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Cumulative effect of orbital resonances in extreme-mass-ratio inspirals

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arxiv 2502.20457 v2 pith:U4XSE4B2 submitted 2025-02-27 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords resonanceeffectsorbitalresonancesemrisaccuratecumulativeevolution
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Orbital resonances in extreme-mass-ratio inspirals (EMRIs) have been proven to be a key feature for accurate gravitational-wave template modeling. Decades of research have led to schemes that can not only model the adiabatic inspiral of such a binary system, but also account for the effects of resonances on their evolution. In this work, we use an effective resonance model that includes analytically derived corrections to the radiation reaction fluxes, to study the combined effects of both dominant (low-order) and subdominant (high-order) orbital resonances in EMRIs. We show that using single, universal shifts for all fluxes overestimates the resonance impact, and therefore individualized shifts for each resonance crossing are needed for accurate modeling. Our analysis reveals that the cumulative effects from multiple resonance crossings can significantly impact the orbital evolution of EMRIs, especially for highly eccentric orbits. Our results provide further evidence that resonance effects have to be included in template production to extract detailed astrophysical parameters from EMRI signals.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Resonant interactions from dynamical perturbers on generic orbits around an extreme mass ratio inspiral

    gr-qc 2025-07 conditional novelty 6.0 of 10

    A numerical scan of 141,130 third-body resonances in EMRI systems finds no action changes above 1% but some waveform phase shifts near 0.1 radian.

  2. Parameter-estimation bias induced by transient orbital resonances in extreme-mass-ratio inspirals

    gr-qc 2026-04 unverdicted novelty 5.0 of 10

    Neglecting transient orbital resonances in EMRIs causes significant SNR losses and biases in recovered parameters, with the sign and amplitude of resonance-induced changes to integrals of motion being critical.

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