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

Documenti analoghi

• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
  di: Huez, Giulia, et al.
  Pubblicazione: (2025)
• Effective-one-body waveform model for non-circularized, planar, coalescing black hole binaries: the importance of radiation reaction
  di: Nagar, Alessandro, et al.
  Pubblicazione: (2024)
• 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
  di: Albertini, Angelica, et al.
  Pubblicazione: (2024)
• Ringdown modeling for effective-one-body waveforms in the test-mass limit for eccentric equatorial orbits around a Kerr black hole
  di: Albanesi, Simone, et al.
  Pubblicazione: (2026)
• Binary black hole merger in the extreme mass ratio limit: a multipolar analysis of the inclined orbit case
  di: Nagni, Luca, et al.
  Pubblicazione: (2025)