利用超流体氦观测银河暗物质的方向性

IF 1.1 3区 物理与天体物理 Q4 PHYSICS, APPLIED Journal of Low Temperature Physics Pub Date : 2024-06-09 DOI:10.1007/s10909-024-03170-6
G. M. Seidel, C. Enss
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引用次数: 0

摘要

在低温下,超流体氦中高度电离粒子从轨道向外传播的准粒子以前曾被证明表现出各向异性。我们讨论了导致这种行为的机制,并证明它发生在反冲能量低至几千伏甚至更低的暗物质核散射中。这种方向性使得我们有可能搜索和区分银河系暗物质,其相互作用截面可以达到中微子雾,而在中微子雾中,相干的中微子-核散射会带来不可还原的背景。
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Use of Superfluid Helium to Observe Directionality of Galactic Dark Matter

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 directionality makes it possible to search for and distinguish galactic dark matter with interaction cross sections that reach into the neutrino fog where coherent neutrino-nucleus scattering presents an irreducible background.

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来源期刊
Journal of Low Temperature Physics
Journal of Low Temperature Physics 物理-物理:凝聚态物理
CiteScore
3.30
自引率
25.00%
发文量
245
审稿时长
1 months
期刊介绍: The Journal of Low Temperature Physics publishes original papers and review articles on all areas of low temperature physics and cryogenics, including theoretical and experimental contributions. Subject areas include: Quantum solids, liquids and gases; Superfluidity; Superconductivity; Condensed matter physics; Experimental techniques; The Journal encourages the submission of Rapid Communications and Special Issues.
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