scholarly journals Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of state

2016 ◽  
Vol 94 (1) ◽  
Author(s):  
Helena Pais ◽  
Constança Providência
Particles ◽  
2020 ◽  
Vol 3 (3) ◽  
pp. 621-629
Author(s):  
Prasanta Char ◽  
Silvia Traversi ◽  
Giuseppe Pagliara

We present a Bayesian analysis on the equation of state of neutron stars based on a class of relativistic mean field models. The priors on the equation of state are related to the properties of nuclear matter at saturation and the posteriors are obtained through the Bayesian procedure by exploiting recent astrophysical constraints on the mass–radius relations of neutron stars. We find indications of a tension (within the adopted model) between the prior on the nuclear incompressibility and its posterior which in turn seems to suggest a possible phase transition at about twice saturation density to a phase where the nucleon effective mass is strongly reduced. A possible relation with the chiral phase transition in dense matter is also discussed.


2000 ◽  
Vol 671 (1-4) ◽  
pp. 447-460 ◽  
Author(s):  
R.J. Furnstahl ◽  
Brian D. Serot

1994 ◽  
Vol 337 (1-2) ◽  
pp. 19-24 ◽  
Author(s):  
Tomoyuki Maruyama ◽  
Hirotsugu Fujii ◽  
Takumi Muto ◽  
Toshitaka Tatsumi

Author(s):  
M. SERRA ◽  
T. OTSUKA ◽  
Y. AKAISHI ◽  
S. HIROSE ◽  
P. RING

2019 ◽  
Vol 99 (4) ◽  
Author(s):  
Odilon Lourenço ◽  
Mariana Dutra ◽  
César H. Lenzi ◽  
César V. Flores ◽  
Débora P. Menezes

Sign in / Sign up

Export Citation Format

Share Document