Total Magnification and Magnification Centroid Due to Strongly Naked Singularity Lensing
Justin DeAndrea, Shreya Patel

TL;DR
This paper analyzes gravitational lensing by a strongly naked singularity at the galactic center, calculating magnification properties and comparing them to black hole lenses, with implications for cosmic censorship hypotheses.
Contribution
It provides detailed calculations of magnification centroid, shift, and total magnification for SNS lensing using the Janis-Newman-Winicour metric, expanding previous work and highlighting observable differences from black holes.
Findings
Magnification centroid increases with source position.
Magnification centroid shift peaks then decreases with source position.
Total magnification decreases to one as source position grows.
Abstract
A strongly naked singularity (SNS) was modelled at the center of the Galaxy. This specific type of naked singularity was characterized in 2008 by Virbhadra and Keeton. The lens is described using the Janis-Newman-Winicour metric, which has an ordinary mass and massless scalar charge parameters. Gravitational lensing by the SNS gives rise to 4 images: 2 images on the same side as the source and 2 images on the opposite side of the source from the optic axis. We compute magnification centroid, magnification centroid shift, and total absolute magnification for many values of the angular source position. The nature of the curve for all three results are qualitatively similar to Schwarzschild black hole lenses, but quantitatively different. Magnification centroid increases as angular source position increases. As angular source position increases, magnification centroid shift increases to a…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
