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Radiation Transfer of Emission Lines in Curved Space-Time

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arxiv astro-ph/0406401 v1 pith:5YVY27N6 submitted 2004-06-17 astro-ph

Steven V. Fuerst , Kinwah Wu This is my paper · ORCID
classification astro-ph
keywords formulationcurvedemissionspace-timeabsorbingaccountaccretionapply
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We present a general formulation for ray-tracing calculations in curved space-time. The formulation takes full account of relativistic effects in the photon transport and the relative motions of the emitters and the light-of-sight absorbing material. We apply the formulation to calculate the emission from accretion disks and tori around rotating black holes.

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  1. Geodesic structure of a rotating regular black hole

    gr-qc 2019-08 conditional novelty 5.0 of 10

    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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