Thomas precession in post-Newtonian gravitoelectromagnetism

Donato Bini, Paolo Carini, Robert T. Jantzen, and Daniel Wilkins
Phys. Rev. D 49, 2820 – Published 15 March 1994
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Abstract

The well-known Thomas precession effect is discussed in the context of the post-Newtonian approximation to general relativity using the language of gravitoelectromagnetism (3-plus-1 splitting of gravitational theory). Preliminary discussion anchors the post-Newtonian coordinate system and choice of gravitational variables in the mathematical structure of fully nonlinear general relativity, linking the post-Newtonian gravitoelectric and gravitomagnetic fields to kinematical properties of the associated observer congruence. The transformation laws for these fields under a change of post-Newtonian coordinate system are derived first within the post-Newtonian theory and then by taking the limit of their fully nonlinear form to reveal the interpretation of the various terms in the post-Newtonian case. These transformation laws are then used to make a case for the existence of a gravitational analogue of the ordinary Thomas precession of the spin of a gyroscope.

  • Received 16 September 1993

DOI:https://doi.org/10.1103/PhysRevD.49.2820

©1994 American Physical Society

Authors & Affiliations

Donato Bini

  • Physics Department and International Center for Relativistic Astrophysics, University of Rome, I-00185 Roma, Italy

Paolo Carini

  • GP-B, Hansen Labs, Stanford University, Stanford, California 94305
  • International Center for Relativistic Astrophysics, University of Rome, I-00185 Roma, Italy

Robert T. Jantzen

  • Department of Mathematical Physics, Villanova University, Villanova, Pennsylvania 19085
  • International Center for Relativistic Astrophysics, University of Rome, I-00185 Roma, Italy

Daniel Wilkins

  • Physics Department, University of Nebraska, Omaha, Nebraska 68182

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Issue

Vol. 49, Iss. 6 — 15 March 1994

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