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QCD at high density: Equation of state for nuclear collisions and neutron stars

  • A unified chiral mean field approach is presented for QCD thermodynamics in a wide range of temperatures and densities. The model simultaneously gives a satisfactory description of lattice QCD thermodynamics and fulfills nuclear matter and astrophysical constraints. The resulting equation of state can be incorporated in relativistic fluid-dynamical simulations of heavy-ion collisions and neutron stars mergers. Access to different regions of the QCD phase diagram can be obtained in simulations of heavy-ion data and observations of neutron star mergers.

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Metadaten
Author:Anton MotornenkoORCiDGND, Volodymyr VovchenkoORCiDGND, Jan SteinheimerORCiDGND, Stefan SchrammGND, Horst StöckerORCiDGND
URN:urn:nbn:de:hebis:30:3-775109
DOI:https://doi.org/10.1016/j.nuclphysa.2018.11.028
ISSN:0375-9474
Parent Title (English):Nuclear Physics A
Publisher:Elsevier
Place of publication:Amsterdam
Document Type:Article
Language:English
Date of Publication (online):2019/01/22
Date of first Publication:2019/01/22
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Contributing Corporation:International Conference on Ultrarelativistic Nucleus-Nucleus Collisions (27. : 2018 : Venedig)
Release Date:2023/10/06
Tag:QCD equation of state; neutron star properties; parity-doublet model
Volume:982
Page Number:4
First Page:891
Last Page:894
HeBIS-PPN:513174605
Institutes:Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - CC BY-NC-ND - Namensnennung - Nicht kommerziell - Keine Bearbeitungen 4.0 International