Dissipation for Euler's Disk and a Desktop Demonstration of Coalescing Neutron Stars

dc.creatorBildsten, Lars
dc.date2001-02-11
dc.date.accessioned2026-07-07T03:25:41Z
dc.date.available2026-07-07T03:25:41Z
dc.descriptionI show that the recent calculation of Moffatt's regarding the viscous dissipation of a spinning coin overlooked the importance of the finite width of the viscous boundary layer. My new estimates are more in accord with that observed. I also point out that the frequency ``chirp'' of the specially designed toy ``Euler's Disk'' is similar to that expected during the last few minutes of the life of a coalescing binary of two neutron stars. As such, this toy is an excellent desktop demonstration for the expected phenomena.
dc.descriptionSubmitted to American Journal of Physics
dc.identifierhttps://arxiv.org/abs/gr-qc/0102046
dc.identifierhttp://arxiv.org/abs/gr-qc/0102046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33803
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleDissipation for Euler's Disk and a Desktop Demonstration of Coalescing Neutron Stars
dc.typetext

Files

Collections