scholarly journals Variational theory of hot nucleon matter. II. Spin-isospin correlations and equation of state of nuclear and neutron matter

2009 ◽  
Vol 79 (4) ◽  
Author(s):  
Abhishek Mukherjee
Keyword(s):  
Equation Of State ◽  
Neutron Matter ◽  
Variational Theory ◽  
Nucleon Matter

Ferromagnetism in neutron matter and its implication for the neutron star equation of state

2011 ◽  
Author(s):  
J. P. W. Diener ◽  
F. G. Scholtz ◽  
Ersin Göğüş ◽  
Ünal Ertan ◽  
Tomaso Belloni
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Neutron Matter

Equation of state for neutron matter

2005 ◽  
Vol 747 (2-4) ◽  
pp. 655-665 ◽  
Author(s):  
Kh. Gad
Keyword(s):  
Equation Of State ◽  
Neutron Matter

Equation of state for pion-condensed neutron matter at finite temperature

1978 ◽  
Vol 78 (5) ◽  
pp. 547-551 ◽  
Author(s):  
H. Toki ◽  
Y. Futami ◽  
W. Weise
Keyword(s):  
Equation Of State ◽  
Finite Temperature ◽  
Neutron Matter

The equation of state for neutron matter

1970 ◽  
Vol 234 (5) ◽  
pp. 479-492 ◽  
Author(s):  
S. Kistler ◽  
P. Mittelstaedt ◽  
W. Weyer
Keyword(s):  
Equation Of State ◽  
Neutron Matter

scholarly journals Variational theory of hot nucleon matter

2007 ◽  
Vol 75 (3) ◽  
Author(s):  
Abhishek Mukherjee ◽  
V. R. Pandharipande
Keyword(s):  
Variational Theory ◽  
Nucleon Matter

Equation of State and Electrical Conductivity of Dense Fluid Hydrogen and Helium

2003 ◽  
Vol 217 (7) ◽  
pp. 783-794 ◽  
Author(s):  
Ronald Redmer ◽  
H. Juranek ◽  
S. Kuhlbrodt ◽  
V. Schwarz
Keyword(s):  
Electrical Conductivity ◽  
Equation Of State ◽  
Linear Response ◽  
Theoretical Work ◽  
Linear Response Theory ◽  
Giant Planets ◽  
Variational Theory ◽  
Response Theory ◽  
Dense Fluid ◽  
Theory Comparison

AbstractThe equation of state of fluid hydrogen, helium, and their mixtures is determined within fluid variational theory. Reactions between the constituents such as dissociation and ionization are considered. Results are given for densities and temperatures relevant for the interior of giant planets. Furthermore, the electrical conductivity is determined within linear response theory. Comparison is performed with available experiments and other theoretical work.

TOWARD A NEW PARAMETERIZATION OF THE GOGNY FORCE: NEUTRON MATTER AND NUCLEAR BINDING ENERGIES

2006 ◽  
Vol 15 (02) ◽  
pp. 339-345 ◽  
Author(s):  
F. CHAPPERT ◽  
M. GIROD
Keyword(s):  
Equation Of State ◽  
Nuclear Matter ◽  
Variational Calculation ◽  
Binding Energies ◽  
Neutron Matter ◽  
Saturation Point ◽  
Nuclear Binding

A new parameterization of the effective Gogny interaction is investigated. It has the property of fitting the neutron matter Equation Of State (EOS) as predicted by a variational calculation. Its properties in nuclear matter (saturation point, compressibility, …) and in nuclei (binding energies) are presented.

EQUATION OF STATE OF HOT NUCLEAR AND NEUTRON MATTER: A STATISTICAL APPROACH

2006 ◽  
Vol 15 (05) ◽  
pp. 1127-1139 ◽  
Author(s):  
H. R. MOSHFEGH
Keyword(s):  
Equation Of State ◽  
Nucleon Nucleon ◽  
Neutron Matter ◽  
Effect Of Temperature ◽  
Variational Parameter ◽  
Experimental Prediction ◽  
Matter System ◽  
Nucleon Nucleon Interaction ◽  
Theoretical Results ◽  
Good Agreement

The symmetric nuclear and neutron matter equation of state at finite temperature are calculated in the frame of the Thomas-Fermi approximation using the effective nucleon-nucleon interaction of Myers and Swiatecki. By introducing an effective mass in distribution function as a variational parameter, the effect of temperature on pressure, entropy, specific heat capacity, incompressibility and binding energy is discussed. A critical temperature of 17.2 MeV and a critical exponent of 0.32 for symmetric nuclear matter is found and we find that there is no phase transition in the neutron matter system. The results of calculations are in good agreement with experimental prediction and other theoretical results.

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