Rotating dirty black hole and its shadow
In this paper, we examine the effect of dark matter to a Kerr black hole of mass m. The metric is derived using the Newman-Janis algorithm, where the seed metric originates from the Schwarzschild black hole surrounded by a spherical shell of dark matter with mass M and thickness ∆rs. The seed metric...
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| Main Authors: | , |
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| 格式: | text |
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Animo Repository
2020
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| 在線閱讀: | https://animorepository.dlsu.edu.ph/faculty_research/11571 |
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| 機構: | De La Salle University |