Incomplete chirality of exceptional points in asymmetric optical microcavity
Creators
Abstract
A chiral exceptional point (EP) in an optical microcavity emerges from the coalescence of even and odd modes with identical azimuthal modal numbers under asymmetric perturbation. While the chirality of such EPs is well understood in circular disks with asymmetrically positioned Rayleigh scatterers, it becomes more intricate in asymmetric microcavities, where the contributing modes can exhibit nontrivial wave morphology according to chaotic deformation. To explore this, we consider a stand-alone microcavity composed of one half ellipse and two quarter ellipses, for which EPs exhibit incomplete chirality. Our analysis reveals that this incomplete chirality originates from prior mode coupling. After the prior mode coupling, only the quasinormal modes within each superposed mode pair that have identical azimuthal modal numbers but opposite parities contribute to the chirality at EPs. Consequently, the chirality of the EP modes remains incomplete, depending on the relative weight of the original mode pair. Finally, we analyze the formation of EPs and their chiral properties in a generic asymmetric microcavity, providing insights into the underlying mechanisms of incomplete chirality.
Copyright and License (English)
©2025 American Physical Society
Funding (English)
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIT; Grant No. RS-2024-00343969); C.-H.Y. acknowledges financial support from the Institute for Basic Science (Grant No. IBS-R024-D1).
Contributions
C.-H.Y. and C.-M.K. contributed equally to this work.
Data Availability
The data that support the findings of this article are not publicly available upon publication because it is not technically feasible and/or the cost of preparing, depositing, and hosting the data would be prohibitive within the terms of this research project. The data are available from the authors upon reasonable request.
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Additional details
Funding
- National Research Foundation of Korea
- Ministry of Science and ICT
- RS-2024-00343969
- Institute for Basic Science
- IBS-R024-D1
Dates
- Submitted
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2025-07-13
- Accepted
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2025-10-01