On the Born approximation for perturbations of a spherical star and the Newman—Penrose constants
- 30 October 1973
- journal article
- Published by The Royal Society in Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences
- Vol. 335 (1601) , 163-190
- https://doi.org/10.1098/rspa.1973.0120
Abstract
The field equations governing perturbations of a spherical star in general relativity are solved by means of a weak field or Born approximation. Formal expressions for the far field of a non-stationary source are obtained and used to discuss the Newman-Penrose constants.This publication has 12 references indexed in Scilit:
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