algebraic quantum field theory (perturbative, on curved spacetimes, homotopical)
quantum mechanical system, quantum probability
interacting field quantization
Given a gauge theory (and/or gravity) on a spacetime with asymptotic boundary, certain would-be gauge transformations (diffeomorphisms) that act non-trivially on asymptotic “boundary data” may in fact be identified as physically observable global symmetries and hence have, in contrast to actual gauge symmetries, “direct empirical significance” (DES, Teh 2016).
A basic example is (the symmetry generated by) the ADM mass and the BMS group of asymptotic symmetries on asymptotically flat spacetimes.
Up to technical fine-print (cf. Borsboom & Posthuma 2015) a group of asymptotic symmetries is the coset space of all gauge symmetries that respect boundary data, by the subgroup of bulk gauge transformations which act as the identity map on the asymptotic boundary (cf. Strominger 2018 (2.10.1), Borsboom & Posthuma 2015 p 2):
Hence if the bulk gauge symmetries form a normal subgroup then the asymptotic symmetries form a quotient group characterized by a short exact sequence of the form
Early usage of the term “asymptotic symmetry”:
(introducing what came to be known as the BMS group)
In D=3 gravity:
General considerations:
In relation to soft graviton theorems:
In relation to superselection sectors:
For electromagnetism:
See also:
Antoine Rignon-Bret, Simone Speziale: General covariance and boundary symmetry algebras [arXiv:2403.00730]
Níckolas de Aguiar Alves, Andre G. S. Landulfo: The Sky as a Killing Horizon [arXiv:2504.12514]
Last revised on April 18, 2025 at 06:13:51. See the history of this page for a list of all contributions to it.