Higher-order corrections to the relativistic perihelion advance and
✍ Scribed by Maurizio M. D’Eliseo
- Publisher
- Springer Netherlands
- Year
- 2010
- Tongue
- English
- Weight
- 289 KB
- Volume
- 332
- Category
- Article
- ISSN
- 0004-640X
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📜 SIMILAR VOLUMES
Employing action angle variables the relation between the Schwarzschild perihelic shift and the Reissner-Nortlstrom perihelic shift of the test particle has been deduced. It is observed that the charge on the gravitating particle instead of helping the matter to curve the space-time more, tlecurves
## Abstract By a gravitational potential Φ′(__r__) = − __G__~0~__M/r__ (I + α + α In __r__) with |α|≪ 1 a motion δφ of the perihelion of a planet is resulting which is neither depending on the central‐mass __M__ nor on the semi‐axis of the KEPLER‐ellipse δφ ≈︁ ‐ απ. Therefore, |α| must be smaller t