Neutrino angular momentum losses in stellar collapse

Details Neutrino angular momentum losses in stellar collapse Neutrino angular momentum losses in stellar collapse

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.267..501k&link_type=abstract

Nature, vol. 267, June 9, 1977, p. 501, 502. NSF-supported research.

Computer Science

16

Angular Momentum, Energy Dissipation, Gravitational Collapse, Momentum Transfer, Neutrinos, Neutron Stars, Stellar Models, Pulsars, Stellar Rotation, Supernovae

Scientific paper

To account for the slow rotation rate of neutron stars, a model is described which permits evaluation of the loss of angular momentum resulting from the escape of neutrinos from a collapsing stellar core. Loss of angular momentum by this mechanism is thought to occur in all rotating collapsing cores, but does not completely account for the slow rotation of the compact supernova remnants (pulsars). Observational effects caused by transfer of angular momentum to the expanding envelope are considered, and results obtained from a more generalized treatment are discussed.

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