Published July 12, 2006
| Version v1
Journal article
Neutrino Flavor Changing Neutral Currents and Stellar Collapse
Creators
- 1. Department of Physics - 0319, University of California - San Diego, La Jolla, CA 92093 (United States)
Description
Flavor changing neutral current interactions are predicted in some extensions of the Standard Model. We discuss a process by which a neutrino can change flavor by scattering with a quark. We show how the stellar collapse environment is sensitive to neutrino flavor changing scattering on heavy nuclei. In particular, when this interaction is included in the stellar collapse model, the dynamics of the core's evolution and outcome of collapse are drastically changed
Additional details
Identifiers
- DOI
- 10.1063/1.2234427;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 847
- Journal Issue
- 1
- Journal Page Range
- p. 365-367
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- New horizon of nuclear astrophysics and cosmology
- Acronym
- International symposium on origin of matter and evolution of galaxies 2005
- Dates
- 8-11 Nov 2005
- Place
- Tokyo (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38045162
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- FLAVOR MODEL; GRAVITATIONAL COLLAPSE; HEAVY NUCLEI; NEUTRAL CURRENTS; NEUTRAL-CURRENT INTERACTIONS; NEUTRINOS; QUARKS; SCATTERING; STANDARD MODEL; SUPERNOVAE
- Descriptors DEC
- ALGEBRAIC CURRENTS; BINARY STARS; COMPOSITE MODELS; CURRENTS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; INTERACTIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NUCLEI; PARTICLE INTERACTIONS; PARTICLE MODELS; QUANTUM FIELD THEORY; QUARK MODEL; STARS; UNIFIED GAUGE MODELS; VARIABLE STARS
Optional Information
- Notes
- (c) 2006 American Institute of Physics