Dark Matter direct detection of classical WIMPs

Summary

This paper supplements lectures on the direct detection of Weakly Interaction Massive Particle (WIMP) dark matter, covering its distribution, nuclear scattering, backgrounds, experimental design, and ongoing/planned experiments.

Key findings

• Direct detection of WIMP dark matter is a high priority in particle physics.
• Understanding dark matter distribution and nuclear scattering is crucial for detection.
• Minimizing backgrounds and careful experimental design are essential for successful detection.

Methods

• Review of theoretical concepts (WIMP properties, nuclear scattering).
• Discussion of experimental considerations (backgrounds, design).
• Survey of planned and ongoing experiments.

Limitations

• Focuses specifically on classical WIMP candidates.
• Content is based on lectures from a specific summer school (2021).

Applications

• Guiding the design and interpretation of dark matter direct detection experiments.
• Educating researchers on the current state of WIMP detection.