The recent observation of a transmitted THz pulse oscillating at three times the frequency of the incident light paves the way to a powerful protocol to access resonant excitations in a superconductor. Here we show that this nonlinear optical process is dominated by light-induced excitation of Cooper pairs, while the collective amplitude (Higgs) fluctuations of the superconducting order parameter give in general a negligible contribution. We also predict a nontrivial dependence of the signal on the direction of the light polarization with respect to the lattice symmetry, which can be tested in systems such as, e.g., cuprate superconductors.

Nonlinear optical effects and third-harmonic generation in superconductors: Cooper pairs versus Higgs mode contribution / Cea, Tommaso; Castellani, Claudio; Benfatto, Lara. - In: PHYSICAL REVIEW. B. - ISSN 2469-9950. - STAMPA. - 93:18(2016), pp. 1-5. [10.1103/PhysRevB.93.180507]

Nonlinear optical effects and third-harmonic generation in superconductors: Cooper pairs versus Higgs mode contribution

CEA, TOMMASO;CASTELLANI, Claudio;BENFATTO, Lara
2016

Abstract

The recent observation of a transmitted THz pulse oscillating at three times the frequency of the incident light paves the way to a powerful protocol to access resonant excitations in a superconductor. Here we show that this nonlinear optical process is dominated by light-induced excitation of Cooper pairs, while the collective amplitude (Higgs) fluctuations of the superconducting order parameter give in general a negligible contribution. We also predict a nontrivial dependence of the signal on the direction of the light polarization with respect to the lattice symmetry, which can be tested in systems such as, e.g., cuprate superconductors.
2016
superconduttori; conduttività ottica; modi collettivi
01 Pubblicazione su rivista::01a Articolo in rivista
Nonlinear optical effects and third-harmonic generation in superconductors: Cooper pairs versus Higgs mode contribution / Cea, Tommaso; Castellani, Claudio; Benfatto, Lara. - In: PHYSICAL REVIEW. B. - ISSN 2469-9950. - STAMPA. - 93:18(2016), pp. 1-5. [10.1103/PhysRevB.93.180507]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/875269
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