nLab Bondi-Metzner-Sachs group

Redirected from "BMS group".

Context

Gravity

gravity, supergravity

Formalism

Definition

Spacetime configurations

Properties

Spacetimes

Quantum theory

Contents

Idea

The Bondi-Metzner-Sach group (BMS group) is the group of asymptotic symmetries of asymptotically flat spacetimes at lightlike infinity.

References

Named after:

Lecture notes and introductions:

In relation to the Wheeler-DeWitt equation:

Similar symmetries of near horizon geometries of black hole spacetimes (with higher curvature corrections):

  • Mariano Chernicoff, Gaston Giribet, Julio Oliva: Higher-curvature corrections and near horizon symmetries [arXiv:2506.21747]

See also:

  • Ratindranath Akhoury, Arielle Schutz, David Garfinkle: Superrotations are Linkages [arXiv:2507.04245]

  • Yu-fan Zheng: Supersymmetric BMS 4BMS_4 Algebras Revisited: Electric/Magnetic Superalgebras and Free Field Realization [arXiv:2508.17925]

  • Xavier Bekaert, Laura Donnay, Yannick Herfray: BMS particles [arXiv:2412.06002]

  • Romain Ruzziconi, Peter West: Extended BMS representations and strings [arXiv:2601.00662]

  • Geoffrey Compère, Sébastien Robert: Conservation law of super-Lorentz charges [arXiv:2606.26848]

  • Diego Hidalgo, Stefan Vandoren, Huaxuan Zeng: BMS 3BMS_3 invariant field theories [arXiv:2607.06826]

Last revised on July 9, 2026 at 04:00:14. See the history of this page for a list of all contributions to it.