In a rotating LQG-corrected black hole model, the polymeric parameter P lowers scalar quasinormal-mode frequencies, while spin raises them.
Bengtsson, Note on Ashtekar’s variables in the spher- ically symmetric case,Class
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Quasinormal Modes of Self-Dual Loop Quantum Gravity Corrected Kerr Black Holes
In a rotating LQG-corrected black hole model, the polymeric parameter P lowers scalar quasinormal-mode frequencies, while spin raises them.