In the quark-meson model on thermal AdS, chiral symmetry is always broken near the boundary with unique regular inhomogeneous condensate solutions; temperature restores symmetry while negative curvature favors breaking, and the phase diagram is modified by the Hawking-Page transition.
Behavior of a chiral condensate around astrophysical-mass Schwarschild and Reissner-Nordstr¨ om black holes
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Chiral symmetry breaking and inhomogeneous phases in thermal anti-de Sitter spacetime
In the quark-meson model on thermal AdS, chiral symmetry is always broken near the boundary with unique regular inhomogeneous condensate solutions; temperature restores symmetry while negative curvature favors breaking, and the phase diagram is modified by the Hawking-Page transition.