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.
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...
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...
