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Terahertz high-sensitivity SIS mixer based on Nb–AlN–NbN hybrid superconducting tunnel junctions

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摘要 The terahertz band,a unique segment of the electromagnetic spectrum,is crucial for observing the cold,dark universe and plays a pivotal role in cutting-edge scientific research,including the study of cosmic environments that support life and imaging black holes.High-sensitivity superconductor–insulator–superconductor(SIS)mixers are essential detectors for terahertz astronomical telescopes and interferometric arrays.Compared to the commonly used classical Nb/AlO_(x)/Nb superconducting tunnel junction,the Nb/AlN/NbN hybrid superconducting tunnel junction has a higher energy gap voltage and can achieve a higher critical current density.This makes it particularly promising for the development of ultra-wideband,high-sensitivity coherent detectors or mixers in various scientific research fields.In this paper,we present a superconducting SIS mixer based on Nb/AlN/NbN parallel-connected twin junctions(PCTJ),which has a bandwidth extending up to490 GHz–720 GHz.The best achieved double-sideband(DSB)noise temperature(sensitivity)is below three times the quantum noise level.
作者 刘博梁 刘冬 姚明 金骏达 王争 李婧 史生才 Artem Chekushkin Michael Fominsky Lyudmila Filippenko Valery Koshelets Bo-Liang Liu;Dong Liu;Ming Yao;Jun-Da Jin;Zheng Wang;Jing Li;Sheng-Cai Shi;Artem Chekushkin;Michael Fominsky;Lyudmila Filippenko;Valery Koshelets(Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210023,China;School of Astronomy and Space Sciences,University of Science and Technology of China,Hefei 230026,China;Kotel'nikov Institute of Radio Engineering and Electronics,Russian Academy of Sciences,Moscow 125009,Russia)
出处 《Chinese Physics B》 SCIE EI CAS CSCD 2024年第5期681-686,共6页 中国物理B(英文版)
基金 Project supported in part by the National Key Research and Development Program of China(Grant Nos.2023YFA1608201 and 2023YFF0722301) the National Natural Science Foundation of China(Grant Nos.11925304,12020101002,12333013,12273119,and 12103093) supported by grant from the Russian Science Foundation(Grant No.23-7900019)。
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