Published August 12, 2010
| Version v1
Journal article
Neutrino interactions in astrophysics and the third neutrino mixing angle θ13
Creators
- 1. Physics Department, University of Wisconsin, Madison, WI 53706 (United States)
Description
The third neutrino mixing angle θ13 is the least known one. In this contribution, after a brief discussion of the current efforts to determine the value of this angle better, various astrophysical implications of a non-zero value of θ13 are summarized.
Additional details
Identifiers
- DOI
- 10.1063/1.3485134;
- arXiv
- arXiv:1006.2836v1;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1269
- Journal Issue
- 1
- Journal Page Range
- p. 195-200
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 10. international symposium on origin of matter and evolution of galaxies
- Acronym
- OMEG-2010
- Dates
- 8-10 Mar 2010
- Place
- Osaka (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42026083
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; NEUTRINO REACTIONS; NEUTRINO-NUCLEON INTERACTIONS; NEUTRINOS; REST MASS; STANDARD MODEL; SUPERNOVAE; WEINBERG ANGLE
- Descriptors DEC
- BINARY STARS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; INTERACTIONS; LEPTON REACTIONS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; LEPTONS; MASS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NUCLEAR REACTIONS; PARTICLE INTERACTIONS; PARTICLE MODELS; PHYSICS; QUANTUM FIELD THEORY; STARS; UNIFIED GAUGE MODELS; VARIABLE STARS
Optional Information
- Notes
- (c) 2010 American Institute of Physics