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It is known that the nonstrictly thermal character of the Hawking radiationspectrum harmonizes Hawking radiation with black hole (BH) quasi-normal modes(QNM). This paramount issue has been recently analyzed in the framework of bothSchwarzschild BHs (SBH) and Kerr BHs (KBH). In this assignment, we generalizethe analysis to the framework of nonextremal Reissner-Nordstr\"{o}m BHs (RNBH).Such a generalization is important because in both SBHs and KBHs an absorbed(or emitted) particle has only mass. Instead, in RNBHs the particle has chargeas well as mass. In doing so, we expose that for the RNBH, QNMs can benaturally interpreted in terms of quantum levels for both particle emission andabsorption. Conjointly, we generalize some concepts concerning the RNBH's"effective states".

Hawking radiation - quasi-normal modes correspondence and effective states for nonextremal Reissner-Nordstr\"{o}m black holes