A class of black holes in dRGT massive gravity and their thermodynamical properties

SG Ghosh, L Tannukij, P Wongjun - The European Physical Journal C, 2016 - Springer
We present an exact spherical black hole solution in de Rham, Gabadadze, and Tolley
(dRGT) massive gravity for a generic choice of the parameters in the theory, and also …

Analysis of birefringence and dispersion effects from spacetime-symmetry breaking in gravitational waves

K O'Neal-Ault, QG Bailey, T Dumerchat, L Haegel… - Universe, 2021 - mdpi.com
In this work, we review the effective field theory framework to search for Lorentz and CPT
symmetry breaking during the propagation of gravitational waves. The article is written so as …

Gauge symmetries and the Higgs mechanism in Quantum Finance

I Arraut - Europhysics Letters, 2023 - iopscience.iop.org
By using the Hamiltonian formulation, we demonstrate that the Merton-Garman equation
emerges naturally from the Black-Scholes equation after imposing invariance (symmetry) …

The Nambu–Goldstone theorem in nonrelativistic systems

I Arraut - International Journal of Modern Physics A, 2017 - World Scientific
In nonrelativistic systems, when there is spontaneous symmetry breaking, the number of
Nambu–Goldstone bosons (n NG) are not necessarily equal to the number of broken …

Time dependent geometry in massive gravity

Y Heydarzade, P Rudra, B Pourhassan… - … of Cosmology and …, 2018 - iopscience.iop.org
In this paper, we will analyze a time dependent geometry in a massive theory of gravity. This
will be done by analyzing Vaidya spacetime in such a massive theory of gravity. As …

Path-integral derivation of black-hole radiance inside the de-Rham–Gabadadze–Tolley formulation of massive gravity

I Arraut - The European Physical Journal C, 2017 - Springer
If we apply the path-integral formulation in order to analyze the particle creation process of
black holes inside the non-linear formulation of massive gravity, it is possible to demonstrate …

The quantum regularization of singular black-hole solutions in covariant quantum gravity

M Tessarotto, C Cremaschini - Entropy, 2021 - mdpi.com
An excruciating issue that arises in mathematical, theoretical and astro-physics concerns the
possibility of regularizing classical singular black hole solutions of general relativity by …

Non-linear massive gravity as a gravitational σ-model

I Arraut, K Chelabi - Europhysics Letters, 2016 - iopscience.iop.org
We show the direct analogy between the ghost-free non-linear formulation of massive
gravity and the standard σ-models well understood in the literature. This issue explains why …

[PDF][PDF] SOLVING THE DARK ENERGY PROBLEM VIA SYMMETRY CONSTRAINT

I Arraut, EM da Ilha Verde - 2024 - researchgate.net
We derive the vacuum energy from the zero-point quantum fluctuations after imposing a
natural constraint emerging from the rotational symmetry inside the de-Sitter metric. The …

[HTML][HTML] How to Determine Initial Starting Time Step with an Initial Hubble Parameter H= 0 after Formation of Causal Structure Leading to Investigation of the Penrose …

AW Beckwith - Journal of High Energy Physics, Gravitation and …, 2018 - scirp.org
We start where we use an inflaton value due to use of a scale factor. Also we use as the
variation of the time component of the metric tensor in Pre-Planckian Space-time. In doing …