collaborators

6 papers

quant-ph2026

Three wave mixing vacuum squeezing generation in a SNAIL-based Traveling-Wave Parametric Amplifier with alternated flux polarity

Isita Chatterjee, Pegah Darvehi, Antonio Orsi +9

Recent demonstrations of squeezing generation using Traveling Wave Parametric Amplifiers (TWPAs) have opened the way for the application of broadband microwave squeezing in quantum…

astro-ph.HE2026

Searches for Binary Mergers with Sub-solar Mass Components in Data from the First Part of LIGO--Virgo--KAGRA's Fourth Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1834

We report on a gravitational wave search for compact binary coalescences involving at least one component with mass between to , and ratio of component m…

quant-ph2025

Quantitative calibration of a TWPA applied to an optomechanical platform

Alexandre Delattre, Ilya Golokolenov, Richard Pedurand +11

In the last decade, the microwave quantum electronics toolbox has been enriched with quantum-limited detection devices such as Traveling Wave Parametric Amplifiers (TWPAs). The ext…

quant-ph2025

Suppression of measurement-induced state transitions in cosϕ-coupling transmon readout

Cyril Mori, Francesca D Esposito, Alexandru Petrescu +12

Drive-induced unwanted state transitions (DUST) are limiting both for microwave readout and parametric operations of superconducting qubits. Among them, measurement-induced state t…

quant-ph2025

High-power readout of a transmon qubit using a nonlinear coupling

Cyril Mori, Vladimir Milchakov, Francesca D'Esposito +13

The field of superconducting qubits is constantly evolving with new circuit designs. However, when it comes to qubit readout, the use of simple transverse linear coupling remains o…

hep-ex2025

Search for post-inflationary QCD axions with a quantum-limited tunable microwave receiver

Giosuè Sardo Infirri, David Alesini, Caterina Braggio +22

A search for cosmological axions has been performed by scanning a frequency region of MHz centered at about GHz, corresponding to an axion mass eV.…