Kerr-AdS and Kerr-dS solutions revisited
A. G. Agnese, M. La Camera (INFN)
TL;DR
This paper revisits Kerr solutions with a cosmological constant, analyzing their properties under a specific boundary condition where frame dragging angular velocity vanishes at spatial boundaries.
Contribution
It introduces a new boundary condition for Kerr-(A)dS solutions and explores the properties of extreme black holes within this framework.
Findings
Properties of extreme black holes are discussed.
The boundary condition affects the angular velocity profile.
Revisited solutions offer new insights into Kerr-(A)dS geometries.
Abstract
We reconsider the Kerr metric with cosmological term imposing the condition that the angular velocity of the dragging of the inertial frames vanishes at spatial boundaries. Some properties of the extreme black holes in the revisited solutions are discussed.
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