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Peeling properties of lightlike signals in General Relativity

G. F. Bressange·P. A. Hogan
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Abstract

The peeling properties of a lightlike signal propagating through a general Bondi-Sachs vacuum spacetime and leaving behind another Bondi-Sachs vacuum space-time are studied. We demonstrate that in general the peeling behavior is the conventional one which is associated with a radiating isolated system and that it becomes unconventional if the asymptotically flat space-times on either side of the history of the light-like signal tend to flatness at future null infinity faster than the general Bondi-Sachs space-time. This latter situation occurs if, for example, the space-times in question are static Bondi-Sachs space- times.

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G. F. Bressange, P. A. Hogan. 2000-02-14. Peeling properties of lightlike signals in General Relativity. https://doi.org/10.1103/physrevd.60.104006

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