Comments on gravitational radiation damping and energy loss in binary systems

Details Comments on gravitational radiation damping and energy loss in binary systems Comments on gravitational radiation damping and energy loss in binary systems

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208l..77e&link_type=abstract

Astrophysical Journal, vol. 208, Sept. 1, 1976, pt. 2, p. L77-L81.

Astronomy and Astrophysics

Astrophysics

103

Binary Stars, Energy Dissipation, Gravitational Waves, Stellar Gravitation, Iterative Solution, Relativity, Stellar Models

Scientific paper

It is argued that a formula for the energy loss due to gravitational radiation of bound systems such as binaries has not yet been derived either exactly or by means of a consistent approximation method within general relativity, a view which contradicts some widely accepted claims in the literature. The main approaches used to obtain such a formula are critically reviewed, and it is pointed out that the derivations presented so far either contain inconsistencies or are incomplete.

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