collaborators

6 papers

astro-ph.CO2025

Testing the cosmic distance duality relation using model-independent approach

Shubham Barua, Sujit K. Dalui, Rikiya Okazaki +1

In this work, we test the cosmic distance duality relation (CDDR) using the arbitrary redshift pivot Padé-(2,1) expansion methodology developed in arXiv:2509.16196. This approach a…

astro-ph.CO2025

Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model

Shubham Barua, Shantanu Desai

Recent DESI results indicate a strong preference for dynamical dark energy (DE) when baryon acoustic oscillation (BAO) measurements are combined with supernovae (SNe) and cosmic mi…

astro-ph.CO2025

On frequentist confidence intervals in a non-Gaussian regime

Shubham Barua, Shantanu Desai, Mauricio Lopez-Hernandez +1

We study frequentist confidence intervals based on graphical profile likelihoods (Wilks' theorem, likelihood integration), and the Feldman-Cousins (FC) prescription, a generalisati…

astro-ph.CO2025

Constraints on Dark Energy Models Using Late Universe Probes

Shubham Barua, Shantanu Desai

We use late Universe probes - Type Ia Supernovae from the PantheonPlus compilation, Quasars, and Dark Energy Spectroscopic Instrument (DESI) Data Release 1 (DR1) BAO data - along w…

astro-ph.IM2025

Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood

Shubham Barua, Vyaas Ramakrishnan, Shantanu Desai

The Megamaser Cosmology Project inferred a value for the Hubble constant given by km/sec/Mpc. This value was obtained using Bayesian inference by marginalizing…

astro-ph.CO2024

Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results

Shubham Barua, Shantanu Desai

We apply data-motivated priors on the peak absolute magnitude of Type Ia supernovae () and the sound horizon at the drag epoch (), to study how the degeneracy affec…