Centro de Excelencia Severo Ochoa
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Grey Room 3/ Zoom
I will discuss holographic renormalization group (RG) flows beyond their infrared (IR) fixed points. Such “trans-IR” flows are a natural framework for describing physics inside of black holes. I will present a holographic a-function that is stationary at the boundary and the horizon and is monotonic in both the exterior and the interior of the black hole. A monotonic a-function can also be constructed for anisotropic black holes.
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