A new formula for the conserved charges in 3+1 gravity for spacetimes with local anti-de Sitter asymptotic geometry is proposed. It is shown that requiring the action to have an extremum for this class of asymptotia sets the boundary term that must be added to the Lagrangian as the Euler density with a fixed weight factor. The resulting action gives rise to the mass and angular momentum as Noether charges associated to the asymptotic Killing vectors without requiring specification of a reference background in order to have a convergent expression. A consequence of this definition is that any negative constant curvature spacetime has vanishing Noether charges. These results remain valid in the Λ = 0 limit. © 2000 American Physical Society
WOS:000458820400006We give a new construction of conserved charges in asymptotically anti-de Sitter ...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. On...
WOS:000458375300008Starting from a divergence-free rank-4 tensor of which the trace is the cosmologi...
Indexación: ScopusA new formula for the conserved charges in 3+1 gravity for spacetimes with local a...
A new formula for the conserved charges in 3+1 gravity for spacetimes with local AdS asymptotic geom...
Mass and other conserved Noether charges are discussed for solutions of gravity theories with locall...
We review issues related to conservation laws for gravity with a negative cosmological constant subj...
We review issues related to conservation laws for gravity with a negative cosmological constant subj...
Indexación: ScopusMass and other conserved Noether charges are discussed for solutions of gravity th...
We give a detailed review of construction of conserved quantities in extended theories of gravity fo...
Energy, and more generally conserved charges, is a subtle issue in general relativity and it is subj...
We extend the Abbott-Deser-Tekin procedure of defining conserved quantities of asymptotically consta...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. On...
The calculation of conserved charges of black holes is a rich problem, for which many methods are kn...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. O...
WOS:000458820400006We give a new construction of conserved charges in asymptotically anti-de Sitter ...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. On...
WOS:000458375300008Starting from a divergence-free rank-4 tensor of which the trace is the cosmologi...
Indexación: ScopusA new formula for the conserved charges in 3+1 gravity for spacetimes with local a...
A new formula for the conserved charges in 3+1 gravity for spacetimes with local AdS asymptotic geom...
Mass and other conserved Noether charges are discussed for solutions of gravity theories with locall...
We review issues related to conservation laws for gravity with a negative cosmological constant subj...
We review issues related to conservation laws for gravity with a negative cosmological constant subj...
Indexación: ScopusMass and other conserved Noether charges are discussed for solutions of gravity th...
We give a detailed review of construction of conserved quantities in extended theories of gravity fo...
Energy, and more generally conserved charges, is a subtle issue in general relativity and it is subj...
We extend the Abbott-Deser-Tekin procedure of defining conserved quantities of asymptotically consta...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. On...
The calculation of conserved charges of black holes is a rich problem, for which many methods are kn...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. O...
WOS:000458820400006We give a new construction of conserved charges in asymptotically anti-de Sitter ...
We discuss the definition of conserved quantities in asymptotically locally de Sitter spacetimes. On...
WOS:000458375300008Starting from a divergence-free rank-4 tensor of which the trace is the cosmologi...