Additional Observational Signatures of Asymmetric Thin-Shell Wormholes within 4D Einstein-Gauss-Bonnet Gravity
Abstract
In this paper, we study the optical appearance of a 4D Einstein-Gauss-Bonnet asymmetric thin-shell wormhole. Using Visser's cut-and-paste construction, we determine the photon sphere radius and critical impact parameter for different values of the Gauss-Bonnet coupling α. We then investigate the effective potential and photon motion inside the wormhole spacetime. It is found that the effective potential, light ray paths, and azimuthal angle are closely tied to the mass ratio of the two spacetimes. Considering an optically thin accretion disk as the only light source, we find that the asymmetric thin-shell wormhole's images exhibit additional photon rings and lensing bands that are absent for a 4D Einstein-Gauss-Bonnet black hole. Furthermore, the size of these extra rings increases with α, contrary to the black hole case. Such exceptionally bright rings provide a reliable criterion for distinguishing and characterizing a thin-shell wormhole spacetime. We also verify that the mass ratio and throat radius significantly tune the morphology of these extra photon rings.
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BibTeX
@misc{song2026additional,
title = {{Additional Observational Signatures of Asymmetric Thin-Shell Wormholes within 4D Einstein-Gauss-Bonnet Gravity}},
author = {J. Song and X. G. Lan},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2607.03673},
eprint = {2607.03673},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2607.03673},
}
RIS
TY - UNPB
TI - Additional Observational Signatures of Asymmetric Thin-Shell Wormholes within 4D Einstein-Gauss-Bonnet Gravity
AU - J. Song
AU - X. G. Lan
PY - 2026
DA - 2026/10/16
PB - arXiv
DO - 10.48550/arxiv.2607.03673
UR - https://arxiv.org/abs/2607.03673
AB - In this paper, we study the optical appearance of a 4D Einstein-Gauss-Bonnet asymmetric thin-shell wormhole. Using Visser's cut-and-paste construction, we determine the photon sphere radius and critical impact parameter for different values of the Gauss-Bonnet coupling α. We then investigate the effective potential and photon motion inside the wormhole spacetime. It is found that the effective potential, light ray paths, and azimuthal angle are closely tied to the mass ratio of the two spacetimes. Considering an optically thin accretion disk as the only light source, we find that the asymmetric thin-shell wormhole's images exhibit additional photon rings and lensing bands that are absent for a 4D Einstein-Gauss-Bonnet black hole. Furthermore, the size of these extra rings increases with α, contrary to the black hole case. Such exceptionally bright rings provide a reliable criterion for distinguishing and characterizing a thin-shell wormhole spacetime. We also verify that the mass ratio and throat radius significantly tune the morphology of these extra photon rings.
ER -