Humboldt-Universität zu Berlin - Mathematisch-Naturwissen­schaft­liche Fakultät - Institut für Physik

Termine im Mai 2024

  • 2024-05-14T15:00:00+02:00
  • 2024-05-14T17:00:00+02:00
  • Zoom & Lise-Meitner-Haus, Christian-Gerthsen-Hörsaal, Newtonstraße 15, 12489 Berlin
Mai 14 Dienstag 2024

Zeit: 15:00

Zoom & Lise-Meitner-Haus, Christian-Gerthsen-Hörsaal, Newtonstraße 15, 12489 Berlin

Vortrag: Interactions between baryons from ab initio QCD

  • 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

  • 2024-05-21T15:00:00+02:00
  • 2024-05-21T17:00:00+02:00
  • Zoom & Lise-Meitner-Haus, Christian-Gerthsen-Hörsaal, Newtonstraße 15, 12489 Berlin
Mai 21 Dienstag 2024

Zeit: 15:00

Zoom & Lise-Meitner-Haus, Christian-Gerthsen-Hörsaal, Newtonstraße 15, 12489 Berlin

Vortrag: Photon-photon interactions in ultracold atomic media: from conditional phase to quantum vortices

  • 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.