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相关论文: The Bondi-Metzner-Sachs group in five spacetime di…

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The asymptotic symmetry algebra of four-dimensional Einstein gravity in the asymptotically flat context has been shown recently to be the direct sum of the Poincar\'e algebra and of an infinite-dimensional abelian algebra (with central…

高能物理 - 理论 · 物理学 2024-02-21 Oscar Fuentealba , Marc Henneaux , Cédric Troessaert

A review of our results on the asymptotic structure of gravity at spatial infinity in four spacetime dimensions is given. Finiteness of the action and integrability of the asymptotic Lorentz boost generators are key criteria that we…

高能物理 - 理论 · 物理学 2023-06-06 Marc Henneaux , Cédric Troessaert

We develop the analysis of the asymptotic properties of gravity in higher spacetime dimensions $D$, with a particular emphasis on the case $D=5$. Our approach deals with spatial infinity and is Hamiltonian throughout. It is shown that the…

高能物理 - 理论 · 物理学 2022-08-10 Oscar Fuentealba , Marc Henneaux , Javier Matulich , Cédric Troessaert

Asymptotically flat spacetimes have been studied in five separate regions: future/past timelike infinity $i^\pm$, future/past null infinity $\mathcal{I}^\pm$, and spatial infinity $i^0$. We formulate assumptions and definitions such that…

广义相对论与量子宇宙学 · 物理学 2023-11-21 Geoffrey Compère , Samuel E. Gralla , Hongji Wei

We propose a consistent set of boundary conditions for gravity in asymptotically flat spacetime at spacelike infinity, which yields an enhancement of the Bondi-Metzner Sachs group with smooth superrotations and new subleading symmetries.…

高能物理 - 理论 · 物理学 2024-11-19 Adrien Fiorucci , Javier Matulich , Romain Ruzziconi

The asymptotic structure of three-dimensional hypergravity without cosmological constant is analyzed. In the case of gravity minimally coupled to a spin-$5/2$ field, a consistent set of boundary conditions is proposed, being wide enough so…

高能物理 - 理论 · 物理学 2015-11-05 Oscar Fuentealba , Javier Matulich , Ricardo Troncoso

In this paper we establish two results concerning four-dimensional asymptotically flat spacetimes at spatial infinity. First, we show that the six conserved Lorentz charges are encoded in two unique, distinct, but mutually dual symmetric…

广义相对论与量子宇宙学 · 物理学 2015-05-27 Geoffrey Compère , François Dehouck , Amitabh Virmani

We analyse the asymptotic symmetries of Maxwell theory at spatial infinity through the Hamiltonian formalism. Precise, consistent boundary conditions are explicitly given and shown to be invariant under asymptotic angle-dependent…

高能物理 - 理论 · 物理学 2018-05-30 Marc Henneaux , Cédric Troessaert

The Bondi-Metzner-Sachs-van der Burg (BMS) group is the asymptotic symmetry group of radiating asymptotically flat spacetimes. It has recently received renewed interest in the context of the flat holography and the infrared structure of…

高能物理 - 理论 · 物理学 2020-09-07 Romain Ruzziconi

It is argued that the symmetry algebra of asymptotically flat spacetimes at null infinity in 4 dimensions should be taken as the semi-direct sum of supertranslations with infinitesimal local conformal transformations and not, as usually…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Glenn Barnich , Cedric Troessaert

Four-dimensional asymptotically flat spacetimes at spatial infinity are defined from first principles without imposing parity conditions or restrictions on the Weyl tensor. The Einstein-Hilbert action is shown to be a correct variational…

高能物理 - 理论 · 物理学 2015-05-28 Geoffrey Compère , François Dehouck

This work is a pedagogical review dedicated to a modern description of the Bondi-Metzner-Sachs group. The curved space-times that will be taken into account are the ones that suitably approach, at infinity, Minkowski space-time. In…

广义相对论与量子宇宙学 · 物理学 2019-01-24 Francesco Alessio , Giampiero Esposito

It is natural to regulate an infinite-sized system by imposing a boundary condition at finite distance, placing the system in a "box." This breaks symmetries, though the breaking is small when the box is large. One should thus be able to…

广义相对论与量子宇宙学 · 物理学 2015-12-16 Tomas Andrade , Donald Marolf

The purpose of this dissertation is to examine the BMS symmetry group, which arises as the asymptotic symmetry group of four-dimensional asymptotically flat spacetimes at null infinity, and to uncover its relation to the Carroll group.…

广义相对论与量子宇宙学 · 物理学 2018-05-28 Yvonne Calò

The asymptotic structure of null and spatial infinities of asymptotically flat spacetimes plays an essential role in discussing gravitational radiation, gravitational memory effect, and conserved quantities in General Relativity. Bondi,…

广义相对论与量子宇宙学 · 物理学 2025-12-01 Mariem Magdy

We present a new set of asymptotic conditions for gravity at spatial infinity that includes gravitational magnetic-type solutions, allows for a non-trivial Hamiltonian action of the complete $BMS_4$ algebra, and leads to a non-divergent…

广义相对论与量子宇宙学 · 物理学 2018-08-15 Marc Henneaux , Cédric Troessaert

We show that the non-linear BMS$_5$ symmetry algebra of asymptotically flat Einstein gravity in five dimensions, as well as the super-BMS$_4$ superalgebra of asymptotically flat supergravity, can be redefined so as to take a direct sum…

高能物理 - 理论 · 物理学 2023-09-15 Oscar Fuentealba , Marc Henneaux

After a review of symmetries and classical solutions involved in the AdS3/CFT2 correspondence, we apply a similar analysis to asymptotically flat spacetimes at null infinity in 3 and 4 dimensions. In the spirit of two dimensional conformal…

高能物理 - 理论 · 物理学 2010-12-09 Glenn Barnich , Cedric Troessaert

We explore the holographic principle in the context of asymptotically flat space-times by means of the asymptotic symmetry group of this class of space-times, the so called Bondi-Metzner-Sachs (BMS) group. In particular we construct a…

高能物理 - 理论 · 物理学 2008-11-26 Claudio Dappiaggi

The symmetry algebra of asymptotically flat spacetimes at null infinity in four dimensions in the sense of Newman and Unti is revisited. As in the Bondi-Metzner-Sachs gauge, it is shown to be isomorphic to the direct sum of the abelian…

广义相对论与量子宇宙学 · 物理学 2013-01-24 Glenn Barnich , Pierre-Henry Lambert
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