Published May 1999 | Version v1
Journal article Metadata-only

Future supernova neutrino detection

Creators

Description

The responses of different neutrino detectors to the signal expected from a gravitational stellar collapse in our Galaxy are analysed and compared in this paper. Energetic and temporal characteristics of the detected neutrino signal are studied in order to investigate their information content concerning the stellar collapse and neutrino properties. Some consequences on ν physics and astrophysics are discussed

Additional details

Identifiers

PII
S0920563299004600;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
77
Journal Issue
1-3
Journal Page Range
p. 435-439
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
18. international conference on neutrino physics and astrophysics
Dates
4-9 Jun 1998
Place
Takayama (Japan)

INIS

Country of Publication
Netherlands
Country of Input or Organization
Ukraine
INIS RN
35052609
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTROPHYSICS; GALAXIES; GRAVITATIONAL COLLAPSE; NEUTRINO DETECTION; NEUTRINOS; RADIATION DETECTORS; SUPERNOVAE
Descriptors DEC
BINARY STARS; DETECTION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; LEPTONS; MASSLESS PARTICLES; MEASURING INSTRUMENTS; PHYSICS; RADIATION DETECTION; STARS; VARIABLE STARS

Optional Information

Copyright
Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.