scholarly journals Asymmetric Nuclear Matter and Neutron Star Properties

1996 ◽  
Vol 469 ◽  
pp. 794 ◽  
Author(s):  
L. Engvik ◽  
E. Osnes ◽  
M. Hjorth-Jensen ◽  
G. Bao ◽  
E. Ostgaard
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Asymmetric Nuclear Matter

Neutron star properties and the relativistic equation of state of asymmetric nuclear matter

1994 ◽  
Vol 50 (3) ◽  
pp. R1287-R1291 ◽  
Author(s):  
H. Huber ◽  
F. Weber ◽  
M. K. Weigel
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Relativistic Equation ◽  
Asymmetric Nuclear Matter

scholarly journals Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star

2021 ◽  
Vol 57 (4) ◽  
Author(s):  
Ngo Hai Tan ◽  
Dao T. Khoa ◽  
Doan Thi Loan
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Asymmetric Nuclear Matter

scholarly journals QMC approach based on the Bogoliubov independent quark model of the nucleon

2016 ◽  
Vol 25 (02) ◽  
pp. 1650007 ◽  
Author(s):  
Henrik Bohr ◽  
Steven A. Moszkowski ◽  
Prafulla K. Panda ◽  
Constança Providência ◽  
João da Providência
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Quark Model ◽  
Effective Mass ◽  
Mass Formula ◽  
Saturation Density ◽  
Nucleon Mass ◽  
Asymmetric Nuclear Matter ◽  
Meson Coupling

The quark–meson coupling (QMC) model due to Guichon is formulated on the basis of the independent quark model of the nucleon proposed by Bogoliubov and is applied to the phenomenological descriptions of symmetric and asymmetric nuclear matter. For symmetric matter, the model predicts, at saturation density, the incompressibility [Formula: see text][Formula: see text]MeV, the quark effective mass [Formula: see text][Formula: see text]MeV and the effective nucleon mass [Formula: see text], where [Formula: see text] is the nucleon mass in vacuum. Neutron star masses above two solar masses are obtained.

scholarly journals Warm asymmetric nuclear matter and proto-neutron star structure

2004 ◽  
Vol 70 (4) ◽  
Author(s):  
Pravat Kumar Jena ◽  
Lambodar Prasad Singh
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Asymmetric Nuclear Matter ◽  
Proto Neutron Star ◽  
Star Structure

scholarly journals Asymmetric Nuclear Matter and Neutron Star Properties

1994 ◽  
Vol 73 (20) ◽  
pp. 2650-2653 ◽  
Author(s):  
L. Engvik ◽  
M. Hjorth-Jensen ◽  
E. Osnes ◽  
G. Bao ◽  
E. Østgaard
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Asymmetric Nuclear Matter

PARAMETRIC COUPLING MODEL: RECENT ADVANCES

2010 ◽  
Vol 19 (08n10) ◽  
pp. 1463-1468
Author(s):  
G. F. MARRANGHELLO ◽  
C. PROVIDÊNCIA ◽  
A. M. S. DOS SANTOS
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Coupling Model ◽  
Heavy Ion ◽  
Small Range ◽  
Heavy Ion Collision ◽  
Asymmetric Nuclear Matter ◽  
Parametric Coupling ◽  
Free Parameters ◽  
Ion Collision

We review the properties of the parametric coupling model and analyze its results when considering neutron star observations and heavy-ion collision experiments, specially those concerning the isospin characteristics of symmetric and asymmetric nuclear matter. By the end of the analysis, we are able to constrain the free parameters to a very small range of acceptable values.

Three-Body Force Effects on EOS of Asymmetric Nuclear Matter and Proton Fraction in Neutron Star Matter

2003 ◽  
Vol 39 (4) ◽  
pp. 439-446 ◽  
Author(s):  
Zuo Wei ◽  
A. Lejeune ◽  
U. Lombardo ◽  
J.f. Mathiot
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Body Force ◽  
Neutron Star Matter ◽  
Asymmetric Nuclear Matter ◽  
Three Body

Nucleon Superfluidity in Asymmetric Nuclear Matter and Neutron Star Matter

2010 ◽  
Author(s):  
Wei Zuo ◽  
U. Lombardo ◽  
Akira Ozawa ◽  
Weiping Lu
Keyword(s):  
Neutron Star ◽  
Nuclear Matter ◽  
Neutron Star Matter ◽  
Asymmetric Nuclear Matter ◽  
Nucleon Superfluidity
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