File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Low-Velocity-Favored Transition Radiation

TitleLow-Velocity-Favored Transition Radiation
Authors
Issue Date15-Sep-2023
PublisherAmerican Physical Society
Citation
Physical Review Letters, 2023, v. 131, n. 11, p. 1-8 How to Cite?
AbstractWhen 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.
Persistent Identifierhttp://hdl.handle.net/10722/346435
ISSN
2023 Impact Factor: 8.1
2023 SCImago Journal Rankings: 3.040

 

DC FieldValueLanguage
dc.contributor.authorChen, Jialin-
dc.contributor.authorChen, Ruoxi-
dc.contributor.authorTay, Fuyang-
dc.contributor.authorGong, Zheng-
dc.contributor.authorHu, Hao-
dc.contributor.authorYang, Yi-
dc.contributor.authorZhang, Xinyan-
dc.contributor.authorWang, Chan-
dc.contributor.authorKaminer, Ido-
dc.contributor.authorChen, Hongsheng-
dc.contributor.authorZhang, Baile-
dc.contributor.authorLin, Xiao-
dc.date.accessioned2024-09-17T00:30:32Z-
dc.date.available2024-09-17T00:30:32Z-
dc.date.issued2023-09-15-
dc.identifier.citationPhysical Review Letters, 2023, v. 131, n. 11, p. 1-8-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10722/346435-
dc.description.abstractWhen 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.-
dc.languageeng-
dc.publisherAmerican Physical Society-
dc.relation.ispartofPhysical Review Letters-
dc.titleLow-Velocity-Favored Transition Radiation-
dc.typeArticle-
dc.identifier.doi10.1103/PhysRevLett.131.113002-
dc.identifier.scopuseid_2-s2.0-85172869379-
dc.identifier.volume131-
dc.identifier.issue11-
dc.identifier.spage1-
dc.identifier.epage8-
dc.identifier.eissn1079-7114-
dc.identifier.issnl0031-9007-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats