Globally stationary but locally static space-times: A gravitational analog of the Aharonov-Bohm effect
- 15 September 1982
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 26 (6) , 1281-1290
- https://doi.org/10.1103/physrevd.26.1281
Abstract
It is well known that gravitational fields may be locally the same but globally distinct due to differences in the topology of their underlying manifolds. Globally stationary but locally static gravitational fields provide an example of gravitational fields which are locally the same but globally distinct in spite of the homeomorphism of their underlying manifolds. Any static metric on a space-time manifold with nonvanishing first Betti number is shown to generate an -parameter family of such solutions. These fields are seen to provide a gravitational analog of the electromagnetic Aharonov-Bohm effect. The exterior field of a rotating infinite cylinder of matter is discussed as an exactly soluble example.
Keywords
This publication has 31 references indexed in Scilit:
- Classical Electromagnetic Interaction of a Charged Particle with a Constant-Current SolenoidPhysical Review D, 1973
- Theorem on the Reality of the Electromagnetic PotentialsAmerican Journal of Physics, 1972
- Aharonov-Bohm Effect—Quantum Effects on Charged Particles in Field-Free RegionsAmerican Journal of Physics, 1970
- Further examples of «machian» effects of rotating bodies in general relativityIl Nuovo Cimento B (1971-1996), 1968
- Nonlocal effects in classical and quantum theoriesAnnals of Physics, 1967
- Particle wave functions in weak gravitational fieldsIl Nuovo Cimento B (1971-1996), 1967
- A gravitational Aharonov-Bohm effectIl Nuovo Cimento B (1971-1996), 1967
- On the "special role" of the electromagnetic potentials in quantum mechanicsUspekhi Fizicheskih Nauk, 1962
- Significance of Electromagnetic Potentials in the Quantum TheoryPhysical Review B, 1959
- On the Hamilton-Jacobi theory and quantization of generalized electrodynamicsProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1938