We report the niobium titanium nitride (NbTiN) superconducting strip photon detectors (SSPDs) with strip widths ranging from 0.1 to 30 µm. The bias current dependences of the detection efficiencies at the 1550 nm wavelength and the dark count rates were systematically evaluated in the wide range of the strip widths. Single-photon detection was confirmed and a saturation trend in the bias current dependence of detection efficiency was also observed for all strip width SSPDs. In addition, we measured the physical properties of the NbTiN films and found the switching current of SSPDs gradually deviated lower from the estimated depairing current with increasing the strip width. Furthermore, the dark counts occurred at the lower bias current relative to the depairing current as the strip width increased. These results suggest that the bias current is unevenly distributed as the strip width increases and the concentrated bias current may induce the dark counts. Our results would provide valuable insights into a better understanding of SSPDs with a wide range of strip widths, the origin of dark counts, and the mechanism of photon detection in superconducting strip.
{"title":"Evaluation of NbTiN Superconducting Strip Photon Detectors With 0.1–30 µm Strip Widths","authors":"Tomohiro Haneishi;Masahiro Yabuno;Hiroki Kutsuma;Shigehito Miki;Taro Yamashita","doi":"10.1109/TASC.2024.3521901","DOIUrl":"https://doi.org/10.1109/TASC.2024.3521901","url":null,"abstract":"We report the niobium titanium nitride (NbTiN) superconducting strip photon detectors (SSPDs) with strip widths ranging from 0.1 to 30 µm. The bias current dependences of the detection efficiencies at the 1550 nm wavelength and the dark count rates were systematically evaluated in the wide range of the strip widths. Single-photon detection was confirmed and a saturation trend in the bias current dependence of detection efficiency was also observed for all strip width SSPDs. In addition, we measured the physical properties of the NbTiN films and found the switching current of SSPDs gradually deviated lower from the estimated depairing current with increasing the strip width. Furthermore, the dark counts occurred at the lower bias current relative to the depairing current as the strip width increased. These results suggest that the bias current is unevenly distributed as the strip width increases and the concentrated bias current may induce the dark counts. Our results would provide valuable insights into a better understanding of SSPDs with a wide range of strip widths, the origin of dark counts, and the mechanism of photon detection in superconducting strip.","PeriodicalId":13104,"journal":{"name":"IEEE Transactions on Applied Superconductivity","volume":"35 5","pages":"1-5"},"PeriodicalIF":1.7,"publicationDate":"2024-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142938211","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
A spacecraft re-entering the Earth's atmosphere must endure extremely high heat loads. These heat loads are created by the rapid deceleration of the spacecraft causing shock waves which in turn create a high-temperature plasma. Passive thermal protection based on ablative materials is the current solution for spacecraft heat shielding, but it is limited by material durability. As an alternative, magnetic heat shielding has shown great potential to deflect and redirect the plasma. However, fully understanding of the concept requires further experimental validation. Paihau-Robinson Research Institute has designed and built a high-temperature superconductor (HTS) system, which will be used to test the magnetic heat shielding concept at the German Aerospace Centre's (DLR) shock tunnel, where realistic flow conditions for hypersonic flight configurations are created. This paper reports the design of the HTS system with some preliminary experimental results on its performance. The shock wave stand-off distance is calculated based on the designed field (2T), which will be compared with the experimental data using a high-speed camera at DLR's shock tunnel in 2025.
{"title":"Investigation of Magnetic Heat Shielding During Spacecraft Re-Entry Using HTS Magnet – Preliminary Experimental Design","authors":"Xiyong Huang;Ben Parkinson;Nicholas Strickland;Steven Smart;Joseph Bailey;Vishnu Asokakumar Sreekala;Tulasi Parashar;Jakub Glowacki;Nicholas Long;Hubertus Weijers","doi":"10.1109/TASC.2024.3521904","DOIUrl":"https://doi.org/10.1109/TASC.2024.3521904","url":null,"abstract":"A spacecraft re-entering the Earth's atmosphere must endure extremely high heat loads. These heat loads are created by the rapid deceleration of the spacecraft causing shock waves which in turn create a high-temperature plasma. Passive thermal protection based on ablative materials is the current solution for spacecraft heat shielding, but it is limited by material durability. As an alternative, magnetic heat shielding has shown great potential to deflect and redirect the plasma. However, fully understanding of the concept requires further experimental validation. Paihau-Robinson Research Institute has designed and built a high-temperature superconductor (HTS) system, which will be used to test the magnetic heat shielding concept at the German Aerospace Centre's (DLR) shock tunnel, where realistic flow conditions for hypersonic flight configurations are created. This paper reports the design of the HTS system with some preliminary experimental results on its performance. The shock wave stand-off distance is calculated based on the designed field (2T), which will be compared with the experimental data using a high-speed camera at DLR's shock tunnel in 2025.","PeriodicalId":13104,"journal":{"name":"IEEE Transactions on Applied Superconductivity","volume":"35 5","pages":"1-6"},"PeriodicalIF":1.7,"publicationDate":"2024-12-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142938165","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-12-24DOI: 10.1109/TASC.2024.3521900
M. de Wit;L. Gottardi;K. Nagayoshi;E. Taralli;D. Vaccaro;K. Ravensberg;M.P. Bruijn;J. van der Kuur;J.R. Gao;J.W.A. den Herder
The X-ray Integral Field Unit (X-IFU) is an imaging spectrometer based on a large array of Transition Edge Sensors (TES) measured using Time Domain Multiplexing (TDM). For the development of a backup detector array, we have designed and realized a cryogenic test setup capable of measuring 9 detectors in a single cooldown under DC bias. We have used this setup to study a small selection of low aspect ratio TES designs, intended to have a low normal resistance suitable for TDM readout. In this work we show how the different designs are affected by magnetic fields. We do this by presenting the impact on the transition shape, detector integrated Noise Equivalent Power (NEP), and sensitivity of the energy scale calibration. We find, in agreement with previous studies, that reducing the width of the TES bilayer greatly improves the detector resilience to magnetic fields, potentially by several orders of magnitude.
{"title":"Transition Edge Sensors for DC Operation and Low Magnetic Field Sensitivity","authors":"M. de Wit;L. Gottardi;K. Nagayoshi;E. Taralli;D. Vaccaro;K. Ravensberg;M.P. Bruijn;J. van der Kuur;J.R. Gao;J.W.A. den Herder","doi":"10.1109/TASC.2024.3521900","DOIUrl":"https://doi.org/10.1109/TASC.2024.3521900","url":null,"abstract":"The X-ray Integral Field Unit (X-IFU) is an imaging spectrometer based on a large array of Transition Edge Sensors (TES) measured using Time Domain Multiplexing (TDM). For the development of a backup detector array, we have designed and realized a cryogenic test setup capable of measuring 9 detectors in a single cooldown under DC bias. We have used this setup to study a small selection of low aspect ratio TES designs, intended to have a low normal resistance suitable for TDM readout. In this work we show how the different designs are affected by magnetic fields. We do this by presenting the impact on the transition shape, detector integrated Noise Equivalent Power (NEP), and sensitivity of the energy scale calibration. We find, in agreement with previous studies, that reducing the width of the TES bilayer greatly improves the detector resilience to magnetic fields, potentially by several orders of magnitude.","PeriodicalId":13104,"journal":{"name":"IEEE Transactions on Applied Superconductivity","volume":"35 5","pages":"1-5"},"PeriodicalIF":1.7,"publicationDate":"2024-12-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142940752","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-12-24DOI: 10.1109/TASC.2024.3522067
Alexander J. Brooks;Jay C. LeFebvre;Joseph A. Forman;Sreekar Vattipalli;Alex Belianinov;Michael Titze;Shane A. Cybart
In this work, we study cobalt (Co) ion implantation into YBCO thin film, and correlate irradiation parameters with electrical transport measurements. 40 keV Co ions were implanted into patterned electrodes at fluences ranging from 1 × 10 13