Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 18, Issue 5, Pages 833-841Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/18/5/306
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In the context of the teleparallel equivalent of general relativity, we obtain the tetrad and the torsion fields of the stationary axisymmetric Kerr spacetime. It is shown that, in the slow rotation and weak-field approximations, the axial-vector torsion plays the role of the gravitomagnetic component of the gravitational field, and is thus responsible for the Lense-Thirring effect.
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