The Euclidean quantisation of Kerr-Newman-de Sitter black holes
Piotr Chru\'sciel, Michael H\"orzinger
TL;DR
This paper investigates Einstein-Maxwell instantons related to Kerr-Newman-de Sitter black holes, revealing a quantisation condition on their masses and charges in Euclidean space.
Contribution
It introduces a novel quantisation condition for the parameters of Kerr-Newman-de Sitter black holes in Euclidean quantum gravity.
Findings
Derivation of a quantisation condition on black hole parameters
Identification of specific Euclidean solutions with discrete properties
Insights into the quantum structure of charged rotating black holes
Abstract
We study the family of Einstein-Maxwell instantons associated with the Kerr-Newman metrics with a positive cosmological constant. This leads to a quantisation condition on the masses and charges of the resulting Euclidean solutions.
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