Humboldt-Universität zu Berlin - Mathematisch-Naturwissen­schaft­liche Fakultät - Experimentelle Elementarteilchenphysik

Vergangene Termine

  • 2024-06-06T13:00:00+02:00
  • 2024-06-06T14:00:00+02:00
  • DESY, Villa | SR5, Platanenallee 6, 15738 Zeuthen
Juni 6 Donnerstag 2024

Zeit: 13:00

DESY, Villa | SR5, Platanenallee 6, 15738 Zeuthen

  • 2024-05-30T13:00:00+02:00
  • 2024-05-30T14:00:00+02:00
  • DESY, Villa | SR5, Platanenallee 6, 15738 Zeuthen
Mai 30 Donnerstag 2024

Zeit: 13:00

DESY, Villa | SR5, Platanenallee 6, 15738 Zeuthen

The cosmos manages to accelerate particles to energies that are unattainable for man-made accelerators, ultra-high energy cosmic rays. The sources in which this happens have been elusive. The arrival directions of these cosmic rays do not point back to their sources, due to their bent trajectories in (extra-)galactic magnetic fields. Their neutral counterpart, the neutrinos, do reveal the sources, however, they require massive detector volumes to be detected. This is in particular true at energies of EeV, which correspond to the highest energy cosmic rays. This talk will introduce you to the Radio Neutrino Observatory in Greenland (RNO-G), the world's largest neutrino detector, currently under construction. We will walk through science case, detection method, experimental challenges, and first data. With being a mid-scale experiment, RNO-G is also a stepping stone towards IceCube-Gen2.

  • 2024-05-16T13:00:00+02:00
  • 2024-05-16T14:00:00+02:00
  • Erwin Schrödinger-Zentrum, Rudower Chaussee 26, 12489 Berlin, Vortragsraum 0'101
Mai 16 Donnerstag 2024

Zeit: 13:00

Erwin Schrödinger-Zentrum, Rudower Chaussee 26, 12489 Berlin, Vortragsraum 0'101

  • 2024-04-25T13:00:00+02:00
  • 2024-04-25T14:00:00+02:00
April 25 Donnerstag 2024

Zeit: 13:00

  • 2024-04-18T13:00:00+02:00
  • 2024-04-18T14:00:00+02:00
  • Erwin Schrödinger-Zentrum, Rudower Chaussee 26, 12489 Berlin, Vortragsraum 0'101
April 18 Donnerstag 2024

Zeit: 13:00

Erwin Schrödinger-Zentrum, Rudower Chaussee 26, 12489 Berlin, Vortragsraum 0'101

Abstract: The European Strategy for Particle Physics identified an high-energy e+e- collider studying the Higgs boson as the next priority collider project. The different proposals to realize such a collider all reach a similar performance on the core Higgs program at 250 GeV, albeit with different choices of luminosity and polarisation - but they differ in capabilities at lower and higher energies. This talk will review the physics capabilities of future e+e- linear colliders in the Higgs sector and beyond, with a specific emphasis illuminating the interplay of the top-level beam parameters luminosity, energy and polarisation.