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Search for axions in streaming dark matter

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arxiv 1703.01436 v1 pith:SINW3IND submitted 2017-03-04 physics.ins-det astro-ph.COastro-ph.IM

classification physics.ins-detastro-ph.COastro-ph.IM
keywords axionaxionssearchsomedarkhaloscopematterstreaming
verification ladder T0 review T1 audit T2 compute T3 formal
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A new search strategy for the detection of the elusive dark matter (DM) axion is proposed. The idea is based on streaming DM axions, whose flux might get temporally enormously enhanced due to gravitational lensing. This can happen if the Sun or some planet (including the Moon) is found along the direction of a DM stream propagating towards the Earth location. The experimental requirements to the axion haloscope are a wide-band performance combined with a fast axion rest mass scanning mode, which are feasible. Once both conditions have been implemented in a haloscope, the axion search can continue parasitically almost as before. Interestingly, some new DM axion detectors are operating wide-band by default. In order not to miss the actually unpredictable timing of a potential short duration signal, a network of co-ordinated axion antennae is required, preferentially distributed world-wide. The reasoning presented here for the axions applies to some degree also to any other DM candidates like the WIMPs.

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Cited by 1 Pith paper

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

  1. ADAMOS: Axion Daily Modulation Searches for Dark Matter at 20 GHz

    hep-ex 2026-02 conditional novelty 5.0 of 10

    ADAMOS, a proposed 20 GHz thin-shell haloscope, would reach g_aγγ≈4.4×10^-13 GeV^-1 in 30 days and simultaneously search for daily-modulated and transient axion signals.

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