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research article

High-temperature ultrafast polariton parametric amplification in semiconductor microcavities

Saba, M.  
•
Ciuti, C.  
•
Bloch, J.
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2001
Nature

Cavity polaritons, the elementary optical excitations of semiconductor microcavities, may be understood as a superposition of excitons and cavity photons(1). Owing to their composite nature, these bosonic particles have a distinct optical response, at the same time very fast and highly nonlinear. Very efficient light amplification due to polariton-polariton parametric scattering has recently been reported in semiconductor microcavities at liquid-helium temperatures(2-11). Here we demonstrate polariton parametric amplification up to 120 K in GaAlAs-based microcavities and up to 220 K in CdTe-based microcavities. We show that the cut-off temperature for the amplification is ultimately determined by the binding energy of the exciton. A 5-mum-thick planar microcavity can amplify a weak light pulse more than 5,000 times. The effective gain coefficient of an equivalent homogeneous medium would be 10(7) cm(-1). The subpicosecond duration and high efficiency of the amplification could be exploited for high-repetition all-optical microscopic switches and amplifiers. 10(5) polaritons occupy the same quantum state during the amplification, realizing a dynamical condensate of strongly interacting bosons which can be studied at high temperature.

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Type
research article
DOI
10.1038/414731a
Web of Science ID

WOS:000172676200042

Author(s)
Saba, M.  
Ciuti, C.  
Bloch, J.
Thierry-Mieg, V.
Andre, R.
Dang, L. S.
Kundermann, S.  
Mura, A.
Bongiovanni, G.
Staehli, J. L.  
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Date Issued

2001

Published in
Nature
Volume

414

Issue

6865

Start page

731

End page

735

Subjects

STIMULATED SCATTERING

•

AMPLIFIER

•

EMISSION

•

COHERENT

•

EXCITONS

•

DEVICES

•

GAIN

Note

Swiss Fed Inst Technol Lausanne, PH Ecublens, Dept Phys, CH-1015 Lausanne EPFL, Switzerland. CNRS, L2M, F-92225 Bagneux, France. Univ Grenoble 1, Spectrometrie Phys Lab, F-38402 St Martin Dheres, France. Univ Cagliari, Dipartimento Fis, I-09042 Monserrato, Italy. Univ Cagliari, Ist Nazl Fis Mat, I-09042 Monserrato, Italy. Saba, M, Swiss Fed Inst Technol Lausanne, PH Ecublens, Dept Phys, CH-1015 Lausanne EPFL, Switzerland.

ISI Document Delivery No.: 501GD

Cited Reference Count: 20

Cited References:

BAUMBERG JJ, 2000, PHYS REV B, V62, P16247

BLOCH J, 1998, APPL PHYS LETT, V73, P1694

CIUTI C, 2000, PHYS REV B, V62

CIUTI C, 2001, PHYS REV B, V63

DANG LS, 1998, PHYS REV LETT, V81, P3920

DASBACH G, 2000, PHYS REV B, V62, P13076

EHRENSTEIN D, 2000, PHYS REV FOCUS, V5

HOUDRE R, 2000, PHYS REV LETT, V85, P2793

HUANG R, 2000, PHYS REV B, V61

IMAMOGLU A, 1996, PHYS REV A, V53, P4250

KELKAR PV, 1997, PHYS REV B, V56, P7564

LIDZEY DG, 1998, NATURE, V395, P53

LIDZEY DG, 2000, SCIENCE, V288, P1620

PEARTON SJ, 1999, J APPL PHYS, V86, P1

PONCE FA, 1997, NATURE, V386, P351

SAVVIDIS PG, 2000, PHYS REV B, V62, P13278

SAVVIDIS PG, 2000, PHYS REV LETT, V84, P1547

STEVENSON RM, 2000, PHYS REV LETT, V85, P3680

WEISBUCH C, 1992, PHYS REV LETT, V69, P3314

YAMAMOTO Y, 2000, NATURE, V405, P629

Editorial or Peer reviewed

REVIEWED

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Available on Infoscience
August 31, 2007
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/11422
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