Ray and wave optics in an optical wormhole

We examine ray trajectories and wave dynamics in an optical wormhole with constant negative Gaussian curvature, analogous to a monolayer graphene sheet or graphene wormholes. Focusing on the elliptic wormhole (EWH), we derive exact solutions for ray trajectories and show that the effective potential is impenetrable at the optical origin u = 0 , but rapidly vanishes at large distances, allowing trajectories to remain unaffected. By solving the Helmholtz equation on the EWH surface, we find that S-waves ( m = 0 ) are indefinitely trapped at the origin by an infinitely attractive effective potential, whereas modes with m ≠ 0 encounter an infinitely repulsive barrier. Additionally, we determine the spatially and frequency-dependent refractive index characterizing the EWH and discuss the corresponding optical response of the background.

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Publication Details

Journal
Physics Letters B
Published
2025-06-03
DOI
https://doi.org/10.1016/j.physletb.2025.139626
Citations
7
Primary Topic
Orbital Angular Momentum in Optics
Type
article
Field-Weighted Citation Impact
8.73
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article

Ray and wave optics in an optical wormhole

Abdullah Güvendi, Semra Gürtaş Doğan, Omar Mustafa
7 citations
Physics Letters B
Orbital Angular Momentum in Optics
8.73
article

Ray and wave optics in an optical wormhole

Abdullah Güvendi, Semra Gürtaş Doğan, Omar Mustafa
article en
7 citations

Abstract

We examine ray trajectories and wave dynamics in an optical wormhole with constant negative Gaussian curvature, analogous to a monolayer graphene sheet or graphene wormholes. Focusing on the elliptic wormhole (EWH), we derive exact solutions for ray trajectories and show that the effective potential is impenetrable at the optical origin u = 0 , but rapidly vanishes at large distances, allowing trajectories to remain unaffected. By solving the Helmholtz equation on the EWH surface, we find that S-waves ( m = 0 ) are indefinitely trapped at the origin by an infinitely attractive effective potential, whereas modes with m ≠ 0 encounter an infinitely repulsive barrier. Additionally, we determine the spatially and frequency-dependent refractive index characterizing the EWH and discuss the corresponding optical response of the background.

Physics Letters BVol. 868
Hakkari University (TR), Erzurum Technical University (TR), Eastern Mediterranean University (CY)
Affordable and clean energy
Openalex Percentile: Top 2%
Orbital Angular Momentum in Optics
8.73
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