Published December 16, 2011
| Version v1
Journal article
The nuclear response of molybdenum to supernova neutrinos
Creators
- 1. Department of Physics, P.O. Box 35 (YFL), FI-40014 University of Jyvskyl (Finland)
Description
Neutrino-nucleus interactions play a prominent role in many astrophysical applications. Knowledge about nuclear responses to neutrinos is therefore of paramount importance. We present cross sections for neutral-current neutrino-nucleus scattering off the stable (A = 92,94,95,96,97,98,100) molybdenum isotopes. The nuclear responses for these nuclei are additionally computed by folding the computed cross sections with a Fermi-Dirac distribution.
Additional details
Identifiers
- DOI
- 10.1063/1.3671055;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1417
- Journal Issue
- 1
- Journal Page Range
- p. 149-153
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Workshop on calculation of double-beta-decay matrix elements
- Acronym
- MEDEX '11
- Dates
- 13-16 Jun 2011
- Place
- Prague (Czech Republic)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43094073
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CROSS SECTIONS; DIRAC EQUATION; MOLYBDENUM 100 TARGET; MOLYBDENUM 92 TARGET; MOLYBDENUM 94 TARGET; MOLYBDENUM 95 TARGET; MOLYBDENUM 96 TARGET; MOLYBDENUM 97 TARGET; MOLYBDENUM 98 TARGET; NEUTRINO REACTIONS; NEUTRINO-NUCLEON INTERACTIONS; NEUTRINOS
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; FIELD EQUATIONS; INTERACTIONS; LEPTON REACTIONS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; LEPTONS; MASSLESS PARTICLES; NUCLEAR REACTIONS; PARTIAL DIFFERENTIAL EQUATIONS; PARTICLE INTERACTIONS; PHYSICS; TARGETS; WAVE EQUATIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics