Kerr-Schild Geometry from Cosmology to Microworld and Space-Time Structure
Alexander Burinskii

TL;DR
This paper explores Kerr-Schild geometry's role in modeling diverse space-times, from cosmology to micro-worlds, revealing insights into vacuum fluctuations, twistorial structures, and the universe's flatness and cosmological constant.
Contribution
It introduces a Kerr-Schild model of the Bubble Universe with rotating de Sitter space, linking micro-world particle models to cosmological structures within a unified geometric framework.
Findings
Universe modeled as a semi-closed rotating de Sitter space
Micro-world models incorporate twistorial and beam-like vacuum fluctuations
Universe likely flat with zero cosmological constant
Abstract
The Kerr-Schild (KS) geometry is linked tightly with the auxiliary \emph{flat} Minkowski background. Nevertheless, it describes many curved space-times and the related physical models, starting from cosmology and black holes to the microworld of the spinning elementary particles and the pre-quantum structure of vacuum fluctuations. We consider here a KS model of the Bubble Universe -- a semi-closed Universe with a rotating de Sitter (or anti-de Sitter) space embedded in an external flat space-time. When the solution has two horizons, it may also be interpreted as an Universe inside a black hole. In micro-world the KS geometry yields a model of the spinning particle consistent with gravity and describes a pre-quantum twistorial structure of space-time with the beam-like fluctuations of metric consistent with the beamlike fluctuations of electromagnetic vacuum. These light-like…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
