Near-horizon quantum gravity fluctuations in an extremal AdS5-Reissner-Nordström black brane make the holographic Wilson loop obey an area law, producing a linear quark-antiquark potential at zero temperature.
We use the quantum-corrected AdS5 metric (12) and drop the subscript of tE for simplicity
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Quantum-Corrected Holographic Wilson Loop Expectation Values and Super-Yang-Mills Confinement
Near-horizon quantum gravity fluctuations in an extremal AdS5-Reissner-Nordström black brane make the holographic Wilson loop obey an area law, producing a linear quark-antiquark potential at zero temperature.