Direct detection of WIMPs

TL;DR

This paper reviews the theoretical framework and current experimental efforts for directly detecting WIMPs, a leading dark matter candidate, by analyzing their elastic scattering signals with target materials.

Contribution

It provides a comprehensive overview of the theoretical calculations and predictions for WIMP direct detection across various particle physics models.

Findings

Summarizes the theoretical calculation methods for WIMP detection rates.

Reviews the different detection signals and experimental approaches.

Discusses the particle physics and astrophysical factors influencing detection prospects.

Abstract

A generic weakly interacting massive particle (WIMP) is one of the most attractive candidates to account for the cold dark matter in our Universe, since it would be thermally produced with the correct abundance to account for the observed dark matter density. WIMPs can be searched for directly through their elastic scattering with a target material, and a variety of experiments are currently operating or planned with this aim. In these notes we overview the theoretical calculation of the direct detection rate of WIMPs as well as the different detection signals. We discuss the various ingredients (from particle physics and astrophysics) that enter the calculation and review the theoretical predictions for the direct detection of WIMPs in particle physics models.