Asymmetric Nuclear Matter with Pion Dressing

2007/11/30 by S. Sarangi, Sarangi, S., P. K. Panda +5
Physics and Astronomy · #FOS: Physical sciences #Nuclear Theory (nucl-th) #nucl-th

paper · pdf · doi:10.48550/arxiv.0711.4874

12 pages, 9 figures, 1 table

arxiv created 2007/11/30 · arxiv updated 2009/12/01

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.

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