By calculating the Newman-Penrose Weyl tensor components of a perturbed spherically symmetric space-time with respect to invariantly defined classes of null tetrads, we give a physical interpretation, in terms of gravitational radiation, of odd parity gauge invariant metric perturbations. We point out how these gauge invariants may be used in setting boundary and/or initial conditions in perturbation theory
We find the transformation between static coordinates and the Newton gauge for the Schwarzschild-De-...
We consider in detail the problem of gauge dependence that exists in relativistic perturbation theor...
Many calculations in general relativity are simplified when using a tetrad formalism. As an importan...
By calculating the Newman-Penrose Weyl tensor components of a perturbed spherically symmetric space-...
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We ...
The study of cosmological perturbations brought to light misleading interpretations and solutions wi...
Abstract. We construct a covariant and gauge-invariant framework to deal with arbitrary high-order p...
We first investigate the gravitational wave in the flat Finsler spacetime. In the Finslerian univers...
We discuss the issue of observables in general-relativistic perturbation theory, adopting the view t...
We present a formalism to study the metric perturbations of the Schwarzschild spacetime. The formali...
We investigate higher than the first order gravitational perturbations in the Newman-Penrose formali...
Perturbation theory of rotating black holes is described in terms of the Weyl scalars $\psi_4$ and $...
An implicit fundamental assumption in relativistic perturbation theory is that there exists a parame...
Perturbation theory of vacuum spherically symmetric spacetimes is a crucial tool for understanding t...
Inspired by the fully non-linear Geodesic Light-Cone (GLC) gauge, we consider its analogous set of c...
We find the transformation between static coordinates and the Newton gauge for the Schwarzschild-De-...
We consider in detail the problem of gauge dependence that exists in relativistic perturbation theor...
Many calculations in general relativity are simplified when using a tetrad formalism. As an importan...
By calculating the Newman-Penrose Weyl tensor components of a perturbed spherically symmetric space-...
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We ...
The study of cosmological perturbations brought to light misleading interpretations and solutions wi...
Abstract. We construct a covariant and gauge-invariant framework to deal with arbitrary high-order p...
We first investigate the gravitational wave in the flat Finsler spacetime. In the Finslerian univers...
We discuss the issue of observables in general-relativistic perturbation theory, adopting the view t...
We present a formalism to study the metric perturbations of the Schwarzschild spacetime. The formali...
We investigate higher than the first order gravitational perturbations in the Newman-Penrose formali...
Perturbation theory of rotating black holes is described in terms of the Weyl scalars $\psi_4$ and $...
An implicit fundamental assumption in relativistic perturbation theory is that there exists a parame...
Perturbation theory of vacuum spherically symmetric spacetimes is a crucial tool for understanding t...
Inspired by the fully non-linear Geodesic Light-Cone (GLC) gauge, we consider its analogous set of c...
We find the transformation between static coordinates and the Newton gauge for the Schwarzschild-De-...
We consider in detail the problem of gauge dependence that exists in relativistic perturbation theor...
Many calculations in general relativity are simplified when using a tetrad formalism. As an importan...