  Transverse oscillations that do not show significant damping in solar coronal
loops are found to be ubiquitous. Recently, the discovery of high-frequency
transverse oscillations in small-scale loops has been accelerated by the
Extreme Ultraviolet Imager onboard Solar Orbiter. We perform a meta-analysis by
considering the oscillation parameters reported in the literature. Motivated by
the power law of the velocity power spectrum of propagating transverse waves
detected with CoMP, we consider the distribution of energy fluxes as a function
of oscillation frequencies and the distribution of the number of oscillations
as a function of energy fluxes and energies. These distributions are described
as a power law. We propose that the power law slope ($\delta=-1.40$) of energy
fluxes depending on frequencies could be used for determining whether
high-frequency oscillations dominate the total heating ($\delta < 1$) or not
($\delta > 1$). In addition, we found that the oscillation number distribution
depending on energy fluxes has a power law slope of $\alpha=1.00$, being less
than 2, which means that oscillations with high energy fluxes provide the
dominant contribution to the total heating. It is shown that, on average,
higher energy fluxes are generated from higher frequency oscillations. The
total energy generated by transverse oscillations ranges from about $10^{20}$
to $10^{25}$ erg, corresponding to the energies for nanoflare
($10^{24}-10^{27}$ erg), picoflare ($10^{21}-10^{24}$ erg), and femtoflare
($10^{18}-10^{21}$ erg). The respective slope results imply that high-frequency
oscillations could provide the dominant contribution to total coronal heating
generated by decayless transverse oscillations.

Solar and Stellar Astrophysics