Wavy way to the Kerr metric and the quantum nature of its ring singularity
O. Gurtug, M. Halilsoy

TL;DR
This paper explores a novel derivation of the Kerr metric via colliding gravitational waves, examines the classical stability of related spacetime structures, and demonstrates that quantum effects can regularize the Kerr ring singularity.
Contribution
It provides an alternative derivation of the Kerr metric using colliding gravitational waves and shows quantum effects can heal the classical ring singularity.
Findings
Kerr metric can be derived from colliding gravitational waves.
Certain spacetime structures are transient black holes under stability conditions.
Quantum probe indicates the Kerr ring singularity is quantum regular.
Abstract
From inherent non-linearity two gravitational waves, unless they are unidirectional, fail to satisfy a superposition law. They collide to develop a new spacetime carrying the imprints of the incoming waves. Same behaviour is valid also for any massless lightlike field. As a result of the violent collision process either a naked singularity or a Cauchy horizon (CH) develops. It was shown by Chandrasekhar and Xanthopoulos (CX) that a particular class of colliding gravitational waves (CGW) spacetime is locally isometric to the Kerr metric for rotating black holes. This relation came to be known as the CX duality. Such a duality can be exploited as an alternative derivation for the Kerr metric as we do herein. Not each case gives rise to a CH but those which do are transient to a black hole state provided stability requirements are met. These classical considerations can be borrowed to shed…
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Taxonomy
TopicsQuantum Mechanics and Non-Hermitian Physics · Quantum chaos and dynamical systems · Black Holes and Theoretical Physics
