English

Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures

Astrophysics of Galaxies 2021-02-24 v2 High Energy Physics - Phenomenology

Abstract

An ultralight scalar boson with mass m11022m_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 m21020m_2\simeq 10^{-20} eV, with the possibility of a third axion with mass m30.5×1018m_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.

Keywords

Cite

@article{arxiv.1811.03771,
  title  = {Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures},
  author = {Hoang Nhan Luu and S. -H. Henry Tye and Tom Broadhurst},
  journal= {arXiv preprint arXiv:1811.03771},
  year   = {2021}
}

Comments

The new version includes a dynamical analysis of UFD galaxies and consistency check for cosmic relic abundance

R2 v1 2026-06-23T05:09:53.624Z