Cosmological constraints on dark energy in f (Q) gravity: A parametrized perspective
A Mussatayeva, N Myrzakulov, M Koussour - Physics of the Dark Universe, 2023 - Elsevier
In this paper, we focus on the parametrization of the effective equation of state (EoS)
parameter within the framework of f (Q) symmetric teleparallel gravity. Here, the gravitational …
parameter within the framework of f (Q) symmetric teleparallel gravity. Here, the gravitational …
[HTML][HTML] Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
We propose a logarithmic parametrization form of energy density for the scalar field dark
energy in the framework of the standard theory of gravity, which supports the necessary …
energy in the framework of the standard theory of gravity, which supports the necessary …
Constrained evolution of effective equation of state parameter in non-linear f R, L m dark energy model: insights from Bayesian analysis of cosmic chronometers and …
We conduct a Bayesian analysis of recent observational datasets, specifically the Cosmic
Chronometers (CC) dataset and Pantheon samples, to investigate the evolution of the EoS …
Chronometers (CC) dataset and Pantheon samples, to investigate the evolution of the EoS …
Observational constraints on the equation of state of viscous fluid in f (R, T) gravity
In this paper, we investigate a cosmological model based on viscous f (R, T) gravity as a
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
Cosmological parameter analyses using transversal BAO data
We investigate observational constraints on cosmological parameters combining 15
measurements of the transversal BAO scale (obtained free of any fiducial cosmology) with …
measurements of the transversal BAO scale (obtained free of any fiducial cosmology) with …
Late-time cosmology in f (Q, Lm) gravity: Analytical solutions and observational fits
In this study, we examined the late-time cosmic expansion of the universe within the
framework of f (Q, L m) gravity, where Q denotes the non-metricity and L m represents the …
framework of f (Q, L m) gravity, where Q denotes the non-metricity and L m represents the …
[HTML][HTML] Barrow holographic dark energy with Granda–Oliveros cutoff
A study on the effects of implementing the Granda–Oliveros infrared cutoff in the recently
introduced Barrow holographic dark energy model is presented, and its cosmological …
introduced Barrow holographic dark energy model is presented, and its cosmological …
Constraining the curvature density parameter in cosmology
P Mukherjee, N Banerjee - Physical Review D, 2022 - APS
The cosmic curvature density parameter has been constrained in the present work
independent of any background cosmological model. The reconstruction is undertaken …
independent of any background cosmological model. The reconstruction is undertaken …
What can Machine Learning tell us about the background expansion of the Universe?
R Arjona, S Nesseris - Physical Review D, 2020 - APS
Machine learning (ML) algorithms have revolutionized the way we interpret data in
astronomy, particle physics, biology, and even economics, since they can remove biases …
astronomy, particle physics, biology, and even economics, since they can remove biases …
[HTML][HTML] Model-independent cosmological insights from three newly reconstructed deceleration parameters with observational data
DM Naik, NS Kavya, L Sudharani, V Venkatesha - Physics Letters B, 2023 - Elsevier
This article introduces three novel parametrizations of the deceleration parameter (DP) to
explore the cosmological scenario. The newly introduced parametric forms of the DP are …
explore the cosmological scenario. The newly introduced parametric forms of the DP are …