The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A
dc.contributor.author | Barbieri, R. | en_US |
dc.contributor.author | Mohapatra, R. N. | en_US |
dc.contributor.author | Yanagida, T. | en_US |
dc.date.accessioned | 2006-05-10T15:37:26Z | |
dc.date.available | 2006-05-10T15:37:26Z | |
dc.date.issued | 1988-10-13 | en_US |
dc.identifier.citation | Barbieri, R., Mohapatra, R. N., Yanagida, T. (1988/10/13)."The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A." Physics Letters B 213(1): 69-72. <http://hdl.handle.net/2027.42/27097> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6TVN-46YSTYR-28Y/2/b3d3bfcc149ae08be63de8b080e36547 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/27097 | |
dc.description.abstract | If the magnetic moment of the neutrino is to provide a resolution of the solar neutrino puzzle without violating the constraints implied by SN1987A observations, there must exist non-standard interactions of the right-handed neutrinos, which are able to trap them in the supernova core. We study one class of such interactions mediated by a singly charged Higgs boson, already proposed to yield a large magnetic moment of the neutrino, and suggest how the same interaction could provide a detectable signal in future neutrino counting experiments, e+e--->[nu][gamma]. | en_US |
dc.format.extent | 15157 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.extent | 257954 bytes | |
dc.format.mimetype | text/plain | |
dc.format.mimetype | text/plain | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | en_US |
dc.publisher | Elsevier | en_US |
dc.title | The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbsecondlevel | Mathematics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationother | INFN, Sezione di Pisa, Pisa, Italy; Dipartimento di Fisica, Universitá di Pisa, I-56100, Pisa, Italy. | en_US |
dc.contributor.affiliationother | Department of Physics and Astronomy, University of Maryland, College Park, MD 20742, USA | en_US |
dc.contributor.affiliationother | Tohuku University, Sendai 980, Japan | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/27097/3/0000088.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0370-2693(88)91049-0 | en_US |
dc.identifier.source | Physics Letters B | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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