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astro-ph.HE2026

Large Gravitational Wave Phase Shifts from Strong 3-body Interactions in Dense Stellar Clusters

Kai Hendriks, Dany Atallah, Miguel Martinez +7

The phase evolution of gravitational waves (GWs) can be modulated by the astrophysical environment surrounding the source, which provides a probe for the origin of individual binar…

astro-ph.HE2025

The construction and use of dephasing prescriptions for environmental effects in gravitational wave astronomy

János Takátsy, Lorenz Zwick, Kai Hendriks +3

In the first part of this work, we provide a curated overview of the theoretical framework necessary for incorporating dephasing due to environmental effects (EE) in gravitational…

astro-ph.HE2025

Amplified capture rate of dark matter in compact binaries and constraints on bosonic dark matter from GW170817

János Takátsy, Lorenz Zwick, David O'Neill +1

The accretion of dark matter (DM) onto compact objects and the potential gravitational collapse of neutron stars due to this accretion has become a promising indirect probe of DM p…

astro-ph.HE2025

Dissecting environmental effects with eccentric gravitational wave sources

Lorenz Zwick, Kai Hendriks, David O'Neill +6

We model the effect of resonances between time-varying perturbative forces and the epi-cyclical motion of eccentric binaries in the gravitational wave (GW) driven regime. These ind…

astro-ph.HE2025

Environmental effects in stellar mass gravitational wave sources I: Expected fraction of signals with significant dephasing in the dynamical and AGN channels

Lorenz Zwick, János Takátsy, Pankaj Saini +5

We present the first overview of the expected quantity of signals which will showcase significant gravitational wave phase shifts caused by astrophysical environments, considering…