dorsal/arxiv
View SchemaOn Einsteinian orbits of celestial bodies
| Authors | A. Loinger |
|---|---|
| Categories | |
| ArXiv ID | physics/0303035 |
| URL | https://arxiv.org/abs/physics/0303035 |
| Journal | Spacetime & Substance, Volume 4, No.2 (17), 2003, pp.74-75 |
Abstract
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.
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"abstract": "It can be demonstrated that no motion of masses can generate gravitational\nwaves. Accordingly: i) the time decrease of the orbital period of the famous\nbinary PSR1913+16 cannot yield an experimental proof of the emission of\ngravitational waves; ii) measurements of the propagation of the quasar\nJ0842+1835 radio-signals past Jupiter cannot reveal the propagation of\ngravitational waves sent forth by the planet in its motion around the Sun:\nindeed, this motion does not generate any gravitational radiation; iii) the\nbinary RX J0806.3+1527 has the shortest known revolution period (only 321 s):\nhowever, it cannot be a candidate for the detection of gravitational waves\nbecause no kind of motion of a mass can give origin to a gravitational wave.",
"arxiv_id": "physics/0303035",
"authors": [
"A. Loinger"
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"journal_ref": "Spacetime \u0026 Substance, Volume 4, No.2 (17), 2003, pp.74-75",
"title": "On Einsteinian orbits of celestial bodies",
"url": "https://arxiv.org/abs/physics/0303035"
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