On Einsteinian orbits of celestial bodies
| dc.creator | Loinger, A. | |
| dc.date | 2003-03-09 | |
| dc.date.accessioned | 2026-07-07T05:48:54Z | |
| dc.date.available | 2026-07-07T05:48:54Z | |
| dc.description | It can be demonstrated that no motion of masses can generate gravitational waves. Accordingly: i) the time decrease of the orbital period of the famous binary PSR1913+16 cannot yield an experimental proof of the emission of gravitational waves; ii) measurements of the propagation of the quasar J0842+1835 radio-signals past Jupiter cannot reveal the propagation of gravitational waves sent forth by the planet in its motion around the Sun: indeed, this motion does not generate any gravitational radiation; iii) the binary RX J0806.3+1527 has the shortest known revolution period (only 321 s): however, it cannot be a candidate for the detection of gravitational waves because no kind of motion of a mass can give origin to a gravitational wave. | |
| dc.description | 3 pages, LaTeX, to be published on Spacetime & Substance | |
| dc.identifier | https://arxiv.org/abs/physics/0303035 | |
| dc.identifier | http://arxiv.org/abs/physics/0303035 | |
| dc.identifier | Spacetime & Substance, Volume 4, No.2 (17), 2003, pp.74-75 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/85200 | |
| dc.subject | General Physics | |
| dc.title | On Einsteinian orbits of celestial bodies | |
| dc.type | text |