1999
DOI: 10.1103/physrevd.60.104006
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Peeling properties of lightlike signals in general relativity

Abstract: The peeling properties of a light-like signal propagating through a general Bondi-Sachs vacuum space-time 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 spac… Show more

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Cited by 3 publications
(11 citation statements)
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“…Furthermore, space-times describing light like signals propagating through a general Bondi-Sachs space-time have peeling properties as well. In certain cases these are different from those of a Bondi-Sachs space-time [5].…”
Section: Introductionmentioning
confidence: 82%
“…Furthermore, space-times describing light like signals propagating through a general Bondi-Sachs space-time have peeling properties as well. In certain cases these are different from those of a Bondi-Sachs space-time [5].…”
Section: Introductionmentioning
confidence: 82%
“…such that ∇ µ g ∼ λν = 0 . The whole set of equations (31), (32) an d (37) describe the dynamics of the shell, however as they are not all independent only part of them need to be used.…”
Section: Iii1 Junction Conditions : the Distributional Descriptionmentioning
confidence: 99%
“…According to the form taken by the functions F (x, y), U + (u, v + ) and V + (u, v + ) diferent types of situations can occur: we can have only a lighlike shell, only an impulsive wave or both. A more extended version describing the geometry of the spacetimes M ± and the properties of the shell and the wave will be presented in forthcoming paper [37].…”
Section: Planar Shells and Impulsive Wavesmentioning
confidence: 99%
“…Regrouping the covariant derivatives and taking into account the relation between spin and torsion given in (15), this equation leads directly to the generalized evolution equation of the spin tensor…”
Section: The Einstein-cartan Theorymentioning
confidence: 99%
“…Using the relations (4), (15) and (29), we can obtain the following useful form of Σ νρ in terms of the spin tensor…”
Section: Figure 1 : Isometric Soldering Of Two Spacetimesmentioning
confidence: 99%