4–8 Dec 2023
CERN
Europe/Zurich timezone

Session

EM-GW detectors

4 Dec 2023, 09:45
4/3-006 - TH Conference Room (CERN)

4/3-006 - TH Conference Room

CERN

110
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Conveners

EM-GW detectors

  • Andreas Ringwald

EM-GW detectors

  • Andrew Geraci

EM-GW detectors

  • Diego Blas (UAB/IFAE)

EM-GW detectors

  • Matthias Schott (CERN / University of Mainz)

EM-GW detectors

  • Asuka Ito

Presentation materials

There are no materials yet.

  1. Sebastian Ellis (Universite de Geneve (CH))
    04/12/2023, 09:45
  2. Krisztian Peters (Deutsches Elektronen-Synchrotron (DE))
    04/12/2023, 10:15

    The former MAGO collaboration, led by INFN Genoa, developed in the past SRF cavities in order to perform R&D with the aim to search for gravitational waves. In a collaborative effort, DESY/U.Hamburg and Fermilab continues this R&D programme. Since July the MAGO cavity is at DESY for measurements and matching simulations to characterise the cavity before surface treatment and cold measurements...

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  3. Bianca Giaccone (Fermi National Accelerator Laboratory)
    04/12/2023, 11:30
  4. Aldo Ejlli
    04/12/2023, 12:00
  5. Camilo Alfredo Garcia Cely (Technical University Munich)
    06/12/2023, 09:30
  6. Kaliroe Pappas (Massachusetts Institute of Technology, Laboratory For Nuclear Science)
    06/12/2023, 10:00

    ABRACADABRA-10cm has had great success as a lumped-element axion dark matter pathfinder experiment. Now, using the electrodynamics of gravitational waves and a simple change of pickup structures, we are using the ABRACADABRA detector to search for high-frequency gravitational wave in the kHz to MHz range. These higher frequencies may indicate signs of in-spiraling primordial black holes, or...

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  7. Elina Fuchs
    06/12/2023, 11:30
  8. Gianluca Gregori (University of Oxford)
    06/12/2023, 12:00
  9. Axel Lindner
    06/12/2023, 15:30

    At DESY in Hamburg, axions search experiments not relying on the dark matter paradigm are taking data (ALPS II) or have good prospects to start construction soon (BabyIAXO). Due to the similarity of axion-photon and GW-photon conversions in background magnetic fields, both experiments will also be sensitive to high frequency gravitational waves (HF-GW). The status of ALPS II and BabyIAXO as...

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  10. Georgios Vacalis
    06/12/2023, 16:00

    We propose a new method for detecting high-frequency gravitational waves (GWs) using high-energy pulsed lasers. Through the inverse Gertsenshtein effect, the interaction between a GW and the laser beam results in the creation of an electromagnetic signal. The latter can be detected using single-photon counting techniques. We present the minimal strain of a detectable GW which only depends on...

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