18th Patras Workshop on Axions, WIMPs and WISPs

Session

Thursday Session 3

6 Jul 2023, 14:10

G-003

102. Status of the BSM and FIPs experiments in PBC

Sasha Rozanov

06/07/2023, 14:10

During last years the Physics Beyond Colliders (PBC) study at CERN explored the scientific potential of the CERN accelerator complex and infrastructure to the projects complementary to LHC and other colliders. This talk presents the status of the proposals presented in the domains of Beyond Standard Model (BSM) physics, especially the search for Feebly Interacting Particles (FIPs) and dark...

20. The ALPS II First Science Run

Aaron Spector (Deutsches Elektronen Synchrotron - DESY)

06/07/2023, 14:55

The Any Light Particle Search II (ALPS II) is a light-shining-through-a-wall (LSW) experiment located at DESY in Hamburg, Germany, that is searching for axions and axion-like particles in the mass range below 0.1 meV. LSW experiments take advantage of the potential interaction between axions and two photons by shining a laser through a region of high magnetic field. This creates an axion field...

14. New results of the DOSUE-RR experiment and future

Dr Shunsuke Adachi (Kyoto University)

06/07/2023, 15:15

Dark photon dark matter (DP-DM) is one of the dark matter candidates. The DP-DM is theoretically predicted to have a weak coupling χ to ordinary photons. This results in the emission of the conversion photon at the electromagnetic boundary such as a metal surface when the DP-DM passes through.
The DOSUE-RR (Dark-photon dark-matter Observing System for Un-Explored Radio-Range) is a series of...

19. WISPFI: WISP Searches on a Fiber Interferometer

Marios Maroudas (University of Hamburg)

06/07/2023, 15:35

WISP Searches on a Fiber Interferometer (WISPFI) is a novel tabletop experiment using interferometric techniques applied to photonic crystal fibers searching for a resonant photon-axion conversion. It is independent of the local dark matter density which can highly reduce the sensitivity of axion experiments and could as well be the reason behind the null results of dark matter searches so...