Constraints on BMS Transformations via Energy Conditions and implications on black hole geometry
Nihar Ranjan Ghosh, Malay K. Nandy

TL;DR
This paper explores how classical energy conditions restrict the supertranslation transformations in the BMS group, revealing that many are physically inadmissible, thus significantly narrowing the allowed supertranslation sector in black hole spacetimes.
Contribution
It develops a perturbative framework to derive explicit inequalities from energy conditions on supertranslations, constraining the BMS group on Schwarzschild backgrounds.
Findings
Energy conditions impose angular restrictions on supertranslations.
SEC and WEC restrict supertranslations at next-to-leading order.
NEC and DEC constraints appear only at higher orders, especially NNLO.
Abstract
We investigate whether the formally infinite-dimensional supertranslation sector of the Bondi-Metzner-Sachs (BMS) group remains fully physically admissible once classical energy conditions are enforced. Working in a perturbative framework , we first develop a general toolkit by expanding the curvature tensors and the Ricci scalar in powers of the perturbation and recast the strong, weak, null and dominant energy conditions (SEC, WEC, NEC and DEC, respectively) as explicit inequalities on following from the Raychaudhuri equation. The formalism is general, but to obtain concrete constraints we specialize to the standard BMS form on a Schwarzschild background and parametrize by a supertranslation function . We find that the SEC and WEC impose nontrivial angular restrictions on already…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations · Noncommutative and Quantum Gravity Theories
