Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Documenti analoghi

• Comparing effective-one-body and Mathisson-Papapetrou-Dixon results for a spinning test particle on circular equatorial orbits around a Kerr black hole
  di: Albertini, Angelica, et al.
  Pubblicazione: (2024)
• Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity
  di: Albertini, Angelica, et al.
  Pubblicazione: (2023)
• Circular equatorial orbits of extended bodies with spin-induced quadrupole around a Kerr black hole: Comparing spin-supplementary conditions
  di: Shahzadi, Misbah, et al.
  Pubblicazione: (2025)
• Hybridization of second-order gravitational self-force and numerical relativity waveforms for quasi-circular and non-spinning black hole binaries
  di: Iglesias, Hector, et al.
  Pubblicazione: (2025)
• Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
  di: Mathews, Josh, et al.
  Pubblicazione: (2025)