Particle motion and tidal force in a non-vacuum-charged naked singularity

dc.contributor.authorJoshi, Pankaj S.
dc.date.accessioned2025-02-05T12:16:31Z
dc.date.available2025-02-05T12:16:31Z
dc.date.issued2024-04-10
dc.descriptionOpen Access
dc.description.abstractWe investigate the gravitational field of a charged, non-vacuum, non-rotating, spherically symmetric body of mass M assuming a static solution to the Einstein–Maxwell field equations. We show the characteristics of perihelion precession of orbits in the case of charged naked singularity (CNS) spacetime. Here we discuss some novel features of light-like geodesics in this spacetime. We also discuss the comparative study of tidal force in the null singularity spacetime and charged naked singularity spacetime.
dc.identifier.citationViththani, D. P., Joshi, A. B., Bhanja, T., & Joshi, P. S. (2024). Particle motion and tidal force in a non-vacuum-charged naked singularity. The European Physical Journal C, 84(4), 383. https://doi.org/10.1140/epjc/s10052-024-12746-1
dc.identifier.urihttps://link.springer.com/article/10.1140/epjc/s10052-024-12746-1
dc.identifier.urihttps://ir.ahduni.edu.in/handle/123456789/4080
dc.language.isoen
dc.publisherSpringer Nature
dc.titleParticle motion and tidal force in a non-vacuum-charged naked singularity
dc.typeArticle

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