Speaker
Enrico Maria Sessolo
(NCBJ, Warsaw)
Description
We analyze the phenomenological status of several models of BSM physics explaining the muon g-2 anomaly and the relic density of dark matter. We consider scenarios requiring extra vector-like matter, some of which are based on supersymmetry. We confront the models with the latest bounds from the LHC 14 TeV run, direct and indirect searches for dark matter, and precision tests of the electroweak theory, highlighting viable regions of the parameter space and expected signatures in future experiments.
Primary author
Enrico Maria Sessolo
(NCBJ, Warsaw)
Co-authors
Kamila Kowalska
(TU Dortmund)
Luc Darmé
(UPMC Paris 6)
Dr
Arghya Choudhury
(University of Sheffield)
Sebastian Trojanowski
(National Centre for Nuclear Research, Poland)
Leszek Roszkowski
