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.

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

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.)

HyperBio (2019)

Vis-NIR Hyperspectral imaging for biomaterial quality control

Read More  

CHIPTRANSFORM (2018)

On-chip optical communication with transformation optics

Read More  

BALANCE (2019)

Mapping Dispersion Spectroscopically in Large Gas-Phase Molecular Ions

Read More