Common perturbation theory problems encountered in quantum mechanics include the calculation of energy shifts and wavefunction corrections for a system when a small perturbation is applied. Solutions to these problems involve using perturbation theory formulas to calculate the first-order and higher-order corrections to the energy levels and wavefunctions of the system. These corrections help to account for the effects of the perturbation on the system's behavior and provide a more accurate description of its quantum properties.
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