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SPA4AstroQIT SIGNED

Broadband Quantum-Limited Parametric Amplifier for Astronomy and Quantum Information Technology

Total Cost €

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EC-Contrib. €

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Partnership

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 SPA4AstroQIT project word cloud

Explore the words cloud of the SPA4AstroQIT project. It provides you a very rough idea of what is the project "SPA4AstroQIT" about.

almost    superconductor    parametric    astronomy    insulator    significantly    radio    ultra    transform    amplifiers    planar    arrays    millimetre    superconducting    circuits    conversion    array    medium    broadband    mobility    limited    construction    frequency    handling    frequencies    wave    spas    instrumentation    potentially    deployment    mixer    bandwidth    profound    front    bits    qubit    bolometric    effect    positive    readout    operate    mm    receivers    sub    architecture    power    experiments    mode    broad    telecommunications    pixel    noise    mechanism    electron    performance    circuit    gain    detector    hard    heat    receiver    cosmic    utilising    thz    amplifier    superior    transmission    passive    successful    mixing    fidelity    huge    sis    sensitivity    performances    transistor    hundreds    background    fabricate    heterodyne    microwave    compact    astronomical    count    medical    revolutionise    quantum    dissipation    hemt    nonlinear    observational    replace    converter    computing   

Project "SPA4AstroQIT" data sheet

The following table provides information about the project.

Coordinator
THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD 

Organization address
address: WELLINGTON SQUARE UNIVERSITY OFFICES
city: OXFORD
postcode: OX1 2JD
website: www.ox.ac.uk

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country United Kingdom [UK]
 Total cost 1˙991˙678 €
 EC max contribution 1˙991˙678 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-STG
 Funding Scheme ERC-STG
 Starting year 2019
 Duration (year-month-day) from 2019-02-01   to  2024-01-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD UK (OXFORD) coordinator 1˙991˙678.00

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 Project objective

The emerging technology of superconducting parametric amplifiers (SPAs) can achieve quantum-limited sensitivity over broad bandwidth, by utilising the wave-mixing mechanism in a passive 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 performances are far superior to the state-of-the-art high electron mobility transistor (HEMT) amplifier, and they can operate from radio to THz frequencies. Therefore, they could potentially revolutionise almost every kind of microwave, millimetre (mm) and sub-millimetre (sub-mm) instrumentation: from observational astronomy to quantum information experiments. Their deployment as readout amplifiers could improve the heterodyne receiver sensitivity significantly, and enable the construction of large bolometric arrays. Their large bandwidth, high power handling and quantum-noise performance could have profound effect on quantum computing architecture, improve the fidelity to process hundreds of quantum bits (qubit). They can be used as front-end high frequency amplifiers operating at THz frequencies, which is hard to achieve with HEMT technology. In this proposal, I aim to develop: 1) ultra-broadband readout amplifiers for mm/sub-mm astronomical receivers and qubit experiments, which would enable the construction of large pixel-count system; 2) front-end amplifiers at mm frequencies for heterodyne receivers and B-mode Cosmic Microwave Background experiments; and 3) parametric frequency down-converter with positive conversion gain to replace Superconductor-Insulator-Superconductor (SIS) as ultra-low noise heterodyne mixer for large array application. The successful development of these programmes not only could transform the mm/sub-mm instrumentation in the future, but could also have huge impact on many other fields such as telecommunications, medical and quantum computing technology.

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