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A small guide to variations in teleparallel gauge theories of gravity and the Kaniel-Itin model

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arxiv gr-qc/9801036 v1 pith:ZS2XC7UK submitted 1998-01-12 gr-qc hep-th

classification gr-qchep-th
keywords modelequationkaniel-itinalphacoframefieldgaugegravitational
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Recently Kaniel & Itin proposed a gravitational model with the wave type equation [\square+\lambda(x)]\vartheta^\alpha=0 as vacuum field equation, where \vartheta^\alpha denotes the coframe of spacetime. They found that the viable Yilmaz-Rosen metric is an exact solution of the tracefree part of their field equation. This model belongs to the teleparallelism class of gravitational gauge theories. Of decisive importance for the evaluation of the Kaniel-Itin model is the question whether the variation of the coframe commutes with the Hodge star. We find a master formula for this commutator and rectify some corresponding mistakes in the literature. Then we turn to a detailed discussion of the Kaniel-Itin model.

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    gr-qc 2019-08 conditional novelty 6.0 of 10

    In the linearized regime of nonlocal gravity, the gravitomagnetic field of a rotating mass acquires a tiny nonlocal correction, below one part in 10^10 of the general-relativistic value for Earth and Moon.

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