Article
Version 1
This version is not peer-reviewed
Theoretical WIMP-Nucleus Scattering Rates For Isomeric Nuclei
Version 1
: Received: 30 July 2024 / Approved: 1 August 2024 / Online: 1 August 2024 (15:32:13 CEST)
How to cite: Vergados, J. D.; Bonatsos, D. Theoretical WIMP-Nucleus Scattering Rates For Isomeric Nuclei. Preprints 2024, 2024080035. https://doi.org/10.20944/preprints202408.0035.v1 Vergados, J. D.; Bonatsos, D. Theoretical WIMP-Nucleus Scattering Rates For Isomeric Nuclei. Preprints 2024, 2024080035. https://doi.org/10.20944/preprints202408.0035.v1
Abstract
The direct detection of dark matter constituents, in particular the weakly interacting
massive particles (WIMPs), is central to particle physics and cosmology. In this paper we develop the
formalism for WIMP-Nucleus induced transitions from isomeric nuclear states. We specialize it in
the case of the experimentally interesting target 180 Ta
Keywords
Dark matter; Isomeric Nuclei; Nuclear structure models and methods; Shell model; Collective models; Nilsson Model
Subject
Physical Sciences, Nuclear and High Energy Physics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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