Gravitational lensing and shadows in the toron solution of Einstein's equations using ray tracing methods
General Relativity and Quantum Cosmology
2025-03-13 v2 Exactly Solvable and Integrable Systems
Abstract
We present a numerical and analytical study of the so-called `toron' solution of the stationary axisymmetric Einstein equations in vacuum expressed in terms of elliptic functions. The asymptotic behavior of this solution coincides with the one of the NUT solution, i.e., it has a `gravimagnetic' mass known as the NUT parameter while the ordinary mass vanishes. The physical properties of this spacetime are studied via ray tracing. The results are compared to known geodesic flows in Schwarzschild, Kerr and NUT spacetimes to discuss similarities and differences, with a particular emphasis on the comparison of NUT and toron spacetimes.
Keywords
Cite
@article{arxiv.2501.04509,
title = {Gravitational lensing and shadows in the toron solution of Einstein's equations using ray tracing methods},
author = {Eddy B. de Leon. C. Klein and D. Korotkin},
journal= {arXiv preprint arXiv:2501.04509},
year = {2025}
}