# Compact stars in the QCD phase diagram VI <br><small><small>(Cosmic matter in heavy-ion collision laboratories?)</small></small>

26-29 September 2017
DUBNA
Europe/Moscow timezone

## Towards a unified quark-hadron equation of state for neutron stars, supernovae and heavy-ion collisions

26 Sep 2017, 10:30
25m
Blokhintsev Hall (4rd floor, BLTP) (DUBNA)

DUBNA RUSSIA

### Speaker

Mr 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.

 Slides