Matching Zerilli to Chandrasekhar-Esposito through the first post-Newtonian order.

Details Matching Zerilli to Chandrasekhar-Esposito through the first post-Newtonian order. Matching Zerilli to Chandrasekhar-Esposito through the first post-Newtonian order.

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983gregr..15.1121a&link_type=abstract

General Relativity and Gravitation, Volume 15, Issue 12, pp.1121-1129

Physics

2

Gravitation Theory:Gravitational Radiation, Gravitational Radiation:Gravitation Theory

Scientific paper

The results obtained from an analysis of the wave zone of the Zerilli equation by Anderson, Kates, Kegeles, and Madonna are reviewed. An asymptotic gauge transformation is then developed in order to transform the metric from Regge-Wheeler gauge to Chandrasekhar and Esposito gauge, through the first post-Newtonian (PN) order. The transformation is carried out and the transformed wave zone metric is matched to the Chandrasekhar-Esposito (CE) metric.

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