Towards a new quark-nuclear matter EoS for applications in astrophysics and heavy-ion collisions
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...
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| Veröffentlicht in: | Journal of physics. Conference series 2016-01, Vol.668 (1), p.12042 |
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| creator | Bastian, Niels-Uwe Blaschke, David |
| 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. We discuss the limitations of a 2-phase description and outline steps beyond it, towards the formulation of a unified quark-nuclear matter EoS on a more fundamental level by a cluster virial expansion. |
| doi_str_mv | 10.1088/1742-6596/668/1/012042 |
| format | Article |
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| subjects | Astrophysics Equations of state Explosions Heavy ions Ionic collisions Neutron stars Neutrons Nuclear matter Physics Quarks |
| title | Towards a new quark-nuclear matter EoS for applications in astrophysics and heavy-ion collisions |
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