Energy deposition due to neutrino pair annihilation near rotating neutron stars

Prasannaa, A. R. ; Goswami, Srubabati (2002) Energy deposition due to neutrino pair annihilation near rotating neutron stars Physics Letters B, 526 (1-2). pp. 27-33. ISSN 0370-2693

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Official URL: http://www.sciencedirect.com/science/article/pii/S...

Abstract

General relativistic effects have been shown to increase the energy deposition rate due to the process in supernovae and neutron stars. In this Letter 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.

Item Type:Article
Source:Copyright of this article belongs to Elsevier Science.
Keywords:Neutrinos; Supernovae; Neutron Stars
ID Code:108720
Deposited On:01 Feb 2018 04:37
Last Modified:01 Feb 2018 04:37

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