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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4229

Full metadata record

DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Constraints on the neutrino magnetic moment		161.09 kB	Adobe PDF	View/Open

DSpace JSPUI