Neutron stars within a relativistic mean field theory compatible with nucleon-nucleon short-range correlations

2019 ◽  
Vol 990 ◽  
pp. 118-136
Author(s):  
Zhen Li ◽  
Zhongzhou Ren ◽  
Bin Hong ◽  
Hao Lu ◽  
Dong Bai
Keyword(s):  
Field Theory ◽  
Neutron Stars ◽  
Short Range ◽  
Mean Field Theory ◽  
Mean Field ◽  
Nucleon Nucleon ◽  
Relativistic Mean Field Theory ◽  
Relativistic Mean Field ◽  
Short Range Correlations

FINITE TEMPERATURE EQUATIONS OF STATE FOR MIXED STARS

2004 ◽  
Vol 13 (07) ◽  
pp. 1249-1253
Author(s):  
DÉBORA P. MENEZES ◽  
C. PROVIDÊNCIA
Keyword(s):  
Field Theory ◽  
Neutron Stars ◽  
Quark Matter ◽  
Finite Temperature ◽  
Equations Of State ◽  
Mean Field Theory ◽  
Mean Field ◽  
Relativistic Mean Field Theory ◽  
Relativistic Mean Field

We investigate the properties of mixed stars formed by hadronic and quark matter in β-equilibrium described by appropriate equations of state (EOS) in the framework of relativistic mean-field theory. The calculations were performed for T=0 and for finite temperatures and also for fixed entropies with and without neutrino trapping in order to describe neutron and proto-neutron stars. The star properties are discussed. Maximum allowed masses for proto-neutron stars are much larger when neutrino trapping is imposed.

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