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) …
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 …
Component of GW190814 and Other Self-bound Strange Stars in f(Q) Gravity Theory …
Observational constraints on maximum mass limit and physical properties of anisotropic strange star models by gravitational decoupling in Einstein–Gauss–Bonnet …
In this work, we are guided by the gravitational wave events GW 170817 and GW 190814
together with observations of neutron stars PSR J1614-2230, PSR J1903+ 6620, and LMC X …
together with observations of neutron stars PSR J1614-2230, PSR J1903+ 6620, and LMC X …
Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in f (Q) f(Q) Gravity
The current theoretical development identified as the gravitational decoupling via Complete
Geometric Deformation (CGD) method that has been introduced to explore the nonmetricity …
Geometric Deformation (CGD) method that has been introduced to explore the nonmetricity …
A simple protocol to construct solutions with vanishing complexity by Gravitational Decoupling
E Contreras, Z Stuchlik - The European Physical Journal C, 2022 - Springer
In this work we develop a simple protocol to construct interior solutions through Gravitational
Decoupling by the Minimal Gemetric Deformation extended satisfying the vanishing …
Decoupling by the Minimal Gemetric Deformation extended satisfying the vanishing …
Role of Complexity on Self‐gravitating Compact Star by Gravitational Decoupling
In this paper, we study novel classes of solutions characterizing the role of complexity on
static and spherically symmetric self‐gravitating systems proposed by L. Herrera (Phys Rev …
static and spherically symmetric self‐gravitating systems proposed by L. Herrera (Phys Rev …
[HTML][HTML] Anisotropic compact stars in complexity formalism and isotropic stars made of anisotropic fluid under minimal geometric deformation (MGD) context in …
In this paper, we present an anisotropic solution for static and spherically symmetric self-
gravitating systems by demanding the vanishing of the complexity factor (Herrera in Phys …
gravitating systems by demanding the vanishing of the complexity factor (Herrera in Phys …
Influence of three parameters on maximum mass and stability of strange star under linear f(Q) − action
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) …
field using gravitational decoupling by means of the complete geometric deformation (CGD) …
Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in f (𝒬) gravity
Our current investigation is inherently linked to the observations of gravitational waves from
the GW190814 event which suggests that the source of the signals can be ascribed to a …
the GW190814 event which suggests that the source of the signals can be ascribed to a …
Energy exchange between relativistic fluids: the polytropic case
We present a simple, analytic and straightforward method to elucidate the effects produced
by polytropic fluids on any other gravitational source, no matter its nature, for static and …
by polytropic fluids on any other gravitational source, no matter its nature, for static and …
Testing strong gravitational lensing effects of various supermassive compact objects for the static and spherically symmetric hairy black hole by gravitational …
We investigate the strong gravitational lensing effects of various supermassive compact
objects for the static and spherically symmetric hairy black hole by gravitational decoupling …
objects for the static and spherically symmetric hairy black hole by gravitational decoupling …