Generation of 11-fs dark pulses via coherent perfect absorption in plasmonic metamaterial
Generation of 11-fs dark pulses via coherent perfect absorption in plasmonic metamaterial
Dark pulses are dips in power of electro magnetic radiation on a constant background that are often accompanied by a phase jump across the intensity minimum. Since their discovery, dark pulses have attracted considerable attention in many fields such as dark solitons and optical communications. Here we report generation of 11 fs dark pulses using the regime of “perfect absorption”. When two coherent counter-propagating electromagnetic waves of the same intensity form a standing wave, a thin absorber placed in the antinode of the wave could completely dissipate energy of both waves if its traveling wave absorption is 50%. If one of the waves is a “gate pulse” in time domain, the “perfect absorption” regime will exist only during the pulse, when a dip in power of “carrier pulse” will be created. “Dark pulses” are generated by positioning plasmonic absorber in the anti-node of the standing wave and balancing peak intensities . These dark pulses are characterized using cross-correlation technique. Measured width of the “dark pulse” is border than 6 fs “gate pulse”, which is nearly 11fs as shown in Fig. 1B. Width of the “dark pulse” is limited by transient plasmonic absorption establishes with completion of the plasmon relaxation time, which is typically 11fs in gold nanostructures. We argue that bandwidth of dark pulses is limited by the plasmon relaxation time of the absorber.
Nalla, V.
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Valente, J.
b1d50ead-5c3d-4416-ad05-3beb1b373146
Sun, H.
24faa0fa-7976-4270-8fc6-9c85e201662d
Zheludev, N.I.
32fb6af7-97e4-4d11-bca6-805745e40cc6
Nalla, V.
13a5bf90-d118-435e-912f-73c457f2713e
Valente, J.
b1d50ead-5c3d-4416-ad05-3beb1b373146
Sun, H.
24faa0fa-7976-4270-8fc6-9c85e201662d
Zheludev, N.I.
32fb6af7-97e4-4d11-bca6-805745e40cc6
Nalla, V., Valente, J., Sun, H. and Zheludev, N.I.
(2017)
Generation of 11-fs dark pulses via coherent perfect absorption in plasmonic metamaterial.
6th International Topical Meeting on Nanophotonics and Metamaterials (NanoMeta 2017), Tirol, Seefeld, Austria.
04 - 07 Jan 2017.
Record type:
Conference or Workshop Item
(Poster)
Abstract
Dark pulses are dips in power of electro magnetic radiation on a constant background that are often accompanied by a phase jump across the intensity minimum. Since their discovery, dark pulses have attracted considerable attention in many fields such as dark solitons and optical communications. Here we report generation of 11 fs dark pulses using the regime of “perfect absorption”. When two coherent counter-propagating electromagnetic waves of the same intensity form a standing wave, a thin absorber placed in the antinode of the wave could completely dissipate energy of both waves if its traveling wave absorption is 50%. If one of the waves is a “gate pulse” in time domain, the “perfect absorption” regime will exist only during the pulse, when a dip in power of “carrier pulse” will be created. “Dark pulses” are generated by positioning plasmonic absorber in the anti-node of the standing wave and balancing peak intensities . These dark pulses are characterized using cross-correlation technique. Measured width of the “dark pulse” is border than 6 fs “gate pulse”, which is nearly 11fs as shown in Fig. 1B. Width of the “dark pulse” is limited by transient plasmonic absorption establishes with completion of the plasmon relaxation time, which is typically 11fs in gold nanostructures. We argue that bandwidth of dark pulses is limited by the plasmon relaxation time of the absorber.
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Accepted/In Press date: 18 November 2016
e-pub ahead of print date: 4 January 2017
Venue - Dates:
6th International Topical Meeting on Nanophotonics and Metamaterials (NanoMeta 2017), Tirol, Seefeld, Austria, 2017-01-04 - 2017-01-07
Organisations:
Optoelectronics Research Centre
Identifiers
Local EPrints ID: 405443
URI: http://eprints.soton.ac.uk/id/eprint/405443
PURE UUID: 84d1d785-f4b5-4e40-bf00-8f4d8e7361ab
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Date deposited: 03 Feb 2017 16:08
Last modified: 16 Mar 2024 02:43
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Contributors
Author:
V. Nalla
Author:
J. Valente
Author:
H. Sun
Author:
N.I. Zheludev
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