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We investigate the existence of Reissner-Nordstr"om (RN) type black holes in f® gravity. Our emphasis is to derive, in the presence of electrostatic source, the necessary conditions which provide such static, spherically symmetric (SSS) black holes available in f® gravity. We also study the thermodynamics of the black hole solution.

生成讲解博客的中文版本

生成AI智能校验的中文版本