Kepler equation for inspiralling compact binaries
Compact binaries consisting of neutron stars/black holes on eccentric orbit undergo a perturbed Keplerian motion. The perturbations are either of relativistic origin or are related to the spin, mass quadrupole, and magnetic dipole moments of the binary components. The post-Newtonian motion of such s...
Elmentve itt :
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| Dokumentumtípus: | Cikk |
| Megjelent: |
American Physical Society
2005
|
| Sorozat: | PHYSICAL REVIEW D
72 No. 10 |
| doi: | 10.1103/PhysRevD.72.104022 |
| mtmt: | 1278979 |
| Online Access: | http://publicatio.bibl.u-szeged.hu/7964 |
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| 024 | 7 | |a 10.1103/PhysRevD.72.104022 |2 doi | |
| 024 | 7 | |a 1278979 |2 mtmt | |
| 040 | |a SZTE Publicatio Repozitórium |b hun | ||
| 041 | |a zxx | ||
| 100 | 1 | |a Keresztes Zoltán | |
| 245 | 1 | 0 | |a Kepler equation for inspiralling compact binaries |h [elektronikus dokumentum] / |c Keresztes Zoltán |
| 260 | |a American Physical Society |c 2005 | ||
| 300 | |a Terjedelem: 7 p.-Azonosító: 104022 | ||
| 490 | 0 | |a PHYSICAL REVIEW D |v 72 No. 10 | |
| 520 | 3 | |a Compact binaries consisting of neutron stars/black holes on eccentric orbit undergo a perturbed Keplerian motion. The perturbations are either of relativistic origin or are related to the spin, mass quadrupole, and magnetic dipole moments of the binary components. The post-Newtonian motion of such systems decouples into radial and angular parts. We present here for the first time the radial motion of such a binary encoded in a generalized Kepler equation, with the inclusion of all above-mentioned contributions, up to linear order in the perturbations. Together with suitably introduced parametrizations, the radial motion is solved completely. | |
| 700 | 0 | 1 | |a Mikóczi Balázs |e aut |
| 700 | 0 | 1 | |a Gergely Árpád László |e aut |
| 856 | 4 | 0 | |u http://publicatio.bibl.u-szeged.hu/7964/1/72_cikk_keresztesetal2005.pdf |z Dokumentum-elérés |
| 856 | 4 | 0 | |u http://publicatio.bibl.u-szeged.hu/7964/2/72_cikk_preprint_0510602v1.pdf |z Dokumentum-elérés |