We consider four-dimensional spacetimes which are asymptotically flat at spatial infinity and show that, in the first-order framework, the action principle for general relativity is well defined without the need of infinite counter terms. It naturally leads to a covariant phase space in which the Hamiltonians generating asymptotic symmetries provide the total energy–momentum and angular momentum of the spacetime. We address the subtle but important problems that arise because of logarithmic translations and super translations both in the Lagrangian and Hamiltonian frameworks. As a forthcoming paper will show, the treatment of higher dimensions is considerably simpler. Our first-order framework also suggests a new direction for generalizing ...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
We show that the on-shell path integral for asymptotically flat Euclidean spacetimes can be given in...
We consider four-dimensional spacetimes which are asymptotically flat at spatial infinity and show t...
18 pages, No figures. Added a footnote 2 and two referencesInternational audienceWe consider 4-dimen...
We consider four-dimensional spacetimes which are asymptotically flat at spatial infinity and show t...
Four-dimensional asymptotically flat spacetimes at spatial infinity are defined from first principle...
Four-dimensional asymptotically flat spacetimes at spatial infinity are defined from first principle...
Proper understanding of the geometry on the boundary of a spacetime is a critical step on the way to...
We present a new set of asymptotic conditions for gravity at spatial infinity that includes gravitat...
Abstract We present a new set of asymptotic conditions for gravity at spatial infinity that includes...
Abstract Proper understanding of the geometry on the boundary of a spacetime is a critical step on t...
International audienceWe present a new set of asymptotic conditions for gravity at spatial infinity ...
We present a new set of asymptotic conditions for gravity at spatial infinity that includes gravitat...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
We show that the on-shell path integral for asymptotically flat Euclidean spacetimes can be given in...
We consider four-dimensional spacetimes which are asymptotically flat at spatial infinity and show t...
18 pages, No figures. Added a footnote 2 and two referencesInternational audienceWe consider 4-dimen...
We consider four-dimensional spacetimes which are asymptotically flat at spatial infinity and show t...
Four-dimensional asymptotically flat spacetimes at spatial infinity are defined from first principle...
Four-dimensional asymptotically flat spacetimes at spatial infinity are defined from first principle...
Proper understanding of the geometry on the boundary of a spacetime is a critical step on the way to...
We present a new set of asymptotic conditions for gravity at spatial infinity that includes gravitat...
Abstract We present a new set of asymptotic conditions for gravity at spatial infinity that includes...
Abstract Proper understanding of the geometry on the boundary of a spacetime is a critical step on t...
International audienceWe present a new set of asymptotic conditions for gravity at spatial infinity ...
We present a new set of asymptotic conditions for gravity at spatial infinity that includes gravitat...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
International audienceThe Hamiltonian analysis for the Einstein's action in G-->0 limit is performed...
We show that the on-shell path integral for asymptotically flat Euclidean spacetimes can be given in...