Charged black holes in Vaidya backgrounds: Hawking's Radiation
Ng. Ibohal, L. Kapil
TL;DR
This paper introduces new solutions to Einstein's equations describing charged black holes within Vaidya backgrounds, enhancing understanding of their properties and radiation behavior.
Contribution
It presents novel embedded solutions for charged and rotating black holes in Vaidya spacetimes, expanding the theoretical framework of black hole models.
Findings
New embedded solutions for Reissner-Nordstrom-Vaidya and Kerr-Newman-Vaidya black holes.
Insights into the structure and properties of charged black holes in dynamic backgrounds.
Potential implications for understanding Hawking radiation in these contexts.
Abstract
In this paper we propose a class of embedded solutions of Einstein's field equations describing non-rotating Reissner-Nordstrom-Vaidya and rotating Kerr-Newman-Vaidya black holes.
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