Unified Treatment of null and Spatial Infinity IV: Angular Momentum at Null and Spatial Infinity
arXiv:2311.14190 · doi:10.1007/JHEP01(2024)085
Abstract
In a companion paper we introduced the notion of asymptotically Minkowski spacetimes. These space-times are asymptotically flat at both null and spatial infinity, and furthermore there is a harmonious matching of limits of certain fields as one approaches in null and space-like directions. These matching conditions are quite weak but suffice to reduce the asymptotic symmetry group to a Poincaré group . Restriction of to future null infinity yields the canonical Poincaré subgroup of the BMS group selected in the companion paper and its restriction to spatial infinity gives the canonical subgroup of the Spi group there. As a result, one can meaningfully compare angular momentum that has been defined at using with that defined on using . We show that the angular momentum charge at equals the sum of the angular momentum charge at any 2-sphere cross-section of and the total flux of angular momentum radiated across the portion of to the past of . In general the balance law holds only when angular momentum refers to subgroups of the Poincaré group .
Version to appear in JHEP. Slightly edited to improve the presentation. Four references added. 30 pages, 1 figure
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Cited by in corpus (8)
- ADM, BMS, and some puzzling interconnections
- Projective and Carrollian geometry at time/space-like infinity on projectively compact Ricci flat Einstein manifolds
- Supertranslation ambiguity in post-Minkowskian expansion
- On supertranslation invariant Lorentz charges
- Ti and Spi, Carrollian extended boundaries at timelike and spatial infinity
- Quasi-local spin-angular momentum and the construction of axial vector fields
- Supertranslations at Spatial and Timelike Infinities in the First-Order Formalism
- Note on post-Minkowskian expansion and Bondi coordinates