We revisit our earlier work and investigate the bound state perturbations in the interior of the Schwarzschild black hole. The bound sates are defined as the perturbations in the interior of the black hole with an imaginary spectrum which are regular at the center of black hole while their time-dependent profile falls off exponentially on the event horizon. Using the scale factor in the expanding direction in the interior of the black hole as the clock, we rewrite the corresponding Regge-Wheeler equation and solve it semianalytically as well as numerically. We confirm that the bound state solutions exist for scalar, vector and axial tensor perturbations. It is shown that for a given value of $\ell >s$, there are total $\ell -s$ such bound states. We obtain the universal lower bound $2GM{\omega }_I>1$ for the spectrum of bound state which is asymptotically saturated in the large $\ell$ limit. Furthermore, we obtain an upper bound on the spectrum of axial perturbations which for large $\ell$ scales like $2GM{\omega }_I\lesssim 0.04{\ell }^4$. As observed recently, these bound states have the curious property that the profile of the total wave function has a nonzero magnitude near the future event horizon.

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• Classical black holes