  We investigate the generation of Primordial Black Holes (PBHs) with the aid
of gravitationally increased friction mechanism originated from the NonMinimal
field Derivative Coupling (NMDC) to gravity framework, with the quartic
potential. Applying the coupling parameter as a two-parted function of inflaton
field and fine-tuning of five parameter assortments we can acquire ultra
slow-roll phase to slow down the inflaton field due to high friction. This
enables us to achieve enough enhancement in the amplitude of curvature
perturbations power spectra to generate PBHs with different masses. The
reheating stage is considered to obtain criteria for PBHs generation during
radiation dominated era. We demonstrate that three cases of asteroid mass PBHs
($10^{-12}M_{\odot}$, $10^{-13}M_{\odot}$, and $10^{-15}M_{\odot})$ can be very
interesting candidates for comprising $100\%$ , $98.3\%$ and $99.1\%$ of the
total Dark Matter (DM) content of the universe. Moreover, we analyse the
production of induced Gravitational Waves (GWs), and illustrate that their
spectra of current density parameter $(\Omega_{\rm GW_0})$ for all parameter
Cases foretold by our model have climaxes which cut the sensitivity curves of
GWs detectors, ergo the veracity of our outcomes can be tested in light of
these detectors. At last, our numerical results exhibit that the spectra of
$\Omega_{\rm GW_0}$ behave as a power-law function with respect to frequency,
$\Omega_{\rm GW_0} (f) \sim (f/f_c)^{n} $, in the vicinity of climaxes. Also,
in the infrared regime $f\ll f_{c}$, the power index satisfies the relation
$n=3-2/\ln(f_c/f)$.
