A general framework isolates the linear term in the holographic quark-antiquark potential for symmetric strings in stationary backgrounds, with explicit hypergeometric and elliptic integral expressions for black brane and Rindler-AdS cases.
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Path integral techniques yield effective actions that unify accreting and evaporating configurations for uncharged non-rotating black holes, with emphasis on non-standard evaporating modes.
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The Static Heavy Quark-Antiquark Potential within String Theory in Arbitrary Stationary Backgrounds
A general framework isolates the linear term in the holographic quark-antiquark potential for symmetric strings in stationary backgrounds, with explicit hypergeometric and elliptic integral expressions for black brane and Rindler-AdS cases.
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Path Integral approach to Black-hole Evaporation and Accretion
Path integral techniques yield effective actions that unify accreting and evaporating configurations for uncharged non-rotating black holes, with emphasis on non-standard evaporating modes.