A set of effective equations for the gauge-invariant gravitational perturbations in the interior of a spherically symmetric, nonrotating black hole is derived within the framework of hybrid loop quantum cosmology. The quantum zero mode of the Hamiltonian constraint, obtained from a perturbative gauge-invariant canonical analysis, is explicitly imposed on a class of quantum states whose wave functions factorize into a background and a perturbative part, related through a geometric relational variable. These states naturally describe regimes with small perturbative backreaction and lead to an effective Hamiltonian and associated dynamics for the perturbations. The resulting equations take the form of Regge-Wheeler equations modified by expectation values of the quantum black hole geometry, providing a clear characterization of quantum corrections to the classical description of the black hole interior. This framework opens the way to investigating hybrid loop quantum gravity effects in the propagation of gravitational waves.

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• Loop quantum gravity
• Quantum aspects of black holes
• Quantum gravity