Publication: Bulk properties of the system formed in Au plus Au collisions at root S-NN=14.5 GeV at the BNL STAR detector
| dc.contributor.author | Adam, J. | |
| dc.contributor.author | Adamczyk, L. | |
| dc.contributor.author | Adams, J. R. | |
| dc.contributor.author | Adkins, J. K. | |
| dc.contributor.author | Alekseev, I. | |
| dc.contributor.author | Brandin, A. V. | |
| dc.contributor.author | Khyzhniak, Y. V. | |
| dc.contributor.author | Kochenda, L. | |
| dc.contributor.author | Kravtsov, P. | |
| dc.contributor.author | Nigmatkulov, G. | |
| dc.contributor.author | Okorokov, V. | |
| dc.contributor.author | Strikhanov, M. | |
| dc.contributor.author | Taranenko, A. | |
| dc.contributor.author | Алексеев, Игорь Геннадьевич | |
| dc.contributor.author | Брандин, Андрей Владимирович | |
| dc.contributor.author | Нигматкулов, Григорий Александрович | |
| dc.contributor.author | Окороков, Виталий Алексеевич | |
| dc.contributor.author | Стриханов, Михаил Николаевич | |
| dc.contributor.author | Тараненко, Аркадий Владимирович | |
| dc.date.accessioned | 2024-11-25T16:41:26Z | |
| dc.date.available | 2024-11-25T16:41:26Z | |
| dc.date.issued | 2020 | |
| dc.description.abstract | We report systematic measurements of bulk properties of the system created in Au + Au collisions at root S-NN = 14.5 GeV recorded by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The transverse momentum spectra of pi(+/-), K-+/-, and p((p) over bar) are studied at midrapidity (vertical bar y vertical bar < 0.1) for nine centrality intervals. The centrality, transverse momentum (p(T)), and pseudorapidity (eta) dependence of inclusive charged particle elliptic flow (v(2)), and rapidity-odd charged particles directed flow (v(1)) results near midrapidity are also presented. These measurements are compared with the published results from Au + Au collisions at other energies, and from Pb Pb collisions at root S-NN = 2.76 TeV. The results at root S-NN = 14.5 GeV show similar behavior as established at other energies and fit well in the energy dependence trend. These results are important as the 14.5-GeV energy fills the gap in mu(B), which is of the order of 100 MeV, between root S-NN = 11.5 and 19.6 GeV. Comparisons of the data with UrQMD and AMPT models show poor agreement in general. | |
| dc.identifier.citation | Bulk properties of the system formed in Au plus Au collisions at root S-NN=14.5 GeV at the BNL STAR detector / Adam, J [et al.] // Physical Review C. - 2020. - 101. - № 2. - 10.1103/PhysRevC.101.024905 | |
| dc.identifier.doi | 10.1103/PhysRevC.101.024905 | |
| dc.identifier.uri | https://www.doi.org/10.1103/PhysRevC.101.024905 | |
| dc.identifier.uri | https://www.scopus.com/record/display.uri?eid=2-s2.0-85082714606&origin=resultslist | |
| dc.identifier.uri | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000513213300003 | |
| dc.identifier.uri | https://openrepository.mephi.ru/handle/123456789/20345 | |
| dc.relation.ispartof | Physical Review C | |
| dc.title | Bulk properties of the system formed in Au plus Au collisions at root S-NN=14.5 GeV at the BNL STAR detector | |
| dc.type | Article | |
| dspace.entity.type | Publication | |
| oaire.citation.issue | 2 | |
| oaire.citation.volume | 101 | |
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