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dc.contributor.authorInghirami, Gabriele
dc.contributor.authorHillmann, Paula Christine
dc.contributor.authorTomášik, Boris
dc.contributor.authorBleicher, Marcus
dc.date.accessioned2019-11-08T14:16:28Z
dc.date.available2019-11-08T14:16:28Z
dc.date.issued2020
dc.identifier.citationInghirami, G., Hillmann, P. C., Tomášik, B., & Bleicher, M. (2020). Temperatures and chemical potentials at kinetic freeze-out in relativistic heavy ion collisions from coarse grained transport simulations. <i>Journal of Physics G: Nuclear and Particle Physics</i>, <i>47</i>(2), Article 025104. <a href="https://doi.org/10.1088/1361-6471/ab53f4" target="_blank">https://doi.org/10.1088/1361-6471/ab53f4</a>
dc.identifier.otherCONVID_33465781
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/66286
dc.description.abstractUsing the UrQMD/coarse graining approach we explore the kinetic freeze-out stage in central Au + Au collisions at various energies. These studies allow us to obtain detailed information on the thermodynamic properties (e.g. temperature and chemical potential) of the system during the kinetic decoupling stage. We explore five relevant collision energies in detail, ranging from √sNN=2.4 GeV (GSI-SIS) to √sNN=200 GeV (RHIC). By adopting a standard Hadron Resonance Gas equation of state, we determine the average temperature〈T〉and the average baryon chemical potential〈μB〉on the space-time hyper-surface of last interaction. The results highlight the nature of the kinetic freeze-out as a continuous process. This differential decoupling is an important aspect often missed when summarizing data as single points in the phase diagram as e.g. done in Blast-Wave fits. We compare the key properties of the system derived by using our approach with other models and we briefly review similarities and differences.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherInstitute of Physics
dc.relation.ispartofseriesJournal of Physics G: Nuclear and Particle Physics
dc.rightsCC BY-NC-ND 3.0
dc.titleTemperatures and chemical potentials at kinetic freeze-out in relativistic heavy ion collisions from coarse grained transport simulations
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201911084802
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineTeoreettinen fysiikkafi
dc.contributor.oppiaineTheoretic Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0954-3899
dc.relation.numberinseries2
dc.relation.volume47
dc.type.versionacceptedVersion
dc.rights.copyright© 2019 IOP Publishing Ltd.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.grantnumber297058
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by-nc-nd/3.0/
dc.relation.doi10.1088/1361-6471/ab53f4
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationG. Inghirami is supported by the Academy of Finland, Project no. 297058. P. Hillmann acknowledges support by the GSI in cooperation with the John von Neumann Institute for Computing; she also acknowledges support from the HGS-HIRe and FIGSS graduate schools. B. Tomasik acknowledges support by the grant No. 17-04505S from the Czech Science Foundation. The computational resources were provided by the Center for Scienti c Computing (CSC) of the Goethe University Frankfurt and by the Frankfurt Institute for Advanced Studies (FIAS). This work was supported by the COST Action CA15213 (THOR).
dc.type.okmA1


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