Cumulative effect of orbital resonances in extreme-mass-ratio inspirals
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.
Authors
- Kyriakos Destounis (ORCID: https://orcid.org/0000-0003-2997-088X)
- Paolo Pani (ORCID: https://orcid.org/0000-0003-4443-1761)
- Alejandro Cárdenas-Avendaño (ORCID: https://orcid.org/0000-0001-9528-1826)
- E. Levati
Institutions
- Los Alamos National Laboratory (US)
- University of Lisbon (PT)
- Wake Forest University (US)
- Sapienza University of Rome (IT)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2025-05-02
- DOI
- https://doi.org/10.1103/physrevd.111.104006
- Citations
- 4
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 4.62
Funders
- U.S. Department of Energy
- Sapienza Università di Roma
- Ministero dell'Università e della Ricerca
- Fundação para a Ciência e a Tecnologia
- Los Alamos National Laboratory