Pressure tuning of light-induced superconductivity in K3C60

被引:87
作者
Cantaluppi, A. [1 ,2 ]
Buzzi, M. [1 ]
Jotzu, G. [1 ]
Nicoletti, D. [1 ,2 ]
Mitrano, M. [1 ]
Pontiroli, D. [3 ]
Ricco, M. [3 ]
Perucchi, A. [4 ]
Di Pietro, P. [4 ]
Cavalleri, A. [1 ,2 ,5 ]
机构
[1] Max Planck Inst Struct & Dynam Matter, Hamburg, Germany
[2] Hamburg Ctr Ultrafast Imaging, Hamburg, Germany
[3] Univ Parma, Dipartimento Sci Matemat Fis & Informat, Parma, Italy
[4] INSTM UdR Trieste ST & Elettra Sincrotrone Triest, Trieste, Italy
[5] Univ Oxford, Dept Phys, Clarendon Lab, Oxford, England
基金
瑞士国家科学基金会; 欧洲研究理事会;
关键词
PHASE; DEPENDENCE;
D O I
10.1038/s41567-018-0134-8
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Optical excitation at terahertz frequencies has emerged as an effective means to dynamically manipulate complex materials. In the molecular solid K(3)C(6)0, short mid-infrared pulses transform the high-temperature metal into a non-equilibrium state with the optical properties of a superconductor. Here we tune this effect with hydrostatic pressure and find that the superconducting-like features gradually disappear at around 0.3 GPa. Reduction with pressure underscores the similarity with the equilibrium superconducting phase of K3C60, in which a larger electronic bandwidth induced by pressure is also 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 hypothesized previously, and rather extends all the way to room temperature.
引用
收藏
页码:837 / 841
页数:5
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