Vacuum C-metric and the Gravitational Stark Effect
arXiv:gr-qc/0401071 · doi:10.1103/PhysRevD.70.044020
Abstract
We study the vacuum C-metric and its physical interpretation in terms of the exterior spacetime of a uniformly accelerating spherically - symmetric gravitational source. Wave phenomena on the linearized C-metric background are investigated. It is shown that the scalar perturbations of the linearized C-metric correspond to the gravitational Stark effect. This effect is studied in connection with the Pioneer anomaly.
New version accepted for publication in Phys. Rev. D
References in corpus (2)
Cited by in corpus (12)
- The Pioneer Anomaly
- A method to measure the resonance transitions between the gravitationally bound quantum states of neutrons in the GRANIT spectrometer
- Centrifugal quantum states of neutrons
- Charged particle interferometry in Plebański--Demiański black hole space--times
- Massless spinning test particles in vacuum algebraically special spacetimes
- Geodesic motion in the vacuum C-metric
- Spinning particles in the vacuum C metric
- C metric: the equatorial plane and Fermi coordinates
- Is the physics within the Solar system really understood?
- Inertial effects in accelerating spacetimes
- Does the Neptunian system of satellites challenge a gravitational origin for the Pioneer anomaly?
- Gravitational radiation of accelerated sources