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Cut-continuity of twistor angular momentum
被引:0
作者:
Helfer, Adam D.
[1
,2
]
机构:
[1] Univ Missouri, Dept Math, Columbia, MO 65211 USA
[2] Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA
关键词:
GRAVITATIONAL WAVES;
GENERAL RELATIVITY;
D O I:
10.1103/PhysRevD.106.084044
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Chen et al. argued recently that, in Bondi-Sachs spacetimes, the angular momentum at scri (null infinity) should vary continuously with the position of the cut (but not depend sensitively on its derivatives); they showed that this property was enjoyed by some definitions but not others. I show here that the twistor definition has this continuity. The argument is rather different from the one of Chen et al., with the invariant geometry of scri at the forefront. The flux, in the sense of the angular momentum emitted between two infinitesimally separated cuts, is calculated; this flux can be interpreted as the first variation of the angular momentum with respect to the cut. Examining the second variation, one finds that the twistor definition, unlike most others, responds to correlations in radiation between different asymptotic directions. The twistor angular momentum is thus sensitive to a qualitatively different structure in the asymptotic field than are the currently more used ones.
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页数:16
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