Thursday, November 20, 2025, 16:00
WBGB/019
Michael Doser, CERN
Abstract:
While dark matter candidates range from ultra-light axions to superheavy
WIMPs, there might be another window in which to look for them: a
hypothetical Standard Model uuddss (sexaquark) state at around 2
GeV/c2 could combine many of the necessary requirements that
a dark matter candidate needs to satisfy. This talk will touch upon a
number of areas related to its possible existence, its properties and
possible formation pathway through the annihilation of antiprotons on
3He, as well as how it could be detected if it exists (and
can be formed).