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

Simple item page
dc.creatorCornish, Neil J.
dc.date2001-01-10
dc.date.accessioned2026-07-07T11:29:52Z
dc.date.available2026-07-07T11:29:52Z
dc.descriptionLevin (gr-qc/9910040) has shown that spinning compact binaries can be chaotic at second post-Newtonian order. However, when higher order dissipational effects are included, the dynamics will no longer be chaotic, though the evolution may still be unpredictable in a practical sense. I discuss some of the additional work that needs to be done to decide how this unpredictability might affect gravitational wave detectors such as LIGO.
dc.description1 page
dc.identifierhttps://arxiv.org/abs/gr-qc/0101041
dc.identifierhttp://arxiv.org/abs/gr-qc/0101041
dc.identifierPhys.Rev.Lett.85:3980,2000
dc.identifierdoi:10.1103/PhysRevLett.85.3980
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196852
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleComment on "Gravity Waves, Chaos, and Spinning Compact Binaries"
dc.typetext

Files

Collections

arXiv