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Abstract: Dark Matter experiments searching for Weakly interacting massive particles (WIMPs) primarily use nuclear recoils (NRs) in their attempt to detect WIMPs. Migdal-induced electronic recoils (ERs) provide additional sensitivity to light Dark Matter with Script O(GeV/c2) masses. In this work, we use Bayesian inference to find the parameter space where future detectors like XENONnT and SuperCDMS SNOLAB will be able to detect WIMP Dark Matter through NRs, Migdal-induced ERs or a combination thereof. We identify regions where each detector is best at constraining the Dark Matter mass and spin independent cross-section and infer where two or more detection configurations are complementary to constraining these Dark Matter parameters through a combined analysis.
Authorship: Angevaare J., Bertone G., Colijn A., Decowski M., Kavanagh B.,
Fuente: Journal of Cosmology and Astroparticle Physics, 2022, 10, 004
Publisher: IOP Publishing
Year of publication: 2022
No. of pages: 24
Publication type: Article
DOI: 10.1088/1475-7516/2022/10/004
ISSN: 1475-7516
Publication Url: https://doi.org/10.1088/1475-7516/2022/10/004
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ANGEVAARE, J.R.
BERTONE, G.
COLIJN, A.P.
DECOWSKIA, M.P.
BRADLEY JAMES KAVANAGH
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