-
Anna Obertacke (Stockholm University)24/11/2025, 11:20
The IceCube Neutrino Observatory in Antarctica is a versatile instrument in neutrino astronomy and particle physics. Over 5000 optical modules fill a volume of a cubic kilometer of ice. When a charged neutrino-secondary passes through the detector Cherenkov light is emitted that is picked up by the optical modules. Even exotic particles predicted beyond the Standard Model of particle physics...
Go to contribution page -
Axel Pontén (Uppsala University)24/11/2025, 11:40
This is the first-ever search for Long-Lived Particles (LLPs) produced by atmospheric muons at the IceCube Neutrino Observatory, a state-of-the-art neutrino telescope located 2 km below the South Pole ice. IceCube’s kilometer-scale detector, optimized for astrophysical neutrino detection, also provides an opportunity for particle physics searches for unique signatures in an unexplored energy...
Go to contribution page -
Torben Flehmke (su.se)24/11/2025, 11:55
The XENONnT experiment is the current iteration of liquid xenon detectors build and operated by the XENON collaboration. It is one of the leading experiments in providing limits on the WIMP-nucleon cross section for WIMPs heavier than 10 GeV/$c^2$. While primarily designed for the detection of more massive WIMPy dark matter, it is also sensitive to lower mass dark matter such as axions and...
Go to contribution page -
Vladimir Kiselev (Ruhr University Bochum)24/11/2025, 12:10
Active galactic nuclei (AGN) are compelling sites for high-energy neutrino production, yet the balance between light-meson ($\pi, K$) and charm-hadron channels in dense, magnetised environments remains unresolved. We present a simulation-driven framework that couples a version of CRPropa designed for the AGN / jet environment and a Hadronic Interaction Module for $pp$ interactions with...
Go to contribution page
Choose timezone
Your profile timezone: