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Neutrino astrophysics with IMB: past, present, and future

dc.contributor.authorCasper, David W.en_US
dc.contributor.authorSulak, Lawrence R.en_US
dc.contributor.authorBionta, Richard M.en_US
dc.contributor.authorBlewitt, G.en_US
dc.contributor.authorBratton, C. B.en_US
dc.contributor.authorClaus, R.en_US
dc.contributor.authorCortez, B. G.en_US
dc.contributor.authorCrouch, M.en_US
dc.contributor.authorDye, S. T.en_US
dc.contributor.authorErrede, S.en_US
dc.date.accessioned2006-04-07T20:23:10Z
dc.date.available2006-04-07T20:23:10Z
dc.date.issued1988-03en_US
dc.identifier.citationCasper, David W., Sulak, Lawrence R., Bionta, R. M., Blewitt, G., Bratton, C. B., Casper, D., Claus, R., Cortez, B., Crouch, M., Dye, S. T., Errede, S. (1988/03)."Neutrino astrophysics with IMB: past, present, and future." Nuclear Physics B - Proceedings Supplements 3(): 463-470. <http://hdl.handle.net/2027.42/27392>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVD-47GJ19S-N/2/43221beaf70ccbca2c019ecfc022d8daen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/27392
dc.description.abstractA burst of eight neutrino interactions occurring over a six second interval had been observed with the IMB detector. The closeness in time of the burst to the optical discovery of Supernova 1987a suggests that the neutrinos originated from stellar collapse. The characteristics of the burst are reviewed together with a recently completed reevaluation of many aspects of the detector's response. Efforts underway to discover past and future supernovae are also briefly discussed.en_US
dc.format.extent429287 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleNeutrino astrophysics with IMB: past, present, and futureen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelNuclear Engineering and Radiological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumThe University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.contributor.affiliationotherno department founden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/27392/1/0000423.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0920-5632(88)90197-1en_US
dc.identifier.sourceNuclear Physics B - Proceedings Supplementsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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