Compatibility of Exotic States with Neutron Star Observation

Details Compatibility of Exotic States with Neutron Star Observation Compatibility of Exotic States with Neutron Star Observation

2007-04-04

arxiv.org/abs/0704.0504v1

Prog.Theor.Phys.Suppl.168:627-630,2007

Physics

Nuclear Physics

Nuclear Theory

4 pages, 1 figure. A contribution to Yukawa International Seminar (YKIS) 2006, "New Frontiers in QCD", Kyoto, Japan, Nov. 20 -

Scientific paper

10.1143/PTPS.168.627

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 $\sim 2 M_\odot$.

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