  We study quantum gravity effects on the thermodynamic character and the
radiation process of the thin accretion disks around Schwarzschild-like black
hole. The quantum gravity correction is invoked through the framework of
generalization of uncertainty which is equivalent to the renormalization group
improved quantum gravity and maintain the limit of the asymptotically safe
preposition of gravity. It admits a free parameter that encodes the quantum
effects on the spacetime geometry. It allows us to study how the thermal
properties of the black hole itself and the the accretion around it disk are
modified in the quantum regime. We computed explicitly the entropy,
temperature, free energy, and enthalpy of the modified black hole and show its
variation with with the free parameter that encodes the quantum effects. We
explicitly make estimations of quantum correction to the time averaged energy
flux, the temperature of the disk, the differential luminosity, and the
conversion efficiency of accreting mass into radiation. We observe a
conspicuous shifting of the radius of the innermost stable circular orbit
(ISCO) toward small values together with an enhancement of the maximum of the
values of the average thermal radiation and greater conversion efficiency of
accreting mass into radiation compared to the classical gravity scenario.
