001     363838
005     20260223232528.0
024 7 _ |a 10.1140/epjs/s11734-025-02088-8
|2 doi
024 7 _ |a 1951-6355
|2 ISSN
024 7 _ |a 1951-6401
|2 ISSN
024 7 _ |a 10.15120/GSI-2026-00048
|2 datacite_doi
024 7 _ |a arXiv:2509.09061
|2 arXiv
024 7 _ |a WOS:001634589300001
|2 WOS
037 _ _ |a GSI-2026-00048
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2509.09061
|2 arXiv
100 1 _ |a Bratkovskaya, Elena
|0 P:(DE-Ds200)OR7813
|b 0
|e Corresponding author
|u gsi
245 _ _ |a Study on the equation-of-state with light clusters and hypernuclei
260 _ _ |a Heidelberg
|c 2025
|b Springer
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1769175533_4016835
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a This article is licensed under a Creative Commons Attribution 4.0 International License
520 _ _ |a Heavy-ion collision experiments offer a unique opportunity to explore the early stages of the Universe by creating matter under extreme conditions of high temperature and baryon density. The properties of such matter are governed by the equation-of-state (EoS), which remains a central focus of investigation from both experimental and theoretical perspectives. Flow harmonics are among the most sensitive observables for probing the EoS, as they strongly reflect the underlying interactions and degrees of freedom of the system. In this article, we review the current status of our understanding of the EoS based on microscopic transport models, emphasizing comparisons with experimental data in the few GeV energy range.
536 _ _ |a 612 - Cosmic Matter in the Laboratory (POF4-612)
|0 G:(DE-HGF)POF4-612
|c POF4-612
|f POF IV
|x 0
536 _ _ |a Physics of hot and dense matter - Theory (HFHF project) (I:(DE-Ds200)HFHF-HI-Th)
|0 I:(DE-Ds200)HFHF-HI-Th
|c I:(DE-Ds200)HFHF-HI-Th
|x 1
588 _ _ |a Dataset connected to CrossRef, Journals: repository.gsi.de
693 _ _ |a theory
|e no experiment theory work (theory)
|1 EXP:(DE-Ds200)theory-20200803
|0 EXP:(DE-Ds200)no_experiment-20200803
|5 EXP:(DE-Ds200)no_experiment-20200803
|x 0
700 1 _ |a Aichelin, Jörg
|b 1
773 _ _ |a 10.1140/epjs/s11734-025-02088-8
|0 PERI:(DE-600)2267176-6
|p 1
|t European physical journal special topics
|v Spec. Top.
|y 2025
|x 1951-6355
856 4 _ |u https://repository.gsi.de/record/363838/files/s11734-025-02088-8.pdf
|y OpenAccess
856 4 _ |u https://repository.gsi.de/record/363838/files/s11734-025-02088-8.pdf?subformat=pdfa
|x pdfa
|y OpenAccess
909 C O |o oai:repository.gsi.de:363838
|p openaire
|p open_access
|p OpenAPC_DEAL
|p driver
|p VDB
|p openCost
|p dnbdelivery
910 1 _ |a GSI Helmholtzzentrum für Schwerionenforschung GmbH
|0 I:(DE-Ds200)20121206GSI
|k GSI
|b 0
|6 P:(DE-Ds200)OR7813
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-612
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Cosmic Matter in the Laboratory
|x 0
914 1 _ |y 2025
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2024-12-12
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0300
|2 StatID
|b Medline
|d 2024-12-12
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0600
|2 StatID
|b Ebsco Academic Search
|d 2024-12-12
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2024-12-12
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2024-12-12
915 _ _ |a DEAL Springer
|0 StatID:(DE-HGF)3002
|2 StatID
|d 2024-12-12
|w ger
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2024-12-12
915 _ _ |a IF < 5
|0 StatID:(DE-HGF)9900
|2 StatID
|d 2024-12-12
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b ASC
|d 2024-12-12
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b EUR PHYS J-SPEC TOP : 2022
|d 2024-12-12
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2024-12-12
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2024-12-12
915 p c |a APC keys set
|2 APC
|0 PC:(DE-HGF)0000
915 p c |a Local Funding
|2 APC
|0 PC:(DE-HGF)0001
915 p c |a DFG OA Publikationskosten
|2 APC
|0 PC:(DE-HGF)0002
915 p c |a DEAL: Springer Nature 01.01.2024
|2 APC
|0 PC:(DE-HGF)0178
920 _ _ |l yes
920 1 _ |0 I:(DE-Ds200)TES-20160901OR397
|k TES
|l Heiße & Dichte QCD Materie
|x 0
920 1 _ |0 I:(DE-Ds200)FHF-20200605OR451
|k FHF
|l Helmholtz ForschAkad Hess. f. FAIR, HFHF
|x 1
980 1 _ |a FullTexts
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a I:(DE-Ds200)TES-20160901OR397
980 _ _ |a I:(DE-Ds200)FHF-20200605OR451
980 _ _ |a UNRESTRICTED
980 _ _ |a APC


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21