activity
20182026
most citedFirst constraint on the dissipative tidal deformability of neutron stars

29 citations · 72 across the 9 of their papers we have counts for

collaborators

9 papers

gr-qc2026

Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum

Ran Chen, Rohit S. Chandramouli, Federico Pozzoli +2

Astrophysical formation channels of stellar-mass binary black holes (sBBHs) can induce significant orbital eccentricities in their early inspiral. We analyze the implications on th…

gr-qc2026★ 1 cited

Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries

Sophia Yi, Francesco Iacovelli, Emanuele Berti +4

The Laser Interferometer Space Antenna (LISA) will observe massive black hole binaries (MBHBs) with astoundingly high signal-to-noise ratio, leaving parameter estimation with these…

gr-qc2025

When vacuum breaks: a self-consistency test for astrophysical environments in extreme mass ratio inspirals

Lorenzo Copparoni, Rohit S. Chandramouli, Enrico Barausse

Gravitational-wave signals are typically interpreted under the vacuum hypothesis, i.e. assuming negligible influence from the astrophysical environment. This assumption is expected…

gr-qc2025★ 8 cited

Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries

Ran Chen, Rohit S. Chandramouli, Federico Pozzoli +2

The population of unresolved stellar-mass black hole binaries (sBBHs) is expected to produce a stochastic gravitational-wave background (SGWB) potentially detectable by the Laser I…

gr-qc2025★ 5 cited

Systematic bias in LISA ringdown analysis due to waveform inaccuracy

Lodovico Capuano, Massimo Vaglio, Rohit S. Chandramouli +3

Inaccurate modeling of gravitational-wave signals can introduce systematic biases in the inferred source parameters. As detector sensitivities improve and signals become louder, mi…

gr-qc2024★ 2 cited

Millilensing induced systematic biases in parameterized tests of General Relativity

Anna Liu, Rohit S. Chandramouli, Otto A. Hannuksela +2

Tests of general relativity (GR) can be systematically biased when our waveform models are inaccurate. We here study systematic biases in tests of general relativity induced by neg…

gr-qc2024★ 27 cited

Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes

Rohit S. Chandramouli, Kaitlyn Prokup, Emanuele Berti +1

We study the robustness of parametrized post-Einsteinian (ppE) tests of General Relativity (GR) with gravitational waves, due to waveform inaccuracy. In particular, we determine th…

gr-qc2023★ 29 cited

First constraint on the dissipative tidal deformability of neutron stars

Justin L. Ripley, Abhishek Hegade K. R., Rohit S. Chandramouli +1

The gravitational waves (GWs) emitted by neutron star binaries probe the physics of matter at supra nuclear densities. During the late inspiral, tidal deformations raised on each s…

cond-mat.stat-mech2018

Efficient implementation of the Wang-Landau algorithm for systems with length-scalable potential energy functions

Santosh Kumar, Girish Kumar, Rohit S. Chandramouli +1

We consider a class of systems where identical particles with positions and momenta are enclosed in a box of size , and e…