Opendata, web and dolomites

SPA4AstroQIT SIGNED

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

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 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.

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

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

Map

 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.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "SPA4ASTROQIT" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

The information about "SPA4ASTROQIT" are provided by the European Opendata Portal: CORDIS opendata.

More projects from the same programme (H2020-EU.1.1.)

KineTic (2020)

New Reagents for Quantifying the Routing and Kinetics of T-cell Activation

Read More  

NEUTRAMENTH (2018)

A redox-neutral process for the cost-efficient and environmentally friendly production of Menthol

Read More  

E-DURA (2018)

Commercialization of novel soft neural interfaces

Read More