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The Hubble tension is analyzed in the framework of quantum cosmologicalapproach. It is found that there arises a new summand in the expression for thetotal energy density stipulated by the quantum Bohm potential. This additionalenergy density modifies the expansion history of the early universe and decayswith scale factor $a$ as $a^{-6}$, faster than radiation, in late universe.Taking account of this matter-energy component of quantum nature can, inprinciple, eliminate a discrepancy between the direct late timemodel-independent measurements of the Hubble constant and its indirect modeldependent estimates. The model been considered allows one to extend thestandard cosmology to quantum sector.

The Hubble tension from the standpoint of quantum cosmology