Abstract
In earlier papers, we have introduced an approach for quantum-gravitational bodies based on the quantum potential written in the form of an equation of state to be added to equations of gravitation theories. In the case of Einsteinian gravitation, we have obtained quantum black holes by rough calculation but, in the case of Newtonian gravitation, with additional assumption on "no-escape" radius for light, the same bodies may be obtained by simple but rigorous mathematical calculation. This paper deals with Newtonian rotating quantum black holes and derives their mass spectrum that is closed to those of some authors based on relativistic treatment.
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