THz emission peak at low voltage bias from stacked intrinsic Josephson junction Bi<sub>2</sub>Sr<sub>2</sub>CaCu<sub>2</sub>O<sub>8</sub> terahertz sources
ORAL
Abstract
The extremely anisotropic high-temperature superconductor Bi2Sr2CaCu2O8 contains stacked 'intrinsic' Josephson junctions with a large superconducting gap energy. Mesa-shaped devices constructed from this material therefore show promise as a source of coherent, continuous-wave radiation in the 'terahertz gap' range.
THz emission from these devices has previously been typically observed at frequencies between around 0.4 THz – 2 THz, corresponding to Josephson voltages of between 0.8 mV and 4 mV per intrinsic junction. However, we have recently observed a new type of emission which occurs at bias currents below the retrapping current of the stacked Josephson junctions. This unusual THz emission state is highly reproducible, is metastable over a timescale of hours, and shows systematic temperature dependence. The maximum emitted THz power that can be generated from this mode is comparable to that generated by the more well-established and better-understood THz emission modes in Bi2Sr2CaCu2O8 mesa sources.
We will discuss possible mechanisms for the unusual emission mode, together with future directions of related research.
THz emission from these devices has previously been typically observed at frequencies between around 0.4 THz – 2 THz, corresponding to Josephson voltages of between 0.8 mV and 4 mV per intrinsic junction. However, we have recently observed a new type of emission which occurs at bias currents below the retrapping current of the stacked Josephson junctions. This unusual THz emission state is highly reproducible, is metastable over a timescale of hours, and shows systematic temperature dependence. The maximum emitted THz power that can be generated from this mode is comparable to that generated by the more well-established and better-understood THz emission modes in Bi2Sr2CaCu2O8 mesa sources.
We will discuss possible mechanisms for the unusual emission mode, together with future directions of related research.
*This research is supported by PSC-CUNY Award 60792-00-48; and by the US Department of Energy, Office of Sciences, Materials Sciences and Engineering Division.
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Presenters
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Karen J Kihlstrom
- Physics, Queens College CUNY