Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap

We report the investigation of the influence of Josephson pair tunnelling on the sensitivity of an SIS mixer near the superconducting gap of niobium. Hot and cold load measurements were carried out from 600 GHz to 700 GHz, without completely supressing the Josephson effect. We have noticed that when...

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Κύριοι συγγραφείς: Tan, B, Yassin, G
Μορφή: Journal article
Έκδοση: Terahertz Science and Technology 2011
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author Tan, B
Yassin, G
author_facet Tan, B
Yassin, G
author_sort Tan, B
collection OXFORD
description We report the investigation of the influence of Josephson pair tunnelling on the sensitivity of an SIS mixer near the superconducting gap of niobium. Hot and cold load measurements were carried out from 600 GHz to 700 GHz, without completely supressing the Josephson effect. We have noticed that when measurements were made at bias points near the first Shapiro step, significantly higher values of Y-factor could be obtained with magnetic field strengths that made the Shapiro step sharper, rather then those that supressed the step. This resulted in a significant improvement in noise temperature of the mixer at those bias points. This observation is important for SIS mixers operating at frequencies near or above gap frequency (ωgap) because the warping of the second negative photon step to the positive display side, narrowing down the bias voltage interval in which measurement of the Y-factor at the first photon step could be done.
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spelling oxford-uuid:ee186fe0-4bac-41da-b4db-bc366f2972d22022-03-27T11:30:07ZJosephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gapJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:ee186fe0-4bac-41da-b4db-bc366f2972d2Symplectic Elements at OxfordTerahertz Science and Technology2011Tan, BYassin, GWe report the investigation of the influence of Josephson pair tunnelling on the sensitivity of an SIS mixer near the superconducting gap of niobium. Hot and cold load measurements were carried out from 600 GHz to 700 GHz, without completely supressing the Josephson effect. We have noticed that when measurements were made at bias points near the first Shapiro step, significantly higher values of Y-factor could be obtained with magnetic field strengths that made the Shapiro step sharper, rather then those that supressed the step. This resulted in a significant improvement in noise temperature of the mixer at those bias points. This observation is important for SIS mixers operating at frequencies near or above gap frequency (ωgap) because the warping of the second negative photon step to the positive display side, narrowing down the bias voltage interval in which measurement of the Y-factor at the first photon step could be done.
spellingShingle Tan, B
Yassin, G
Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title_full Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title_fullStr Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title_full_unstemmed Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title_short Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap
title_sort josephson pair tunnelling influence on the performance of an sis mixer near its superconducting gap
work_keys_str_mv AT tanb josephsonpairtunnellinginfluenceontheperformanceofansismixernearitssuperconductinggap
AT yassing josephsonpairtunnellinginfluenceontheperformanceofansismixernearitssuperconductinggap