22–26 Jan 2024
Europe/Berlin timezone

Session

Thursday Morning Session

25 Jan 2024, 09:00
Bormio, Italy

Bormio, Italy

Presentation materials

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  1. Prof. Mike Lisa (Ohio State University)
    25/01/2024, 09:00
  2. Matthias Schott (Uni. Mainz)
    25/01/2024, 09:45
  3. Prof. Kate Scholberg (Duke University, Durham)
    25/01/2024, 10:50

    This talk will be an overview of the physics of coherent elastic neutrino-nucleus scattering (CEvNS) and the current status and prospects of CEvNS experiments.

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  4. Prof. Wolfram Weise (Technical University of Munich)
    25/01/2024, 11:25

    The heaviest neutron stars progressively tighten the constraints on the equation-of-state of strongly interacting, dense baryonic matter. Using the observational data base, results are presented of a detailed Bayes inference program, with focus on prerequisites and limitations for hypothetical phase transitions at the baryon densities realized in neutron star cores. Consequences for the...

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  5. Prof. Michael Block (GSI / HIM / JGU)
    25/01/2024, 12:00

    Exploring the limits of nuclear existence is one of the forefront topics in nuclear physics. One
    limit is concerned with the heaviest nucleus that may exist. Theoretical models have predicted
    that superheavy nuclei with Z ? 120 exist and feature a region of long-lived superheavy nuclides
    around N = 184, the so-called the island of stability. Since the first predictions new elements
    up to Z...

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  6. Dr Edda Gschwendtner (CERN)

    The construction of ever larger accelerator facilities has its limits, and new technologies will be needed to push the energy frontier. Plasma wakefield acceleration is a rapidly developing field which appears to be an auspicious candidate technology for future high-energy accelerators; acceleration gradients up to 1000 times superior to those achieved with radiofrequency cavities have been...

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