Thermal properties of nuclear matter in a variational framework with relativistic corrections

2014 ◽  
Vol 89 (1) ◽  
Author(s):  
S. Zaryouni ◽  
M. Hassani ◽  
H. R. Moshfegh
Keyword(s):  
Thermal Properties ◽  
Nuclear Matter ◽  
Relativistic Corrections ◽  
Variational Framework

Thermal properties of nuclear matter with a momentum-dependent effective interaction

1993 ◽  
Vol 47 (4) ◽  
pp. 1519-1528 ◽  
Author(s):  
V. K. Mishra ◽  
G. Fai ◽  
L. P. Csernai ◽  
E. Osnes
Keyword(s):  
Thermal Properties ◽  
Nuclear Matter ◽  
Effective Interaction

EFFECTS OF THE ω MESON SELF COUPLING ON THE THERMAL PROPERTIES OF ASYMMETRIC NUCLEAR MATTER

2009 ◽  
Vol 24 (11n13) ◽  
pp. 1067-1070
Author(s):  
S. WIBOWO ◽  
A. SULAKSONO
Keyword(s):  
Phase Transition ◽  
Thermal Properties ◽  
Nuclear Matter ◽  
Gas Phase ◽  
Mean Field ◽  
Binodal Curve ◽  
Asymmetric Nuclear Matter ◽  
Relativistic Mean Field ◽  
Chemical Instabilities ◽  
Rmf Model

Effects of the ω meson self coupling (OMSC) on the thermal properties of asymmetric nuclear matter (ANM) are studied within the framework of relativistic mean field (RMF) model that includes contributions of all possible mixed interactions among meson fields involved up to quartic order. In particular, we study the mechanical and chemical instabilities (spinodal), as well as the liquid-gas phase transition (binodal) at finite temperature. It is found that the onset of spinodal instabilities and the binodal curve are only marginally affected by variation of the OMSC parameter, whereas the binodal curve shows a strong correlation to the symmetry energy. Comparison with other ERMF parameter sets is also performed.

Microscopic study of thermal properties of the nuclear matter formed in heavy-ion collisions

1992 ◽  
Vol 542 (4) ◽  
pp. 671-698 ◽  
Author(s):  
Dao T. Khoa ◽  
N. Ohtsuka ◽  
Amand Faessler ◽  
M.A. Matin ◽  
S.W. Huang ◽  
...  
Keyword(s):  
Thermal Properties ◽  
Nuclear Matter ◽  
Microscopic Study ◽  
Heavy Ion Collisions ◽  
Heavy Ion ◽  
Ion Collisions

RELATIVISTIC CORRECTIONS TO THE NUCLEAR AND NEUTRON MATTER ENERGY IN THE LOCV FRAMEWORK

2005 ◽  
Vol 14 (02) ◽  
pp. 297-314 ◽  
Author(s):  
S. ZARYOUNI ◽  
H. R. MOSHFEGH
Keyword(s):  
Equation Of State ◽  
Kinetic Energy ◽  
Nuclear Matter ◽  
Cluster Expansion ◽  
Binding Energies ◽  
Symmetric Nuclear Matter ◽  
Neutron Matter ◽  
Relativistic Corrections ◽  
Pure Neutron Matter ◽  
Matter Energy

We calculate the two-body relativistic boost interaction corrections as well as relativistic one-body and two-body kinetic energy corrections in cluster expansion of energy with AV18 and the new charge dependent Reid93 potentials within the lowest order constrained variational (LOCV) method. The equation of state of symmetric nuclear matter and pure neutron matter are calculated using the non-relativistic (H NR ), non-relativistic plus boost interaction corrections [Formula: see text] and [Formula: see text] plus kinetic energy corrections [Formula: see text] Hamiltonians. The relativistic boost interaction effects reduce the binding energies of symmetric nuclear matter for the AV18 interaction by ~3 MeV .

On the thermal properties of polarised nuclear matter

1980 ◽  
Vol 6 (10) ◽  
pp. 1229-1236 ◽  
Author(s):  
M Y M Hassan ◽  
S S Montasser ◽  
S Ramadan
Keyword(s):  
Thermal Properties ◽  
Nuclear Matter
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