/files/Fig6_Kstar2Km_phi2Km_mult3.png$$y00008 (Color online) K$^{*0}$/K$^{-}$ and $\phi$/K$^{-}$ ratios as a function of $\langle\mathrm{d}N_{\mathrm{ch}}/\mathrm{d}\eta\rangle^{1/3}$ measured at mid-rapidity~\cite{Aamodt:2011mr} in pp collisions at $\sqrt{s}$ = 2.76 TeV and 7 TeV~\cite{Abelev:2012hy}, and Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. For Pb--Pb collisions, the $\phi$/K$^{-}$ values are exclusively from~\cite{Abelev:2014uua}; the previously published K$^{*0}$/K$^{-}$ measurements are compared to new measurements in finer centrality classes. Bars represent the statistical uncertainties, empty boxes represent the total systematic uncertainties, and shaded boxes represent the systematic uncertainties that are uncorrelated between centrality classes. The expectations from a thermal model calculation with chemical freeze-out temperature of 156 MeV for the most central collisions~\cite{Stachel:2013zma} are shown. The EPOS3 calculation of the K$^{*0}$/K and $\phi$/K ratios are also shown as a violet band for different centrality intervals~\cite{Knospe:2015nva}. 002244366 8564_ $$82206977$$s57144$$uhttps://cds.cern.ch/record/2244366/files/Fig4b_InvYield_Phi_pp2760GeV.png$$y00005 (Color online) Invariant yields for (a) K$^{*0}$ and (b) $\phi$ mesons normalized to the number of inelastic pp collisions at $\sqrt{s}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical uncertainties on the data are shown by bars and the systematic uncertainties by boxes. The results are compared with model calculations from PYTHIA 8.14~\cite{Sjostrand:2007gs}, PHOJET~\cite{Engel:1994vs, Engel:1995yda}, PYTHIA D6T~\cite{Field:2008zz}, PYTHIA ATLAS-CSC~\cite{Buttar:2004iy} and PYTHIA PERUGIA~\cite{Skands:2010ak} as shown by different dashed lines. The lower panel for both K$^{*0}$ and $\phi$ shows the model to data ratio. 002244366 8564_ $$82206978$$s50542$$uhttps://cds.cern.ch/record/2244366/files/Fig9_RAA_KStar_Phi_ChrgHadron-eps-converted-to.png$$y00011 (Color online) The nuclear modification factor, $R_\mathrm{AA}$, as a function of $p_{\mathrm{T}}$ for K$^{*0}$ and $\phi$ mesons in Pb--Pb collisions for different centrality classes. The results are compared with the $R_\mathrm{AA}$ of charged hadrons measured by ALICE~\cite{Abelev:2012hxa}. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The boxes around unity indicate the uncertainty on the normalization of $R_\mathrm{AA}$, including the uncertainty on the nuclear overlap function $\langle T_{\mathrm{AA}} \rangle$ and the normalization uncertainty given in Table~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206979$$s49193$$uhttps://cds.cern.ch/record/2244366/files/Fig1_Invmass_Kstar_pp_PbPb_2760GeV.png$$y00000 (Color online) Invariant-mass distributions of $\pi$K pairs for pp and the 0--5$\%$ most central Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 2.76 TeV for the momentum ranges 0.6 $\textless$ $p_{\mathrm{T}}$ $\textless$ 0.9 GeV/$c$ (upper panel) and 10 $\textless$ $p_{\mathrm{T}}$ $\textless$ 15 GeV/$c$ (lower panel), respectively. Panels (a) and (c) show the unlike charge $\pi$K invariant-mass distribution from the same event and normalized mixed event background. Panels (b) and (d) report the invariant-mass distribution after subtraction of the combinatorial background for K$^{*0}$. The statistical uncertainties are shown by bars. The solid curves represent fits to the distributions and the red dashed curves are the components of those fits that describe the residual background. 002244366 8564_ $$82206980$$s56583$$uhttps://cds.cern.ch/record/2244366/files/Fig4b_InvYield_Phi_pp2760GeV_v3-eps-converted-to.png$$y00005 (Color online) Invariant yields for (a) K$^{*0}$ and (b) $\phi$ mesons normalized to the number of inelastic pp collisions at $\sqrt{s}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical uncertainties on the data are shown by bars and the systematic uncertainties by boxes. The results are compared with model calculations from PYTHIA 8.14~\cite{Sjostrand:2007gs}, PHOJET~\cite{Engel:1994vs, Engel:1995yda}, PYTHIA D6T~\cite{Field:2008zz}, PYTHIA ATLAS-CSC~\cite{Buttar:2004iy} and PYTHIA PERUGIA~\cite{Skands:2010ak} as shown by different dashed lines. The lower panel for both K$^{*0}$ and $\phi$ shows the model to data ratio. 002244366 8564_ $$82206981$$s30674$$uhttps://cds.cern.ch/record/2244366/files/Fig7_Ratio_Phi_Kstar_by_pion_kaon.png$$y00009 (Color online) Ratios of particle yields K$^{*0}$/K and $\phi/$K in panel (a) and K$^{*0}/\pi$ and $\phi/\pi$ in panel (b) as a function of $p_{\mathrm{T}}$ in central Pb--Pb and pp collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV are shown. Here, (K$^{*0}$+$\overline{\mathrm{K}}^{*0}$), ($\mathrm{K}^{+}$+$\mathrm{K}^{-}$) and ($\pi^{+}$+$\pi^{-}$) are denoted as K$^{*0}$, K, $\pi$, respectively. The statistical and systematic uncertainties are shown as bars and caps respectively. 002244366 8564_ $$82206982$$s10632$$uhttps://cds.cern.ch/record/2244366/files/Fig3_left_Eff_pp_2760GeV.png$$y00002 (Color online) The acceptance and efficiency ($A \times$ $\epsilon_{\mathrm{rec}}$) correction as a function of $p_{\mathrm{T}}$ for K$^{*0}$ (red marker) and $\phi$ (blue marker) mesons in pp (left panel) and 0-5$\%$ centrality in Pb--Pb (right panel) collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. 002244366 8564_ $$82206983$$s701805$$uhttps://cds.cern.ch/record/2244366/files/arXiv:1702.00555.pdf 002244366 8564_ $$82206984$$s58199$$uhttps://cds.cern.ch/record/2244366/files/Fig2_Invmass_Phi_pp_PbPb_2760-eps-converted-to.png$$y00001 (Color online) Invariant-mass distributions of KK pairs for pp and the 0--5$\%$ most central Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 2.76 TeV for the momentum ranges 0.5 $\textless$ $p_{\mathrm{T}}$ $\textless$ 0.8 GeV/$c$ (upper panel) and 10 $\textless$ $p_{\mathrm{T}}$ $\textless$ 13 GeV/$c$ (lower panel), respectively. In panels (a) and (c) the unlike charge KK invariant-mass distribution from the same event and normalized mixed event background are shown. In panels (b) and (d) the invariant-mass distribution after subtraction of the combinatorial background for $\phi$ is shown. The statistical uncertainties are shown by bars. The solid curves are the fits to the distributions and the red dashed curves are the components of those fits that describe the residual background. 002244366 8564_ $$82206985$$s58186$$uhttps://cds.cern.ch/record/2244366/files/Fig2_Invmass_Phi_pp_PbPb_2760.png$$y00001 (Color online) Invariant-mass distributions of KK pairs for pp and the 0--5$\%$ most central Pb--Pb collisions at $\sqrt{s_{\mathrm{NN}}}$ = 2.76 TeV for the momentum ranges 0.5 $\textless$ $p_{\mathrm{T}}$ $\textless$ 0.8 GeV/$c$ (upper panel) and 10 $\textless$ $p_{\mathrm{T}}$ $\textless$ 13 GeV/$c$ (lower panel), respectively. In panels (a) and (c) the unlike charge KK invariant-mass distribution from the same event and normalized mixed event background are shown. In panels (b) and (d) the invariant-mass distribution after subtraction of the combinatorial background for $\phi$ is shown. The statistical uncertainties are shown by bars. The solid curves are the fits to the distributions and the red dashed curves are the components of those fits that describe the residual background. 002244366 8564_ $$82206986$$s9836$$uhttps://cds.cern.ch/record/2244366/files/Fig3_right_Eff_pp_2760GeV.png$$y00003 (Color online) The acceptance and efficiency ($A \times$ $\epsilon_{\mathrm{rec}}$) correction as a function of $p_{\mathrm{T}}$ for K$^{*0}$ (red marker) and $\phi$ (blue marker) mesons in pp (left panel) and 0-5$\%$ centrality in Pb--Pb (right panel) collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. 002244366 8564_ $$82206987$$s38618$$uhttps://cds.cern.ch/record/2244366/files/Fig10_RAA_Kstar_Phi_Pi_K_P.png$$y00012 (Color online) The $R_\mathrm{AA}$ for K$^{*0}$ and $\phi$ mesons as a function of $p_{\mathrm{T}}$ in 0--5$\%$ Pb--Pb collisions. The results are compared with the $R_\mathrm{AA}$ of $\pi$, K and p~\cite{Abelev:2014laa}. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The boxes around unity indicate the uncertainty on the normalization of $R_\mathrm{AA}$, including the uncertainty on the nuclear overlap function $\langle T_{\mathrm{AA}} \rangle$ and the normalization uncertainty given in Tab.~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206988$$s30708$$uhttps://cds.cern.ch/record/2244366/files/Fig7_Ratio_Phi_Kstar_by_pion_kaon-eps-converted-to.png$$y00009 (Color online) Ratios of particle yields K$^{*0}$/K and $\phi/$K in panel (a) and K$^{*0}/\pi$ and $\phi/\pi$ in panel (b) as a function of $p_{\mathrm{T}}$ in central Pb--Pb and pp collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV are shown. Here, (K$^{*0}$+$\overline{\mathrm{K}}^{*0}$), ($\mathrm{K}^{+}$+$\mathrm{K}^{-}$) and ($\pi^{+}$+$\pi^{-}$) are denoted as K$^{*0}$, K, $\pi$, respectively. The statistical and systematic uncertainties are shown as bars and caps respectively. 002244366 8564_ $$82206989$$s41221$$uhttps://cds.cern.ch/record/2244366/files/Fig5a_Spectra_Kstar_PbPb_2760GeV_v3-eps-converted-to.png$$y00006 (Color online) Invariant yields of (a) K$^{*0}$ and (b) $\phi$ mesons in various centrality classes in Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The normalization uncertainty is not shown here, but is given in Table~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206990$$s8969$$uhttps://cds.cern.ch/record/2244366/files/Fig3_right_Eff_PbPb_2760GeV_v2-eps-converted-to.png$$y00003 (Color online) The acceptance and efficiency ($A \times$ $\epsilon_{\mathrm{rec}}$) correction as a function of $p_{\mathrm{T}}$ for K$^{*0}$ (red marker) and $\phi$ (blue marker) mesons in pp (left panel) and 0-5$\%$ centrality in Pb--Pb (right panel) collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. 002244366 8564_ $$82206991$$s56329$$uhttps://cds.cern.ch/record/2244366/files/Fig4a_InvYield_Kstar_pp2760GeV.png$$y00004 (Color online) Invariant yields for (a) K$^{*0}$ and (b) $\phi$ mesons normalized to the number of inelastic pp collisions at $\sqrt{s}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical uncertainties on the data are shown by bars and the systematic uncertainties by boxes. The results are compared with model calculations from PYTHIA 8.14~\cite{Sjostrand:2007gs}, PHOJET~\cite{Engel:1994vs, Engel:1995yda}, PYTHIA D6T~\cite{Field:2008zz}, PYTHIA ATLAS-CSC~\cite{Buttar:2004iy} and PYTHIA PERUGIA~\cite{Skands:2010ak} as shown by different dashed lines. The lower panel for both K$^{*0}$ and $\phi$ shows the model to data ratio. 002244366 8564_ $$82206992$$s38350$$uhttps://cds.cern.ch/record/2244366/files/Fig10_RAA_Kstar_Phi_Pi_K_P-eps-converted-to.png$$y00012 (Color online) The $R_\mathrm{AA}$ for K$^{*0}$ and $\phi$ mesons as a function of $p_{\mathrm{T}}$ in 0--5$\%$ Pb--Pb collisions. The results are compared with the $R_\mathrm{AA}$ of $\pi$, K and p~\cite{Abelev:2014laa}. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The boxes around unity indicate the uncertainty on the normalization of $R_\mathrm{AA}$, including the uncertainty on the nuclear overlap function $\langle T_{\mathrm{AA}} \rangle$ and the normalization uncertainty given in Table~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206993$$s47607$$uhttps://cds.cern.ch/record/2244366/files/Fig5b_Spectra_Phi_PbPb_2760GeV.png$$y00007 (Color online) Invariant yields of (a) K$^{*0}$ and (b) $\phi$ mesons in various centrality classes in Pb--Pb collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. Invariant yield is calculated by taking the value of $p_{\mathrm{T}}$ at the corresponding bin center. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The normalization uncertainty is not shown here, but is given in Tab.~\ref{tab_kstar_by_k}. 002244366 8564_ $$82206994$$s23641$$uhttps://cds.cern.ch/record/2244366/files/Fig8_Ratio_Proton_to_Kstar_Phi-eps-converted-to.png$$y00010 (Color online) Ratios of particle yields p/K$^{*0}$ in panel (a) and p/$\phi$ in panel (b) as a function of $p_{\mathrm{T}}$ in central and peripheral Pb--Pb collisions and pp collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. The p/$\phi$ ratio for $p_{\mathrm{T}}$ $\textless$ 4 GeV/$c$ is from~\cite{Abelev:2014uua}. The statistical and systematic uncertainties are shown as bars and boxes respectively. 002244366 8564_ $$82206995$$s9759$$uhttps://cds.cern.ch/record/2244366/files/Fig3_left_Eff_pp_2760GeV_v2-eps-converted-to.png$$y00002 (Color online) The acceptance and efficiency ($A \times$ $\epsilon_{\mathrm{rec}}$) correction as a function of $p_{\mathrm{T}}$ for K$^{*0}$ (red marker) and $\phi$ (blue marker) mesons in pp (left panel) and 0-5$\%$ centrality in Pb--Pb (right panel) collisions at $\sqrt{s_\mathrm{NN}}$ = 2.76 TeV. 002244366 8564_ $$82206996$$s50641$$uhttps://cds.cern.ch/record/2244366/files/Fig9_RAA_KStar_Phi_ChrgHadron.png$$y00011 (Color online) The nuclear modification factor, $R_\mathrm{AA}$, as a function of $p_{\mathrm{T}}$ for K$^{*0}$ and $\phi$ mesons in Pb--Pb collisions for different centrality classes. The results are compared with the $R_\mathrm{AA}$ of charged hadrons measured by ALICE~\cite{Abelev:2012hxa}. The statistical and systematic uncertainties are shown as bars and boxes, respectively. The boxes around unity indicate the uncertainty on the normalization of $R_\mathrm{AA}$, including the uncertainty on the nuclear overlap function $\langle T_{\mathrm{AA}} \rangle$ and the normalization uncertainty given in Tab.~\ref{tab_kstar_by_k}. 002244366 9031_ $$aApproval requested for number CERN-EP-2017-010$$bCERN-EP-2017-010$$cEPPHAPP$$d2017-01-18 10:11:20$$e2017-01-25 10:11:[email protected]$$swaiting 002244366 9031_ $$aDocument approved$$bCERN-EP-2017-010$$cEPPHAPP$$d2017-01-19 16:34:[email protected]$$sapproved 002244366 916__ $$sn$$w201703 002244366 960__ $$a13 002244366 981__ $$a2242352 002244366 980__ $$aArticle 002244366 980__ $$aALICE_Papers 002244366 980__ $$aARTICLE