A Relativistic Mean Field Theory for Nuclear Matter with σ,δ Meson Couplings at T ≠ 0

2004 ◽  
Author(s):  
Bardo E. J. Bodmann
1997 ◽  
Vol 391 (3-4) ◽  
pp. 255-260 ◽  
Author(s):  
Amand Faessler ◽  
A.J. Buchmann ◽  
M.I. Krivoruchenko ◽  
B.V. Martemyanov

2003 ◽  
Vol 12 (01) ◽  
pp. 125-133
Author(s):  
S. HADDAD

Nuclear matter incompressibility is calculated in the framework of the relativistic mean field theory. Asymmetry reduces the incompressibility. The isothermal incompressibility decreases with increasing temperature, and the isentropic one decreases with increasing entropy. Attention is given to the incompressibility at supernova collapse conditions.


2007 ◽  
Vol 16 (02n03) ◽  
pp. 297-302 ◽  
Author(s):  
TOMAZ PASSAMANI ◽  
MARIA LUIZA CESCATO

The nuclear matter density at finite temperature was evaluated analytically in the relativistic mean field theory using Sommerfeld approximation at low temperature. These analytical results are interesting since they allow a more transparent analysis of the contributions of the involved parameters.


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