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gr-qc2025
BOB the (Waveform) Builder: Analyzing Analytical Black-Hole Binary Merger Waveforms with the Backwards One Body Formalism
Anuj Kankani, Sean T. McWilliams
The Backwards-One-Body (BOB) model provides a fully analytical and physically motivated description of the merger-ringdown gravitational radiation emanating from a black hole binar…
gr-qc2025
Spinning Effective-to-Backwards One Body (): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries
Siddharth Mahesh, Sean T. McWilliams, Zachariah Etienne
High-fidelity gravitational waveform models are essential for realizing the scientific potential of next-generation gravitational-wave observatories. While highly accurate, state-o…
gr-qc2025★ 1 cited
Modeling Relative Peak Times of Gravitational Wave Harmonics
Anuj Kankani, Sean T. McWilliams
Accurate modeling of gravitational waves from binary black hole mergers is essential for extracting their rich physics. A key detail for understanding the physics of mergers is pre…