Published February 26, 2007 | Version v1
Journal article

Neutrino Probes of Galactic and Extragalactic Supernovae

  • 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

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