Physics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.262..671k&link_type=abstract
Nature, vol. 262, Aug. 19, 1976, p. 671, 672. NSF-NASA-supported research.
Physics
9
Gravitational Waves, Neutrinos, Neutron Stars, Pulsed Radiation, Star Formation, Supernovae, Damping, Gravitational Collapse, Radiation Detectors, Supernova Remnants, Temperature Distribution, Thermodynamics
Scientific paper
An investigation is conducted concerning the possibility that neutrino radiation rather than gravitational radiation may be the dominant way by which nonradial pulsations are damped out in a collapsing star. The effects of neutrino radiation on the nonradial oscillations of such objects are examined and damping times corresponding to a particular neutrino production mechanism are evaluated. The obtained results imply that neutrino radiation, by more rapid damping of the nonradial oscillations of a newly formed neutron star in a supernova explosion, would hinder gravitational radiation, thus reducing the possibility of its detection.
Kazanas Demos
Schramm David N.
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