Deformation of the Planetary Orbits Caused by the Time Dependent Gravitational Potential in the Universe
arXiv:gr-qc/0403067 · doi:10.1007/s10714-005-0039-6
Abstract
In the paper are studied the deformations of the planetary orbits caused by the time dependent gravitational potential in the universe. It is shown that the orbits are not axially symmetric and the time dependent potential does not cause perihelion precession. It is found a simple formula for the change of the orbit period caused by the time dependent gravitational potential and it is tested for two binary pulsars.
arXiv comment7 pages
References in corpus (10)
- Study of the anomalous acceleration of Pioneer 10 and 11
- Indication, from Pioneer 10/11, Galileo, and Ulysses Data, of an Apparent Anomalous, Weak, Long-Range Acceleration
- Dynamics with a non-standard inertia-acceleration relation: an alternative to dark matter
- Measuring and Understanding the Universe
- Measurement of Relativistic Orbital Decay in the PSR B1534+12 Binary System
- Neutrino Oscillations in Brans-Dicke Theory of Gravity
- A mirror world explanation for the Pioneer spacecraft anomalies?
- Effective time variation of G in a model universe with variable space dimension
- Effect of a scale-dependent cosmological term on the motion of small test particles in a Schwarzschild background
- Possible manifestations of the graviton background