  In this work, we analyzed the effect of different prescriptions of the IR
cutoffs, namely the Hubble horizon cutoff, particle horizon cutoff, Granda and
Oliveros horizon cut off, and the Ricci horizon cutoff on the growth rate of
clustering for the Tsallis holographic dark energy (THDE) model in an FRW
universe devoid of any interactions between the dark Universe. Furthermore, we
used the concept of configurational entropy to derive constraints
(qualitatively) on the model parameters for the THDE model in each IR cutoff
prescription from the fact that the rate of change of configurational entropy
hits a minimum at a particular scale factor $a_{DE}$ which indicate precisely
the epoch of dark energy domination predicted by the relevant cosmological
model as a function of the model parameter(s). By using the current
observational constraints on the redshift of transition from a decelerated to
an accelerated Universe, we derived constraints on the model parameters
appearing in each IR cutoff definition and on the non-additivity parameter
$\delta$ characterizing the THDE model and report the existence of simple
linear dependency between $\delta$ and $a_{DE}$ in each IR cutoff setup.
