A fast quench into a superconducting state can make the oscillating Higgs mode parametrically amplify reflected light and create an idler photon; optically driven K3C60 shows inferred reflectivity above 1.
Pressure tuning of light-induced superconductivity in K3C60
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abstract
Optical excitation at terahertz frequencies has emerged as an effective means to manipulate complex solids dynamically. In the molecular solid K3C60, coherent excitation of intramolecular vibrations was shown to transform the high temperature metal into a non-equilibrium state with the optical conductivity of a superconductor. Here we tune this effect with hydrostatic pressure, and we find it to disappear around 0.3 GPa. Reduction with pressure underscores the similarity with the equilibrium superconducting phase of K3C60, in which a larger electronic bandwidth is detrimental for pairing. Crucially, our observation excludes alternative interpretations based on a high-mobility metallic phase. The pressure dependence also suggests that transient, incipient superconductivity occurs far above the 150 K hypothesised previously, and rather extends all the way to room temperature.
fields
cond-mat.supr-con 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
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Higgs-mediated optical amplification in a non-equilibrium superconductor
A fast quench into a superconducting state can make the oscillating Higgs mode parametrically amplify reflected light and create an idler photon; optically driven K3C60 shows inferred reflectivity above 1.