Disruption time due to FDM fluctuation-induced heating as a function of orbital distance for the 171 GCs in the MW, as provided by Gaia (Vasiliev & Baumgardt 2021). The disruption time was computed using Equation (11), assuming m₂₂ = 0.3 for an FDM halo with a total mass of 10¹² M_⊙. The disruption process is exceedingly slow for MW GCs, even in the central region, with timescales ranging from 30 to 400 Gyr within the inner 1 kpc. In addition, the timescale of the process increases with the boson mass m₂₂