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Superconducting Parametric Amplifier Receiver Technology for Astronomy and Fundamental Physics Experiments

Project description

Superconducting amplifiers for ultra-sensitive instrumentation in scientific research

Superconducting parametric amplifiers are cutting-edge devices that boost the detection of extremely weak signals. Compact, energy-efficient with negligible heat dissipation, they offer ultra-low noise quantum-limited performance, limited only by nature, across a wide frequency range. The ERC-funded SPARTAN-FX project aims to enhance and extend the functionality of these amplifiers for use in astronomy and physics, including the search for dark matter and high-fidelity readout of quantum computational platforms. Researchers will develop improved versions to replace current technologies in large telescopes and ultra-sensitive experiments while also exploring new materials to enable operation at higher temperatures and frequencies. These advancements could also benefit fields like quantum communication and remote sensing.

Objective

The emerging technology of superconducting parametric amplifiers (SPAs) can achieve quantum-limited sensitivity over a broad bandwidth by utilizing the wave-mixing mechanism in a nonlinear transmission medium. They are compact, easy to fabricate with planar circuit technology, have ultra-low heat dissipation, and can be integrated directly with other detector circuits. Their performance surpasses that of the state-of-the-art high electron mobility transistor (HEMT) amplifiers, and they can operate from radio to THz frequencies. Therefore, they have the potential to revolutionize almost every kind of microwave, millimetre (mm), and sub-mm instrumentation, from observational astronomy to fundamental physics experiments such as dark matter searches, quantum information platforms, and neutrino mass determination.

In this proposal, I will:
1. Develop practical ultra-broadband quantum amplifiers for deployment to mm/sub-mm/THz astronomical receivers and fundamental physics experiments.
2. Develop novel ultra-compact parametric frequency converters to replace traditional superconductor-insulator-superconductor (SIS) mixers and Schottky local oscillator (LO) technologies, enabling the construction of large pixel-count systems for mm-wave heterodyne receivers such as the Atacama Large Millimetre/sub-mm Array (ALMA) and Event Horizon Telescopes (EHT).
3. Explore high critical temperature superconductors to extend the operation of these parametric devices into higher bath temperatures and frequencies in the supra-THz regime, potentially replacing hot electron bolometer (HEB) mixers and quantum cascade lasers (QCLs).

The successful delivery of these outcomes marks a paradigm shift in mm/sub-mm/THz instrumentation, replacing all the core technologies used in this regime with a single integratable SPA technology. This will also have a significant impact on many other fields such as telecommunications, medical applications, and remote sensing, among others.

Fields of science (EuroSciVoc)

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Programme(s)

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Topic(s)

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Funding Scheme

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HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

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(opens in new window) ERC-2024-COG

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Host institution

THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 2 999 974,00
Address
WELLINGTON SQUARE UNIVERSITY OFFICES
OX1 2JD Oxford
United Kingdom

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Region
South East (England) Berkshire, Buckinghamshire and Oxfordshire Oxfordshire
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 2 999 974,00

Beneficiaries (1)

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