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Prof. Mike Lisa (Ohio State University)25/01/2024, 09:00
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Matthias Schott (Uni. Mainz)25/01/2024, 09:45
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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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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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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
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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... -
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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