scholarly journals Relativistic mean-field models with scaled hadron masses and couplings: Hyperons and maximum neutron star mass

2016 ◽  
Vol 950 ◽  
pp. 64-109 ◽  
Author(s):  
K.A. Maslov ◽  
E.E. Kolomeitsev ◽  
D.N. Voskresensky
2010 ◽  
Vol 19 (08n10) ◽  
pp. 1575-1582
Author(s):  
L. FERRARI ◽  
P. C. R. ROSSI ◽  
M. MALHEIRO

In this paper we use a polytropic approximation to the equation of state for the interior of neutrons stars, described by relativistic hadronic mean field models. In this approximation, it is possible to obtain analytic expressions for the sound velocity and the incompressibility at the star center. We found a correlation between these quantities and the star mass. Using two well-known parametrizations of the nonlinear Walecka model for nuclear matter composed only of protons, neutrons and electron in β equilibrium, we obtain for a star mass of 1.43 M⊙ a central incompressibility Kc = (3000±100), around ten times the nuclear matter incompressibility, and a central sound velocity (v/c)2 ~ 0.3.


2021 ◽  
Vol 104 (6) ◽  
Author(s):  
W. Z. Shangguan ◽  
Z. Q. Huang ◽  
S. N. Wei ◽  
W. Z. Jiang

2017 ◽  
Vol 961 ◽  
pp. 106-141 ◽  
Author(s):  
E.E. Kolomeitsev ◽  
K.A. Maslov ◽  
D.N. Voskresensky

2015 ◽  
Vol 46 (5) ◽  
pp. 830-834 ◽  
Author(s):  
M. Oertel ◽  
C. Providencia ◽  
F. Gulminelli ◽  
A. R. Raduta

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