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Charged particle interferometry in Plebański–Demiański black hole spacetimes

Valeria KagramanovaInstitut für Physik, Universität Oldenburg, 26111 Oldenburg, GermanyJutta KunzInstitut für Physik, Universität Oldenburg, 26111 Oldenburg, GermanyCláus LämmerzahlZARM, Universität Bremen, Am Fallturm, 28359 Bremen, Germany
2008en
ABI

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The Pleba\'{n}ski--Demia\'{n}ski 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 Pleba\'{n}ski--Demia\'{n}ski 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.

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