Theoretical Estimate of the Sensitivity of the CUORE Detector to Solar
  Axions
  In this paper we calculate the potential sensitivity of the CUORE detector to
axions produced in the Sun through the Primakoff process and detected by the
inverse coherent Bragg-Primakoff process. The conversion rate is calculated
using density functional theory for the electron density and realistic
expectations for the energy resolution and background of CUORE. Monte Carlo
calculations for $5~$y$\times741~$kg=$3705~$kg y of exposure are analyzed using
time correlation of individual events with the theoretical time-dependent
counting rate and lead to an expected limit on the axion-photon coupling
$g_{a\gamma\gamma}<3.83\times 10^{-10}~GeV^{-1}$ for axion masses less than
$100$ eV.
