collaborators

6 papers

astro-ph.CO2026

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy

Mohit Yadav, Tapomoy Guha Sarkar

We investigate nonlinear structure formation in a cosmological model combining one-body decaying dark matter (DDM) with a semi-cosmographic reconstruction of dark energy. In this s…

astro-ph.CO2026

Semi-cosmographic constraints on decaying dark matter and dynamical dark energy: DESI DR2 BAO and 21\, cm intensity-mapping forecasts

Mohit Yadav, Pankaj Chavan, Tapomoy Guha Sarkar

Cosmographic reconstructions provide a model-agnostic approach towards constraining cosmic evolution. In this work, we develop a semi-cosmographic framework that adopts a Padé-rat…

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

Probing Decaying Dark Matter Using the Post-EoR HI 21-cm signal

Mohit Yadav, Tapomoy Guha Sarkar

We propose the HI 21-cm power spectrum from the post-reionization epoch as a probe of a cosmological model with decaying dark matter particles. The unstable particles are assumed t…

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…