Gravity Waves, Chaos, and Spinning Compact Binaries
arXiv:gr-qc/9910040 · doi:10.1103/PhysRevLett.84.3515
Abstract
Spinning compact binaries are shown to be chaotic in the Post-Newtonian expansion of the two body system. Chaos by definition is the extreme sensitivity to initial conditions and a consequent inability to predict the outcome of the evolution. As a result, the spinning pair will have unpredictable gravitational waveforms during coalescence. This poses a challenge to future gravity wave observatories which rely on a match between the data and a theoretical template.
Final version published in PRL
Cited by in corpus (76)
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