Published October 24, 2008
| Version v1
Journal article
Identifying Neutrino Mass Hierarchy at Extremely Small θ13 through Earth Matter Effects in a Supernova Signal
- 1. Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005 (India)
- 2. Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Muenchen (Germany)
Description
Collective neutrino flavor transformations deep inside a supernova are sensitive to the neutrino mass hierarchy even at extremely small values of θ13. Exploiting this effect, we show that comparison of the antineutrino signals from a galactic supernova in two megaton class water Cherenkov detectors, one of which is shadowed by Earth, will enable us to distinguish between the hierarchies if sin2θ13 < or approx. 10-5, where long baseline neutrino experiments would be ineffectual
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.101.171801;
- arXiv
- arXiv:0802.1481v3;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 101
- Journal Issue
- 17
- Journal Page Range
- p. 171801-171801.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40054040
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- ANTINEUTRINOS; CHERENKOV COUNTERS; FLAVOR MODEL; MASS; SIGNALS; SUPERNOVAE
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; BINARY STARS; COMPOSITE MODELS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATTER; MEASURING INSTRUMENTS; NEUTRINOS; PARTICLE MODELS; QUARK MODEL; RADIATION DETECTORS; STARS; VARIABLE STARS
Optional Information
- Notes
- (c) 2008 The American Physical Society