On the Born Approximation for Perturbations of a Spherical Star and the Newman-Penrose Constants

Details On the Born Approximation for Perturbations of a Spherical Star and the Newman-Penrose Constants On the Born Approximation for Perturbations of a Spherical Star and the Newman-Penrose Constants

Oct 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973rspsa.335..163f&link_type=abstract

Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 335, Issue 1601, pp. 163-190

Physics

8

Scientific paper

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.

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