Self-heating, phase coherence, and sidewall angle in 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 are therefore a promising source of coherent, continuous-wave radiation in the 'terahertz gap' range.
To optimize the THz emission power and linewidth performance of these devices, it is essential to create a phase-coherent state among the stacked IJJs. This in turn requires minimizing the spread in their drive voltages, which is far from trivial when the IJJs are current-biased and shunted in series. This is further complicated by self-heating in the mesa, due to the poor c-axis thermal conductivity of Bi2Sr2CaCu2O8 .
The drive voltage spread can be minimized by the correct choice of mesa sidewall angle. Here we calculate the optimal sidewall angle as a function of device geometry, doping state, emission frequency, and intended operating temperature. We find that the optimal sidewall angle varies dramatically depending on the above parameters, and we discuss its implications for THz mesa source engineering.
To optimize the THz emission power and linewidth performance of these devices, it is essential to create a phase-coherent state among the stacked IJJs. This in turn requires minimizing the spread in their drive voltages, which is far from trivial when the IJJs are current-biased and shunted in series. This is further complicated by self-heating in the mesa, due to the poor c-axis thermal conductivity of Bi2Sr2CaCu2O8 .
The drive voltage spread can be minimized by the correct choice of mesa sidewall angle. Here we calculate the optimal sidewall angle as a function of device geometry, doping state, emission frequency, and intended operating temperature. We find that the optimal sidewall angle varies dramatically depending on the above parameters, and we discuss its implications for THz mesa source engineering.
*This research is supported by PSC-CUNY Award 60792-00-48; and by the US Department of Energy, Office of Basic Energy Sciences, under Contract No. DEAC02-06CH11357.
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Presenters
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Karen Kihlstrom
- Physics, CUNY Queens College