Antipodal identification in the Schwarschild spacetime
Miguel Socolovsky

TL;DR
This paper investigates the effects of antipodal identification on Schwarzschild spacetime, revealing changes in topology, light cone structure, and singularities through a Möbius transformation analysis.
Contribution
It introduces a novel analysis of antipodal identification in Schwarzschild spacetime, including topology and geometric properties, and addresses the suppression of conical singularities.
Findings
Non simply-connected topology: R^{2*} x S^2
Bending of light cones observed
Transformation affects horizons and singularities
Abstract
Through a M\"obius transformation, we study aspects like topology, ligth cones, horizons, curvature singularity, lines of constant Schwarzschild coordinates and , null geodesics, and transformed metric, of the spacetime that results from: i) the antipode identification in the Schwarzschild-Kruskal-Szekeres () spacetime, and ii) the suppression of the consequent conical singularity. In particular, one obtains a non simply-connected topology: and, as expected, bending light cones.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
