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gr-qcJan 5, 2001
11
citations (OpenAlex)
authors
  • Scott A. Hughes
institutions
  • California Institute of Technology
arXiv abstractPDF
paper

Comment on "Gravity Waves, Chaos, and Spinning Compact Binaries"

arXiv:gr-qc/0101024 · doi:10.1103/PhysRevLett.85.5480

Abstract

In this comment, I argue that chaotic effects in binary black hole inspiral will not strongly impact the detection of gravitational waves from such systems.

1 page, comment on gr-qc/9910040

Cited by in corpus (8)

  • Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits
  • Chaos and Order in Models of Black Hole Pairs
  • Computing waveforms for spinning compact binaries in quasi-eccentric orbits
  • Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
  • Extended phase-space symplectic-like integrators for coherent post-Newtonian Euler-Lagrange equations
  • Resonant Islands of Effective-One-Body Dynamics
  • Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings
  • Chaotic Emission from Electromagnetic Systems Considering Self-Interaction
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