In several areas of theoretical physics it is useful to know how a quasilocal energy transforms under conformal rescalings or generalized Kerr–Schild mappings. We derive the transformation properties of the Brown–York quasilocal energy in spherical symmetry and we contrast them with those of the Misner–Sharp–Hernandez energy
Restricted Access.We present a detailed examination of the variational principle for metric general ...
Dynamics at large redshift near the horizon of an extreme Kerr black hole are governed by an infinit...
Based on the quasi-local energy definition of Brown and York, we compute the integral of the trace o...
A key feature of the Brown-York definition of quasilocal energy is that, under local boosts of the f...
We derive a formula describing the transformation of the Hawking-Hayward quasi-local energy under a ...
The Misner–Sharp–Hernandez mass defined in general relativity and in spherical symmetry has been rec...
In this work we investigate current research on quasilocal energy and conservation laws in general r...
We propose a method to define and investigate finite size systems in general relativity in terms of...
Quasilocal definitions of stress-energy-momentum-that is, in the form of boundary densities (rather ...
We construct a Hamiltonian formulation of quasi-local general relativity using an extended phase spa...
Consider the definition E of quasilocal energy stemming from the Hamilton-Jacobi method as applied t...
The quasilocal energy of gravitational and matter fields in a spatially bounded region is obtained b...
We investigate the thermodynamics of Einstein–Maxwell (-dilaton) theory for an asymptotically flat s...
The problems of the tolal energy and quasilocalenergy density or an isolated spherically symmetric s...
We show that in a generic scalar-tensor theory of gravity, the ``referenced'' quasilocal mass of a s...
Restricted Access.We present a detailed examination of the variational principle for metric general ...
Dynamics at large redshift near the horizon of an extreme Kerr black hole are governed by an infinit...
Based on the quasi-local energy definition of Brown and York, we compute the integral of the trace o...
A key feature of the Brown-York definition of quasilocal energy is that, under local boosts of the f...
We derive a formula describing the transformation of the Hawking-Hayward quasi-local energy under a ...
The Misner–Sharp–Hernandez mass defined in general relativity and in spherical symmetry has been rec...
In this work we investigate current research on quasilocal energy and conservation laws in general r...
We propose a method to define and investigate finite size systems in general relativity in terms of...
Quasilocal definitions of stress-energy-momentum-that is, in the form of boundary densities (rather ...
We construct a Hamiltonian formulation of quasi-local general relativity using an extended phase spa...
Consider the definition E of quasilocal energy stemming from the Hamilton-Jacobi method as applied t...
The quasilocal energy of gravitational and matter fields in a spatially bounded region is obtained b...
We investigate the thermodynamics of Einstein–Maxwell (-dilaton) theory for an asymptotically flat s...
The problems of the tolal energy and quasilocalenergy density or an isolated spherically symmetric s...
We show that in a generic scalar-tensor theory of gravity, the ``referenced'' quasilocal mass of a s...
Restricted Access.We present a detailed examination of the variational principle for metric general ...
Dynamics at large redshift near the horizon of an extreme Kerr black hole are governed by an infinit...
Based on the quasi-local energy definition of Brown and York, we compute the integral of the trace o...