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Use of Superfluid Helium to Observe Directionality of Galactic Dark Matter

2022/10/12 by G. M. Seidel, Seidel, George M., C. Enss +1
Physics and Astronomy · #Anisotropy #Astrophysics #Atomic and Subatomic Physics Research #Atomic physics #Condensed matter physics #Dark Matter and Cosmic Phenomena #Dark matter #FOS: Physical sciences #Helium #Helium-4 #High Energy Physics - Phenomenology (hep-ph) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Neutrino #Nuclear physics #Physics #Quantum mechanics #Quantum, superfluid, helium dynamics #Recoil #Scattering #Superfluid helium-4 #Superfluidity #WIMP

paper · pdf · doi:10.48550/arxiv.2210.06283

published in arXiv (Cornell University) (Cornell University)

openalex publication_date 2022/10/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The quasiparticle propagation away from the track of a highly ionizing particle in superfluid helium at low temperatures has previously been shown to exhibit anisotropy. We discuss the mechanism responsible for this behavior and show that it occurs for nuclear scattering by dark matter for recoil energies down to a few keV, and perhaps lower. This makes it possible to extend WIMP searches with interaction cross sections that reach into the neutrino floor in a meaningful energy range.

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