SUMMARY
No particles within the Standard Model of Particle Physics possess all the properties of Weakly Interacting Massive Particles (WIMPs). While neutrinos exhibit some characteristics of WIMPs, they do not meet the mass criteria, which typically ranges around 100 GeV. The WIMP concept has evolved, and while neutrinos and other candidates like keV sterile neutrinos are discussed, they do not fit the traditional WIMP definition. The ongoing search for dark matter candidates includes various alternatives such as axion-like particles and supersymmetric particles, indicating a complex landscape beyond the WIMP paradigm.
PREREQUISITES
- Understanding of the Standard Model of Particle Physics
- Knowledge of dark matter candidates, particularly WIMPs and neutrinos
- Familiarity with particle mass scales, specifically in the GeV range
- Basic concepts of supersymmetry and its implications for particle physics
NEXT STEPS
- Research the properties and implications of WIMPs in dark matter theory
- Explore the role of neutrinos in cosmology and their potential as dark matter candidates
- Investigate the concept of supersymmetry and its proposed particles
- Study alternative dark matter candidates such as axion-like particles and WIMPzillas
USEFUL FOR
Particle physicists, cosmologists, and researchers interested in dark matter theories and the properties of fundamental particles.