Computer Science – Numerical Analysis
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..81..483s&link_type=abstract
Astrophysics and Space Science, vol. 81, no. 1-2, Jan. 1982, p. 483-488.
Computer Science
Numerical Analysis
2
Gravitational Collapse, Neutrinos, Particle Energy, Pulsed Radiation, Scintillation Counters, Supernovae, Energy Spectra, Galactic Evolution, Numerical Analysis, Relativistic Particles, Stellar Radiation, Temporal Distribution
Scientific paper
The effect induced in the neutrino detector by a supernova neutrino pulse is investigated, taking into account three factors: (1) the duration of the neutrino radiation, (2) the energy spectrum of the neutrino radiation, and (3) the neutrino rest mass. Domogatsky et al. (1978) had considered the first two of these factors, but neglected the neutrino rest mass. Results show that the shape of the neutrino scintillation detector response depends on both the neutrino radiation characteristics and the neutrino rest mass. It is also noted that the very short and even instantaneous neutrino radiative bursts due to relativistic collapses are lengthened up to several seconds, a fact which should be considered when choosing detector-events-data-analysis systems.
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