collaborators

7 papers

astro-ph.CO2025

Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future

Harsh Mehta, Suvodip Mukherjee

The massive and bright galaxies observed by the James Webb Space Telescope (JWST) at high redshifts () have challenged our understanding of the Universe. This may require re…

astro-ph.CO2025

Gravitational Wave Burst from Bremsstrahlung in Milky Way Can Discover Sub-Solar Dark Matter in Near Future

Samsuzzaman Afroz, Suvodip Mukherjee

What is Dark Matter, and what is its concentration in the Milky Way remains an open question in physics. We show that if a significant fraction of dark matter is composed of sub-so…

astro-ph.CO2025

Illuminating Dark Energy with Bright Standard Sirens from Future Detectors

Samsuzzaman Afroz, Suvodip Mukherjee, Gianmassimo Tasinato

Understanding the nature and evolution of dark energy (DE) is a central challenge in modern cosmology. In this work, we explore the constraining power of bright standard sirens --…

gr-qc2025

The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA

Aniruddha Chakraborty, Suvodip Mukherjee

The lensing of Gravitational Waves (GWs) due to intervening matter distribution in the universe can lead to chromatic and achromatic signatures in the wave-optics and geometrical-o…

astro-ph.CO2024

Multi-Messenger Cosmology: A Route to Accurate Inference of Dark Energy Beyond CPL Parametrization from XG Detectors

Samsuzzaman Afroz, Suvodip Mukherjee

One of the central challenges in modern cosmology is understanding the nature of dark energy and its evolution throughout the history of the Universe. Dark energy is commonly model…

gr-qc2024

Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe

Guillaume Dideron, Suvodip Mukherjee, Luis Lehner

New physics and systematic errors can lead to deviations between the models used to analyze gravitational wave data and the actual signal. Such deviations will generally be correla…