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Levin (gr-qc/9910040) has shown that spinning compact binaries can be chaoticat second post-Newtonian order. However, when higher order dissipationaleffects are included, the dynamics will no longer be chaotic, though theevolution may still be unpredictable in a practical sense. I discuss some ofthe additional work that needs to be done to decide how this unpredictabilitymight affect gravitational wave detectors such as LIGO.Comment: 1 pag

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