Speaker
Niels-Uwe Bastian
(University of Wroclaw)
Description
The aim of our work is to develop a unified equation of state (EoS) for nuclear and quark matter for a wide range in temperature, density and isospin so that it becomes applicable for heavy-ion collisions as well as for the astrophysics of neutron stars, their mergers and supernova explosions. As a first step, we use improved EoS for the hadronic and quark matter phases and join them via Maxwell construction.
For this we work with a generalized density functional approach for the self energies in a quasi particle picture, which gives us the possibility to start with a reasonable physical basis and apply improvements to fit certain constraints from lattice QCD and neutron star measurements.
| List of tracks | QCD phase diagram (BES) |
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Primary author
Niels-Uwe Bastian
(University of Wroclaw)
Co-authors
David Blaschke
(University of Wroclaw)
Dr
Tobias Fischer
(Institute of Theoretical Physics, University of Wroclaw)
Mr
Mark Alexander Randolph Kaltenborn
(The George Washington University)
Dr
Stefan Typel
(GSI Helmholtzzentrum f¨ur Schwerionenforschung GmbH)
Peer reviewing
Paper
Paper files:
