Self-similarity in general relativity

BJ Carr, AA Coley - Classical and Quantum Gravity, 1999 - iopscience.iop.org
The different kinds of self-similarity in general relativity are discussed, with special emphasis
on similarity of thefirst'kind, corresponding to spacetimes admitting a homothetic vector. We …

Structure scalars of spherically symmetric dissipative fluids with gravity

Z Yousaf - Astrophysics and Space Science, 2018 - Springer
The aim of this study is to analyze the role of modification of gravity on some dynamical
properties of spherically symmetric relativistic systems. In this settings, the mathematical …

The Final fate of spherical inhomogeneous dust collapse

TP Singh, PS Joshi - Classical and Quantum Gravity, 1996 - iopscience.iop.org
We examine, in a general manner, the role played by the initial density and velocity
distributions in the gravitational collapse of a spherically symmetric inhomogeneous dust …

Gravitational collapse: the story so far

PS Joshi - Pramana, 2000 - Springer
An outstanding problem in gravitation theory and relativistic astrophysics today is to
understand the final outcome of an endless gravitational collapse. Such a continual collapse …

Tilted Lemaitre-Tolman-Bondi spacetimes: hydrodynamic and thermodynamic properties

L Herrera, A Di Prisco, J Ibáñez - … Review D—Particles, Fields, Gravitation, and …, 2011 - APS
We consider Lemaitre-Tolman-Bondi spacetimes from the point of view of a tilted observer,
ie one with respect to which the fluid is radially moving. The imperfect fluid and the …

Invariant characterization of the growing and decaying density modes in LTB dust models

RA Sussman - Classical and Quantum Gravity, 2013 - iopscience.iop.org
We obtain covariant expressions that generalize the growing and decaying density modes of
linear perturbation theory of dust sources by means of the exact density perturbation from …

Hypothesis of path integral duality. I. Quantum gravitational corrections to the propagator

T Padmanabhan - Physical Review D, 1998 - APS
The action for a relativistic free particle of mass m receives a contribution− m R (x, y) from a
path of length R (x, y) connecting the events xi and y i. Using this action in a path integral …

Collapsing scenario for the k-essence emergent generalized Vaidya spacetime in the context of massive gravity's rainbow

S Ray, A Panda, B Majumder, MR Islam… - Chinese Physics …, 2022 - iopscience.iop.org
In this study, we investigate the collapsing scenario for the k-essence emergent Vaidya
spacetime in the context of massive gravity's rainbow. For this study, we consider that the …

Initial data and the end state of spherically symmetric gravitational collapse

PS Joshi, IH Dwivedi - Classical and Quantum Gravity, 1999 - iopscience.iop.org
Generalizing earlier results on the initial data and the final fate of dust collapse, we study
here the relevance of the initial state of a spherically symmetric matter cloud towards …

Hyperbolically symmetric versions of Lemaitre–Tolman–Bondi spacetimes

L Herrera, A Di Prisco, J Ospino - Entropy, 2021 - mdpi.com
We study fluid distributions endowed with hyperbolic symmetry, which share many common
features with Lemaitre–Tolman–Bondi (LTB) solutions (eg, they are geodesic, shearing, and …