Perturbations of the Vaidya metric in the frequency domain: Quasinormal modes and tidal response
The mass of a black hole can dynamically evolve due to various physical processes, such as
for instance accretion, Hawking radiation, absorption of gravitational/electromagnetic waves …
for instance accretion, Hawking radiation, absorption of gravitational/electromagnetic waves …
Love numbers and Love symmetries for p-form and gravitational perturbations of higher-dimensional spherically symmetric black holes
P Charalambous - Journal of High Energy Physics, 2024 - Springer
A bstract The static Love numbers of four-dimensional asymptotically flat, isolated, general-
relativistic black holes are known to be identically vanishing. The Love symmetry proposal …
relativistic black holes are known to be identically vanishing. The Love symmetry proposal …
Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
S Iteanu, MM Riva, L Santoni, N Savić… - arxiv preprint arxiv …, 2024 - arxiv.org
The induced conservative tidal response of self-gravitating objects in general relativity is
parametrized in terms of a set of coefficients, which are commonly referred to as Love …
parametrized in terms of a set of coefficients, which are commonly referred to as Love …
Existence and stability of relativistic fluid spheres supported by thin shells
JL Rosa, P Piçarra - Physical Review D, 2020 - APS
We propose two models for constant density relativistic perfect-fluid spheres supported by
thin-shell configurations. These models are obtained from the Schwarzschild constant …
thin-shell configurations. These models are obtained from the Schwarzschild constant …
Tidal Love numbers of Proca stars
Proca stars [1] are everywhere regular, asymptotically flat self-gravitating solitons composed
of complex, massive vector bosons, forming a macroscopic, star-sized, Bose-Einstein …
of complex, massive vector bosons, forming a macroscopic, star-sized, Bose-Einstein …
Ladder Symmetries and Love Numbers of Reissner--Nordstr\" om Black Holes
It is well known that asymptotically flat black holes in general relativity have vanishing tidal
Love numbers. In the case of Schwarzschild and Kerr black holes, this property has been …
Love numbers. In the case of Schwarzschild and Kerr black holes, this property has been …
[HTML][HTML] Effect of torsion on the radiation fields in curved spacetime
S Mandal - Physics Letters B, 2020 - Elsevier
The torsion-free connection is one of the important assumptions in Einstein's General theory
of Relativity which has not been verified so far from experimental observation. In this article …
of Relativity which has not been verified so far from experimental observation. In this article …