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Conformal Carroll groups and BMS symmetry (1402.5894v2)

Published 24 Feb 2014 in gr-qc, hep-th, math-ph, and math.MP

Abstract: The Bondi-Metzner-Sachs (BMS) group is shown to be the conformal extension of Levy-Leblond's "Carroll" group. Further extension to the Newman-Unti (NU) group is also discussed in the Carroll framework.

Citations (282)

Summary

  • The paper formulates the conformal Carroll group, establishing its link with BMS symmetry in asymptotically flat spacetimes.
  • It applies rigorous Lie algebra techniques to reveal that the conformal Carroll group constitutes an infinite-dimensional structure including super-translations.
  • The work broadens insights into gravitational radiation and quantum gravity, paving the way for further exploration of asymptotic symmetry frameworks.

An Examination of Conformal Carroll Groups and BMS Symmetry

The paper "Conformal Carroll groups and BMS symmetry" explores the intricate relationship between the Bondi-Metzner-Sachs (BMS) group and the conformal extension of the so-called "Carroll" group, originally proposed by Lévy-Leblond. Additionally, the work outlines the extension of these ideas to the Newman-Unti (NU) group within the Carroll framework. This exploration enriches the theoretical understanding of asymptotic symmetries in general relativity, particularly concerning gravitational radiation and its related symmetry groups in asymptotically flat spacetimes.

Overview of the BMS Group and Carroll Group

The BMS group emerged as a notable asymptotic symmetry group of a four-dimensional asymptotically flat spacetime, notably when dealing with gravitational radiation. Unlike the expected Poincaré group, the BMS group represents an infinite-dimensional structure that comprises numerous copies of the Poincaré group. Remarkably, none of these copies are invariant due to the presence of gravitational radiation, challenging traditional expectations of asymptotic symmetry.

On the other hand, the Carroll group provides an unconventional contraction of the Poincaré group. When the speed of light approaches zero, Carroll structures emerge, suggesting intriguing parallels and distinctions with non-relativistic counterparts such as the Newton-Cartan framework. By examining the conformal extensions of the Carroll group, this paper highlights the versatility of Carrollian mechanics in bridging various aspects of symmetry and spacetime geometries.

Mathematical Formulation

The paper's essential contribution lies in its formulation of the conformal Carroll group, denoted as CCarrN(C, g, ξ), for a given Carroll manifold C. This group consists of transformations preserving a tensor field associated with the Carrollian structure. The investigation reveals that these transformations form a semi-direct product of the conformal Lie algebra so(d + 1,1) with ν-densities on R, resulting in infinite-dimensional Lie algebras due to the presence of super-translations.

A critical insight is provided in the case of the punctured future light-cone within Minkowski spacetime, which emerges as a Carroll manifold known to support BMS symmetry. This manifold's conformal Carroll group is rigorously formulated and validated using a sequence of transformations, establishing a connection to the BMS group for specific settings of the conformal parameter N.

Implications and Future Prospects

The theoretical advancements made in this paper clarify the role of the BMS and NU groups in the context of Carrollian structures, demonstrating their conformal nature and broadening the applicability of Carroll groups in high-energy physics and gravitational theory. This understanding could significantly impact the paper of spacetime symmetries, especially in gravitational wave physics and other related domains.

In terms of future prospects, understanding the conformal properties and Carroll symmetries may lead to new insights in the formulation of quantum gravity theories and might influence the approach toward analyzing gravitational radiation beyond the classical regime. Furthermore, the interchangeability and duality between Carroll and Newton-Cartan structures provoke a deeper inquiry into their potential applications across physical systems, including perhaps in contexts such as brane worlds or the ultra-relativistic limits of string theory.

By shedding new light on these generalized symmetries, the paper offers a substantial contribution to the discussions surrounding asymptotic symmetry groups, inviting further research into their mathematical and physical potential.