TY - JOUR
T1 - Simulations for direct dark matter searches using ALPS II's TES detection system
AU - Schwemmbauer, Christina
AU - Hochberg, Yonit
AU - Isleif, Katharina Sophie
AU - Januschek, Friederike
AU - Lehmann, Benjamin V.
AU - Lindner, Axel
AU - Meyer, Manuel
AU - Othman, Gulden
AU - Gimeno, José Alejandro Rubiera
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2024/4/17
Y1 - 2024/4/17
N2 - Transition Edge Sensors (TES) are superconducting microcalorimeters that can be used for singlephoton detection with extremely low backgrounds. When they are within their superconducting transition region, small temperature fluctuations-like the energy deposited by single photons- lead to large resistance variations. These variations can be measured using Superconducting Quantum Interference Devices (SQUIDs). This technology is planned to be used as a singlephoton detector for later runs of the ALPS II experiment, a light-shining-through-walls experiment at DESY Hamburg, searching for Axion-Like Particles (ALPs), which are possible Dark Matter (DM) candidates. Due to the very low dark count rates in our setup, our TES system might be viable for direct DM searches at sub-MeV masses through electron-scattering of DM in the superconducting chip, as well. Simulations concerning background rejection and calibration methods demonstrate the needed sub-eV sensitivity already.
AB - Transition Edge Sensors (TES) are superconducting microcalorimeters that can be used for singlephoton detection with extremely low backgrounds. When they are within their superconducting transition region, small temperature fluctuations-like the energy deposited by single photons- lead to large resistance variations. These variations can be measured using Superconducting Quantum Interference Devices (SQUIDs). This technology is planned to be used as a singlephoton detector for later runs of the ALPS II experiment, a light-shining-through-walls experiment at DESY Hamburg, searching for Axion-Like Particles (ALPs), which are possible Dark Matter (DM) candidates. Due to the very low dark count rates in our setup, our TES system might be viable for direct DM searches at sub-MeV masses through electron-scattering of DM in the superconducting chip, as well. Simulations concerning background rejection and calibration methods demonstrate the needed sub-eV sensitivity already.
UR - http://www.scopus.com/inward/record.url?scp=85190940842&partnerID=8YFLogxK
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AN - SCOPUS:85190940842
SN - 1824-8039
VL - 454
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 055
T2 - 1st General Meeting and 1st Training School of the COST Action COSMIC WISPers, COSMICWISPers 2023
Y2 - 5 September 2023 through 14 September 2023
ER -