Orbital evolution for extreme mass-ratio binaries: conservative self forces

Simple item page
dc.creatorBurko, Lior M.
dc.date2007-01-02
dc.date.accessioned2026-07-07T10:37:11Z
dc.date.available2026-07-07T10:37:11Z
dc.descriptionThe conservative dephasing effects of gravitational self forces for extreme mass-ratio inspirals are studied. Both secular and non-secular conservative effects may have a significant effect on LISA waveforms that is independent of the mass ratio of the system. Such effects need to be included in generated waveforms to allow for accurate gravitational wave astronomy that requires integration times as long as a year.
dc.description3 figures, in Proceedings of the Sixth International LISA Symposium (AIP, 2006)
dc.identifierhttps://arxiv.org/abs/gr-qc/0701022
dc.identifierhttp://arxiv.org/abs/gr-qc/0701022
dc.identifierAIPConf.Proc.873:269-273,2006
dc.identifierdoi:10.1063/1.2405054
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180296
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOrbital evolution for extreme mass-ratio binaries: conservative self forces
dc.typetext

Files

Collections

arXiv