Axion minicluster streams in the solar neighbourhood
Ciaran A. J. O'Hare, Giovanni Pierobon, Javier Redondo

TL;DR
This paper investigates how tidal streams from axion miniclusters in the solar neighborhood affect direct detection prospects, suggesting that overlapping streams create a distinctive, spiky signal shape that can reveal axion cosmology history.
Contribution
It demonstrates that tidal disruption leads to overlapping axion streams, significantly altering local dark matter density and signal shape, providing new experimental signatures.
Findings
Most local axion dark matter is in overlapping streams.
Streams produce a spiky, non-Maxwellian signal shape.
Density in the solar neighborhood remains close to the average dark matter density.
Abstract
A consequence of QCD axion dark matter being born after inflation is the emergence of small-scale substructures known as miniclusters. Although miniclusters merge to form minihalos, this intrinsic granularity is expected to remain imprinted on small scales in our galaxy, leading to potentially damaging consequences for the campaign to detect axions directly on Earth. This picture, however, is modified when one takes into account the fact that encounters with stars will tidally strip mass from the miniclusters, creating pc-long tidal streams that act to refill the dark matter distribution. Here we ask whether or not this stripping rescues experimental prospects from the worst-case scenario in which the majority of axions remain bound up in unobservably small miniclusters. We find that the density sampled by terrestrial experiment on mpc-scales will be, on average, around 70--90\% of the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Astronomy and Astrophysical Research
