activity
20122025
most citedStringent constraints on neutron-star radii from multimessenger observations and nuclear theory

389 citations · 1.5k across the 21 of their papers we have counts for

collaborators

22 papers

gr-qc2025★ 3 cited

Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation

Sumit Kumar, Max Melching, Frank Ohme

The PE for GW merger events relies on a waveform model calibrated using numerical simulations. Within the Bayesian framework, this waveform model represents the GW signal produced…

astro-ph.CO2023★ 15 cited

Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass

Luca Amendola, Davi C. Rodrigues, Sumit Kumar +1

We test the possibility that the black holes (BHs) detected by LIGO-Virgo-KAGRA (LVK) may be cosmologically coupled and grow in mass proportionally to the cosmological scale factor…

gr-qc2022★ 1 cited

Constraining mass of the graviton with GW170817

Andrey A. Shoom, Sumit Kumar, N. V. Krishnendu

We consider the massive graviton phenomenological model based on the graviton's dispersion terms included into phase of gravitational wave's waveform. Such model was already consid…

gr-qc2022

A novel ringdown amplitude-phase consistency test

Xisco Jiménez Forteza, Swetha Bhagwat, Sumit Kumar +1

The ringdown signal emitted during a binary black hole coalescence can be modeled as a linear superposition of the characteristic damped modes of the remnant black hole that get ex…

astro-ph.CO2022★ 3 cited

Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves

Sumit Kumar

The third-generation (3G) gravitational wave (GW) detectors such as the Einstein telescope (ET) or Cosmic Explorer (CE) are expected to play an important role in cosmology. With th…

astro-ph.IM2022★ 9 cited

Parameter Estimation with Nonstationary Noise in Gravitational-wave Data

Sumit Kumar, Alexander H. Nitz, Xisco Jiménez Forteza

The sensitivity of gravitational-wave (GW) detectors is characterized by their noise curves, which determine the detector's reach and ability to measure the parameters of astrophys…