16–20 Sept 2024
Europe/Rome timezone

Session

Morning 4

19 Sept 2024, 09:00

Conveners

Morning 4: Session 4

  • Mihaela Parvu (Faculty of Physics, University of Bucharest)

Presentation materials

There are no materials yet.

  1. Michael Doser (CERN)
    19/09/2024, 09:00
    Overview lecture
  2. Dr Alessio Rettaroli (Istituto Nazionale di Fisica Nucleare)
    19/09/2024, 09:45
    Talk

    In recent years, we witnessed an increasing growth in the research of light Dark Matter (DM) candidates, addressing in particular axions and axion-like particles (ALPs).
    The axion observation technique is based upon its in- verse Primakoff conversion into one photon, stimulated by a static magnetic field.

    Here, recent results of the QUAX experiment are presented.
    In particular, the...

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  3. Juan P.A. Maldonado (Max Planck Institute for Physics)
    19/09/2024, 10:05
    Talk

    MADMAX, the MAgnetized Disc and Mirror Axion eXperiment, is a novel dielectric haloscope concept to detect the axion in the mass range 40-400 ueV through enhancement of the inverse Primakoff process. In this overview talk, I will review the experiment's design concept and discuss the status of ongoing research on the critical path of the experiment, including advancements in magnet...

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  4. Samet Lezki
    19/09/2024, 10:25
    Talk

    The NA62 experiment at CERN, designed to measure the highly-suppressed decay $K^{+} \rightarrow \pi^{+}\nu\bar{\nu}$, has the capability to collect data in a beam-dump mode, where 400GeV protons are dumped on an absorber. In this configuration, New Physics (NP) particles, including dark photons, dark scalars and axion-like particles, may be produced and reach a decay volume beginning 80m...

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  5. Prof. Anastasia Fialkov (IoA, Cambridge University)
    19/09/2024, 10:45
    Talk

    Ultra-light axions is one of the most widely considered models of dark matter. In my talk, I will focus on the formation of cosmic web, first structures, stars and galaxies in a fuzzy dark matter universe. We model star and galaxy formation using a hydrodynamical code AREPO coupled to the ultra-light dark matter component solved using Schrodinger-Poisson code. We explore properties of the...

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  6. Julian Walter (Helmholtz-Institut, GSI Helmholtzzentrum für Schwerionenforschung, 55128 Mainz, Germany // Johannes Gutenberg-Universität Mainz, 55128 Mainz, Germany)
    19/09/2024, 11:30
    Talk

    Axions and other light pseudoscalar bosons with masses below $1\,\mathrm{eV}/c^2$, collectively referred to as axionlike particles (ALPs), are among the most well-motivated dark matter (DM) candidates.
    The Cosmic Axion Spin Precession Experiment (CASPEr)\,[1] aims at detecting axionlike DM with nuclear magnetic resonance techniques.
    CASPEr-Gradient in Mainz probes the coupling of nuclear...

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  7. Gabe Hoshino (University of Chicago)
    19/09/2024, 11:50
    Talk

    We present the status and recent results of the room temperature BREAD gigahertz pilot experiment (GigaBREAD) which is looking for axion-like particles in the $\sim 50 \ \mu\mathrm{eV}$ range. Reflector-based searches allow for wave-like dark matter searches at higher mass regimes where resonant cavity searches lose sensitivity due to scaling limitations. BREAD is a novel reflector concept...

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  8. Marianne Moore (MIT)
    19/09/2024, 12:10
    Talk

    The sexaquark, a hypothetical stable and neutral six-quark state, has been recently proposed as a dark matter candidate. Here, I argue it is very unlikely sexaquarks could consistently compose more than a billionth of the dark matter abundance for a wide range of scattering cross sections and annihilation rates. To draw these conclusions, I connect the sexaquark freeze-out abundance to...

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  9. Prof. Michael Tobar (Department of Physics, UWA)
    19/09/2024, 12:30
    Talk

    In this presentation I will provide an update on research at the Quantum Technologies and Dark Matter Laboratories at the University of Western Australia to develop new techniques to search for wave-like dark matter candidates and to test fundamental physics using precision low-energy metrology.

    In particular we will focus on techniques which utilize low-loss and low-noise electromagnetic...

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