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- W3103226722 abstract "A naive introduction of a dependency of the mass of a black hole on the Schwarzschild time coordinate results in singular behavior of curvature invariants at the horizon, violating expectations from complementarity. If instead a temporal dependence is introduced in terms of a coordinate akin to the river time representation, the Ricci scalar is nowhere singular away from the origin. It is found that for a shrinking mass scale due to evaporation, the null radial geodesics that generate the horizon are slightly displaced from the coordinate singularity. In addition, a changing horizon scale significantly alters the form of the coordinate singularity in diagonal (orthogonal) metric coordinates representing the space-time. A Penrose diagram describing the growth and evaporation of an example black hole is constructed to examine the evolution of the coordinate singularity." @default.
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- W3103226722 date "2007-05-15" @default.
- W3103226722 modified "2023-10-16" @default.
- W3103226722 title "Coordinates with Non-Singular Curvature for a Time Dependent Black Hole Horizon" @default.
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- W3103226722 doi "https://doi.org/10.1007/s10701-007-9146-4" @default.
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