Published February 26, 2007
| Version v1
Journal article
Neutrino Probes of Galactic and Extragalactic Supernovae
Creators
- 1. California Institute of Technology, Mail Code 130-33, Pasadena, CA 91125 (United States)
Description
Neutrinos are a messenger of extreme condition inside a supernova core and a new-born neutron star. Since current ground-based detectors have potential to detect 10 000 neutrinos from supernova at the galactic center, they could tell us lots of important physics. It includes: explosion mechanism, shock wave propagation, core temperature, and gravitational binding energy, as well as neutrino properties as elementary particle. In addition to the galactic supernova neutrino burst, one can still learn about them with diffuse supernova neutrino background, which is also soon to be detected. We review current situation from both points of view, and discuss prospects for future neutrino astrophysics
Additional details
Identifiers
- DOI
- 10.1063/1.2713526;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 891
- Journal Issue
- 1
- Journal Page Range
- p. 263-271
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 6. Symposium on nuclear physics
- Dates
- 5-8 Sep 2006
- Place
- Tours (France)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39073960
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINDING ENERGY; GRAVITATION; NEUTRINO DETECTION; NEUTRINOS; NEUTRON STARS; PARTICLE PROPERTIES; REVIEWS; SHOCK WAVES; SUPERNOVAE; WAVE PROPAGATION
- Descriptors DEC
- BINARY STARS; DETECTION; DOCUMENT TYPES; ELEMENTARY PARTICLES; ENERGY; ERUPTIVE VARIABLE STARS; FERMIONS; LEPTONS; MASSLESS PARTICLES; RADIATION DETECTION; STARS; VARIABLE STARS
Optional Information
- Notes
- (c) 2007 American Institute of Physics