dc.creator |
Butler, Malcolm |
|
dc.creator |
Malaney, R. A. |
|
dc.creator |
Starkman, G. D. |
|
dc.date.accessioned |
2015-04-30T12:47:42Z |
|
dc.date.available |
2015-04-30T12:47:42Z |
|
dc.date.issued |
1994-06-01 |
|
dc.identifier.issn |
0556-2821 |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/26089 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
Applying the phenomenon of neutrino lasing in the solar interior we show how the rate for the generic neutrino decay process [nu] [right arrow] fermion + boson can in principle be enhanced by many orders of magnitude over its normal decay rate. Such a large enhancement could be of import to neutrino-decay models invoked in response to the apparent deficit of electron neutrinos observed from the Sun. The significance of this result to such models depends on the specific form of the neutrino decay, and the particle model within which it is embedded. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2015-04-30T12:47:42Z
No. of bitstreams: 1
Butler_M_N_article_1994.pdf: 293765 bytes, checksum: 48e1f73197d5c59725341b14454dbf46 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2015-04-30T12:47:42Z (GMT). No. of bitstreams: 1
Butler_M_N_article_1994.pdf: 293765 bytes, checksum: 48e1f73197d5c59725341b14454dbf46 (MD5)
Previous issue date: 1994-06-01 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Physical Society |
en_CA |
dc.relation.uri |
http://dx.doi.org/10.1103/PhysRevD.49.6232 |
|
dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
|
dc.subject.lcsh |
Solar neutrinos |
|
dc.title |
Neutrino lasing in the Sun |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Physical Review D 49(11), 6232-6235. (1994) |
en_CA |