Compatibility of Exotic States with Neutron Star Observation
| dc.creator | Hyun, Chang Ho | |
| dc.date | 2007-04-04 | |
| dc.date.accessioned | 2026-07-07T11:40:56Z | |
| dc.date.available | 2026-07-07T11:40:56Z | |
| dc.description | 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 $\sim 2 M_\odot$. | |
| dc.description | 4 pages, 1 figure. A contribution to Yukawa International Seminar (YKIS) 2006, "New Frontiers in QCD", Kyoto, Japan, Nov. 20 - Dec. 8, 2006 | |
| dc.identifier | https://arxiv.org/abs/0704.0504 | |
| dc.identifier | http://arxiv.org/abs/0704.0504 | |
| dc.identifier | Prog.Theor.Phys.Suppl.168:627-630,2007 | |
| dc.identifier | doi:10.1143/PTPS.168.627 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/200367 | |
| dc.subject | Nuclear Theory | |
| dc.title | Compatibility of Exotic States with Neutron Star Observation | |
| dc.type | text |