Background rates of x-ray transition-edge sensor micro-calorimeters under a frequency domain multiplexing readout for solar axion-like particles’ detection

Journal Article (2023)
Authors

D. Vaccaro (SRON–Netherlands Institute for Space Research)

Luciano Gottardi (SRON–Netherlands Institute for Space Research)

H. Akamatsu (SRON–Netherlands Institute for Space Research)

J. van der Kuur (SRON–Netherlands Institute for Space Research)

K. Nagayoshi (SRON–Netherlands Institute for Space Research)

Emanuele Taralli (SRON–Netherlands Institute for Space Research)

M. de Wit (SRON–Netherlands Institute for Space Research)

K. Ravensberg (SRON–Netherlands Institute for Space Research)

Jian Gao (SRON–Netherlands Institute for Space Research, TU Delft - ImPhys/Adam group)

J. W. den Herder (Universiteit van Amsterdam, SRON–Netherlands Institute for Space Research)

Research Group
ImPhys/Adam group
Copyright
© 2023 D. Vaccaro, L. Gottardi, H. Akamatsu, J. van der Kuur, K. Nagayoshi, E. Taralli, M. de Wit, K. Ravensberg, J.R. Gao, J. W.A. den Herder
To reference this document use:
https://doi.org/10.1063/5.0142367
More Info
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Publication Year
2023
Language
English
Copyright
© 2023 D. Vaccaro, L. Gottardi, H. Akamatsu, J. van der Kuur, K. Nagayoshi, E. Taralli, M. de Wit, K. Ravensberg, J.R. Gao, J. W.A. den Herder
Research Group
ImPhys/Adam group
Issue number
4
Volume number
94
DOI:
https://doi.org/10.1063/5.0142367
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Abstract

We report on the x-ray background rate measured with transition-edge sensors (TES) micro-calorimeters under frequency-domain multiplexing (FDM) readout as a possible technology for future experiments aiming at a direct detection of axion-like particles. Future axion helioscopes will make use of large magnets to convert axions into photons in the keV range and x-ray detectors to observe them. To achieve this, a detector array with high spectral performance and extremely low background is necessary. TES are single-photon, non-dispersive, high-resolution micro-calorimeters and represent a possible candidate for this application. We have been developing x-ray TES micro-calorimeters and an FDM readout technology in the framework of the space-borne x-ray astronomical observatories. We show that the current generation of our detectors is already a promising technology for a possible axion search experiment, having measured an x-ray background rate of 2.2(2) × 10−4 cm−2 s−1 keV−1 with a cryogenic demonstrator not optimized for this specific application. We then make a prospect to further improve the background rate down to the required value ( < 1 0 − 7 cm−2 s−1 keV−1) for an axion-search experiment, identifying no fundamental limits to reach such a level.

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