Compatibility of Exotic States with Neutron Star Observation
Nuclear Theory
2008-11-26 v1
Abstract
We consider the effect of hard core repulsion in the baryon-baryon interaction at short distance to the properties of a neutron star. We obtain that, even with hyperons in the interior of a neutron star, the neutron star mass can be as large as .
Keywords
Cite
@article{arxiv.0704.0504,
title = {Compatibility of Exotic States with Neutron Star Observation},
author = {Chang Ho Hyun},
journal= {arXiv preprint arXiv:0704.0504},
year = {2008}
}
Comments
4 pages, 1 figure. A contribution to Yukawa International Seminar (YKIS) 2006, "New Frontiers in QCD", Kyoto, Japan, Nov. 20 - Dec. 8, 2006