Prospects of a Solar Axion Search with CUORE

The Cryogenic Underground Observatory for Rare Events (CUORE) is an array of 988 TiO₂ crystal bolometers currently operating at Gran Sasso National Laboratory. The primary analysis of CUORE is to search for the ultra-rare process of neutrinoless double-beta (0νββ) in Te-130, which has an energy region of interest (ROI) of 2490-2575 keV. As an extremely low background experiment with high energy resolution and exposure, CUORE has the potential to perform other rare-event searches such as for solar axions or Axion Like Particles (ALPs). Axions are a well-motivated dark matter candidate that also provides a solution for the QCD Strong CP problem. This talk will discuss the prospects of performing a search in CUORE data for solar axions from the Fe-57 transition, which would produce a signal at 14.4 keV. In this talk, I will also discuss the analysis tools for processing and analyzing data that have been developed to enable analyses in CUORE below 100 keV.