In this paper we consider gauge invariant linear perturbations of the metric and matter tensors describing the self-similar Lemaitre-Tolman-Bondi (timelike dust) spacetime containing a naked singularity. We decompose the angular part of the perturbation in terms of spherical harmonics and perform a Mellin transform to reduce the perturbation equations to a set of ordinary differential equations with singular points. We fix initial data so the perturbation is finite on the axis and the past null cone of the singularity, and follow the perturbation modes up to the Cauchy horizon. There we argue that certain scalars formed from the modes of the perturbation remain finite, indicating linear stability of the Cauchy horizon
Abstract. We construct a covariant and gauge-invariant framework to deal with arbitrary high-order p...
The background of this thesis is the cosmic censorship hypothesis, which states that the gravitation...
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We ...
In this paper we consider gauge invariant linear perturbations of the metric and matter tensors desc...
In this paper we consider gauge invariant linear perturbations of the metric and matter tensors desc...
We study even parity metric and matter perturbations of all angular modes in self-similar Vaidya spa...
Certain classes of solutions to Einstein’s field equations admit singularities from which light can ...
We carry out an analytic study of odd-parity perturbations of the self-similar Vaidya space-times th...
Lemaitre-Tolman-Bondi (LTB) solutions are used frequently to describe the collapse or expansion of s...
The naked singularity occurs in the generic collapse of an inhomogeneous dust ball. We study even-pa...
The motion of a spherical dust cloud is described by the Lemaitre-Tolman-Bondi solution and is compl...
It has been suggested that a naked singularity is a good candidate for a strong gravita-tional wave ...
Perturbation theory of vacuum spherically symmetric spacetimes is a crucial tool for understanding t...
By calculating the Newman-Penrose Weyl tensor components of a perturbed spherically symmetric space-...
The covariant gauge-invariant perturbation theory of scalar cosmological perturbations is developed ...
Abstract. We construct a covariant and gauge-invariant framework to deal with arbitrary high-order p...
The background of this thesis is the cosmic censorship hypothesis, which states that the gravitation...
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We ...
In this paper we consider gauge invariant linear perturbations of the metric and matter tensors desc...
In this paper we consider gauge invariant linear perturbations of the metric and matter tensors desc...
We study even parity metric and matter perturbations of all angular modes in self-similar Vaidya spa...
Certain classes of solutions to Einstein’s field equations admit singularities from which light can ...
We carry out an analytic study of odd-parity perturbations of the self-similar Vaidya space-times th...
Lemaitre-Tolman-Bondi (LTB) solutions are used frequently to describe the collapse or expansion of s...
The naked singularity occurs in the generic collapse of an inhomogeneous dust ball. We study even-pa...
The motion of a spherical dust cloud is described by the Lemaitre-Tolman-Bondi solution and is compl...
It has been suggested that a naked singularity is a good candidate for a strong gravita-tional wave ...
Perturbation theory of vacuum spherically symmetric spacetimes is a crucial tool for understanding t...
By calculating the Newman-Penrose Weyl tensor components of a perturbed spherically symmetric space-...
The covariant gauge-invariant perturbation theory of scalar cosmological perturbations is developed ...
Abstract. We construct a covariant and gauge-invariant framework to deal with arbitrary high-order p...
The background of this thesis is the cosmic censorship hypothesis, which states that the gravitation...
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We ...