Characterizing geodesic deviations in a topological star spacetime: Massive, charged, spinning, and stringylike objects

Donato Bini; Giorgio Di Russo

doi:10.1103/6xc4-wm2f

Characterizing geodesic deviations in a topological star spacetime: Massive, charged, spinning, and stringylike objects

Donato Bini ¹ and Giorgio Di Russo ²

¹Istituto per le Applicazioni del Calcolo “M. Picone,” CNR, I-00185 Rome, Italy
²School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS, Hangzhou 310024, China

PDF

Phys. Rev. D 112, 024021 – Published 8 July, 2025

DOI: https://doi.org/10.1103/6xc4-wm2f

Abstract

We study deviations from geodesic motions in a topological star spacetime for either massive, charged and spinning particles, elucidating different behaviors with the Schwarzschild spacetime. We also consider the deviations for the motion of electrically charged stringy probes in $D = 5$ , framing all cases within a unified picture.

Physics Subject Headings (PhySH)

Authorization Required

We need you to provide your credentials before accessing this content.

Physical Review D

Export citation

Export citation

Characterizing geodesic deviations in a topological star spacetime: Massive, charged, spinning, and stringylike objects

Abstract

Physics Subject Headings (PhySH)

Authorization Required

Other Options

References (Subscription Required)

Outline

Information

Filter

Filter

Article Lookup

Enter a citation

Characterizing geodesic deviations in a topological star spacetime: Massive, charged, spinning, and stringylike objects

Abstract

Physics Subject Headings (PhySH)

Authorization Required

Log in via your institution

Log in via APS Member Subscription

Other Options

References (Subscription Required)