Published 1994 | Version v1
Report Open

Comment on the preprint Neutrino Flavor Evolution Near a Supernova's Core

Creators

Description

The revised version of the widely circulated preprint ''Neutrino Flavor Evolution Near A Supernova's Core'' by J. Pantaleone (astro-ph 9405008 on the bulletin Board, Indiana University preprint IUHET-276) is wrong. It contains two errors which lead to incorrect conclusions regarding neutrino flavor transformation in the supernova environment. In this short note we discuss these errors

Availability note (English)

MF available from INIS under the Report Number; Also available from OSTI as DE94017576; NTIS; US Govt. Printing Office Dep.

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Additional details

Publishing Information

Imprint Pagination
7 p.
Report number
DOE/ER/40561--149

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
26012889
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
COSMIC NEUTRINOS; FLAVOR MODEL; HAMILTONIANS; QUANTUM MECHANICS; SUPERNOVAE
Descriptors DEC
BINARY STARS; COMPOSITE MODELS; COSMIC RADIATION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATHEMATICAL OPERATORS; MECHANICS; NEUTRINOS; PARTICLE MODELS; QUANTUM OPERATORS; QUARK MODEL; RADIATIONS; STARS; VARIABLE STARS

Optional Information

Contract/Grant/Project number
Contract FG06-90ER40561; Grant PHY-9121623
Funding organization
USDOE, Washington, DC (United States); National Science Foundation, Washington, DC (United States).