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© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.

Abstract

Transition-edge sensor (TES) microcalorimeters are advanced cryogenic detectors that use a superconducting film for particle or photon detection. We are establishing a new production line for TES detectors to serve as cryogenic anticoincidence (i.e., veto) devices. These detectors are made with a superconducting bilayer of titanium (Ti) and gold (Au) thin films deposited via electron beam evaporation in a high vacuum condition on a monocrystalline silicon substrate. In this work, we report on the development of such sensors, aiming to achieve stable sensing performance despite the effects of aging. For this purpose, patterned and non-patterned Ti/Au bilayer samples with varying geometries and thicknesses were fabricated using microfabrication technology. To characterize the detectors, we present and discuss initial results from repeated resistance–temperature (R–T) measurements over time, conducted on different samples, thereby augmenting existing literature data. Additionally, we present a discussion of the sensor’s degradation over time due to aging effects and test a potential remedy based on an easy annealing procedure. In our opinion, this work establishes the groundwork for our new TES detector production line.

Details

Title
Assessing the Aging Effect on Ti/Au Bilayers for Transition-Edge Sensor (TES) Detectors
Author
Gambelli, Maria 1   VIAFID ORCID Logo  ; Matteo D’Andrea 2   VIAFID ORCID Logo  ; Asquini, Rita 3   VIAFID ORCID Logo  ; Buzzin, Alessio 3   VIAFID ORCID Logo  ; Macculi, Claudio 2   VIAFID ORCID Logo  ; Torrioli, Guido 1   VIAFID ORCID Logo  ; Cibella, Sara 1   VIAFID ORCID Logo 

 Institute for Photonics and Nanotechnologies, National Research Council of Italy (CNR), Via del Fosso del Cavaliere 100, 00133 Rome, Italy; [email protected] (G.T.); [email protected] (S.C.) 
 Institute of Space Astrophysics and Planetology, Italian National Institute for Astrophysics (INAF), Via del Fosso del Cavaliere 100, 00133 Rome, Italy; [email protected] (M.D.); [email protected] (C.M.) 
 Department of Information Engineering, Electronics and Telecommunications, Via Eudossiana 18, Sapienza University of Rome, 00184 Rome, Italy; [email protected] (R.A.); [email protected] (A.B.) 
First page
3995
Publication year
2024
Publication date
2024
Publisher
MDPI AG
e-ISSN
14248220
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3072728448
Copyright
© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.