activity
20052026
most citedBrans-Dicke Scalar Field as a Chameleon

128 citations · 291 across the 17 of their papers we have counts for

collaborators

26 papers

hep-ph2026

Probing Scalar-Induced First-Order Phase Transitions with the Diffuse Supernova Neutrino Background

Sudipta Das, Shamik Niyogi, Manibrata Sen

We investigate the possibility of probing a scalar-induced first-order phase transition (FOPT) inside core-collapse supernovae through the diffuse supernova neutrino background (DS…

gr-qc2023

Ideal Gas Thermodynamics with an Invariant Energy Scale

Sudipta Das

A viable approach towards Quantum Gravity is the Doubly Special Relativity (DSR) framework in which an observer-independent finite energy upper bound (or a finite smallest length s…

hep-ph2023

Present and future constraints on flavor-dependent long-range interactions of high-energy astrophysical neutrinos

Sanjib Kumar Agarwalla, Mauricio Bustamante, Sudipta Das +1

The discovery of new, flavor-dependent neutrino interactions would provide compelling evidence of physics beyond the Standard Model. We focus on interactions generated by the anoma…

hep-ph2023★ 9 cited

Constraining Lorentz Invariance Violation with Next-Generation Long-Baseline Experiments

Sanjib Kumar Agarwalla, Sudipta Das, Sadashiv Sahoo +1

Unified theories such as string theory and loop quantum gravity allow the Lorentz Invariance Violation (LIV) at the Planck Scale ( GeV). Using an effective field…

hep-ph2022

Enhancing Sensitivity to Leptonic CP Violation using Complementarity among DUNE, T2HK, and T2HKK

Sanjib Kumar Agarwalla, Sudipta Das, Alessio Giarnetti +2

After the landmark discovery of non-zero by the modern reactor experiments, unprecedented precision on neutrino mass-mixing parameters has been achieved over the past deca…

gr-qc2022★ 4 cited

Perturbation in an interacting dark universe

Srijita Sinha, Manisha Banerjee, Sudipta Das

In this paper we have considered an interacting model of dark energy and have looked into the evolution of the dark sectors. By solving the perturbation equations numerically, we h…