papers

Publications (21)

gr-qc2014

Causal heat flow in Bianchi type-V universe

M. Govender, S. Thirukkanesh

In this paper we investigate the role of causal heat transport in a spatially homogeneous, locally-rotationally symmetric Bianchi type-V cosmological model. In particular, the caus…

gr-qc2021

Gravitationally decoupled strange star model beyond standard maximum mass limit in Einstein-Gauss-Bonnet gravity

S. K. Maurya, Ksh. Newton Singh, M. Govender +1

The recent theoretical advance known as the Minimal Geometric Deformation (MGD) method has initiated a renewed interest in investigating higher curvature gravitational effects in r…

gr-qc2017

Anisotropic stars for spherically symmetric spacetimes satisfying the Karmarkar condition

S. K. Maurya, B. S. Ratanpal, M. Govender

A new class of solution describing an anisotropic stellar configuration satisfying Karmarkar's condition i.e. spherically symmetric metric of embedding class 1, is reported. It has…

gr-qc2002

Radiating spherical collapse with heat flow

M. Govender

We present here a simple model of radiative gravitational collapse with radial heat flux which describes qualitatively the stages close to the formation of a superdense cold star.…

gr-qc2017

A family of charged compact objects with anisotropic pressure

S. K. Maurya, M. Govender

Utilizing an ansatz developed by Maurya and co-workers we present a class of exact solutions of the Einstein-Maxwell field equations describing a spherically symmetric compact obje…

gr-qc2026

Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows

A. Errehymy, S. K. Maurya, M. Govender +4

In this work, we explore for the first time slowly rotating traversable wormholes embedded in holographic dark energy. We focus on three representative holographic dark energy mode…

gr-qc2010

Thermal Behaviour of Euclidean Stars

G. Govender, M. Govender, K. S. Govinder

A recent study of dissipative collapse considered a contracting sphere in which the areal and proper radii are equal throughout its evolution. The interior spacetime was matched to…

gr-qc2025

Anisotropic Spacetimes in -gravity: Bianchi I, Bianchi III and Kantowski-Sachs Cosmologies

R. Bogadi, A. Giacomini, M. Govender +3

We investigate the evolution of cosmological anisotropies within the framework of -gravity. Specifically, we consider a locally rotationally symmetric geometry in…

gr-qc2023

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

S. K. Maurya, K. N. Singh, M. Govender +2

Inspired by the conundrum of the gravitational event, GW190814 which brings to light the coalescence of a 23 black hole with a yet to be determined secondary component…

gr-qc2014

Non-adiabatic spherical collapse with a two-fluid atmosphere

M. Govender

In this work we present an exact model of a spherically symmetric star undergoing dissipative collapse in the form of a radial heat flux. The interior of the star is matched smooth…

gr-qc2022

Thermodynamical aspects of Bianchi type-I Universe in quadratic form of gravity and observational constraints

M. Koussour, S. H. Shekh, M. Govender +1

In this paper, we discuss the Bianchi type-I cosmological model in the framework of symmetric teleparallel gravity say gravity in which the non-metricity term is respons…

gr-qc2024

Dynamical stability of new wormhole solutions via cold dark matter and solitonic quantum wave halos in gravity

G. Mustafa, Faisal Javed, S. K. Maurya +2

This current analysis offers novel wormhole solutions in the background of newly developed extended gravity. We use an anisotropic matter source and…

physics.gen-ph2017

Generating physically realizable stellar structures via embedding

S. K. Maurya, M. Govender

In this work we present an exact solution of the Einstein-Maxwell field equations describing compact, charged objects within the framework of classical general relativity. Our mode…

gr-qc2013

The role of shear in dissipative gravitational collapse

M. Govender, K. P. Reddy, S. D. Maharaj

In this paper we investigate the physics of a radiating star undergoing dissipative collapse in the form of a radial heat flux. Our treatment clearly demonstrates how the presence…

physics.gen-ph2016

Anisotropic compact stars in Karmarkar spacetime

Ksh. Newton Singh, Neeraj Pant, M. Govender

We present a new class of solutions to the Einstein field equations for an anisotropic matter distribution in which the interior space-time obeys the Karmarkar condition. The neces…

gr-qc2013

Radiating stars with generalised Vaidya atmospheres

S. D. Maharaj, G. Govender, M. Govender

We model the gravitational behaviour of a radiating star when the exterior geometry is the generalised Vaidya spacetime. The interior matter distribution is shear-free and undergoi…

gr-qc2026

Asymptotic Solutions of Radiating Stars

R. S. Bogadi, G. Leon, M. Govender +3

We investigate the evolution of the surface of radiating stars by studying the asymptotic behaviour of exact solutions initiated via the stationary boundary condition. This boundar…

gr-qc2024

Influence of pressure anisotropy and non-metricity parameter on mass-radius relation and stability of millisecond pulsar in gravity

S. K. Maurya, Ksh. Newton Singh, G. Mustafa +3

In this study we explore the astrophysical implications of pressure anisotropy on the physical characteristics of millisecond pulsars within the framework of gravity, {in pa…

gr-qc2017

Physical viability of fluid spheres satisfying the Karmarkar condition

Ksh. Newton Singh, Neeraj Pant, M. Govender

We obtain a new solution of the TOV-equation for an anisotropic fluid distribution by imposing the Karmarkar condition. In order to close the system of equations we postulate an in…

gr-qc2020

Charged anisotropic strange stars in Brans-Dicke gravity with a massive scalar field through embedding approach

S. K. Maurya, Ksh. Newton Singh, M. Govender +1

In this exposition, we seek solutions of the Einstein-Maxwell field equations in the presence of a massive scalar field cast in the Brans-Dicke (BD) formalism which describes charg…

gr-qc2022

Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in gravity

S. K. Maurya, G. Mustafa, M. Govender +1

In this work we take our cue from the observations of gravitational waves of the GW190814 event which suggests that source of the signals can be ascribed to a compact binary coales…