Possible CP-violation effects in core-collapse supernovae
Creators
- 1. Department of Physics, University of Wisconsin Madison, WI 53706 (United States)
- 2. Institut de Physique Nucleaire, F-91406 Orsay cedex (France)
Description
We study CP-violation effects when neutrinos are present in dense matter, such as outside the proto-neutron star formed in a core-collapse supernova. Using general arguments based on the Standard Model, we confirm that there are no CP-violating effects at the tree level on the electron neutrino and anti-neutrino fluxes in a core-collapse supernova. On the other hand significant effects can be obtained for muon and tau neutrinos even at the tree level. We show that CP-violating effects can be present in the supernova electron (anti-)neutrino fluxes as well, if muon and tau neutrinos have different fluxes at the neutrinosphere. Such differences could arise due to physics beyond the Standard Model, such as the presence of flavor-changing interactions
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physletb.2008.03.038Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2008.03.038;
- arXiv
- arXiv:0710.3112v3;
- PII
- S0370-2693(08)00364-X;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 662
- Journal Issue
- 5
- Journal Page Range
- p. 396-404
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40046814
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CP INVARIANCE; ELECTRON NEUTRINOS; FLAVOR MODEL; MUONS; NEUTRON STARS; NUCLEOSYNTHESIS; R PROCESS; STANDARD MODEL; SUPERNOVAE; TAU NEUTRINOS
- Descriptors DEC
- BINARY STARS; COMPOSITE MODELS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; EVOLUTION; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; HEAVY LEPTONS; INVARIANCE PRINCIPLES; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NEUTRINOS; PARTICLE MODELS; QUANTUM FIELD THEORY; QUARK MODEL; STAR EVOLUTION; STARS; SYNTHESIS; UNIFIED GAUGE MODELS; VARIABLE STARS
Optional Information
- Copyright
- Copyright (c) 2008 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.