DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ikeda, M | ko |
dc.contributor.author | Takeda, A | ko |
dc.contributor.author | Fukuda, Y | ko |
dc.contributor.author | Vagins, M | ko |
dc.contributor.author | Yoo, Jonghee | ko |
dc.date.accessioned | 2016-07-25T09:44:11Z | - |
dc.date.available | 2016-07-25T09:44:11Z | - |
dc.date.created | 2016-07-21 | - |
dc.date.created | 2016-07-21 | - |
dc.date.issued | 2007-11 | - |
dc.identifier.citation | ASTROPHYSICAL JOURNAL, v.669, no.1, pp.519 - 524 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://hdl.handle.net/10203/212202 | - |
dc.description.abstract | We report the results of a search for neutrino bursts from supernova explosions using the Super-Kamiokande detector. Super-Kamiokande is sensitive to core-collapse supernova explosions via observation of their neutrino emissions. The expected number of events comprising such a burst is similar to 10(4), and the average energy of the neutrinos is in the range of a few tens of MeV for a core-collapse supernova explosion at a typical distance in our galaxy ( 10 kpc); this strong signal means that the detection efficiency anywhere within our galaxy and well past the Magellanic Clouds should be 100%. We examined a data set taken from 1996 May to 2001 July, and from 2002 December to 2005 October, corresponding to 2589.2 live days. However, there is no evidence of such a supernova explosion during the data-taking period. The 90% C. L. upper limit on the rate of core-collapse supernova explosions out to distances of 100 kpc is found to be 0.32 SN yr(-1). | - |
dc.language | English | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.subject | CORE-COLLAPSE SUPERNOVAE | - |
dc.subject | 23 FEBRUARY 1987 | - |
dc.subject | DETECTOR | - |
dc.subject | SIGNAL | - |
dc.title | Search for supernova neutrino bursts at super-kamiokande | - |
dc.type | Article | - |
dc.identifier.wosid | 000250480600039 | - |
dc.identifier.scopusid | 2-s2.0-39049152843 | - |
dc.type.rims | ART | - |
dc.citation.volume | 669 | - |
dc.citation.issue | 1 | - |
dc.citation.beginningpage | 519 | - |
dc.citation.endingpage | 524 | - |
dc.citation.publicationname | ASTROPHYSICAL JOURNAL | - |
dc.identifier.doi | 10.1086/521547 | - |
dc.contributor.localauthor | Yoo, Jonghee | - |
dc.contributor.nonIdAuthor | Ikeda, M | - |
dc.contributor.nonIdAuthor | Takeda, A | - |
dc.contributor.nonIdAuthor | Fukuda, Y | - |
dc.contributor.nonIdAuthor | Vagins, M | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | CORE-COLLAPSE SUPERNOVAE | - |
dc.subject.keywordPlus | 23 FEBRUARY 1987 | - |
dc.subject.keywordPlus | DETECTOR | - |
dc.subject.keywordPlus | SIGNAL | - |
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