Abstract
The Kerr-type solution in the Brans-Dicke theory should contain three parameters: a massm, a rotational parametera 0, and a coupling parameterω It goes over to the Kerr solution in Einstein's theory of general relativity in the limitω → 8. Using these conditions, we construct a special solution from Bruckman's solutions which can be regarded as a Kerr-type solution in the Brans-Dicke theory.
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