Universality of Sypersymmetric Attractors
Sergio Ferrara, Renata Kallosh

TL;DR
This paper demonstrates that the entropy-area relation for supersymmetric black holes is universal across various theories and dimensions, based on the behavior of central charges and duality invariants at the attractor point.
Contribution
It proves the universality of the entropy formula for supersymmetric black holes and extends the results to different dimensions and theories, providing duality symmetric expressions for ground state energy.
Findings
Entropy-area formula is universal for N=2,4,8 supersymmetric black holes.
All central charges except Z=M vanish at the attractor point for N=4,8.
Ground state energy expressed via duality invariants and horizon area.
Abstract
The macroscopic entropy-area formula for supersymmetric black holes in N=2,4,8 theories is found to be universal: in d=4 it is always given by the square of the largest of the central charges extremized in the moduli space. The proof of universality is based on the fact that the doubling of unbroken supersymmetry near the black hole horizon requires that all central charges other than Z=M vanish at the attractor point for N=4,8. The ADM mass at the extremum can be computed in terms of duality symmetric quartic invariants which are moduli independent. The extension of these results for d=5, N=1,2,4 is also reported. A duality symmetric expression for the energy of the ground state with spontaneous breaking of supersymmetry is provided by the power 1/2 (2/3) of the black hole area of the horizon in d=4 (d=5). It is suggested that the universal duality symmetric formula for the energy of…
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