Advancing the Effective-One-Body Framework in the Test-Mass Limit
Nami Nishimura, Alessandra Buonanno, Guglielmo Faggioli, Maarten van de Meent, Gaurav Khanna

TL;DR
This paper introduces SEOB-TML, an advanced EOB framework optimized for test-mass limit black hole binaries, achieving higher accuracy and reduced errors in waveform modeling through innovative prescriptions and mode modeling techniques.
Contribution
The paper presents novel quadrupole-factorized flux mapping, a phenomenological transition ansatz, and explicit mode-mixing modeling, significantly improving EOB waveform accuracy in the test-mass limit.
Findings
Reduced fractional flux errors with Q-factorized prescription
Enhanced waveform accuracy in late inspiral-merger-ringdown stages
Better agreement with numerical waveforms compared to previous models
Abstract
We present SEOB-TML, an enhanced effective-one-body (EOB) framework for the test-mass limit, optimized for quasi-circular, spin-aligned binary black holes. On the dynamical side, we introduce a quadrupole-factorized (Q-factorized) prescription that maps the total energy flux-including horizon absorption-onto a single (2,2) mode baseline. This approach effectively captures higher-order multipole contributions without explicit mode summation, while simultaneously leading to a dramatic reduction in fractional flux errors. To ensure a smooth transition to the post-merger stage, we replace traditional next-to-quasicircular corrections with a phenomenological ansatz, enabling a flexible, mode-dependent attachment prescription. For the merger-ringdown stage, we utilize quasi-normal mode coefficients extracted from numerical waveforms via qnmfinder to explicitly model mode-mixing effects. These…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Gamma-ray bursts and supernovae
