📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

DarkSide-20K Photon-detector pre-production development

Lead Research Organisation: University of Liverpool
Department Name: Physics

Abstract

This proposal is for Bridge funding for pre-production work linked to the project "Silicon Photosensor Development for the Low-Background Frontier" (ST/V001906/1). The pre-funding is for items 1 and 2 in the attached "DarkSide-UK Bridging Case For Support", which cover work to be done in preparation for: Work Strand 1- Work package 1 - Task 1.1 - sub-task Epoxy Die Bonding of the main proposal.


Summary of the full proposal:

This proposal aims to leverage the UK's world-leading silicon detector integration capability to grow UK leadership in large silicon photo-multiplier (SiPM) array detectors for low-background physics.
Low background physics experiments address some of the most fundamental open questions in science today: what is most of the matter in the universe made of? how does dark matter interact with us? why do we live in a matter-dominated universe? Experiments studying these questions at the cosmic and intensity frontiers of particle physics increasingly employ detectors filled with liquid noble gases. Liquid nobles produce scintillation light when particles interact, which is detected with arrays of photo-sensor detectors.

Silicon detectors have revolutionised particle physics at the energy frontier, and are increasingly important at the intensity and cosmic frontiers. The major challenge in dark matter and low-energy neutrino physics is to maximise signal detection efficiency whilst achieving ultra-low background interaction rates. There is a growing consensus across liquid noble dark matter and neutrino experiments that silicon photo-multiplier (SiPM) detectors are the key enabling technology to meet these challenges. The importance of developing UK leadership in this area was recognised in the recent STFC Dark Matter Strategic Review:

"The development of SiPMs for future large-scale direct-DM searches using noble gases provides the opportunity for the UK to invest in early R&D in order to achieve technological leadership in any future next generation experiment. R&D would focus on the design, production and testing of large SiPM tile arrays including electronics."

This proposal focuses on the design, production and testing of large SiPM tile arrays including electronics. The state-of-the-art in integration of large SiPM tile arrays for low-background experiments today is the DarkSide photon detector module (PDM). The PDM consists of an array of ~1 cm2 SiPMs ('tiles') bonded to a substrate to form a 25 cm2 photosensitive area, connected to cryogenic front end electronics that combine the signal from all tiles and condition it. This proposal aims to develop technological leadership for the future through:
1. R&D: on developing tiled Si array detectors for low-background experiments beyond the current state-of-the-art. We will develop new integration and readout strategies to reduce radioactivity and expand the physics reach of future experiments, potentially hosted at Boulby Underground Laboratory;
2. Knowledge Exchange: leveraging knowledge built up in the Global Argon Dark Matter Collaboration and world-leading UK facilities, we will develop production processes and expertise to manufacture and test improved, lower-background PDMs; and,
3. Capacity building: demonstrating capacity to build and test PDMs for the global next-generation liquid noble gas experiment through producing PDMs for a sub-system of DarkSide's outer detector.

To execute this ambitious programme we bring together a team of experts that have built silicon detectors for the Large Hadron Collider and space-based experiments, dark matter and neutrino physics experimentalists pushing the frontiers of ultra-low radioactivity, and theorists expanding the horizons for new physics searches based on advances in instrumentation.
 
Description The grant funded the pre-production stage preparing tooling and processes for the assembly of nearly 40,000 Silicon Photo-multiplier sensors into up to 2,400 sensor arrays in the UK for the outer detector of the Darkside-20k experiment in Gran Sasso. Darkside-20k will search for dark matter candidates with competitive sensitivity over a large range of masses.
Work funded under this pre-production grant led to a highly successful subsequent production phase in which Liverpool manufactured more than its intended share of the 2,400 module needed. Produced Silicon photomulitplier tiles have shown excellent performance. Installation of the first UK outer detector photon detection module is scheduled to start in the second half of 2025.
Exploitation Route Silicon Photo-multiplier arrays are the likely technology of choice for future large low-background experiments, with large arrays with hundreds of thousands of SiPM sensors foreseen to be deployed. Through the Darkside-20k pre-production work and subsequent production we have developed a production capacity in the UK with highly efficient assembly processes, consistent with the tight radio-purity constraints.
Sectors Aerospace

Defence and Marine

Digital/Communication/Information Technologies (including Software)

Electronics

 
Description LIVERPOOL REQUEST FOR POSTDOCTORAL RESEARCH ASSISTANTS 2022
Amount £864,004 (GBP)
Funding ID ST/X00595X/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 03/2023 
End 09/2025
 
Description Silicon Photosensor Development for the Low-Background Frontier
Amount £346,013 (GBP)
Funding ID ST/V001795/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 03/2021 
End 03/2024