Boosted Horizon of a Boosted Space-Time Geometry
Emmanuele Battista, Giampiero Esposito, Paolo Scudellaro, Francesco, Tramontano

TL;DR
This paper studies the ultrarelativistic limit of Schwarzschild-de Sitter spacetime, revealing a shock-wave singularity, a scalar curvature singularity within a 3-sphere, and a novel 'boosted horizon' that exhibits antigravity-like effects on particles.
Contribution
It introduces a new ultrarelativistic boosting method for Schwarzschild-de Sitter spacetime and uncovers unique geometric features like the 'boosted horizon' and associated antigravity effects.
Findings
Identification of a shock-wave singularity in the boosted spacetime
Discovery of a scalar curvature singularity within a 3-sphere
Existence of a 'boosted horizon' acting as an elastic wall for particles
Abstract
We apply the ultrarelativistic boosting procedure to map the metric of Schwarzschild-de Sitter spacetime into a metric describing de Sitter spacetime plus a shock-wave singularity located on a null hypersurface, by exploiting the picture of the embedding of an hyperboloid in a five-dimensional Minkowski spacetime. After reverting to the usual four-dimensional formalism, we also solve the geodesic equation and evaluate the Riemann curvature tensor of the boosted Schwarzschild-de Sitter metric by means of numerical calculations, which make it possible to reach the ultrarelativistic regime gradually by letting the boost velocity approach the speed of light. Eventually, the analysis of the Kretschmann invariant (and of the geodesic equation) shows the global structure of space- time, as we demonstrate the presence of a "scalar curvature singularity" within a 3-sphere and find that it is…
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