348516 20260319130055.0 10.3390/universe9100433 doi Sinyukov:2023jjn INSPIRETeX inspire:2705664 inspire arXiv:2310.16233 arXiv 10.15120/GSI-2024-00340 datacite_doi altmetric:155766048 altmetric WOS:001093538300001 WOS GSI-2024-00340 English 530 arXiv:2310.16233 arXiv Sinyukov, Yu. M. P:(DE-HGF)0 0 Space–Time Structure of Particle Emission and Femtoscopy Scales in Ultrarelativistic Heavy-Ion Collisions Basel 2023 MDPI article DRIVER Output Types/Journal article DataCite Journal Article journal journal PUB:(DE-HGF)16 1706745384_2344681 PUB:(DE-HGF) ARTICLE BibTeX JOURNAL_ARTICLE ORCID Journal Article 0 EndNote 28 pages, 9 figures. 'Author edition' of the recently published articleThe research was carried out within the NAS of the Ukraine Targeted Research Program “Collaboration in advanced international projects on high-energy physics and nuclear physics”, Agreement No. 7/2023 between the NAS of Ukraine and BITP of the NAS of Ukraine. The work was also supported by a grant from the Simons Foundation (Grant Number 1039151, Y.S., V.S., and M.A.). The author Yu.S. is supported by the Excellence Initiative Research University grant of the Warsaw University of Technology.Y.S. is also grateful to the ExtreMe Matter Institute (EMMI) at GSI in Darmstadt, where he was affiliated at the beginning of the work on the current paper, and to Hanna Zbroszczyk for her invitation to continue these studies in Warsaw University of Technology (WUT) as the Visiting Professor. "This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/)." The analysis of the spatiotemporal picture of particle radiation in relativistic heavy-ion collisions in terms of correlation femtoscopy scales, emission, and source functions allows one to probe the character of the evolution of the system created in the collision. Realistic models, such as the integrated hydrokinetic model (iHKM), used in the present work, are able to simulate the entire evolution process of strongly interacting matter produced in high-energy nuclear collisions. The mentioned model describes all the stages of the system’s evolution, including thermalisation and hydrodynamisation, which can help researchers figure out the specific details of the process and better understand the formation mechanisms of certain observables. In the current paper, we investigated the behaviour of the pion and kaon interferometry radii and their connection with emission functions in ultrarelativistic heavy-ion collisions at the Large Hadron Collider within iHKM. We focused on the study of the emission time scales at different energies for both particle species (pions and kaons) aiming to gain deeper insight into relation of these scales and the peculiarities of the mentioned system’s collective expansion and decay with the experimentally observed femtoscopy radii. One of our main interests was the problem of the total system’s lifetime estimation based on the femtoscopy analysis. 612 - Cosmic Matter in the Laboratory (POF4-612) G:(DE-HGF)POF4-612 POF4-612 POF IV 0 Dataset connected to CrossRef, INSPIRE, Journals: repository.gsi.de heavy ion: scattering INSPIRE matter: interaction INSPIRE space-time INSPIRE collective INSPIRE interferometer INSPIRE interpretation of experiments: CERN LHC Coll INSPIRE formation INSPIRE correlation INSPIRE lifetime INSPIRE nucleus INSPIRE structure INSPIRE numerical calculations INSPIRE kaon autogen pion autogen femtoscopy radius autogen emission function autogen emission time autogen particlisation autogen theory no experiment theory work (theory) EXP:(DE-Ds200)theory-20200803 EXP:(DE-Ds200)no_experiment-20200803 EXP:(DE-Ds200)no_experiment-20200803 0 Shapoval, Volodymyr P:(DE-HGF)0 1 Adzhymambetov, Musfer 0000-0001-7311-7830 2 Corresponding author 10.3390/universe9100433 Vol. 9, no. 10, p. 433 - PERI:(DE-600)2813994-X 10 433 - Universe 9 2023 2218-1997 http://repository.gsi.de/record/348516/files/universe-09-00433.pdf OpenAccess http://repository.gsi.de/record/348516/files/universe-09-00433.pdf?subformat=pdfa pdfa OpenAccess oai:repository.gsi.de:348516 openaire open_access VDB driver dnbdelivery DE-HGF Forschungsbereich Materie Matter and the Universe G:(DE-HGF)POF4-610 G:(DE-HGF)POF4-612 G:(DE-HGF)POF4 G:(DE-HGF)POF4-600 G:(DE-HGF)POF Cosmic Matter in the Laboratory 0 2023 OpenAccess StatID:(DE-HGF)0510 StatID Creative Commons Attribution CC BY 4.0 LIC:(DE-HGF)CCBY4 HGFVOC JCR StatID:(DE-HGF)0100 StatID UNIVERSE-BASEL : 2022 2023-10-26 DBCoverage StatID:(DE-HGF)0200 StatID SCOPUS 2023-10-26 DBCoverage StatID:(DE-HGF)0501 StatID DOAJ Seal 2023-04-12T15:03:23Z DBCoverage StatID:(DE-HGF)0500 StatID DOAJ 2023-04-12T15:03:23Z Peer Review StatID:(DE-HGF)0030 StatID DOAJ : Anonymous peer review 2023-04-12T15:03:23Z DBCoverage StatID:(DE-HGF)0600 StatID Ebsco Academic Search 2023-10-26 Peer Review StatID:(DE-HGF)0030 StatID ASC 2023-10-26 DBCoverage StatID:(DE-HGF)0199 StatID Clarivate Analytics Master Journal List 2023-10-26 DBCoverage StatID:(DE-HGF)0150 StatID Web of Science Core Collection 2023-10-26 DBCoverage StatID:(DE-HGF)1150 StatID Current Contents - Physical, Chemical and Earth Sciences 2023-10-26 IF < 5 StatID:(DE-HGF)9900 StatID 2023-10-26 yes I:(DE-Ds200)EXM-20080818OR100 EXM ExtreMe Matter Institute, EMMI 0 journal VDB I:(DE-Ds200)EXM-20080818OR100 UNRESTRICTED FullTexts