We show how to calculate pseudotensor-based conserved quantities for isolated systems in general relativity, in a way which allows an arbitrary asymptotic behavior of the coordinate system used. Our method is a generalization of that given by Persides [1], and allows the asymptotic evaluation of energy, momentum, and angular momentum in any coordinate system. We carry out the calculation for the Schutz-Sorkin gravitational Noether operator, which is a pseudotensorial operator on vector fields that reduces to the familiar pseudotensors for particular choices of the fields
Indexación: ScopusA new formula for the conserved charges in 3+1 gravity for spacetimes with local a...
Using a formalism introduced by Feynman, Deser, Grishchuk, Petrov and Popova, the pseudotensors, suc...
A new formula for the conserved charges in 3+1 gravity for spacetimes with local anti-de Sitter asym...
We show how to calculate pseudotensor-based conserved quantities for isolated systems in general rel...
A method for calculating pseudotensor-based conserved quantities for isolated systems in general rel...
By using a suitable two-point scalar field, a covariant formulation of the Einstein pseudotensor is ...
The problem of finding a covariant expression for the distribution and conservation of gravitational...
As is known, the role of the energy-momentum pseudotensors of the gravitational field is to extend t...
The Lagrangian scenario is applied both to Einstein's rst and Hilbert's second order Lagra...
We derive the gravitational energy-momentum pseudotensor τσλ in metric f(R) gravity and in teleparal...
We derive conservation laws in Symmetric Teleparallel Equivalent of General Relativity (STEGR) with ...
The problem of finding a covariant expression for the distribution and conservation of gravitational...
The problem of non-localizability and the non-uniqueness of gravitational energy in general relativi...
We examine various methods of constructing conserved quantities in the Teleparallel Equivalent of Ge...
A new, general, field theoretic approach to the derivation of asymptotic conservation laws is presen...
Indexación: ScopusA new formula for the conserved charges in 3+1 gravity for spacetimes with local a...
Using a formalism introduced by Feynman, Deser, Grishchuk, Petrov and Popova, the pseudotensors, suc...
A new formula for the conserved charges in 3+1 gravity for spacetimes with local anti-de Sitter asym...
We show how to calculate pseudotensor-based conserved quantities for isolated systems in general rel...
A method for calculating pseudotensor-based conserved quantities for isolated systems in general rel...
By using a suitable two-point scalar field, a covariant formulation of the Einstein pseudotensor is ...
The problem of finding a covariant expression for the distribution and conservation of gravitational...
As is known, the role of the energy-momentum pseudotensors of the gravitational field is to extend t...
The Lagrangian scenario is applied both to Einstein's rst and Hilbert's second order Lagra...
We derive the gravitational energy-momentum pseudotensor τσλ in metric f(R) gravity and in teleparal...
We derive conservation laws in Symmetric Teleparallel Equivalent of General Relativity (STEGR) with ...
The problem of finding a covariant expression for the distribution and conservation of gravitational...
The problem of non-localizability and the non-uniqueness of gravitational energy in general relativi...
We examine various methods of constructing conserved quantities in the Teleparallel Equivalent of Ge...
A new, general, field theoretic approach to the derivation of asymptotic conservation laws is presen...
Indexación: ScopusA new formula for the conserved charges in 3+1 gravity for spacetimes with local a...
Using a formalism introduced by Feynman, Deser, Grishchuk, Petrov and Popova, the pseudotensors, suc...
A new formula for the conserved charges in 3+1 gravity for spacetimes with local anti-de Sitter asym...