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SUPERGALAX SIGNED

Highly sensitive detection of single microwave photons with coherent quantum network of superconducting qubits for searching galactic axions

Total Cost €

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EC-Contrib. €

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Partnership

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Project "SUPERGALAX" data sheet

The following table provides information about the project.

Coordinator
CONSIGLIO NAZIONALE DELLE RICERCHE 

Organization address
address: PIAZZALE ALDO MORO 7
city: ROMA
postcode: 185
website: www.cnr.it

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 Italy [IT]
 Total cost 2˙456˙232 €
 EC max contribution 2˙456˙232 € (100%)
 Programme 1. H2020-EU.1.2.1. (FET Open)
 Code Call H2020-FETOPEN-2018-2019-2020-01
 Funding Scheme RIA
 Starting year 2020
 Duration (year-month-day) from 2020-01-01   to  2022-12-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    CONSIGLIO NAZIONALE DELLE RICERCHE IT (ROMA) coordinator 424˙348.00
2    LOUGHBOROUGH UNIVERSITY UK (LOUGHBOROUGH) participant 386˙463.00
3    ISTITUTO NAZIONALE DI RICERCA METROLOGICA IT (TORINO) participant 370˙000.00
4    LEIBNIZ-INSTITUT FUER PHOTONISCHE TECHNOLOGIEN E.V. DE (JENA) participant 363˙500.00
5    KARLSRUHER INSTITUT FUER TECHNOLOGIE DE (KARLSRUHE) participant 348˙170.00
6    RUHR-UNIVERSITAET BOCHUM DE (BOCHUM) participant 337˙500.00
7    ISTITUTO NAZIONALE DI FISICA NUCLEARE IT (FRASCATI) participant 226˙250.00

Map

 Project objective

Detection of single photons in the microwave range has a number of applications ranging from galactic dark matter axions searches to quantum computing and metrology. We propose a novel approach to acquisition of extremely low energy microwave signals (~1 GHz), based on the general concept of a passive quantum detection. For such highly sensitive detector (quantum antenna) the key novel concept we intend to use is the coherent quantum network composed of a large amount of strongly interacting superconducting qubits embedded in a low dissipative superconducting resonator. We will fabricate and explore the dynamics of coherent quantum networks based on two types of superconducting qubits: transmons and flux qubits. A spatially distributed network of superconducting qubits interacting off-resonance with the incoming radiation, shows the collective ac Stark effect that can be measured even in the limit of single photon counting. The interaction of the signal with the collective quantum states occurring in the network of superconducting qubits has the fundamental character of a quantum non-demolition measurement, whereby the quantum states of the signal and the collective states of qubits become gradually entangled. In particular, by employment of the network of large number of qubits (N) and utilization of a collective mode established in the network, we expect to exceed the standard quantum limit and reach the so-called Heisenberg limit of sensitivity which is proportional to 1/N instead of ~1/√N in case of N non directly interacting qubits. Assessment of the progress will be done by testing arrays with increasing number of superconducting qubits by using complementary experiments with different single photon sources. The feasibility of the superconducting network detector for galactic dark matter axions search will be finaly tested by axion conversion experiment in a magnetic field.

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

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