On The Direct Detection of Dark Matter- Exploring all the signatures of the neutralino-nucleus interaction
J.D. Vergados (University of Ioannina, Ioannina, Greece)

TL;DR
This paper reviews methods and signatures for direct detection of supersymmetric dark matter, focusing on neutralino interactions with nuclei, and explores experimental signatures like modulation and directional detection to improve detection prospects.
Contribution
It provides a comprehensive analysis of all potential signatures of neutralino-nucleus interactions, including novel considerations for directional experiments and alternative detection channels.
Findings
Derived constraints on nucleon cross sections from current experimental limits.
Identified characteristic signatures such as modulation effects and directional asymmetries.
Extended analysis to include detection of excited states, recoiling electrons, and X-ray emissions.
Abstract
Various issues related to the direct detection of supersymmetric dark matter are reviewed. Such are: 1) Construction of supersymmetric models with a number of parameters, which are constrained from the data at low energies as well as cosmological observations. 2) A model for the nucleon, in particular the dependence on the nucleon cross section on quarks other than u and d. 3) A nuclear model, i.e. the nuclear form factor for the scalar interaction and the spin response function for the axial current. 4) Information about the density and the velocity distribution of the neutralino (halo model). Using the present experimental limits on the rates and proper inputs in 3)-4) we derive constraints in the nucleon cross section, which involves 1)-2). Since the expected event rates are extremely low we consider some additional signatures of the neutralino nucleus interaction, such as the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Cosmology and Gravitation Theories
