“School of Astronomy”
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| Paper IPM / Astronomy / 15716 |
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Real black holes in the universe are located in the expanding accelerating background which is called the cosmological black holes. Hence, to study the background effects, it is necessary to model these black holes in the cosmological background where the dark energy is the dominant energy. In this paper, we argue that most of the dynamical cosmological black holes can be modeled by point mass cosmological black holes. Considering the de Sitter background for the accelerating universe, we present the point mass cosmological background in the cosmological de Sitter spacetime. Our work also includes the point mass black holes which have charge and angular momentum. We study the mass, horizons, redshift structure and geodesics properties for these black holes.
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