Asymmetric Nuclear Matter with Pion Dressing
Nuclear Theory
2007-12-03 v1
Abstract
We discuss a self-consistent method to calculate the properties of cold asymmetric nuclear matter which is dressed with isoscalar scalar pion condensates. The nucleon-nucleon interaction is mediated by these pion pairs, omega- and rho- mesons. The parameters of these interactions are evaluated self-consistently using the saturation properties of nuclear matter like binding energy, pressure, compressibility and symmetry energy. The computed equation of state of pure neutron matter (PNM) is used to calculate mass and radius of a pure neutron star.
Cite
@article{arxiv.0711.4874,
title = {Asymmetric Nuclear Matter with Pion Dressing},
author = {S. Sarangi and P. K. Panda and S. K. Sahu and L. Maharana},
journal= {arXiv preprint arXiv:0711.4874},
year = {2007}
}
Comments
12 pages, 9 figures, 1 table