Publication: Equilibration and baryon densities attainable in relativistic heavy-ion collisions
| dc.contributor.author | Ivanov, Y. B. | |
| dc.contributor.author | Soldatov, A. A. | |
| dc.contributor.author | Солдатов, Алексей Анатольевич | |
| dc.date.accessioned | 2024-11-25T16:49:55Z | |
| dc.date.available | 2024-11-25T16:49:55Z | |
| dc.date.issued | 2020 | |
| dc.description.abstract | Kinetic equilibration of the matter and baryon densities attained in the central region of colliding Au+Au nuclei in the energy range of root s(NN) = 3.3-39 GeV are examined within the model of three-fluid dynamics. It is found that the kinetic equilibration is faster at higher collision energies: the equilibration time (in the center-of-mass frame of colliding nuclei) rises from approximate to 5 fm/c at root s(NN) = 3.3 GeV to approximate to 1 fm/c at 39 GeV. The chemical equilibration, and thus thermalization, takes longer. We argue that the presented time evolution of the net-baryon and energy densities in the central region is a necessary prerequisite of proper reproduction of bulk observables in midrapidity. We suggest that for informative comparison of predictions of different models it is useful to calculate an invariant four-volume (V-4), where the proper density of the equilibrated matter exceeds a certain value. The advantage of this four-volume is that it does not depend on specific choice of the three-volume in different studies and takes into account the lifetime of the high-density region, which also matters. The four-volume V-4 = 100 fm(4)/c is chosen to compare the baryon densities attainable at different energies. It is found that the highest proper baryon density increases with the collision energy rise, from n(B)/n(0) approximate to 4 at 3.3 GeV to n(B)/n(0) approximate to 30 at 39 GeV. These highest densities are achieved in the central region of the colliding system. | |
| dc.identifier.citation | Ivanov, Y. B. Equilibration and baryon densities attainable in relativistic heavy-ion collisions / Ivanov, YB, Soldatov, AA // Physical Review C. - 2020. - 101. - № 2. - 10.1103/PhysRevC.101.024915 | |
| dc.identifier.doi | 10.1103/PhysRevC.101.024915 | |
| dc.identifier.uri | https://www.doi.org/10.1103/PhysRevC.101.024915 | |
| dc.identifier.uri | https://www.scopus.com/record/display.uri?eid=2-s2.0-85082751013&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:000517222700005 | |
| dc.identifier.uri | https://openrepository.mephi.ru/handle/123456789/20371 | |
| dc.relation.ispartof | Physical Review C | |
| dc.title | Equilibration and baryon densities attainable in relativistic heavy-ion collisions | |
| dc.type | Article | |
| dspace.entity.type | Publication | |
| oaire.citation.issue | 2 | |
| oaire.citation.volume | 101 | |
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