Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures

Details Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures

1998-03-09

arxiv.org/abs/nucl-th/9803026v1

Phys.Rev.C57:3484-3487,1998

Physics

Nuclear Physics

Nuclear Theory

8 pages, 9 figures, submitted in a shorter version to Phys. Rev. C

Scientific paper

10.1103/PhysRevC.57.3484

The properties of hot matter are studied in the frame of the relativistic Brueckner-Hartree-Fock theory. The equations are solved self-consistently in the full Dirac space. For the interaction we used the potentials given by Brockmann and Machleidt. The obtained critical temperatures are smaller than in most of the nonrelativistic investigations. We also calculated the thermodynamic properties of hot matter in the relativistic Hartree--Fock approximation, where the force parameters were adjusted to the outcome of the relativistic Brueckner--Hartree--Fock calculations at zero temperature. Here, one obtains higher critical temperatures, which are comparable with other relativistic calculations in the Hartree scheme.

Affiliated with

Also associated with

No associations

Rating

Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-420331