International audienceIn General Relativity, the allowed set of diffeomorphisms or gauge transformations at asymptotic infinity forms the BMS group, an infinite-dimensional extension of the Poincaré group. We focus on the structure of the BMS group in two distinct forms of Hamiltonian dynamics - the instant and front forms. Both similarities and differences in these two forms are examined while emphasising the role of non-covariant approaches to symmetries in gravity
International audienceNew boundary conditions for asymptotically flat spacetimes are given at spatia...
Diffeomorphisms in general relativity can act non-trivially on the boundary of spacetimes. Of partic...
We show that we can derive the asymptotic Einstein's equations that arises at order 1/r in asymptoti...
International audienceIn General Relativity, the allowed set of diffeomorphisms or gauge transformat...
International audienceIn General Relativity, the allowed set of diffeomorphisms or gauge transformat...
In General Relativity, the allowed set of diffeomorphisms or gauge transformations at asymptotic inf...
A short overview of the role of BMS symmetries in various approaches to the flat spacetime holograph...
The Bondi-Metzner-Sachs-van der Burg (BMS) group is the asymptotic symmetry group of radiating asymp...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
Abstract The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asympt...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asymptotically ...
We work out the description of the gauge symmetry of unimodular gravity in the constrained Hamiltoni...
Abstract New boundary conditions for asymptotically flat spacetimes are given at spatial infinity. T...
International audienceNew boundary conditions for asymptotically flat spacetimes are given at spatia...
Diffeomorphisms in general relativity can act non-trivially on the boundary of spacetimes. Of partic...
We show that we can derive the asymptotic Einstein's equations that arises at order 1/r in asymptoti...
International audienceIn General Relativity, the allowed set of diffeomorphisms or gauge transformat...
International audienceIn General Relativity, the allowed set of diffeomorphisms or gauge transformat...
In General Relativity, the allowed set of diffeomorphisms or gauge transformations at asymptotic inf...
A short overview of the role of BMS symmetries in various approaches to the flat spacetime holograph...
The Bondi-Metzner-Sachs-van der Burg (BMS) group is the asymptotic symmetry group of radiating asymp...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
Abstract The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asympt...
International audienceThe spacetime in the interior of a black hole can be described by an homogeneo...
The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asymptotically ...
We work out the description of the gauge symmetry of unimodular gravity in the constrained Hamiltoni...
Abstract New boundary conditions for asymptotically flat spacetimes are given at spatial infinity. T...
International audienceNew boundary conditions for asymptotically flat spacetimes are given at spatia...
Diffeomorphisms in general relativity can act non-trivially on the boundary of spacetimes. Of partic...
We show that we can derive the asymptotic Einstein's equations that arises at order 1/r in asymptoti...