Published November 1, 2008 | Version v1
Journal article Metadata-only

Collective three-flavor oscillations of supernova neutrinos

Creators

  • 1. Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai (India)

Description

We present a formalism to study three-flavor effects in flavor conversions of dense neutrino ensembles. The main idea is to use the smallness of Δm2o-dotΔm2atm and θ13. The formalism has immediate applications to neutrinos from supernovae or the early Universe. We outline some consequences for supernova neutrino phenomenology, e.g hierarchy determination at extremely small θ13.

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/136/4/042072

Additional details

Identifiers

DOI
10.1088/1742-6596/136/4/042072;

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
136
Journal Issue
4
Journal Page Range
[1 p.]
ISSN
1742-6596

Conference

Title
23. international conference on neutrino physics and astrophysics
Dates
25-31 May 2008
Place
Christchurch (New Zealand)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41050670
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMIC NEUTRINOS; FLAVOR MODEL; KOBAYASHI-MASKAWA MATRIX; NEUTRINO OSCILLATION; REST MASS; SUPERNOVAE; UNIVERSE; WEINBERG ANGLE
Descriptors DEC
BINARY STARS; COMPOSITE MODELS; COSMIC RADIATION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATRICES; NEUTRINOS; PARTICLE MODELS; QUARK MODEL; RADIATIONS; STARS; VARIABLE STARS