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Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution
We systematically review some standard issues and also the latest developments of
modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time …
modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time …
Heavy baryons in compact stars
We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …
covariant density functional approach to the equation of state and composition of dense …
Physical characteristics and maximum allowable mass of hybrid star in the context of f(Q) gravity
In this study, we explore several new characteristics of a static anisotropic hybrid star with
strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we use …
strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we use …
[HTML][HTML] Causal limit of neutron star maximum mass in f (R) gravity in view of GW190814
We investigate the causal limit of maximum mass for stars in the framework of f (R) gravity.
We choose a causal equation of state, with variable speed of sound, and with the transition …
We choose a causal equation of state, with variable speed of sound, and with the transition …
Stellar structure models in modified theories of gravity: Lessons and challenges
The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …
nuclear force and the gravitational interaction under the most extreme conditions observably …
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) …
[HTML][HTML] Extended gravity description for the GW190814 supermassive neutron star
Very recently a compact object with a mass in the range 2.50÷ 2.67 M⊙ has been
discovered via gravitational waves detection of a compact binary coalescence. The mass of …
discovered via gravitational waves detection of a compact binary coalescence. The mass of …
Finch–Skea Stellar structures obeying Karmarkar condition in modified f (G) gravity
The current research addresses the composition and modeling of compact dense
astrophysical objects in a renowned modified gravity namely f (G) theory, where G denotes …
astrophysical objects in a renowned modified gravity namely f (G) theory, where G denotes …
Extending Anisotropic Interiors admitting Vanishing Complexity in Charged f (R, T) Theory
This paper extends the definition of the complexity factor for a charged self‐gravitating
structure in the background of f (R, T) f(R,T) gravity. For this purpose, the modified Einstein …
structure in the background of f (R, T) f(R,T) gravity. For this purpose, the modified Einstein …
Anisotropic charged stellar models with modified Van der Waals EoS in f(Q) gravity
This paper is based on the study of compact stars in the context of electric fields and the
nonmetricity effects of gravity. Due to this, we are motivated to build stellar models based on …
nonmetricity effects of gravity. Due to this, we are motivated to build stellar models based on …