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gr-qc2026

Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333

Massimo Vaglio, Amodio Carleo, Abhimanyu Susobhanan +5

We constrain Einstein-aether gravity -- a Lorentz-violating extension of General Relativity in which a dynamical, unit timelike vector field selects a preferred frame -- using upda…

gr-qc2025

Hierarchical modeling of gravitational-wave populations for disentangling environmental and modified-gravity effects

Shubham Kejriwal, Enrico Barausse, Alvin J. K. Chua

The upcoming Laser Interferometer Space Antenna (LISA) will detect up to thousands of extreme-mass-ratio inspirals (EMRIs). These sources will spend cycles in band, and…

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 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

Reconstructing the LISA massive black hole binary population via iterative kernel density estimation

Jam Sadiq, Kallol Dey, Thomas Dent +1

Reconstructing the properties of the astrophysical population of binary compact objects in the universe is a key science goal of gravitational wave detectors. This goal is hindered…