Constant-polymerization loop quantization of Schwarzschild-de Sitter in Kantowski-Sachs gauge generates a spurious low-curvature black hole horizon, while Schwarzschild-anti-de Sitter does not.
On the other hand, in the region T < TT , b(T ) re- mains almost constant for T ≳ TWH (≃ −22.1844), but suddenly drops to zero at T ≃ TWH
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Lessons from gauge fixing and polymerization of loop quantum black holes with a cosmological constant
Constant-polymerization loop quantization of Schwarzschild-de Sitter in Kantowski-Sachs gauge generates a spurious low-curvature black hole horizon, while Schwarzschild-anti-de Sitter does not.