Dark Matter Particle Predictions with Python
Dr. John Harrison
Texas A&M University-Corpus Christi
Abstract
High-energy neutrino flavor transitions provide a sensitive probe of physics beyond the Standard Model, particularly in regimes where ultra-high-energy cross-sections and extended mixing structures become relevant. In this work, we model neutrino flavor evolution using the PMNS framework and higher-order transition indices to generalize the standard oscillation probability structure. These calculations incorporate cosmic-ray-scale interaction cross-sections, where neutrino-electron scattering reaches approximately 1.691 × 10−33 cm2 for Eν ∼ 1000 GeV.
We then explore conditions under which neutrino states may mix with supersymmetric neutralinos—fermionic combinations of photino, zino, and higgsino fields—commonly proposed as WIMP dark matter candidates. In R-parity-violating SUSY scenarios, modified neutral fermion mass matrices and non-zero sneutrino vacuum expectation values can enable neutrino-neutralino mixing, allowing oscillations into heavier neutralino-like states over long baselines or extreme energies. Representative density transitions are computed to illustrate how such extended mixing could influence flavor populations and potentially connect neutrino oscillation phenomenology with dark matter signatures.
These results highlight a mathematically consistent pathway for linking neutrino flavor physics with supersymmetric dark matter models and motivate further investigation into observational consequences for cosmic neutrino experiments and next-generation dark matter searches.