Cerenkov radiation in vacuum from a superluminal grating
File(s)PhysRevResearch.4.013064.pdf (1.12 MB)
Published version
Author(s)
Oue, Daigo
Ding, Kun
Pendry, John
Type
Journal Article
Abstract
Nothing can physically travel faster than light in vacuum. There are several ways proposed to bypass the light barrier and produce ˇCerenkov radiation ( ˇCR) in vacuum. In this article, we theoretically predict ˇCR in vacuum from a spatiotemporally modulated boundary. We consider the modulation of traveling wave type and apply a uniform electrostatic field on the boundary to generate electric dipoles. Since the induced dipoles stick to the interface, they travel at the modulation speed. When the grating travels faster than light, it emits ˇCR. In order to quantitatively examine this argument, we need to calculate the field scattered at the boundary. We utilise a dynamical
differential method, which we developed in the previous paper, to quantitatively evaluate the field distribution in such a situation. We can confirm that all scattered fields are evanescent if the modulation speed is slower than light while some become propagating if the modulation is faster
than light.
differential method, which we developed in the previous paper, to quantitatively evaluate the field distribution in such a situation. We can confirm that all scattered fields are evanescent if the modulation speed is slower than light while some become propagating if the modulation is faster
than light.
Date Issued
2022-01-31
Date Acceptance
2021-12-29
Citation
Physical Review Research, 2022, 4, pp.1-6
ISSN
2643-1564
Publisher
American Physical Society
Start Page
1
End Page
6
Journal / Book Title
Physical Review Research
Volume
4
Copyright Statement
© 2022 The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.
License URL
Sponsor
Gordon and Betty Moore Foundation
Identifier
https://journals.aps.org/prresearch/abstract/10.1103/PhysRevResearch.4.013064
Grant Number
00009581
Publication Status
Published
Date Publish Online
2022-01-31