Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
We construct a set of equations of state (EoS) of dense and hot matter with a 1st order phase transition from a hadronic system to a deconfined quark matter state. In this two-phase approach, hadrons are described using the relativistic mean field theory with different parametrisations and the decon...
Guardat en:
| Autors principals: | , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2019-08-01
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| Col·lecció: | Universe |
| Matèries: | |
| Accés en línia: | https://www.mdpi.com/2218-1997/5/8/186 |
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