I recently had the pleasure of taking part in the 8th general meeting of the FASER Collaboration, hosted by the University of Bern. It was a wonderful week full of great science, exciting results, and plenty of ideas for the future.
The programme spanned the full breadth of the collaboration’s efforts: from neutrino cross-sections at TeV energies to forward charm production; from searches for dark photons, axion-like particles, and quirks to muon deep-inelastic scattering at the energy frontier as a probe of proton structure; and from new detector concepts to innovative reconstruction algorithms and out-of-the-box theory insights. There is no shortage of initiatives to further enrich an already blossoming programme.
While reaping the fruits of the recently completed Run 3 dataset and planning some of its legacy analyses, we also discussed at length the prospects for a thriving TeV neutrino and muon programme, alongside long-lived-particle and BSM searches, during Run 4 in the High-Luminosity LHC era, when FASER would be exposed to an unprecedented luminosity. It was clear from the discussions that, cliché but true, the best is yet to come.
It was a pleasure to attend with a strong delegation from the Nikhef Theory group and VU Physics and Astronomy: Jelle Koorn, Paulina Hernandez Sainz, Peter Krack, and Elie Hammou, and to meet in person so many of our friends and close collaborators from FASER, including Felix Kling, Jamie Boyd, Jonathan Feng, and many others, after months of interaction over Mattermost and Zoom.
Many thanks to Akitaka Ariga and his Bern colleagues for the flawless organisation. We return home fully energised and full of ideas for the next steps. The coming months will be intense but also very interesting, so stay tuned for news from FASER!











