期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 510, 期 1, 页码 1425-1430出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab3520
关键词
galaxies: high-redshift; cosmology: theory; cosmology: dark matter; cosmology: early Universe
Fuzzy dark matter, composed of ultra-light axions, is an alternative theory designed to address the small-scale problems faced by the standard cold dark matter proposal. It alleviates some of the apparent discrepancies faced by the standard ACDM paradigm.
Fuzzy dark matter (FDM) or wave dark matter is an alternative theory designed to solve the small-scale problems faced by the standard cold dark matter proposal for the primary material component of the Universe. It is made up of ultra-light axions having mass similar to 10(-22) eV that typically have de Broglie wavelength of several kpc, alleviating some of the apparent small-scale discrepancies faced by the standard ACDM paradigm. In this paper, we calculate the halo mass function for the FDM using a sharp-k window function and compare it with one calculated using numerical simulations, finding the peak mass at roughly 10(10 )M(circle dot) for a particle mass of 2 x 10(-22) eV. We also constrain the mass of FDM particle to be greater than or similar to 2 x 10(-22) eV using the observations of high-redshift (z similar to 10) lensed galaxies from CLASH survey.
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