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Evolution of inspiral orbits around a Schwarzschild black hole

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arxiv 1111.6908 v3 pith:DMB4LPBF submitted 2011-11-29 gr-qc astro-ph.HE

Niels Warburton , Sarp Akcay , Leor Barack , Jonathan R. Gair , Norichika Sago This is my paper · ORCID
classification gr-qcastro-ph.HE
keywords blackconservativecorrectionsevolutionincludinginspiralorbitsanalytic
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We present results from calculations of the orbital evolution in eccentric binaries of nonrotating black holes with extreme mass-ratios. Our inspiral model is based on the method of osculating geodesics, and is the first to incorporate the full gravitational self-force (GSF) effect, including conservative corrections. The GSF information is encapsulated in an analytic interpolation formula based on numerical GSF data for over a thousand sample geodesic orbits. We assess the importance of including conservative GSF corrections in waveform models for gravitational-wave searches.

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Cited by 4 Pith papers

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

  1. Approach to the separatrix with eccentric orbits

    gr-qc 2024-12 conditional novelty 7.0 of 10

    The adiabatic inspiral near the separatrix for eccentric orbits is solved analytically, with the Lambert W_{-1} function controlling the late-time decay of the distance to the separatrix.

  2. Geometric properties of slowly rotating black holes embedded in matter environments

    gr-qc 2026-02 conditional novelty 6.0 of 10

    The rotation of a surrounding dark-matter halo shifts the light ring, ISCO, epicyclic frequencies, and resonance locations of a slowly spinning black hole in a way that depends on the halo's angular velocity.

  3. Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA

    gr-qc 2024-04 unverdicted novelty 6.0 of 10

    Bayesian inference on LVK O1-O3 events with eccentric aligned-spin waveforms yields log10 Bayes factors of 1.77-4.75 favoring eccentricity for GW200129, GW190701 and GW200208_22, and >99.5% probability that at least o...

  4. Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms

    gr-qc 2025-02 conditional novelty 5.0 of 10

    A PN-anchored waveform-based eccentricity estimator using envelope fits to the universal eccentric modulation, with an empirically added half-PN term.

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