Published 2011 | Version v1
Book

Effects of resonant spin-flavor conversion of supernova neutrinos in supernova neutrino event

  • 1. Dept. of Astronomy University of Tokyo, Tokyo (JAPAN)
  • 2. Dept. of Mathematics, Toyota National College of Technology (JAPAN)
  • 3. Dept. of Physics, Nagoya University (JAPAN)

Description

We investigate the effects of the resonant spin-flavor (RSF) conversion of Majorana neutrinos in the time variation of supernova νe spectrum. The time evolution of electron mole fraction in the innermost region of supernova ejecta is considered. Large time variation of the supernova νe spectrum would be observed if the RSF conversion is effective in the inverted mass hierarchy and adiabatic high-density MSW resonance.

Part of:
Neutrino Telescope

Additional details

Publishing Information

Publisher
Edizioni Papergraf
Imprint Place
Padova (Italy)
ISBN
978-88-97645-01-6
Imprint Title
Neutrino Telescope
Imprint Pagination
481 p.
Journal Page Range
p. 413-415

Conference

Title
14. International Workshop on Neutrino Telescopes
Dates
15-18 Mar 2011
Place
Venezia (Italy)

INIS

Country of Publication
Italy
Country of Input or Organization
Italy
INIS RN
44036226
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
FLAVOR MODEL; FREQUENCY MEASUREMENT; NEUTRINO BEAMS; NEUTRINO OSCILLATION; SPIN; SUPERNOVAE
Descriptors DEC
ANGULAR MOMENTUM; BEAMS; BINARY STARS; COMPOSITE MODELS; ERUPTIVE VARIABLE STARS; LEPTON BEAMS; MATHEMATICAL MODELS; PARTICLE BEAMS; PARTICLE MODELS; PARTICLE PROPERTIES; QUARK MODEL; STARS; VARIABLE STARS

Optional Information