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Searching for low mass dark matter via phonon creation in superfluid 4He

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arxiv 2005.08824 v3 pith:Z2P5FY4B submitted 2020-05-18 hep-ph astro-ph.COcond-mat.othercond-mat.supr-con

classification hep-phastro-ph.COcond-mat.othercond-mat.supr-con
keywords phononphononsdarkmatterenergyomegashowersingle
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abstract

We consider the scattering of dark matter particles from superfluid liquid $^4$He, which has been proposed as a target for their direct detection. Focusing on dark matter masses below ~1 MeV, we demonstrate from sum-rule arguments the importance of the production of single phonons with energies $\omega \lesssim 1$ meV. We show further that the anomalous dispersion of phonons in liquid $^4$He at low pressures [i.e., $d^2\omega(q)/dq^2>0$, where $q$ and $\omega(q)$ are the phonon momentum and energy] has the important consequence that a single phonon will decay over a relatively short distance into a shower of lower energy phonons centered on the direction of the original phonon. Thus the experimental challenge in this regime is to detect a shower of low energy phonons, not just a single phonon. Additional information from the distribution of phonons in such a shower could enhance the determination of the dark matter mass.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  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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