Low-velocity-favored transition radiation
When a charged particle penetrates through an optical interface, photon emissions emerge-a phenomenon known as transition radiation. Being paramount to fundamental physics, transition radiation has enabled many applications from high-energy particle identification to novel light sources. A rule of t...
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sg-ntu-dr.10356-1740152024-03-12T01:31:41Z Low-velocity-favored transition radiation Chen, Jialin Chen, Ruoxi Tay, Fuyang Gong, Zheng Hu, Hao Yang, Yi Zhang, Xinyan Wang, Chan Kaminer, Ido Chen, Hongsheng Zhang, Baile Lin, Xiao School of Physical and Mathematical Sciences School of Electrical and Electronic Engineering Centre for Disruptive Photonic Technologies (CDPT) Physics Low-velocity Optical interfaces When a charged particle penetrates through an optical interface, photon emissions emerge-a phenomenon known as transition radiation. Being paramount to fundamental physics, transition radiation has enabled many applications from high-energy particle identification to novel light sources. A rule of thumb in transition radiation is that the radiation intensity generally decreases with the decrease of particle velocity v; as a result, low-energy particles are not favored in practice. Here, we find that there exist situations where transition radiation from particles with extremely low velocities (e.g., v/c<10^{-3}) exhibits comparable intensity as that from high-energy particles (e.g., v/c=0.999), where c is the light speed in free space. The comparable radiation intensity implies an extremely high photon extraction efficiency from low-energy particles, up to 8 orders of magnitude larger than that from high-energy particles. This exotic phenomenon of low-velocity-favored transition radiation originates from the interference of the excited Ferrell-Berreman modes in an ultrathin epsilon-near-zero slab. Our findings may provide a promising route toward the design of integrated light sources based on low-energy electrons and specialized detectors for beyond-standard-model particles. National Research Foundation (NRF) X. L. acknowledges the support partly from the National Natural Science Fund for Excellent Young Scientists Fund Program (Overseas) of China, the National Natural Science Foundation of China under Grant No. 62175212, Zhejiang Provincial Natural Science Fund Key Project under Grant No. LZ23F050003, and the Fundamental Research Funds for the Central Universities (2021FZZX001-19). H. C. acknowledges the support from the Key Research and Development Program of the Ministry of Science and Technology under Grants No. 2022YFA1404704, No. 2022YFA1404902, and No. 2022YFA1405200, the National Natural Science Foundation of China under Grants No. 11961141010 and No. 61975176. J. C. acknowledges the support from the Chinese Scholarship Council (CSC No. 202206320287). I. K. acknowledges the support from the Israel Science Foundation under Grant No. 3334/19 and the Israel Science Foundation under Grant No. 830/19. Y. Y. acknowledges the support from the start-up fund of the University of Hong Kong and the National Natural Science Foundation of China Excellent Young Scientists Fund (HKU 12222417). B. Z. acknowledges the support from Singapore National Research Foundation Competitive Research Program No. NRF-CRP23-2019-0007. 2024-03-12T01:31:41Z 2024-03-12T01:31:41Z 2023 Journal Article Chen, J., Chen, R., Tay, F., Gong, Z., Hu, H., Yang, Y., Zhang, X., Wang, C., Kaminer, I., Chen, H., Zhang, B. & Lin, X. (2023). Low-velocity-favored transition radiation. Physical Review Letters, 131(11), 113002-. https://dx.doi.org/10.1103/PhysRevLett.131.113002 0031-9007 https://hdl.handle.net/10356/174015 10.1103/PhysRevLett.131.113002 37774266 2-s2.0-85172869379 11 131 113002 en NRF-CRP23-2019-0007 Physical Review Letters © 2023 American Physical Society. All rights reserved. |
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Physics Low-velocity Optical interfaces Chen, Jialin Chen, Ruoxi Tay, Fuyang Gong, Zheng Hu, Hao Yang, Yi Zhang, Xinyan Wang, Chan Kaminer, Ido Chen, Hongsheng Zhang, Baile Lin, Xiao Low-velocity-favored transition radiation |
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When a charged particle penetrates through an optical interface, photon emissions emerge-a phenomenon known as transition radiation. Being paramount to fundamental physics, transition radiation has enabled many applications from high-energy particle identification to novel light sources. A rule of thumb in transition radiation is that the radiation intensity generally decreases with the decrease of particle velocity v; as a result, low-energy particles are not favored in practice. Here, we find that there exist situations where transition radiation from particles with extremely low velocities (e.g., v/c<10^{-3}) exhibits comparable intensity as that from high-energy particles (e.g., v/c=0.999), where c is the light speed in free space. The comparable radiation intensity implies an extremely high photon extraction efficiency from low-energy particles, up to 8 orders of magnitude larger than that from high-energy particles. This exotic phenomenon of low-velocity-favored transition radiation originates from the interference of the excited Ferrell-Berreman modes in an ultrathin epsilon-near-zero slab. Our findings may provide a promising route toward the design of integrated light sources based on low-energy electrons and specialized detectors for beyond-standard-model particles. |
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School of Physical and Mathematical Sciences |
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School of Physical and Mathematical Sciences Chen, Jialin Chen, Ruoxi Tay, Fuyang Gong, Zheng Hu, Hao Yang, Yi Zhang, Xinyan Wang, Chan Kaminer, Ido Chen, Hongsheng Zhang, Baile Lin, Xiao |
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Article |
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Chen, Jialin Chen, Ruoxi Tay, Fuyang Gong, Zheng Hu, Hao Yang, Yi Zhang, Xinyan Wang, Chan Kaminer, Ido Chen, Hongsheng Zhang, Baile Lin, Xiao |
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Chen, Jialin |
title |
Low-velocity-favored transition radiation |
title_short |
Low-velocity-favored transition radiation |
title_full |
Low-velocity-favored transition radiation |
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Low-velocity-favored transition radiation |
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Low-velocity-favored transition radiation |
title_sort |
low-velocity-favored transition radiation |
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2024 |
url |
https://hdl.handle.net/10356/174015 |
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1794549364180385792 |