New Description of Pseudo-newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes
نویسنده
چکیده
We present a pseudo-Newtonian potential for accretion disk modeling around rotating black holes. This potential can describe the general relativistic effects in accretion disk properly. As the inclusion of rotation in a proper way is very important at the inner edge of the disk we derived our potential starting from the Kerr metric. This potential can reproduce all the essential properties of general relativity with 10% error at most even for rapidly rotating black holes. Subject headings: pseudo-Newtonian potential — Kerr geometry — accretion disk
منابع مشابه
Description of Pseudo-newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes
We present a pseudo-Newtonian potential for accretion disk modeling around the rotating black holes. This potential can describe the general relativistic effects on accretion disk. As the inclusion of rotation in a proper way is very important at an inner edge of disk the potential is derived from the Kerr metric. This potential can reproduce all the essential properties of general relativity w...
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