  We consider a decaying scalar dark matter (DM) with mass $m_\chi$ in the
range 10 GeV - 10 TeV and vary the branching ratios of all possible two-body SM
final states (excluding and including $\nu\bar{\nu}$) in the range $0\%-100\%$
to derive constraints on the total decay width $\Gamma$ using the data
collected by several astrophysical and cosmological observations. We find that,
$\Gamma \lesssim 10^{-26} - 10^{-27}\,{\rm s}^{-1}$ (excluding $\nu\bar{\nu}$)
and $\Gamma \lesssim 10^{-24} - 10^{-26}\,{\rm s}^{-1}$ (including
$\nu\bar{\nu}$) are allowed, depending on the values of $m_\chi$, which are
most robust upper limits on $\Gamma$ for a generic decaying scalar DM. We then
investigate the prospect of the upcoming Square Kilometre Array (SKA) radio
telescope in detecting the DM decay induced radio signals originating inside
the dwarf spheroidal (dSph) galaxies. We have classified the DM parameter
space, allowed by the existing observations, independently of the branching
ratio of each individual two-body SM final state, based on the detectability at
the SKA. Excluding the $\nu\bar{\nu}$ decay mode, we find that, throughout the
DM mass range considered, $\Gamma \gtrsim 10^{-30}\,{\rm s}^{-1} -
10^{-29}\,{\rm s}^{-1}$ is detectable for all possible branching ratio
combinations at the SKA (assuming 100 hours of observation time), with
conservative choices for the relevant astrophysical parameters. On the other
hand, when arbitrary branching ratios are allowed also for the $\nu\bar{\nu}$
decay mode, DM decays can be probed independently of the branching ratio of
each SM final state for $\Gamma \gtrsim 2 \times 10^{-29}\,{\rm s}^{-1}$,
provided DM masses are greater than a few hundreds of GeV.

High Energy Physics - Phenomenology;High Energy Astrophysical Phenomena