Black hole entropy in f(Q) gravity obeys a universal integral relation involving horizon data and a residue-induced temperature shift, with an explicit first-order correction for the quadratic model.
Calculating the hawking temperature of black holes inf(q) gravity using the rvb method: A residue-based approach.Canadian Journal of Physics, 103:531–542
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Black Hole Entropy in f(Q) Gravity from the RVB Residue Method
Black hole entropy in f(Q) gravity obeys a universal integral relation involving horizon data and a residue-induced temperature shift, with an explicit first-order correction for the quadratic model.