Characterizing geodesic deviations in a Topological Star spacetime: massive, charged, spinning and stringy-like objects
Donato Bini, Giorgio Di Russo

TL;DR
This paper investigates how geodesic deviations behave in a Topological Star spacetime for various particles, revealing differences from Schwarzschild spacetime and unifying cases including stringy probes in five dimensions.
Contribution
It provides a comprehensive analysis of geodesic deviations for different particles in Topological Star spacetimes, including charged, spinning, and stringy probes, within a unified framework.
Findings
Distinct deviation behaviors compared to Schwarzschild spacetime
Unified description for massive, charged, spinning, and stringy probes
Insights into higher-dimensional stringy effects on geodesics
Abstract
We study deviations from geodesic motions in a Topological Star spacetime for either massive, charged and spinning particles, elucidating different behaviours with the Schwarzschild spacetime. We also consider the deviations for the motion of electrically charged stringy probes in , framing all cases within a unified picture.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
