  The current LIGO-Virgo observing run has been pushing the sensitivity limit
to touch the stochastic gravitational-wave backgrounds (SGWBs). However, no
significant detection has been reported to date for any single dominated source
of SGWBs with a single broken-power-law (BPL) spectrum. Nevertheless, it could
equally well escape from existing Bayesian searches from, for example, two
comparable dominated sources with two separate BPL spectra (double-peak case)
or a single source with its power-law behavior in the spectrum broken twice
(doubly broken case). In this paper, we put constraints on these two cases but
specifically for the model with cosmological first-order phase transitions from
Advanced LIGO-Virgo's first three observing runs. We found strong negative
evidence for the double-peak case and hence place 95\% C.L. upper limits
$\Omega_\mathrm{BPL,1}<5.8\times10^{-8}$ and
$\Omega_\mathrm{BPL,2}<4.4\times10^{-8}$ on the two BPL spectra amplitudes with
respect to the unresolved compact binary coalescence (CBC) amplitude
$\Omega_\mathrm{CBC}<5.6\times10^{-9}$. We further found weak negative evidence
for the doubly broken case and hence place 95\% C.L. upper limit
$\Omega_\mathrm{DB}<1.2\times10^{-7}$ on the overall amplitude of the doubly
broken spectrum with respect to $\Omega_\mathrm{CBC}<6.0\times10^{-9}$. In
particular, the results from the double-peak case have marginally ruled out the
strong super-cooling first-order phase transitions at LIGO-Virgo band.
