  White dwarf-black hole tidal disruption events (herein WTDEs) present an
opportunity to probe the quiescent intermediate mass black hole population in
the universe. We run an extensive set of Monte-Carlo based simulations to
explore SRG/eROSITA's detection sensitivity to WTDEs as a function of black
hole mass, redshift and time offset between event flaring and it first being
observed. A novel estimate of WTDE rate densities from globular clusters and
dwarf galaxies is also presented. We combine this with estimated detection
sensitivities to infer the rate of eROSITA detecting these events. Depending on
the estimate of the intrinsic rate of WTDEs, we anticipate that eROSITA may
detect $\sim 3$ events over its 4 year all-sky survey. eROSITA will be most
sensitive to systems with black hole masses above $10^4M_{\odot}$, and is most
likely to catch these within 5 days of flaring.
