Question What do we know about Higginson and Gauginos

[Harry Costas]

Lets go back 2019

[Submitted on 31 Dec 2018 (v1), last revised 18 Jun 2019 (this version, v2)]

Peccei-Quinn Symmetry and Nucleon Decay in Renormalizable SUSY SO(10)​

K.S. Babu, Takeshi Fukuyama, Saki Khan, Shaikh Saad

We suggest simple ways of implementing Peccei-Quinn (PQ) symmetry to solve the strong CP problem in renormalizable SUSY SO(10) models with a minimal Yukawa sector. Realistic fermion mass generation requires that a second pair of Higgs doublets survive down to the PQ scale. We show how unification of gauge couplings can be achieved in this context. Higgsino mediated proton decay rate is strongly suppressed by a factor of (MPQ/MGUT)2, which enables all SUSY particles to have masses of order TeV. With TeV scale SUSY spectrum, p→ν⎯⎯⎯K+ decay rate is expected to be in the observable range. Lepton flavor violating processes μ→eγ decay and μ−e conversion in nuclei, induced by the Dirac neutrino Yukawa couplings, are found to be within reach of forthcoming experiments.

 

[Harry Costas]

And what's a Wino and a Chargino.
Chiral Supersymmetry a property to be research in explaining Spin in condensates found in Cores of stars, Neutron Stars and Black Hole.

[Submitted on 10 Jan 2019 (v1), last revised 17 Jun 2019 (this version, v2)]

Discovery reach for wino and higgsino dark matter with a disappearing track signature at a 100 TeV pp collider​

Masahiko Saito, Ryu Sawada, Koji Terashi, Shoji Asai

Within the theory of supersymmetry, the lightest neutralino is a dark matter candidate and is often assumed to be the lightest supersymmetric particle (LSP) as well. If the neutral wino or higgsino is dark matter, the upper limit of the LSP mass is determined by the observed relic density of dark matter. If the LSP is a nearly-pure neutral state of the wino or higgsino, the lightest chargino state is expected to have a significant lifetime due to a tiny mass difference between the LSP and the chargino. This article presents discovery potential of the 100 TeV future circular hadron collider (FCC) for the wino and higgsino dark matter using a disappearing-track signature. The search strategy to extend the discovery reach to the thermal limits of wino/higgsino dark matter is discussed with detailed studies on the background rate and the reference design of the FCC-hadron detector under possible running scenarios of the FCC-hadron machine. A proposal of modifying the detector layout and several ideas to improve the sensitivity further are also discussed.