Published December 1998
| Version v1
Journal article
Neutrino absorption efficiency of an 40Ar detector from the β decay of 40Ti
Creators
- 1. University of Notre Dame, Notre Dame, Indiana, 46556 (United States)
- 2. University of Washington, Seattle, Washington, 98195 (United States)
- 3. GANIL, BP 5027, F-14021, Caen Cedex (France)
- 4. Institut de Physique Nucleaire, IN2P3-CNRS, F-91406, Orsay Cedex (France)
Description
We studied β-delayed proton and γ emission from 40Ti decay. We found t1/2=52.7±1.5 ms and observed 28 proton groups that we organized into a 40Ti decay scheme with 21 branches. The reduced transition strengths of these decay branches were then used to compute the neutrino detection efficiency of the ICARUS liquid argon time-projection chamber. We found 40Ar(ν,e) cross sections (for an electron energy threshold W=5 MeV) of (14.0±0.3)x10-43 cm2, (75.1±1.8)x10-43 cm2, and (3.2±0.1)x10-41 cm2 for 8B neutrinos, hep neutrinos, and supernova neutrinos characterized by a temperature of 4.5 MeV. copyright 1998 The American Physical Society
Additional details
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 58
- Journal Issue
- 6
- Journal Page Range
- p. 3677-3687
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 30021320
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ARGON 40; BETA DECAY; NEUTRINO DETECTION; NEUTRINO REACTIONS; SUPERNOVAE; TIME PROJECTION CHAMBERS; TITANIUM 40
- Descriptors DEC
- ARGON ISOTOPES; BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; BINARY STARS; DECAY; DETECTION; DRIFT CHAMBERS; ERUPTIVE VARIABLE STARS; EVEN-EVEN NUCLEI; ISOTOPES; LEPTON REACTIONS; LIGHT NUCLEI; MEASURING INSTRUMENTS; MILLISEC LIVING RADIOISOTOPES; MULTIWIRE PROPORTIONAL CHAMBERS; NUCLEAR DECAY; NUCLEAR REACTIONS; NUCLEI; PROPORTIONAL COUNTERS; RADIATION DETECTION; RADIATION DETECTORS; RADIOISOTOPES; STABLE ISOTOPES; STARS; TITANIUM ISOTOPES; VARIABLE STARS