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E(7) Symmetric Area of the Black Hole Horizon

Renata Kallosh, Barak Kol

TL;DR

The supergravity nonrenormalization theorem for the area of the horizon in the {ital N}=8 case protects the unique {ital U}-duality invariant.

Abstract

Extreme black holes with 1/8 of unbroken N=8 supersymmetry are characterized by the non-vanishing area of the horizon. The central charge matrix has four generic eigenvalues. The area is proportional to the square root of the invariant quartic form of $E_{7(7)}$. It vanishes in all cases when 1/4 or 1/2 of supersymmetry is unbroken. The supergravity non-renormalization theorem for the area of the horizon in N=8 case protects the unique U-duality invariant.

E(7) Symmetric Area of the Black Hole Horizon

TL;DR

The supergravity nonrenormalization theorem for the area of the horizon in the {ital N}=8 case protects the unique {ital U}-duality invariant.

Abstract

Extreme black holes with 1/8 of unbroken N=8 supersymmetry are characterized by the non-vanishing area of the horizon. The central charge matrix has four generic eigenvalues. The area is proportional to the square root of the invariant quartic form of . It vanishes in all cases when 1/4 or 1/2 of supersymmetry is unbroken. The supergravity non-renormalization theorem for the area of the horizon in N=8 case protects the unique U-duality invariant.

Paper Structure

This paper contains 26 equations.