X-ray pulse-shape analysis on bridge-type microcalorimeters with Ti-Au transition-edge sensors

Masahiro Ukibe*, Keiichi Tanaka, Fuminori Hirayama, Taku Mizuki, Tomotaka Hikosaka, Toshimitsu Morooka, Kazuo Chinone, Ushio Kawabe, Toshio Nemoto, Masao Koyanagi, Masataka Ohkubo, Naoto Kobayashi

*この研究の対応する著者

研究成果: Conference contribution

1 被引用数 (Scopus)

抄録

We have fabricated a bridge-type structure for microcalorimeters with superconducting transition-edge sensors (TES). Instead of open space under a SiN x membrane in conventional TES microcalorimeters, the bridge-type calorimeters have a SiNx membrane floating on the Si substrate covered by a SiO 2 layer with a small gap of 30-50 μm. The bridge-type structure ensures that the calorimeters are mechanically tough. In addition, the thermal conductance can easily be controlled by changing the width, length, or thickness of the SiNx bridge. The calorimeters, of which operating temperature is 0.43 K, consist of a Ti/Au bilayer TES and an Au absorber. The x-ray events were read out by a DC-SQUID current amplifier with a 200-series array of SQUIDs placed on a 4.2 K stage. By analyzing the output pulse shapes, it has been found that the pulses are put into two categories. One has a fast rise time of approximately 3 μs and two decay components with time constants of approximately 10 μs and about approximately 130 μs. Another one has a longer rise time of approximately 10 μs and a single decay component of approximately 130 μs. It is considered that the pulse shapes depend on the x-ray absorption positions and the heat-flow pass.

本文言語English
ホスト出版物のタイトルProceedings of SPIE - The International Society for Optical Engineering
ページ376-383
ページ数8
4140
DOI
出版ステータスPublished - 2000
外部発表はい
イベントX-Ray and Gamma-Ray Instrumentation for Astronomy XI - San Diego, CA,USA
継続期間: 2000 8月 22000 8月 4

Other

OtherX-Ray and Gamma-Ray Instrumentation for Astronomy XI
CitySan Diego, CA,USA
Period00/8/200/8/4

ASJC Scopus subject areas

  • 電子工学および電気工学
  • 凝縮系物理学

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