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(2.6) This equation allows for real solutions for the radius depending on the values of the parametersa andg

Horizons The horizons are defined by the relation grr→∞ which is equivalent to set ∆ =r2− 2M(r)r +a2 = 0

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Geodesic structure of a rotating regular black hole

gr-qc · 2019-08-05 · conditional · novelty 5.0

Timelike geodesics in the rotating Hayward regular black hole admit a Carter-like fourth constant of motion, and out-of-plane orbits differ from Kerr mainly at low spin and large length parameter g.

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  • Geodesic structure of a rotating regular black hole gr-qc · 2019-08-05 · conditional · none · ref 1

    Timelike geodesics in the rotating Hayward regular black hole admit a Carter-like fourth constant of motion, and out-of-plane orbits differ from Kerr mainly at low spin and large length parameter g.