First Simulations of Axion Minicluster Halos
arXiv:1911.09417 · doi:10.1103/PhysRevLett.125.041301
Abstract
We study the gravitational collapse of axion dark matter fluctuations in the post-inflationary scenario, so-called axion miniclusters, with N-body simulations. Largely confirming theoretical expectations, overdensities begin to collapse in the radiation-dominated epoch and form an early distribution of miniclusters with masses up to . After matter-radiation equality, ongoing mergers give rise to a steep power-law distribution of minicluster halo masses. The density profiles of well-resolved halos are NFW-like to good approximation. The fraction of axion dark matter in these bound structures is at redshift .
8 pages, 6 figures, accepted by PRL
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