activity
20242026
collaborators

10 papers

gr-qc2026

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data

Enrico Specogna, Shahnawaz A. Adil, Emre Ozulker +4

In this work, we present updated observational constraints on the parameter space of the DMS20 dark energy model, a member of the omnipotent dark energy (ODE) class. Our analysis c…

astro-ph.CO2026

The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction

Pankaj Chavan, Tapomoy Guha Sarkar, Anjan A Sen

The Baryon Acoustic Oscillation (BAO) feature, imprinted in the transverse and radial clustering of dark matter tracers, enables the simultaneous measurement of the angular diamete…

astro-ph.CO2025

Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data

Hanyu Cheng, Eleonora Di Valentino, Luis A. Escamilla +2

We explore an extension of the CDM model in which the pressure of the dark energy (DE) fluid evolves with the expansion of the Universe, expressed as a function of the scal…

astro-ph.CO2025

Disentangling the growth rate of perturbations from the HI bias using only clustering data from galaxy surveys

Pankaj Chavan, Tapomoy Guha Sarkar, Anjan A Sen

This work serves two-fold purpose. Firstly, we provide an alternative to the traditional method of determining the growth rate of density perturbations . In usual practice, $…

astro-ph.CO2025

A semi-cosmographic approach to study cosmological evolution in phase space

Pankaj Chavan, Tapomoy Guha Sarkar, Chandrachud B. V. Dash +1

The signature of Baryon Acoustic Oscillation in the clustering of dark-matter tracers allows us to measure independently. Treating these as conjugate variables, we…

astro-ph.CO2025

Inferring dark energy properties from the scale factor parametrisation

Upala Mukhopadhyay, Sandeep Haridasu, Anjan A Sen +1

We propose and implement a novel test to assess deviations from well-established concordance CDM cosmology while inferring dark energy properties. In contrast to the commonly i…