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We quantize the Oppenheimer-Snyder model of black hole using the integralquantization method. We treat spatial and temporal coordinates on the samefooting both at classical and quantum levels. Our quantization resolves orsmears the singularities of the classical curvature invariants. Quantumtrajectories with bounces can replace singular classical ones. The consideredquantum black hole may have finite bouncing time. As a byproduct, we obtain theresolution of the gravitational singularity of the Schwarzschild black hole atquantum level.

Quantum system ascribed to the Oppenheimer-Snyder model of massive star