Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures

preprint2020arXivOpen access

Abstract

An ultralight scalar boson with mass m1≃10−22m_1 \simeq 10^{-22} eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in String Theory, with multiple light axions predicted in this context. We examine the possibility of soliton structures over a wide range of scales, accounting for galaxy core masses and the common presence of nuclear star clusters. We present a diagnostic soliton core mass-radius plot that provides a global view, indicating the existence of an additional axion with mass m2≃10−20m_2\simeq 10^{-20} eV, with the possibility of a third axion with mass m3≳0.5×10−18m_3 \gtrsim 0.5 \times 10^{-18} eV. We also argue that the relative mass densities measured for these axions are consistent with their cosmological production via the mis-alignment mechanism.

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