DC Field | Value | Language |
---|---|---|
dc.contributor.author | In-Gyu Koh | ko |
dc.date.accessioned | 2013-02-27T21:46:31Z | - |
dc.date.available | 2013-02-27T21:46:31Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 1996 | - |
dc.identifier.citation | PHYSICAL REVIEW D, v.53, no.4, pp.2236 - 2239 | - |
dc.identifier.issn | 0556-2821 | - |
dc.identifier.uri | http://hdl.handle.net/10203/71028 | - |
dc.description.abstract | We investigate a boson star with a self-interacting scalar field as a model of galactic halos. The model has slightly increasing rotation curves and allows wider ranges of the mass (m) and coupling (lambda) of the halo dark matter particle than the noninteracting model previously suggested. The two quantities are related by lambda(1/2)(m(p)/m)(2) greater than or similar to 10(50). | - |
dc.language | English | - |
dc.publisher | AMERICAN PHYSICAL SOC | - |
dc.subject | STELLAR CONFIGURATIONS | - |
dc.subject | SOLITON STARS | - |
dc.subject | FERMION STARS | - |
dc.subject | STABILITY | - |
dc.subject | EVOLUTION | - |
dc.subject | MATTER | - |
dc.title | Galactic halos as boson stars | - |
dc.type | Article | - |
dc.identifier.wosid | A1996TW98200051 | - |
dc.identifier.scopusid | 2-s2.0-0000728692 | - |
dc.type.rims | ART | - |
dc.citation.volume | 53 | - |
dc.citation.issue | 4 | - |
dc.citation.beginningpage | 2236 | - |
dc.citation.endingpage | 2239 | - |
dc.citation.publicationname | PHYSICAL REVIEW D | - |
dc.identifier.doi | 10.1103/PhysRevD.53.2236 | - |
dc.contributor.localauthor | In-Gyu Koh | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | STELLAR CONFIGURATIONS | - |
dc.subject.keywordPlus | SOLITON STARS | - |
dc.subject.keywordPlus | FERMION STARS | - |
dc.subject.keywordPlus | STABILITY | - |
dc.subject.keywordPlus | EVOLUTION | - |
dc.subject.keywordPlus | MATTER | - |
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