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Cosmological observational constraints on the power law f(Q) type modified gravity theory
In modern cosmology, the curiosity of ultimately understanding the nature of the dark energy
controlling the recent acceleration of the Universe motivates us to explore its properties by …
controlling the recent acceleration of the Universe motivates us to explore its properties by …
Late-time cosmology with phantom dark-energy in f (Q) gravity
Motivated by the exciting features and a recent proposed general form of the function of non-
metricity scalar Q, we investigate the cosmological implications in f (Q) gravity, through the …
metricity scalar Q, we investigate the cosmological implications in f (Q) gravity, through the …
Dark matter as a Weyl geometric effect
We investigate the possibility that the observed behavior of test particles outside galaxies,
which is usually explained by assuming the existence of dark matter, is the result of the …
which is usually explained by assuming the existence of dark matter, is the result of the …
Linear redshift parametrization of deceleration parameter in f (R, Lm) gravity
In this study, we investigate the linear redshift parametrization of q (z) within the framework
of f (R, L m) gravity, using constraints derived from H (z)/P antheon samples. We consider a …
of f (R, L m) gravity, using constraints derived from H (z)/P antheon samples. We consider a …
Palatini formulation of the conformally invariant f R, L m gravity theory
We investigate the field equations of the conformally invariant models of gravity with
curvature-matter coupling, constructed in Weyl geometry, using the Palatini formalism. We …
curvature-matter coupling, constructed in Weyl geometry, using the Palatini formalism. We …
Self-similar cosmological solutions in symmetric teleparallel theory: Friedmann-Lemaître-Robertson-Walker spacetimes
The existence of self-similar solutions is discussed in symmetric teleparallel f (Q) theory for a
Friedmann-Lemaître-Robertson-Walker background geometry with zero and nonzero spatial …
Friedmann-Lemaître-Robertson-Walker background geometry with zero and nonzero spatial …
Accelerating Universe scenario in anisotropic f (Q) cosmology
In this paper, we investigate the exact solution of an anisotropic space-time in the context of f
(Q) gravity, where f Q is the arbitrary function of the non-metricity scalar Q. Here, we consider …
(Q) gravity, where f Q is the arbitrary function of the non-metricity scalar Q. Here, we consider …
Cosmological sudden singularities in f(R, T) gravity
In this work, we study the possibility of finite-time future cosmological singularities appearing
in f (R, T) gravity, where R is the Ricci scalar and T is the trace of the stress-energy tensor …
in f (R, T) gravity, where R is the Ricci scalar and T is the trace of the stress-energy tensor …
Transit cosmological models in gravity theory
In the present paper, we investigate some exact cosmological models in F (R, T¯) gravity
theory. We have considered the arbitrary function F (R, T¯)= R+ λ T¯ where λ is an arbitrary …
theory. We have considered the arbitrary function F (R, T¯)= R+ λ T¯ where λ is an arbitrary …
Compact stellar structures in Weyl geometric gravity
We consider the structure and physical properties of specific classes of neutron, quark, and
Bose-Einstein condensate stars in the conformally invariant Weyl geometric gravity theory …
Bose-Einstein condensate stars in the conformally invariant Weyl geometric gravity theory …