Observational properties of black hole in quantum fluctuation modified gravity

Abstract: This study investigates the properties of the thin accretion disk around a black hole in quantum fluctuation modified gravity (QFMGBH) using the Novikov-Thorne model. We restrict the parameter ( \alpha ) characterizing the quantum fluctuation of metric and compute the ISCO radius, examining its effect on the energy flux, the radiation temperature, the luminosity spectrum, the energy efficiency, and the shadow size for various values of the parameter ( \omega ) characterizing the matter around the black hole. Our findings show that the ISCO radius increases with ( \alpha ) for ( \omega = 1/3, 0, -2/3 ), but decreases for ( \omega = -4/3 ). As ( \alpha ) increases, the energy flux and the temperature show distinct trends, with changes in the luminosity spectrum and the efficiency. The shadow size increases for ( \omega = 1/3, 0, -2/3 ), and decreases for ( \omega = -4/3 ). The accretion disk around the QFMGBH is smaller, hotter, and brighter than that surrounded the Schwarzschild BH in GR, suggesting that the observable differences can potentially distinguish quantum fluctuation modified gravity from standard GR.