Kepler Equation for the Compact Binaries under the Spin-spin Interaction
| dc.creator | Keresztes, Zoltán | |
| dc.creator | Mikóczi, Balázs | |
| dc.date | 2006-10-10 | |
| dc.date.accessioned | 2026-07-07T07:26:54Z | |
| dc.date.available | 2026-07-07T07:26:54Z | |
| dc.description | In this work we consider compact binaries on eccentric orbit under the spin-spin interaction. Using the post-Newtonian formalism, the binaries undergo a perturbed Keplerian motion. Here we investigate only the radial motion and derive the contribution of the second post-Newtonian order spin-spin effect to the solution. | |
| dc.description | 4 pages, $g_t$ from Kepler equation removed as compared to the published version, in Proceedings of the Astrophysics of Variable Stars | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610287 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610287 | |
| dc.identifier | ASP Conference Series, 349, 265-268 (2006) | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/117193 | |
| dc.subject | Astrophysics | |
| dc.title | Kepler Equation for the Compact Binaries under the Spin-spin Interaction | |
| dc.type | text |