Interacting dark energy axions in light of the Hubble tension
  A current problem within the {\Lambda}CDM framework is the tension between
late and early time measurements of the Hubble parameter today, H0. We
entertain the possibility that dark energy modeled as multiple interacting
axion-like-particle species can alleviate the current Hubble tension. We then
test these parameters against the milder tension between the CMB and large
scale structure (LSS) observations of {\sigma}8 to ensure that these models do
not exacerbate the tension. We find that there exist parameter spaces for
models of two and three axion-like-particles which can potentially alleviate
the Hubble tension as well as the {\sigma}8 tension.
