On underestimation of the inelastic interactions in the direct dark matter search
Vadim A. Bednyakov

TL;DR
This paper derives expressions for direct dark matter detection rates considering both elastic and inelastic interactions, highlighting the importance of detecting gamma radiation from nuclear deexcitation to avoid underestimating inelastic contributions.
Contribution
It introduces a comprehensive method to estimate detection rates including inelastic channels and emphasizes the need for dual-signal detection to fully observe dark matter interactions.
Findings
Inelastic interactions can dominate at higher recoil energies.
Detection of gamma radiation is crucial for observing inelastic events.
Elastic-only detectors may significantly underestimate dark matter signals.
Abstract
In the paper expressions are obtained for the event rates expected in experiments aimed at direct detection of dark matter (DM) particles. These expressions allow one to estimate the rates taking into account simultaneously elastic (coherent) and inelastic (incoherent) channels of DM particle interaction with nuclei. The nonzero nuclear excitation energies are used in the calculation of the inelastic scattering contributions. A strong correlation between the excitation energy and the recoil energy of the excited nucleus limits the possibility of the inelastic channel detection with a number of nuclei. Together with the standard model of the DM distribution in the Galaxy some models are considered, which allow higher speeds of the DM particle. As the nuclear recoil energy, TA, increases, the dominance of the elastic interaction channel is smoothly replaced by the dominance of the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Radioactive Decay and Measurement Techniques · Advanced Semiconductor Detectors and Materials
