Charged particle interferometry in Plebański--Demiański black hole space--times
arXiv:0801.4514 · doi:10.1088/0264-9381/25/10/105023
Abstract
The Plebański--Demiański solution is a very general axially symmetric analytical solution of the Einstein field equations generalizing the Kerr solution. This solution depends on seven parameters which under certain circumstances are related to mass, rotation, cosmological constant, NUT parameter, electric and magnetic charges, and acceleration. In this paper we present a general description of matter wave interferometry in the general Plebański--Demiański black hole space--time. Particular emphasis is placed on a gauge invariant description of the symmetries of the gauge field. We show that it is possible to have access to all parameters separately except the acceleration. For neutral particles there is only access to a combination of electric and magnetic charge.
17 pages, 2 figures, referees' remarks included, to appear in Class. Quantum Grav. V. 25
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- Penrose Process in Kerr-Taub-NUT Spacetime
- Strong field limit analysis of gravitational lensing in Kerr-Taub-NUT spacetime
- Acceleration of particles by black hole with gravitomagnetic charge immersed in magnetic field
- Magnetized Particle Capture Cross Section for Braneworld Black Hole
- Quantum Interference Effects in Slowly Rotating NUT Space-time
- Quantum Interference Effects in Horava-Lifshitz Gravity
- External Electromagnetic Fields of a Slowly Rotating Magnetized Star with Gravitomagnetic Charge
- Quantum Interference Effects in Spacetime of Slowly Rotating Compact Objects in Braneworld
- Upper limit on NUT charge from the observed terrestrial Sagnac effect
- Potentials for general-relativistic geodesy
- Remarks on the black hole shadows in Kerr-de Sitter space times