Energy deposition due to neutrino pair annhilation near rotating neutron stars

Details Energy deposition due to neutrino pair annhilation near rotating neutron stars Energy deposition due to neutrino pair annhilation near rotating neutron stars

2001-09-05

arxiv.org/abs/astro-ph/0109058v1

Phys.Lett.B526:27-33,2002

Astronomy and Astrophysics

Astrophysics

10 pages, latex, 2 figures

Scientific paper

10.1016/S0370-2693(01)01470-8

General relativistic effects have been shown to increase the energy deposition rate due to the process $\nu \bar{\nu} \to e^{+}e^{-}$ in supernovae and neutron stars. In this paper we study the effect of inclusion of the rotation of the star in the general relativistic treatment. We show that inclusion of rotation results in a reduction in the heating rate as compared to the no rotation case.

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