Horizon Dynamics of Evaporating Black Holes in a Higher Dimensional Inflationary Universe
Manasse Mbonye
TL;DR
This paper investigates the behavior and structure of horizons in higher-dimensional, evaporating black holes within an inflationary universe, focusing on their dynamics and location in a de Sitter spacetime.
Contribution
It provides a detailed analysis of horizon dynamics and structure for Vaidya-type black holes in higher-dimensional de Sitter space, extending previous studies to more complex cosmological models.
Findings
Horizon locations are explicitly determined.
Horizon dynamics are characterized in higher dimensions.
Insights into black hole evaporation in an inflationary context.
Abstract
Spherically symmetric Black Holes of the Vaidya type are examined in an asymptotically de Sitter, higher dimensional spacetime. The various horizons are located. The structure and dynamics of such horizons are studied.
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