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| Funder | Science and Technology Facilities Council |
|---|---|
| Recipient Organization | The University of Manchester |
| Country | United Kingdom |
| Start Date | Sep 30, 2021 |
| End Date | Mar 30, 2025 |
| Duration | 1,277 days |
| Number of Grantees | 2 |
| Roles | Student; Supervisor |
| Data Source | UKRI Gateway to Research |
| Grant ID | 2659474 |
Silicon Photomultiplier (SiPM) technology has advanced in recent years with better photon detection efficiency, low power consumption, single-photon sensitivity, compactness, robustness, high precision position, and time resolution. The recent advancement has shown SIPMs as an alternative to the traditionally used photomultiplier tube in detecting scintillation light in noble gas detectors.
To fully benefit from the excellent performance of SiPM technology, it is necessary to understand and simulate the features concerned with their operation.
This project aims to characterise the performance of cutting-edge silicon photosensors produced for the DarkSide-20k direct dark matter detection experiment through study of features such as the dark count rate, cross talk, after pulsing, gain, time resolution, Sound to noise ratio (SNR), and breakdown voltage. The performance characteristics of the sensors measured in Manchester will be used to inform an updated simulation of the response of the DarkSide detector to dark matter interactions and inform data analysis optimisation and estimates of the ultimate dark matter sensitivity of the experiment when data-taking begins.
These studies will also be used to inform R&D toward the design of future quantum sensors for future experiments requiring the use of high efficiency low radioactivity large-area photosensor arrays operating with photon signals in the vacuum ultraviolet range.
The University of Manchester
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