Constraints on the neutrino magnetic moment from stellar evolution and supernovae type Ia

dc.contributor.author	Sivaram, C
dc.date.accessioned	2009-01-02T11:14:35Z
dc.date.available	2009-01-02T11:14:35Z
dc.date.issued	1993
dc.identifier.citation	D. A. Leahy, R. B. Hickws, and D. Venkatesan.eds., 23rd International Cosmic Ray Conference, Vol. 4, held 19 - 30 July, 1993 at University of Calgary, Alberta, Canada.pp. 645 - 647	en
dc.identifier.uri	http://hdl.handle.net/2248/4229
dc.description.abstract	There are several interesting consequences of a neutrino magnetic moment(NMM) such as possibility of a time varying solar neutrino signal (ENS), increased cooling of red giants and enhanced evolution of horizontal branch stars. Earlier Sn 1987A was used to put constraints on NMM. Here we use effects of NMM in preventing carbon-oxygen deflagrations that cause Sn type Ia to give µ/subν<10/sup-13µB. Constraints on CP- violating weak interactions are also put.	en
dc.language.iso	en	en
dc.publisher	University of Calgary	en
dc.relation.ispartofseries	International Cosmic Ray Conference; Vol. 4
dc.relation.uri	http://adsabs.harvard.edu/abs/1993ICRC....4..645S	en
dc.title	Constraints on the neutrino magnetic moment from stellar evolution and supernovae type Ia	en
dc.type	Article	en