Gravity waves from relativistic binaries

Details Gravity waves from relativistic binaries Gravity waves from relativistic binaries

1999-09-16

arxiv.org/abs/gr-qc/9909051v1

Phys.Rev. D62 (2000) 024023

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX file

Scientific paper

10.1103/PhysRevD.62.024023

The stability of binary orbits can significantly shape the gravity wave signal which future Earth-based interferometers hope to detect. The inner most stable circular orbit has been of interest as it marks the transition from the late inspiral to final plunge. We consider purely relativistic orbits beyond the circular assumption. Homoclinic orbits are of particular importance to the question of stability as they lie on the boundary between dynamical stability and instability. We identify these, estimate their rate of energy loss to gravity waves, and compute their gravitational waveforms.

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