
TL;DR
This paper clarifies the classical symplectic structure of $SU(2)$ isolated horizons, highlighting a rescaling parameter's role, refuting some claims, and questioning the foundation of certain quantum gravity entropy calculations.
Contribution
It demonstrates that the symplectic structure involves a rescaling parameter unrelated to surface gravity, challenging previous assumptions and the classical basis of some quantum horizon models.
Findings
The symplectic structure depends on a rescaling parameter $\sigma$.
The divergence occurs at $\sigma^2=(1+\gamma^2)^{-1}$, violating rescaling symmetry.
Quantum $SU(2)$ horizon theory is based on a flawed classical setup.
Abstract
We point out that the symplectic structure, written in terms of the Sen-Ashtekar-Immirzi-Barbero variables, of a spacetime admitting an isolated horizon as the inner boundary, involves a positive constant parameter, say , if , where is the Barbero-Immirzi parameter. The parameter represents the rescaling freedom that characterizes the equivalence class of null generators of the isolated horizon. We reiterate the fact that the laws of mechanics associated with the isolated horizon does not depend on the choice of and, in particular, while one uses the value of standard surface gravity as input, that does not fix to a particular value. This fact contradicts the claims made in certain parts of the concerned literature that we duly refer to. We do the calculations by taking Schwarzschild metric as an example so that the…
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