Neutrino angular momentum loss in rotating stars

Details Neutrino angular momentum loss in rotating stars Neutrino angular momentum loss in rotating stars

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219l..39e&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 219, Jan. 1, 1978, p. L39-L41.

Astronomy and Astrophysics

Astrophysics

7

Angular Momentum, Energy Distribution, Momentum Transfer, Neutrinos, Stellar Rotation, Gravitational Collapse, Gravitational Waves

Scientific paper

We consider how an axisymmetric, uniformly and slowly rotating homogeneous star might be affected by the loss of energy and angular momentum via neutrino emission. For example, these losses can cause a collapsing, rotating star to flatten either faster or slower than would be the case if these losses were not taken fully into account, depending on the efficiency of the angular momentum loss mechanism.

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