• Editors' Suggestion

Optical Time Reversal from Time-Dependent Epsilon-Near-Zero Media

Stefano Vezzoli, Vincenzo Bruno, Clayton DeVault, Thomas Roger, Vladimir M. Shalaev, Alexandra Boltasseva, Marcello Ferrera, Matteo Clerici, Audrius Dubietis, and Daniele Faccio
Phys. Rev. Lett. 120, 043902 – Published 26 January 2018
PDFHTMLExport Citation

Abstract

Materials with a spatially uniform but temporally varying optical response have applications ranging from magnetic field-free optical isolators to fundamental studies of quantum field theories. However, these effects typically become relevant only for time variations oscillating at optical frequencies, thus presenting a significant hurdle that severely limits the realization of such conditions. Here we present a thin-film material with a permittivity that pulsates (uniformly in space) at optical frequencies and realizes a time-reversing medium of the form originally proposed by Pendry [Science 322, 71 (2008)]. We use an optically pumped, 500 nm thick film of epsilon-near-zero (ENZ) material based on Al-doped zinc oxide. An incident probe beam is both negatively refracted and time reversed through a reflected phase-conjugated beam. As a result of the high nonlinearity and the refractive index that is close to zero, the ENZ film leads to time reversed beams (simultaneous negative refraction and phase conjugation) with near-unit efficiency and greater-than-unit internal conversion efficiency. The ENZ platform therefore presents the time-reversal features required, e.g., for efficient subwavelength imaging, all-optical isolators and fundamental quantum field theory studies.

  • Figure
  • Figure
  • Figure
  • Received 21 September 2017
  • Corrected 29 January 2018

DOI:https://doi.org/10.1103/PhysRevLett.120.043902

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & OpticalCondensed Matter, Materials & Applied Physics

Corrections

29 January 2018

Correction: The AFOSR grant number contained an error and was corrected.

Authors & Affiliations

Stefano Vezzoli1, Vincenzo Bruno1, Clayton DeVault2, Thomas Roger1, Vladimir M. Shalaev3, Alexandra Boltasseva3, Marcello Ferrera1, Matteo Clerici4, Audrius Dubietis5, and Daniele Faccio1,6,*

  • 1Institute of Photonics and Quantum Sciences, Heriot-Watt University, SUPA, Edinburgh EH14 4AS, United Kingdom
  • 2Department of Physics and Astronomy and Birck Nanotechnology Center, Purdue University, 1205 West State Street, West Lafayette, Indiana 47907-2057, USA
  • 3School of Electrical and Computer Engineering and Birck Nanotechnology Center, Purdue University, 1205 West State Street, West Lafayette, Indiana 47907-2057, USA
  • 4School of Engineering, University of Glasgow, G12 8LT Glasgow, United Kingdom
  • 5Laser Research Center, Vilnius University, Sauletekio Avenue 10, LT-10223 Vilnius, Lithuania
  • 6School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom

  • *d.faccio@hw.ac.uk

Article Text (Subscription Required)

Click to Expand

Supplemental Material (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 120, Iss. 4 — 26 January 2018

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×