Photon Detector Development for the Vacuum Ultraviolet Frontier

STFC · United Kingdom government procurement

GlobalGov surfaces government procurement from around the world, including the markets your competitors overlook.

March 30, 2029
Response Due
Active
Status

Opportunity Overview

How is the universe evolving and what roles do dark matter and dark energy play? What is the nature of dark matter and dark energy? What are the fundamental particles and fields? Why is there more matter than antimatter? What is the nature of neutrinos?
To answer these fundamental physics questions, the next generation flagship experiments in neutrino and dark matter will employ noble elements (argon and xenon) as active targets for particle detection. These internationally-leading experiments will rely on detection of light emitted in the vacuum ultraviolet (VUV) wavelength range. Argon and xenon scintillate in the 120-140 nm range and 165-185 range, respectively. This is a problematic region for light detection, where current photodetection technologies perform poorly. Indeed, efficient detection of light down to a single photon using optoelectronic devices is a key theme in the UK’s Quantum Strategy, and extending the detectable spectral range is an established goal of quantum imaging research. We target this extension to VUV, where the decreasing wavelength poses challenges for detection due to the rapid increase of the reflectivity. The state of the art in large-area silicon sensor array technology is Silicon Photomultipliers (SiPMs) with unsatisfactory performances of photon detection efficiency between 15% (Hamamatsu, at 178 nm) and 22% (FBK Low Field UV optimized), dropping to 10% for 128 nm.
With this project, we aim at boosting the quantum efficiency and collected number of photons for VUV sensitive photon sensors via a strategy that combines smart sensor designs, the use of 2D materials, and the application of novel readouts. This will unlock the potential of a wide range of tonne- and kilotonne-scale neutrino and dark matter experiments such as DUNE, NEXT, DarkSide, LZ and nEXO. These experiments will need to instrument large readout areas (10–100 m2) both at room temperature (DUNE near detector and NEXT experiments) and in cryogenic conditions (DUNE...

This is one of 1,833 active United Kingdom Research Development opportunities most of your competitors will never see.

Your competitors are watching the same crowded contracts everyone else is. Track this opportunity and every one like it worldwide, set deadline alerts, and win where they aren’t. Free for 14 days, no card.

Start Free

Solicitation Details

Issuing agencySTFC
CountryUnited Kingdom
CategoryResearch Development
PublishedMarch 30, 2026
Procurement stageActive solicitation
Response dueMarch 30, 2029
StatusOpen — accepting responses
Official sourceView original notice
Last verifiedAugust 09, 2026

Source: UK Research and Innovation (UKRI) — Open Government Licence v3.0.

Related Opportunities in United Kingdom

EMCCD detector development for space applications: from the Nancy Grace Roman Space Telescope to future mission opportunities
BUTTON-30
GridPP7 QMUL Staff Grant
Neutron Detector Development Using Novel 3He
Imperial College Astrophysics PATT Linked Grant: 2025
Origin and structure of the interplanetary magnetic field
Runaway stars from young star clusters as probes of cluster formation
Neutrino oscillation at T2K and Hyper Kamiokande and development of the Hyper Kamiokande light injection calibration system

See every United Kingdom Research Development opportunity your competition is missing. Free for 14 days.

Get real-time alerts, competitive intelligence, and deadline tracking for this and every market worldwide.

Start Free Trial — No Card Required

Free 14-day trial · no card required

See who is already competing here →

Get a free United Kingdom Research Development intelligence report in your inbox

A personalized report on United Kingdom Research Development opportunities, emailed in 5-10 minutes. One per month, no account needed.