Quantum Sensing with HeRALD: Analyzing Vibrational Parasitic Power Coupling in Transition Edge Sensors for Direct Detection of Dark Matter
POSTER
Abstract
Astronomical observations have consistently suggested that dark matter constitutes a substantial portion of our universe. Despite this strong evidence, detecting dark matter directly remains a formidable challenge. This difficulty arises primarily from the very weak interactions of dark matter with ordinary matter. Consequently, the quest for direct detection continues to push the boundaries of current experimental techniques.
The Helium Roton Apparatus for Light Dark Matter (HeRALD) experiment is part of the TESSERACT Collaboration ( Transition Edge Sensors with Sub-EV Resolution and Cryogenic Targets). The HeRALD experiment employs superfluid helium-4 as the target material with transition edge sensors (TES) for readout.
I will describe recent efforts to calibrate the HeRALD testbed at Lawrence Berkeley National Laboratory using photons from a calcium fluoride scintillator. This study aims to analyze different sources of noise and vibrational parasitic power coupling in our transition edge sensor channels. Through this, the optimal bandwidth for HeRALD signals is assessed, which is crucial to design the necessary filters and reduce noise for future experiments.
The Helium Roton Apparatus for Light Dark Matter (HeRALD) experiment is part of the TESSERACT Collaboration ( Transition Edge Sensors with Sub-EV Resolution and Cryogenic Targets). The HeRALD experiment employs superfluid helium-4 as the target material with transition edge sensors (TES) for readout.
I will describe recent efforts to calibrate the HeRALD testbed at Lawrence Berkeley National Laboratory using photons from a calcium fluoride scintillator. This study aims to analyze different sources of noise and vibrational parasitic power coupling in our transition edge sensor channels. Through this, the optimal bandwidth for HeRALD signals is assessed, which is crucial to design the necessary filters and reduce noise for future experiments.
*Work supported by the U.S. Department of Energy, Office of Science, Division of High Energy Physics, RENEW-Initiative, GROWTH-MSI Program #DE-SC0023725
Presenters
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Bahareh Adami Ardestani
- Sonoma State University