scholarly journals Analysis of critical parameters for nonrelativistic models of symmetric nuclear matter

2021 ◽  
Vol 103 (3) ◽  
Author(s):  
Mariana Dutra ◽  
Odilon Lourenço ◽  
Xavier Viñas ◽  
C. Mondal
Keyword(s):  
Nuclear Matter ◽  
Symmetric Nuclear Matter ◽  
Critical Parameters

EVAPORATION OF SYMMETRIC NUCLEAR MATTER IN WEAKLY CURVED SPACE

2006 ◽  
Vol 15 (03) ◽  
pp. 561-570
Author(s):  
A. V. NAZARENKO
Keyword(s):  
Phase Transition ◽  
Nuclear Matter ◽  
Gas Phase ◽  
Flat Space ◽  
Space Time ◽  
Symmetric Nuclear Matter ◽  
Critical Parameters ◽  
Conformally Flat ◽  
Curved Space ◽  
Walecka Model

Symmetric nuclear matter, described by the linear Walecka model, is considered in conformally flat space-time. The dependence of the critical parameters of liquid-gas phase transition on magnitude of the conformal step-like factor is investigated.

Hyperonic stars within the Bogoliubov quark meson model for nuclear matter

2019 ◽  
Vol 28 (05) ◽  
pp. 1950034
Author(s):  
Prafulla K. Panda ◽  
Constança Providência ◽  
Steven A. Moszkowski ◽  
Henrik Bohr ◽  
João da Providência
Keyword(s):  
Neutron Stars ◽  
Nuclear Matter ◽  
Quark Matter ◽  
Present Model ◽  
Massive Stars ◽  
Symmetric Nuclear Matter ◽  
The Core ◽  
Meson Coupling

We generalize the Bogoliubov quark-meson coupling (QMC) model to also include hyperons. The hyperon-[Formula: see text]-meson couplings are fixed by the model and the hyperon-[Formula: see text]-meson couplings are fitted to the hyperon potentials in symmetric nuclear matter. The present model predicts neutron stars with masses above 2[Formula: see text] and the radius of a 1.4[Formula: see text] star [Formula: see text]14[Formula: see text]km. In the most massive stars, bags overlap at the core of the star, and this may be interpreted as a transition to deconfined quark matter.

Pion condensation in symmetric nuclear matter

1991 ◽  
Vol 17 (6) ◽  
pp. 887-900 ◽  
Author(s):  
T Shamsunnahar ◽  
S Saha ◽  
K Kabir ◽  
L M Nath
Keyword(s):  
Nuclear Matter ◽  
Symmetric Nuclear Matter ◽  
Pion Condensation

scholarly journals Possible Structures of Pion Condensate in Symmetric Nuclear Matter

1980 ◽  
Vol 63 (5) ◽  
pp. 1665-1687 ◽  
Author(s):  
T. Matsui ◽  
T. Otofuji ◽  
K. Sakai ◽  
M. Yasuno
Keyword(s):  
Nuclear Matter ◽  
Symmetric Nuclear Matter ◽  
Pion Condensate

Finite temperature RPA in symmetric nuclear matter with Skyrme interactions

1996 ◽  
Vol 597 (1) ◽  
pp. 1-18 ◽  
Author(s):  
E.S. Hernández ◽  
J. Navarro ◽  
A. Polls ◽  
J. Ventura
Keyword(s):  
Nuclear Matter ◽  
Finite Temperature ◽  
Symmetric Nuclear Matter

DELTA MATTER FORMATION IN DENSE ASYMMETRIC NUCLEAR MEDIUM

2000 ◽  
Vol 15 (24) ◽  
pp. 1529-1537 ◽  
Author(s):  
J. C. T. DE OLIVEIRA ◽  
M. KYOTOKU ◽  
M. CHIAPPARINI ◽  
H. RODRIGUES ◽  
S. B. DUARTE
Keyword(s):  
Nuclear Matter ◽  
Mean Field Theory ◽  
Mean Field ◽  
Symmetric Nuclear Matter ◽  
Coupling Constants ◽  
Nuclear Medium ◽  
Delta Resonance ◽  
Relativistic Mean Field ◽  
Meson Coupling ◽  
Resonance Coupling

In the context of a relativistic mean field theory the delta-resonance matter formation in a highly compressed nuclear medium is investigated. For a given set of nucleon–meson coupling constants, the delta-resonance formation is studied by changing the delta-meson coupling constants. The effect on the equation of state and on the delta-resonance population with respect to changes in the delta-resonance coupling constants values is discussed for very asymmetric and quasi-symmetric nuclear matter, as an extension of works restricted to the symmetric nuclear matter treatment.5,6

Sign in / Sign up

Export Citation Format

Share Document