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dc.contributor.CRUESPUNIVERSIDADE ESTADUAL DE CAMPINASpt_BR
dc.contributor.authorunicampChinellato, David Dobrigkeitpt_BR
dc.contributor.authorunicampDash, Ajay Kumarpt_BR
dc.contributor.authorunicampTakahashi, Junpt_BR
dc.typeArtigopt_BR
dc.titleK*(892)(0) and Phi(1020) production in Pb-pb collisions at root S(nn)=2.76 Tevpt_BR
dc.contributor.authorAbdelwahab, N. M.pt_BR
dc.contributor.authorAdamczyk, L.pt_BR
dc.contributor.authorAdkins, J. K.pt_BR
dc.contributor.authorAgakishiev, G.pt_BR
dc.contributor.authorAggarwal, M. M.pt_BR
dc.contributor.authorAhammed, Z.pt_BR
dc.contributor.authorAlekseev, I.pt_BR
dc.contributor.authorAlford, J.pt_BR
dc.contributor.authorAnson, C. D.pt_BR
dc.contributor.authorAparin, A.pt_BR
dc.contributor.authorArkhipkin, D.pt_BR
dc.contributor.authorAschenauer, E. C.pt_BR
dc.contributor.authorAverichev, G. S.pt_BR
dc.contributor.authorBanerjee, A.pt_BR
dc.contributor.authorBeavis, D. R.pt_BR
dc.contributor.authorBellwied, R.pt_BR
dc.contributor.authorBhasin, A.pt_BR
dc.contributor.authorBhati, A. K.pt_BR
dc.contributor.authorBhattarai, P.pt_BR
dc.contributor.authorBielcik, J.pt_BR
dc.contributor.authorBielcikova, J.pt_BR
dc.contributor.authorBland, L. C.pt_BR
dc.contributor.authorBordyuzhin, I. G.pt_BR
dc.contributor.authorBorowski, W.pt_BR
dc.contributor.authorBouchet, J.pt_BR
dc.contributor.authorBrandin, A. V.pt_BR
dc.contributor.authorBrovko, S. G.pt_BR
dc.contributor.authorBultmann, S.pt_BR
dc.contributor.authorBunzarov, I.pt_BR
dc.contributor.authorBurton, T. P.pt_BR
dc.contributor.authorButterworth, J.pt_BR
dc.contributor.authorCaines, H.pt_BR
dc.contributor.authorSanchez, M. C. D.pt_BR
dc.contributor.authorCampbell, J. M.pt_BR
dc.contributor.authorCebra, D.pt_BR
dc.contributor.authorCendejas, R.pt_BR
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dc.contributor.authorChaloupka, P.pt_BR
dc.contributor.authorChang, Z.pt_BR
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dc.contributor.authorChen, L.pt_BR
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dc.contributor.authorCherney, M.pt_BR
dc.contributor.authorChikanian, A.pt_BR
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dc.contributor.authorCodrington, M. J. M.pt_BR
dc.contributor.authorContin, G.pt_BR
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dc.contributor.authorDu, C. M.pt_BR
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dc.contributor.authorHaag, B.pt_BR
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dc.contributor.authorHarris, J. W.pt_BR
dc.contributor.authorHeppelmann, S.pt_BR
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dc.contributor.authorHoffmann, G. W.pt_BR
dc.contributor.authorHofman, D. J.pt_BR
dc.contributor.authorHorvat, S.pt_BR
dc.contributor.authorHuang, B.pt_BR
dc.contributor.authorHuang, H. Z.pt_BR
dc.contributor.authorHuang, X.pt_BR
dc.contributor.authorHuck, P.pt_BR
dc.contributor.authorHumanic, T. J.pt_BR
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dc.contributor.authorMa, G. L.pt_BR
dc.contributor.authorMa, Y. G.pt_BR
dc.contributor.authorMahapatra, D. P.pt_BR
dc.contributor.authorMajka, R.pt_BR
dc.contributor.authorMargetis, S.pt_BR
dc.contributor.authorMarkert, C.pt_BR
dc.contributor.authorMasui, H.pt_BR
dc.contributor.authorMatis, H. S.pt_BR
dc.contributor.authorMcDonald, D.pt_BR
dc.contributor.authorMcShane, T. S.pt_BR
dc.contributor.authorMinaev, N. G.pt_BR
dc.contributor.authorMioduszewski, S.pt_BR
dc.contributor.authorMohanty, B.pt_BR
dc.contributor.authorMondal, M. M.pt_BR
dc.contributor.authorMorozov, D. A.pt_BR
dc.contributor.authorMustafa, M. K.pt_BR
dc.contributor.authorNandi, B. K.pt_BR
dc.contributor.authorNasim, M.pt_BR
dc.contributor.authorNayak, T. K.pt_BR
dc.contributor.authorNelson, J. M.pt_BR
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dc.contributor.authorPawlak, T.pt_BR
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dc.contributor.authorPei, H.pt_BR
dc.contributor.authorPerkins, C.pt_BR
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dc.contributor.authorPlaninic, M.pt_BR
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dc.contributor.authorPoljak, N.pt_BR
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dc.contributor.authorPoskanzer, A. M.pt_BR
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dc.contributor.authorXu, Q. H.pt_BR
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dc.contributor.authorXu, Z.pt_BR
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dc.contributor.authorYang, Y.pt_BR
dc.contributor.authorYe, Z.pt_BR
dc.contributor.authorYepes, P.pt_BR
dc.contributor.authorYi, L.pt_BR
dc.contributor.authorYip, K.pt_BR
dc.contributor.authorYoo, I. K.pt_BR
dc.contributor.authorYu, N.pt_BR
dc.contributor.authorZbroszczyk, H.pt_BR
dc.contributor.authorZha, W.pt_BR
dc.contributor.authorZhang, J. B.pt_BR
dc.contributor.authorZhang, J. L.pt_BR
dc.contributor.authorZhang, S.pt_BR
dc.contributor.authorZhang, X. P.pt_BR
dc.contributor.authorZhang, Y.pt_BR
dc.contributor.authorZhang, Z. P.pt_BR
dc.contributor.authorZhao, F.pt_BR
dc.contributor.authorZhao, J.pt_BR
dc.contributor.authorZhong, C.pt_BR
dc.contributor.authorZhu, X.pt_BR
dc.contributor.authorZhu, Y. H.pt_BR
dc.contributor.authorZoulkarneeva, Y.pt_BR
dc.contributor.authorZyzak, M.pt_BR
dc.subjectHádronspt_BR
dc.subjectColisões entre íonspt_BR
dc.subjectCromodinâmica quânticapt_BR
dc.subject.otherlanguageHadronspt_BR
dc.subject.otherlanguageIon-ion collisionspt_BR
dc.subject.otherlanguageQuantum chromodynamicspt_BR
dc.description.abstractThe yields of the K*(892)(0) and phi(1020) resonances are measured in Pb-Pb collisions at root s(NN) = 2.76 TeV through their hadronic decays using the ALICE detector. The measurements are performed in multiple centrality intervals at mid-rapidity (vertical bar y vertical bar < 0.5) in the transverse-momentum ranges 0.3 < p(T) < 5 GeV/c for the K*(892)(0) and 0.5 < p(T) < 5 GeV/c for the phi(1020). The yields of K*(892)(0) are suppressed in central Pb-Pb collisions with respect to pp and peripheral Pb-Pb collisions (perhaps due to rescattering of its decay products in the hadronic medium), while the longer-lived phi(1020) meson is not suppressed. These particles are also used as probes to study the mechanisms of particle production. The shape of the pT distribution of the phi(1020) meson, but not its yield, is reproduced fairly well by hydrodynamic models for central Pb-Pb collisions. In central Pb-Pb collisions at low and intermediate p(T), the p/phi(1020) ratio is flat in p(T), while the p/pi and phi(1020)/pi ratios show a pronounced increase and have similar shapes to each other. These results indicate that the shapes of the p(T) distributions of these particles in central Pb-Pb collisions are determined predominantly by the particle masses and radial flow. Finally, phi(1020) production in Pb-Pb collisions is enhanced, with respect to the yield in pp collisions and the yield of charged pions, by an amount similar to the Lambda and Xi.en
dc.description.abstractThe yields of the K*(892)(0) and phi(1020) resonances are measured in Pb-Pb collisions at root s(NN) = 2.76 TeV through their hadronic decays using the ALICE detector. The measurements are performed in multiple centrality intervals at mid-rapidity (vertical bar y vertical bar < 0.5) in the transverse-momentum ranges 0.3 < p(T) < 5 GeV/c for the K*(892)(0) and 0.5 < p(T) < 5 GeV/c for the phi(1020). The yields of K*(892)(0) are suppressed in central Pb-Pb collisions with respect to pp and peripheral Pb-Pb collisions (perhaps due to rescattering of its decay products in the hadronic medium), while the longer-lived phi(1020) meson is not suppressed. These particles are also used as probes to study the mechanisms of particle production. The shape of the pT distribution of the phi(1020) meson, but not its yield, is reproduced fairly well by hydrodynamic models for central Pb-Pb collisions. In central Pb-Pb collisions at low and intermediate p(T), the p/phi(1020) ratio is flat in p(T), while the p/pi and phi(1020)/pi ratios show a pronounced increase and have similar shapes to each other. These results indicate that the shapes of the p(T) distributions of these particles in central Pb-Pb collisions are determined predominantly by the particle masses and radial flow. Finally, phi(1020) production in Pb-Pb collisions is enhanced, with respect to the yield in pp collisions and the yield of charged pions, by an amount similar to the Lambda and Xi.pt_BR
dc.relation.ispartofPhysical review. C, Nuclear physicspt_BR
dc.relation.ispartofabbreviationPhys. rev. Cpt_BR
dc.publisher.cityCollege Park, MDpt_BR
dc.publisher.countryEstados Unidospt_BR
dc.publisherAmerican Physical Societypt_BR
dc.date.issued2015pt_BR
dc.date.monthofcirculationFeb.pt_BR
dc.identifier.citationK*(892)(0) And Phi(1020) Production In Pb-pb Collisions At Root S(nn)=2.76 Tev. Amer Physical Soc, v. 91, p. FEB-2015.pt_BR
dc.language.isoengpt_BR
dc.description.volume91pt_BR
dc.description.issuenumber2pt_BR
dc.description.firstpage1pt_BR
dc.description.lastpage26pt_BR
dc.rightsabertopt_BR
dc.sourceWOSpt_BR
dc.identifier.issn0556-2813pt_BR
dc.identifier.eissn1089-490Xpt_BR
dc.identifier.doi10.1103/PhysRevC.91.024609pt_BR
dc.identifier.urlhttp://journals.aps.org/prc/abstract/10.1103/PhysRevC.91.024609pt_BR
dc.description.sponsorshipCNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorshipFINEP - FINANCIADORA DE ESTUDOS E PROJETOSpt_BR
dc.description.sponsorshipFAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsorship1CNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorship1FINEP - FINANCIADORA DE ESTUDOS E PROJETOSpt_BR
dc.description.sponsorship1FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.date.available2016-06-07T13:13:39Z-
dc.date.accessioned2016-06-07T13:13:39Z-
dc.description.provenanceMade available in DSpace on 2016-06-07T13:13:39Z (GMT). No. of bitstreams: 1 wos_000352303500007.pdf: 1009888 bytes, checksum: d43081cbf3f5570cb1ef89d7c4dc0e7c (MD5) Previous issue date: 2015 Bitstreams deleted on 2020-09-02T13:39:52Z: wos_000352303500007.pdf,. Added 1 bitstream(s) on 2020-09-02T13:43:50Z : No. of bitstreams: 1 000352303500007.pdf: 1454088 bytes, checksum: a6c12eb8290b919bdc1a7f23df8436e6 (MD5)en
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/241512-
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.identifier.source000352303500007pt_BR
dc.creator.orcid0000-0002-9982-9577pt_BR
dc.creator.orcidSem informaçãopt_BR
dc.creator.orcid0000-0002-4091-1779pt_BR
dc.type.formArtigopt_BR
dc.identifier.articleid024609pt_BR
dc.description.sponsorNoteThe ALICE Collaboration would like to thank all its engineers and technicians for their invaluable contributions to the construction of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collaboration gratefully acknowledges the resources and support provided by all Grid centres and the Worldwide LHC Computing Grid (WLCG) collaboration. The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: State Committee of Science, World Federation of Scientists (WFS) and Swiss Fonds Kidagan, Armeniapt_BR
dc.description.sponsorNoteConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)pt_BR
dc.description.sponsorNoteNational Natural Science Foundation of China (NSFC), the Chinese Ministry of Education (CMOE), and the Ministry of Science and Technology of China (MSTC)pt_BR
dc.description.sponsorNoteMinistry of Education and Youth of the Czech Republicpt_BR
dc.description.sponsorNoteDanish Natural Science Research Council, the Carlsberg Foundation, and the Danish National Research Foundationpt_BR
dc.description.sponsorNoteThe European Research Council under the European Community's Seventh Framework Programmept_BR
dc.description.sponsorNoteHelsinki Institute of Physics and the Academy of Finlandpt_BR
dc.description.sponsorNoteFrench CNRS-IN2P3, the Region Pays de Loire, Region Alsace, Region Auvergne, and CEA, Francept_BR
dc.description.sponsorNoteGerman BMBF and the Helmholtz Associationpt_BR
dc.description.sponsorNoteGeneral Secretariat for Research and Technology, Ministry of Development, Greecept_BR
dc.description.sponsorNoteHungarian OTKA and National Office for Research and Technology (NKTH)pt_BR
dc.description.sponsorNoteDepartment of Atomic Energy and Department of Science and Technology of the Government of Indiapt_BR
dc.description.sponsorNoteIstituto Nazionale di Fisica Nucleare (INFN) and Centro Fermi–Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Italypt_BR
dc.description.sponsorNoteMEXT Grant-in-Aid for Specially Promoted Research, Japanpt_BR
dc.description.sponsorNoteJoint Institute for Nuclear Research, Dubnapt_BR
dc.description.sponsorNoteNational Research Foundation of Korea (NRF)pt_BR
dc.description.sponsorNoteCONACYT, DGAPA, México, ALFA-EC and the EPLANET Program (European Particle Physics Latin American Network)pt_BR
dc.description.sponsorNoteStichting voor Fundamenteel Onderzoek der Materie (FOM) and the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlandspt_BR
dc.description.sponsorNoteResearch Council of Norway (NFR)pt_BR
dc.description.sponsorNotePolish Ministry of Science and Higher Educationpt_BR
dc.description.sponsorNoteNational Science Centre, Polandpt_BR
dc.description.sponsorNoteMinistry of National Education/Institute for Atomic Physics and CNCS-UEFISCDI–Romaniapt_BR
dc.description.sponsorNoteMinistry of Education and Science of Russian Federation, Russian Academy of Sciences, Russian Federal Agency of Atomic Energy, Russian Federal Agency for Science and Innovations, and The Russian Foundation for Basic Researchpt_BR
dc.description.sponsorNoteMinistry of Education of Slovakiapt_BR
dc.description.sponsorNoteDepartment of Science and Technology, South Africapt_BR
dc.description.sponsorNoteCIEMAT, EELA, Ministerio de Economía y Competitividad (MINECO) of Spain, Xunta de Galicia (Consellería de Educación), CEADEN, Cubaenergía, Cuba, and IAEA (International Atomic Energy Agency)pt_BR
dc.description.sponsorNoteSwedish Research Council (VR) and Knut & Alice Wallenberg Foundation (KAW)pt_BR
dc.description.sponsorNoteUkraine Ministry of Education and Sciencept_BR
dc.description.sponsorNoteUnited Kingdom Science and Technology Facilities Council (STFC)pt_BR
dc.description.sponsorNoteThe United States Department of Energy, the United States National Science Foundation, the State of Texas, and the State of Ohio.pt_BR
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