Speaker:
Roland Allen (Texas A&M University)
Location:
Address:
Mitchell Institute for Fundamental Physics & Astronomy
College Station, Texas 77843
We propose a dark matter scenario which is ideal in the sense that (1) all of the well-known successes of supersymmetry are preserved, (2) the parameters can satisfy naturalness, (3) the addition of an extended Higgs sector implies a doubly rich plethora of new particles and new physics, (4) the mass of the dominant dark matter WIMP is ≤125 GeV/c2, (5) the gauge couplings of this particle are precisely defined, and (6) naturalness implies that its Higgs-mediated couplings are comparable to those of a neutralino with optimal parameters for direct, indirect, and collider detection. Although direct detection has so far not yielded a verified observation, and both CMS and ATLAS have placed approximately 20% limits on branching ratios for invisible Higgs decays (for collider detection), two recent analyses of antiproton observations by AMS-02 (for indirect detection) have shown evidence for dark matter particles in our predicted range (“100 GeVish”) at the 3 sigma to 5 sigma level, depending on the model.
This seminar is based on conference talks and a series of papers [1-4].Copyright © 2023. All rights reserved, Texas A&M University Trademark | Texas A&M University, College Station, Texas 77843