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6 papers

gr-qc2026

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

Lorenzo Copparoni, Rohit S. Chandramouli, Enrico Barausse

The paper introduces a non‑parametric self‑consistency test that checks whether gravitational‑wave parameter estimates from different parts of an extreme mass ratio inspiral signal…

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

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-qc2026

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

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

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…