QNM frequencies and GUP-corrected Hawking temperatures of BTZ black holes in f(R) and Ricci-Inverse gravity are expressed in terms of an effective cosmological constant, but key derivations contain errors.
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Quasinormal Modes and GUP-Corrected Hawking Radiation of BTZ Black Holes within Modified Gravity Frameworks
QNM frequencies and GUP-corrected Hawking temperatures of BTZ black holes in f(R) and Ricci-Inverse gravity are expressed in terms of an effective cosmological constant, but key derivations contain errors.