17–19 Mar 2025
Europe/Rome timezone

Session

Quantum sensors and technologies

17 Mar 2025, 16:30

Conveners

Quantum sensors and technologies

  • Jean-Pierre Zendri (INFN)
  • Federica Mantegazzini (FBK / INFN-TIFPA)

Presentation materials

There are no materials yet.

  1. Federica Mantegazzini (FBK / INFN-TIFPA)
    17/03/2025, 16:30
    Review talk
  2. Marcello Filippo Faggionato (Istituto Nazionale di Fisica Nucleare)
    17/03/2025, 16:40
    "Rapid fire" talk

    Superconducting circuits have proven to be one of the most promising platforms for quantum computing and sensing applications with Josephson junctions as one of their fundamental building blocks. Therefore, a reliable fabrication process and characterization apparatus of these components is of crucial importance for every experimental group in this field.

    Traditional characterization of...

    Go to contribution page
  3. Danilo Labranca
    17/03/2025, 16:45
    Quantum sensors and technologies
    "Rapid fire" talk

    Superconducting transmon qubits have emerged as powerful tools for precision sensing
    applications [1, 2], particularly in the search for light dark matter candidates such as axions
    and hidden photons [3–9]. These weakly interacting particles may leave detectable signatures
    through their coupling to electromagnetic fields, making highly sensitive quantum devices
    essential for their...

    Go to contribution page
  4. Caterina Braggio
    17/03/2025, 16:52
    Quantum sensors and technologies
    "Rapid fire" talk

    Devices and methods of quantum information science can bring significant upgrades to current and future particle physics detectors. In particular, I will discuss experiments testing the hypothesis that dark matter is composed of very light particles, detectable as an effective field with a specific frequency set by their mass. As the signal to noise ratio is very poor in these experiments, new...

    Go to contribution page
  5. Dr Federico Paolucci (Istituto Nazionale di Fisica Nucleare)
    17/03/2025, 17:02
    Quantum sensors and technologies
    "Rapid fire" talk

    The challenges of modern fundamental physics lie in low energy phenomena, such as gravitational waves, cosmological inflation and dark matter. Indeed, different phenomena in astronomy (such as radio burst sources, cosmic microwave background, and GHz-peaked radio sources) need the development of sensitive bolometers operating in the GHz-THz bands. Furthermore, low energy particle physics...

    Go to contribution page
  6. Enrico Bogoni (Istituto Nazionale di Fisica Nucleare)
    17/03/2025, 17:12
    "Rapid fire" talk

    Recent particle physics experiments requiring excellent energy resolution involve cryogenic detector arrays composed of hundreds of detector pixels, such as Transition Edge Sensors (TESs). To preserve the intrinsically excellent energy resolution of these detector arrays while maintaining minimal system complexity, a broadband, multiplexed read-out chain, with minimal noise addition is...

    Go to contribution page
  7. Mr Leonardo Limongi (TIFPA)
    17/03/2025, 17:19
    Quantum sensors and technologies
    "Rapid fire" talk

    We present the design of a hybrid photon number-resolving detector (PNRD) on a lithium niobate-on-insulator (LNOI) platform, aiming to combine superconducting nanowire single-photon detectors (SNSPDs) in a multiplexed configuration for high-fidelity quantum sensing. Finite element method (FEM) simulations have been conducted to assess key performance factors such as propagation losses,...

    Go to contribution page
  8. Mario De Lucia (Istituto Nazionale di Fisica Nucleare)
    17/03/2025, 17:24
    Quantum sensors and technologies
    "Rapid fire" talk

    Superconducting detectors are currently being developed, optimised and deployed for all forms of physics experiments due to their incredible performance that combines moderate-to-elevate energy resolution, time and spatial resolution with high quantum efficiency and effectively near-zero dark counts. At the Pisa section we are moving the first steps in detector design and fabrication, with the...

    Go to contribution page
  9. Jean-Pierre Zendri (INFN)
    17/03/2025, 17:35
    Review talk
  10. Francesco De Marco (Sapienza University of Rome & Istituto Nazionale di Fisica Nucleare, Sezione di Roma1)
    17/03/2025, 17:45
    Quantum sensors and technologies
    "Rapid fire" talk

    In the last years, gravitational-wave (GW) Earth-based detectors have seen a great improvement in sensitivity, leading to the detection of more than 100 events during the joint observing runs of the LIGO-Virgo-KAGRA (LVK) Collaboration. This has opened the way to a completely new field of study, i.e. multimessenger astrophysics.
    The contribution presented here is about taming quantum noise to...

    Go to contribution page
  11. Andrea Grimaldi
    17/03/2025, 17:52
    Quantum sensors and technologies
    "Rapid fire" talk

    Quantum noise is a fundamental limitation in gravitational wave detectors, restricting their sensitivity and scientific reach. To overcome this challenge, current detectors rely on frequency-dependent squeezing, implemented using long filter cavities to reduce quantum noise across a broad frequency range. While effective, this approach is difficult to scale, particularly for next-generation...

    Go to contribution page
  12. Wajid Ali (University of Genova, Italy)
    17/03/2025, 17:59
    Quantum sensors and technologies
    "Rapid fire" talk

    Abstract for IFD 2025 - INFN Workshop on Future Detectors, on March 17-19, 2025

                                                 (https://agenda.infn.it/event/43956/abstracts/#submit-abstract)
    

    Title: Entangled Squeezed Light for Quantum Noise Reduction in Small-Scale suspended Interferometers

    Presentation type: SIPS

    Authors: W. Ali¹ ² (On behalf of the EPR-SIPS team) ...

    Go to contribution page
  13. Barbara Garaventa (Istituto Nazionale di Fisica Nucleare)
    Quantum sensors and technologies
    "Rapid fire" talk

    The sensitivity of future Gravitational Wave (GW) detectors, such as the Einstein Telescope (ET), will be significantly limited by various noise sources, particularly magnetic noise, especially at low frequencies (from a few Hz to around 100 Hz). Magnetic noise arises from the interaction between environmental magnetic fields and magnetized elements, such as magnet-coil actuators. These...

    Go to contribution page
Building timetable...