Elastic nucleon-nucleon cross section in nuclear matter at finite temperature

1998 ◽  
Vol 57 (2) ◽  
pp. 806-810 ◽  
Author(s):  
A. Schnell ◽  
G. Röpke ◽  
U. Lombardo ◽  
H.-J. Schulze
Keyword(s):  
Nuclear Matter ◽  
Cross Section ◽  
Finite Temperature ◽  
Nucleon Nucleon

The nucleon-nucleon cross section in ground-state and colliding nuclear matter

1996 ◽  
Vol 601 (3-4) ◽  
pp. 505-525 ◽  
Author(s):  
C. Fuchs ◽  
L. Sehn ◽  
H.H. Wolter
Keyword(s):  
Nuclear Matter ◽  
Cross Section ◽  
Ground State ◽  
Nucleon Nucleon

CRITICAL NEUTRON-PROTON ASYMMETRY OF HOT NUCLEAR MATTER

1986 ◽  
Vol 01 (02) ◽  
pp. 71-80 ◽  
Author(s):  
R.K. SU ◽  
S.D. YANG ◽  
G.L. LI ◽  
T.T.S. KUO
Keyword(s):  
Nuclear Matter ◽  
Finite Temperature ◽  
Mean Field ◽  
Nucleon Nucleon ◽  
Nucleon Interaction ◽  
Effective Interactions ◽  
Normal Pair ◽  
Nucleon Nucleon Interaction ◽  
Density Equation ◽  
Temperature Green’S Function

We derive an equation of state for asymmetric nuclear matter at finite temperature, using the Skyrme effective nucleon-nucleon interaction and a mean field approach based on a real-time finite temperature Green’s function method with a normal pair cutoff approximation. With the temperature held constant, it is found that nuclear matter can exist only in the gaseous phase when its neutron excess coefficient a has surpassed a certain critical value αc. We have calculated αc for a number of different Skyrme effective interactions. Phase diagrams involving a are obtained, and a low-density equation for the phase boundary is derived.

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.

VMC CALCULATIONS OF THE GROUND STATE PROPERTIES OF NUCLEAR MATTER

2005 ◽  
Vol 14 (02) ◽  
pp. 255-267 ◽  
Author(s):  
KAAN MANİSA ◽  
ÜLFET ATAV ◽  
RIZA OGUL
Keyword(s):  
Nuclear Matter ◽  
Ground State ◽  
Nucleon Nucleon ◽  
Neutron Matter ◽  
Potential Term ◽  
Ground State Properties ◽  
Dependent Potential ◽  
Variational Monte Carlo Method ◽  
Kinetic And Potential Energies ◽  
Good Agreement

A Variational Monte Carlo method (VMC) is described for the evaluation of the ground state properties of nuclear matter. Equilibrium properties of symmetric nuclear matter and neutron matter are calculated by the described VMC method. The Urbana ν14 potential is used for the nucleon–nucleon interactions in the calculations. Three- and more-body interactions are included as a density dependent potential term. Total, kinetic and potential energies per particle are obtained for nuclear and neutron matter. Pressure values of nuclear and neutron matter are also calculated at various densities. The binding energy of nuclear matter is found to be -16.06 MeV at a saturation density of 0.16 fm -3. The results obtained are in good agreement with those obtained by various authors with different potentials and techniques.

scholarly journals Open-charm mesons in nuclear matter at finite temperature beyond the zero-range approximation

2011 ◽  
Vol 84 (1) ◽  
Author(s):  
C. E. Jiménez-Tejero ◽  
A. Ramos ◽  
L. Tolós ◽  
I. Vidaña
Keyword(s):  
Nuclear Matter ◽  
Finite Temperature ◽  
Open Charm ◽  
Charm Mesons ◽  
Zero Range
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