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Phys. Rev. D 70, 044020 (2004) [7 pages]

Vacuum C metric and the gravitational Stark effect

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D. Bini*
Istituto per le Applicazioni del Calcolo “M. Picone,” CNR, I-00161 Rome, Italy
International Center for Relativistic Astrophysics-I.C.R.A., University of Rome “La Sapienza,” I-00185 Rome, Italy

C. Cherubini
Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 2EG, England, United Kingdom;
Dipartimento di Fisica “E.R. Caianiello,” Università di Salerno, I-84081, Italy;
International Center for Relativistic Astrophysics-I.C.R.A., University of Rome “La Sapienza,” I-00185 Rome, Italy

B. Mashhoon
Department of Physics and Astronomy, University of Missouri-Columbia, Columbia, Missouri 65211, USA

Received 16 January 2004; revised 30 March 2004; published 18 August 2004

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.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.70.044020
DOI:
10.1103/PhysRevD.70.044020
PACS:
04.20.Cv, 04.25.Nx

*Electronic address: binid@icra.it

Present address: Faculty of Engineering, University Campus Bio-Medico of Rome, via E. Longoni 47, 00155 Rome, Italy. Electronic address: cherubini@icra.it

Electronic address: MashhoonB@missouri.edu