The equation of state for cold nuclear matter as seen in nucleus-nucleus scattering

1998 ◽  
Vol 111 (8-9) ◽  
pp. 971-975 ◽  
Author(s):  
F. Nuoffer ◽  
G. Bartnitzky ◽  
H. Clement ◽  
A. Blazevic ◽  
H. G. Bohlen ◽  
...  
Keyword(s):  
Equation Of State ◽  
Nuclear Matter ◽  
Cold Nuclear Matter ◽  
Nucleus Scattering

scholarly journals Holographic cold nuclear matter and neutron star

2014 ◽  
Vol 29 (10) ◽  
pp. 1450060 ◽  
Author(s):  
Kazuo Ghoroku ◽  
Kouki Kubo ◽  
Motoi Tachibana ◽  
Fumihiko Toyoda
Keyword(s):  
Gauge Theory ◽  
Neutron Star ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Fermi Momentum ◽  
The Other ◽  
Holographic Model ◽  
Cold Nuclear Matter ◽  
Theoretical Approaches ◽  
New Phase

We have previously found a new phase of cold nuclear matter based on a holographic gauge theory, where baryons are introduced as instanton gas in the probe [Formula: see text] branes. In our model, we could obtain the equation of state (EOS) of our nuclear matter by introducing Fermi momentum. Then, here we apply this model to the neutron star and study its mass and radius by solving the Tolman–Oppenheimer–Volkoff (TOV) equations in terms of the EOS given here. We give some comments for our holographic model from a viewpoint of the other field theoretical approaches.

Equation of State for Cold Nuclear Matter from RefractiveO16+O16Elastic Scattering

1995 ◽  
Vol 74 (1) ◽  
pp. 34-37 ◽  
Author(s):  
Dao T. Khoa ◽  
W. von Oertzen ◽  
H. G. Bohlen ◽  
G. Bartnitzky ◽  
H. Clement ◽  
...  
Keyword(s):  
Equation Of State ◽  
Nuclear Matter ◽  
Cold Nuclear Matter

Onset Transition to Cold Nuclear Matter from Lattice QCD with Heavy Quarks

2014 ◽  
Author(s):  
Mathias Neuman ◽  
Jens Langelage ◽  
Owe Philipsen
Keyword(s):  
Nuclear Matter ◽  
Lattice Qcd ◽  
Heavy Quarks ◽  
Cold Nuclear Matter

EQUATION OF STATE OF ASYMMETRIC NUCLEAR MATTER WITH GOGNY AND COULOMB INTERACTIONS

1990 ◽  
Vol 05 (14) ◽  
pp. 1071-1080 ◽  
Author(s):  
S. W. HUANG ◽  
M. Z. FU ◽  
S. S. WU ◽  
S. D. YANG
Keyword(s):  
Equation Of State ◽  
Nuclear Matter ◽  
Coulomb Interaction ◽  
Chemical Potential ◽  
Compression Modulus ◽  
Nucleon Nucleon ◽  
Effective Density ◽  
Coulomb Interactions ◽  
Asymmetric Nuclear Matter ◽  
Nucleon Nucleon Interaction

The equation of state of the asymmetric nuclear matter is calculated with the Gogny D1 effective density-dependent nucleon-nucleon interaction and the Coulomb interaction in the framework of the finite-temperature HF method with the rearrangement term. The dependence of the thermodynamical properties such as the critical temperature of the liquid-gas phase transition, the chemical potential, the compression modulus and the entropy on the Coulomb interaction in nuclear matter is treated by using a shielded two-body Coulomb potential and this method has been found to be a reasonable and effective approach.

scholarly journals Constraining the equation of state of dense nuclear matter using thermal emission of neutron stars

2020 ◽  
Vol 1667 ◽  
pp. 012001
Author(s):  
Nicolas Baillot d’Étivaux ◽  
Jérôme Margueron ◽  
Sebastien Guillot ◽  
Natalie Webb ◽  
Màrcio Catelan ◽  
...  
Keyword(s):  
Equation Of State ◽  
Neutron Stars ◽  
Nuclear Matter ◽  
Thermal Emission ◽  
Dense Nuclear Matter
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