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Giant Enhancement of the Optical Second-Harmonic Emission ofWSe2Monolayers by Laser Excitation at Exciton Resonances

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Wang, G., Marie, X., Gerber, I., Amand, T., Lagarde, D., Bouet, L., Vidal, M., Balocchi, A., Urbaszek, B.·2015·Physical Review Letters

Abstract

We show that the light-matter interaction in monolayer WSe_{2} is strongly enhanced when the incoming electromagnetic wave is in resonance with the energy of the exciton states of strongly Coulomb bound electron-hole pairs below the electronic band gap. We perform second harmonic generation (SHG) spectroscopy as a function of laser energy and polarization at T=4 K. At the exciton resonance energies we record an enhancement by up to 3 orders of magnitude of the SHG efficiency, due to the unusual combination of electric dipole and magnetic dipole transitions. The energy and parity of the exciton states showing the strong resonance effects are identified in 1- and 2-photon photoluminescence excitation experiments, corroborated by first principles calculations. Targeting the identified exciton states in resonant 2-photon excitation allows us to maximize k-valley coherence and polarization.

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Metadata

Authors
Wang, G., Marie, X., Gerber, I., Amand, T., Lagarde, D., Bouet, L., Vidal, M., Balocchi, A., & Urbaszek, B.
Venue
Physical Review Letters
Published
2015-03-04
Volume
114
Issue
9
Pages
097403-097403
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W1489642512
Cited by
640
References
61
FWCI
28.91
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Giant Enhancement of the Optical Second-Harmonic Emission ofWSe2Monolayers by Laser Excitation at Exciton Resonances. https://app.cochat.ai/papers/10.1103/physrevlett.114.097403
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Wang, G., Marie, X., Gerber, I., Amand, T., Lagarde, D., Bouet, L., Vidal, M., Balocchi, A., & Urbaszek, B. (2015). Giant Enhancement of the Optical Second-Harmonic Emission ofWSe2Monolayers by Laser Excitation at Exciton Resonances. Physical Review Letters. https://doi.org/10.1103/physrevlett.114.097403

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