activity
20162025
most citedConstraining cosmic curvature by using age of galaxies and gravitational lenses

72 citations · 85 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2025

Spectral Chebyshev Approximation of Cosmic Expansion in Gravity

Akshay Rana

We present a numerical framework to study the cosmological background evolution in gravity by employing a \textit{spectral Chebyshev collocation approach}. Unlike standard i…

astro-ph.CO2025★ 2 cited

Testing the Constancy of Type Ia Supernova Luminosities with Gaussian Process

Akshay Rana

Type Ia supernovae (SNe~Ia) are central to studies of cosmic expansion, under the assumption that their absolute magnitude does not evolve with redshift. Even small drifts in…

astro-ph.CO2022

Examining Temporal Variation of the Fermi Coupling Constant using SNe Ia Light Curves

Akshay Rana, Vedanta Thapar, Hari Prasad S. V. +1

In standard model, the Fermi coupling constant, , sets the strength of electroweak decay. We attempt an approach to constrain the temporal variation of the Fermi coupling cons…

astro-ph.CO2022★ 11 cited

Constraints on the Transition Redshift using Hubble Phase Space Portrait

Darshan Kumar, Deepak Jain, Shobhit Mahajan +2

One of the most significant discoveries in modern cosmology is that the universe is currently in a phase of accelerated expansion after a switch from a decelerated expansion. The r…

astro-ph.CO2021

A non-parametric test of variability of Type Ia supernovae luminosity and CDDR

Darshan Kumar, Akshay Rana, Deepak Jain +3

The first observational evidence for cosmic acceleration appeared from Type Ia supernovae (SNe Type Ia) Hubble diagram from two different groups. However, the empirical treatment o…

astro-ph.CO2021

Strong lensing systems and galaxy cluster observations as probe to the cosmic distance duality relation

R. F. L. Holanda, F. S. Lima, Akshay Rana +1

{In this paper, we use large scale structure observations to test the redshift dependence of cosmic distance duality relation (CDDR), }, with $D…