23–27 Jan 2023
Bormio, Italy
Europe/Berlin timezone

Session

Tuesday Morning

24 Jan 2023, 09:00
Bormio, Italy

Bormio, Italy

Presentation materials

There are no materials yet.

  1. Stefano Di Falco (INFN Pisa)
    24/01/2023, 09:00
    Overview Talk

    The muon anomalous magnetic moment, 𝑎𝜇=(𝑔−2)/2, provides one of the most precise tests of the Standard Model allowing to discover signs of the presence of new particles and forces in the subatomic quantum fluctuations surrounding the muon.
    A previous experiment performed two decades ago at Brookhaven National Laboratory (BNL) has shown an intriguing discrepancy between the theoretical...

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  2. Dr Wolfgang Trautmann (GSI)
    24/01/2023, 09:45
    Overview Talk
  3. Dr Akira Ohnishi (Yukawa Institute, Kyoto University)
    24/01/2023, 10:50
    Overview Talk

    I discuss femtoscopic studies of hadron-hadron interactions mainly from a theoretical point of view. Femtoscopy denotes studies using two-(or more- )particle momentum correlation functions, which are given by the convolution of the source function and the relative
    wave function squared. Thus when the source function is known, one can obtain information on the wave function including the...

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  4. David Hornidge (Mount Allison University)
    24/01/2023, 11:25
    Extended Contribution

    The Electron−Ion Collider is a major new facility scheduled to be built at Brookhaven National Laboratory on Long Island, NY, by the US Department of Energy. Polarized electrons will collide with polarized protons, light ions, and heavy nuclei at luminosities far beyond what is presently available, with the goal of answering fundamental questions central to nuclear physics today. Canadian...

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  5. Stephan Koenigstorfer (Technical University Munich)
    24/01/2023, 12:00
    Short Contribution

    Antinuclei in cosmic rays are considered a unique probe for signals from exotic physics, such as WIMP Dark Matter annihilations. Indeed, these channels are characterised by a very low astrophysical background, which comes from antinuclei produced by high energy cosmic ray interaction with ordinary matter.
    In order to make quantitative predictions for antinuclei fluxes near earth, both the...

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