Asymmetric lepton production in a universe with non-zero baryon number

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3973

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2008-10-25T10:28:15Z	-
dc.date.available	2008-10-25T10:28:15Z	-
dc.date.issued	1982-03	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 82, No. 2, pp. 485 - 488	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/3973	-
dc.description.abstract	Due to processes occurring during different stages of stellar evolution, a universe with a net baryon number develops an excess of neutrinos and positrons over antineutrinos of the same order as the observed relative strength of CP violation, over the course of a Hubble age. Since the neutrinos have a left-handed helicity, an initially symmetric universe would become weakly left-handed after a period of about 10 to the 10th years.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/w8vu32240588w284/	en
dc.subject	Baryons	en
dc.subject	Cosmic Rays	en
dc.subject	Leptons	en
dc.subject	Particle Production	en
dc.subject	Stellar Evolution	en
dc.subject	Black Holes (Astronomy)	en
dc.subject	Electrons	en
dc.subject	Main Sequence Stars	en
dc.subject	Neutron Stars	en
dc.subject	Positrons	en
dc.subject	Supernovae	en
dc.title	Asymmetric lepton production in a universe with non-zero baryon number	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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