Neutrino emission from supernovae in the presence of magnetic fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4362

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2009-03-02T11:39:30Z	-
dc.date.available	2009-03-02T11:39:30Z	-
dc.date.issued	1989	-
dc.identifier.citation	Michele Caffo [et al.]... eds., Astronomy, cosmology and fundamental physics; Proceedings of the Third ESO-CERN symposium held in Bologna,Palazzo Re Enzo,May 16 - 20, 1988, Vol. 155, pp. 471 - 472	en
dc.identifier.isbn	0-7923-0258-3	-
dc.identifier.uri	http://hdl.handle.net/2248/4362	-
dc.description	Restricted Access	-
dc.description.abstract	Neutrino burst observations from SN1987A indicate that the density and the temperature of the source and the propagation of the neutrinos in the medium are markedly different from those of solar and terrestrial conditions. If the magnetic field rises to as much as 10 to the 8th G at the neutrino source, then for a neutrino diffusion time-scale of 10 sec the neutrinos could flip helicity even in the case of a neutrino magnetic moment as small as 10 to the -24th micro-B.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.ispartofseries	Astrophysics and Space Science Library;Vol. 155	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1989ASSL..155..471S	en
dc.subject	Neutrino Beams	en
dc.subject	Particle Emission	en
dc.subject	Stellar Magnetic Fields	en
dc.subject	Supernova 1987a	en
dc.subject	Particle Diffusion	en
dc.subject	Particle Trajectories	en
dc.title	Neutrino emission from supernovae in the presence of magnetic fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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