arXiv · 2608.21532
Chiral symmetry and black hole isospectrality
Abstract
We prove that black-hole isospectrality between linearly independent solutions follows whenever radiative metric and matter perturbations are reconstructed from complex master variables obeying a closed, complex-linear system with complex-linear boundary conditions. If a phase rotation maps one parity sector to the other, then the even- and odd-parity QNM spectra coincide, and the perturbations are parity isospectral. A broad class of chiral-aligned theories satisfies these criteria. As an application, we demonstrate that subextremal Kerr--de Sitter black holes are parity isospectral.
Explore related subjects
Keep this discovery
Colin Weller, Dongjun Li, Pratik Wagle, Andrew Laeuger, Yanbei Chen, Nicolás Yunes. 2026-08-21. Chiral symmetry and black hole isospectrality. https://arxiv.org/abs/2608.21532
Cite the original work for its findings. Save a collection to share your selection of sources.