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Signatures and Detection Prospects for sub-GeV Dark Matter with Superfluid Helium

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arxiv 2208.14474 v1 pith:L6IBUGM4 submitted 2022-08-30 hep-ph astro-ph.COcond-mat.supr-conhep-ex

classification hep-phastro-ph.COcond-mat.supr-conhep-ex
keywords darkdetectionheliummatterquasi-particlessub-gevfluxresulting
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We explore the possibility of using superfluid helium for direct detection of sub-GeV dark matter (DM). We discuss the relevant phenomenology resulting from the scattering of an incident dark matter particle on a Helium nucleus. Rather than directly exciting quasi-particles, DM in this mass range will interact with a single He atom, triggering an atomic cascade which eventually also includes emission and thermalization of quasi-particles. We present in detail the analytical framework needed for modeling these processes and determining the resulting flux of quasi-particles. We propose a novel method for detecting this flux with modern force-sensitive devices, such as nanoelectro-mechanical system (NEMS) oscillators, and derive the sensitivity projections for a generic sub-GeV DM detection experiment using such sensors.

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  1. Hunting axion dark matter with anti-ferromagnets: a case study with nickel oxide

    hep-ph 2024-11 conditional novelty 5.0 of 10

    Axion dark matter with meV-scale masses could be absorbed by magnons in nickel oxide, producing both resonant and broadband detection channels.

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