22–26 Jan 2018
Bormio, Italy
Europe/Berlin timezone

Session

Wednesday Morning

24 Jan 2018, 09:00
Bormio, Italy

Bormio, Italy

Presentation materials

There are no materials yet.

  1. Anton Andronic (GSI Darmstadt)
    24/01/2018, 09:00
    Relativistic Heavy Ion Physics
    Overview Talk
    Deconfined matter is produced in the laboratory at highest energy densities in heavy-ion collisions at the LHC. A selection of recent results from ALICE will be presented, spanning observables from the soft sector (bulk particle production and correlations) to hard probes (charmed hadrons and jets).
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  2. Prof. Zimmer Oliver
    24/01/2018, 09:45
    Fundamental Interactions
    Overview Talk
    Ultracold neutrons (UCNs) can be confined and manipulated in traps and are an excellent probe to study fundamental symmetries and interactions. Storage lifetimes of several hundred seconds enable high-precision experiments with impact on astrophysics and cosmology, complementary to high-energy physics. Although longstanding, the search for a non-vanishing electric dipole moment of the neutron...
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  3. Prof. HIROKAZU TAMURA (Department of Physics, Tohoku University)
    24/01/2018, 11:00
    Hadron Physics
    Overview Talk
    Nuclear Physics with Strangeness
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  4. Prof. Volker Metag (II. Physikalisches Insititut)
    24/01/2018, 11:40
    Hadron Physics
    Overview Talk
    Chiral model calculations, assuming a partial restoration of chiral symmetry in a nuclear medium, predict modifications of meson properties within nuclei. An overview will be given on current experiments studying in-medium properties of mesons and the meson-nucleus interaction to extract meson-nucleus potentials. The real part of the meson nucleus potential describes whether the interaction is...
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  5. Dr Darko Veberic (Karlsruhe Institute of Technology)
    24/01/2018, 12:10
    Nuclear Structure and Astrophysics
    Overview Talk
    The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays with energies above $10^{17}$ eV and to study the interactions of these most energetic particles observed in nature. The Observatory design features an array of 1660...
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