Electron–positron pairs in physics and astrophysics: from heavy nuclei to black holes

R Ruffini, G Vereshchagin, SS Xue - Physics Reports, 2010 - Elsevier
Due to the interaction of physics and astrophysics we are witnessing in these years a
splendid synthesis of theoretical, experimental and observational results originating from …

Construction of fuzzy black holes and self-gravitational droplets in exponential f (R) gravity

S Khan, Z Yousaf - Physica Scripta, 2024 - iopscience.iop.org
Construction of fuzzy black holes and self-gravitational droplets in exponential f(R) gravity -
IOPscience Skip to content IOP Science home Accessibility Help Search Search all IOPscience …

[HTML][HTML] Decoupling gravitational sources in general relativity: The extended case

J Ovalle - Physics Letters B, 2019 - Elsevier
We show how to decoupling two spherically symmetric and static gravitational sources
through the most general possible extension of the so-called Minimal Geometric …

The effect of gravitational decoupling on constraining the mass and radius for the secondary component of GW190814 and other self-bound strange stars in f (Q) …

SK Maurya, KN Singh, M Govender… - The Astrophysical …, 2023 - iopscience.iop.org
The Effect of Gravitational Decoupling on Constraining the Mass and Radius for the Secondary
Component of GW190814 and Other Self-bound Strange Stars in f(Q) Gravity Theory …

[图书][B] Exact space-times in Einstein's general relativity

JB Griffiths, J Podolský - 2009 - books.google.com
Einstein's theory of general relativity is a theory of gravity and, as in the earlier Newtonian
theory, much can be learnt about the character of gravitation and its effects by investigating …

Stable and self-consistent compact star models in teleparallel gravity

GGL Nashed, S Capozziello - The European Physical Journal C, 2020 - Springer
In the framework of Teleparallel Gravity, we derive a charged non-vacuum solution for a
physically symmetric tetrad field with two unknown functions of radial coordinate. The field …

[图书][B] Inhomogeneous cosmological models

A Krasinski - 1997 - ui.adsabs.harvard.edu
This unique volume provides a comprehensive survey of our understanding of the Universe
based on the exact solutions of the theory of relativity. More precisely, it describes those …

Influence of three parameters on maximum mass and stability of strange star under linear f(Q) − action

SV Lohakare, SK Maurya, KN Singh… - Monthly Notices of …, 2023 - academic.oup.com
This study simulates strange stars in f (Q) gravity with an additional source under an electric
field using gravitational decoupling by means of the complete geometric deformation (CGD) …

Effects of charge and gravitational decoupling on complexity and isotropization of anisotropic models

M Sharif, T Naseer - Physics of the Dark Universe, 2023 - Elsevier
This paper constructs two immediate extensions of the existing anisotropic solutions in the
context of Einstein–Maxwell framework by employing minimal geometric deformation. To …

Study of Charged Anisotropic Karmarkar Stars in f (R, T 2) f(R,T^2) Theory

M Sharif, MZ Gul - Fortschritte der Physik, 2023 - Wiley Online Library
This paper examines the viable attributes of charged compact stars with anisotropic matter
configuration in f (R, T 2) f(R,T^2) theory. For this purpose, we use the embedding class‐1 …