  The existence of intermediate-mass black holes (IMBHs) in globular clusters
(GCs) remains a crucial problem. Searching IMBHs in GCs reveals a discrepancy
between radio observations and dynamical modelings: the upper mass limits
constrained by radio observations are systematically lower than that of
dynamical modelings. One possibility for such a discrepancy is that, as we
suggest in this work, there exist outflows in accretion flows. Our results
indicate that, for most sources, current radio observations cannot rule out the
possibility that IMBHs may exist in GCs. In addition, we adopt an \dot{M}-L_{R}
relation to revisit this issue, which confirms the results obtained by the
Fundamental Plane relation.
