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Bormio Conference

22–26 Jan 2024
Europe/Berlin timezone

Bormio Organizers

Session

Wednesday Morning Session

24 Jan 2024, 09:00
Bormio, Italy

Bormio, Italy

Presentation materials

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  1. 56. Recent Developments in Ab Initio Nuclear Many-Body Calculations
    Prof. Heiko Hergert (FRIB, Michigan State University)
    24/01/2024, 09:00

    The capabilities of ab initio many-body calculations for nuclear structure and reactions have expanded dramatically within recent years. We have seen first converged calculations for nuclei as heavy as Pb208, a first attempt at a mass table up to the iron region, as well as studies of fusion and reactions of light nuclei that are of astrophysical importance. Efforts are now focusing on nuclei...

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  2. 44. Recent highlights from experiments with muons and neutrons at PSI
    Prof. Klaus Kirch (PSI & ETHZ)
    24/01/2024, 09:45

    The high intensity proton accelerator facility at the Paul Scherrer Institute (PSI) in Switzerland provides high intensities of pions, muons and ultracold neutrons for fundamental atomic, nuclear and particle physics measurements. Aspects of the facility will be shown and some of the latest experimental results will be presented.

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  3. 85. Testing Fundamental Symmetries by High Precision Comparisons of Matter / Antimatter Conjugates at CERN
    Prof. Stefan Ulmer (HHU Düsseldorf)
    24/01/2024, 11:00

    The Standard Model of particle physics is incredibly successful and glaringly incomplete. Among the questions left open is the striking imbalance of matter and antimatter in our universe, which inspires experiments to compare the fundamental properties of matter/antimatter conjugates with high precision. The BASE collaboration at the antiproton decelerator of CERN is performing such...

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  4. 9. Core-collapse supernovae and neutron star mergers
    Prof. Almudena Arcones (TU Darmstadt & GSI)
    24/01/2024, 11:35

    In 2017, a multimessenger era started with the first gravitational wave detection from the merger of two neutron stars (GW170817) and the rich electromagnetic follow-up. The most exciting electromagnetic counterpart was the kilonova. This provides an answer to the long-standing question of how and where heavy elements are produced in the universe. The neutron-rich material ejected during the...

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  5. 41. Axion Searches
    Dr Babette Döbrich (Max Planck Institute for Physics)
    24/01/2024, 12:10
  6. 69. Open and hidden heavy flavor as probes of deconfinement
    Prof. Johanna Stachel (University of Heidelberg)

    The experimental data on heavy flavor production in nuclear collisions at the LHC will be discussed in terms of their connection to deconfinement in the high energy density medium above the chiral phase transition

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