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 |