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http://hdl.handle.net/2248/4231
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sivaram, C | - |
dc.date.accessioned | 2009-01-02T11:17:18Z | - |
dc.date.available | 2009-01-02T11:17:18Z | - |
dc.date.issued | 1995 | - |
dc.identifier.citation | N. Iucci and E. Lamanna. ed., 24th International Cosmic Ray Conference, Vol. 2, held August 28 - September 8, 1995 in Rome, Italy. | en |
dc.identifier.uri | http://hdl.handle.net/2248/4231 | - |
dc.description.abstract | Two possible merger modes of gamma ray bursts are considered. The merger of two white dwarfs leading to a neutrino bursts accompanying the gamma ray burst. However the merger of two neutron stars should give rise to only a gamma ray burst with a much smaller neutrino flux. Observable signatures to discriminate between these pictures is clarified. | en |
dc.language.iso | en | en |
dc.publisher | International Union of Pure and Applied Physics | en |
dc.relation.ispartofseries | International Union of Pure and Applied Physics; | - |
dc.relation.uri | http://adsabs.harvard.edu/abs/1995ICRC....2..164S | en |
dc.title | Merger Models of Gamma-Ray Bursts: A Comparison | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Merger Models of Gamma-Ray Bursts | 113.58 kB | Adobe PDF | ![]() View/Open |
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