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      Topology, Entropy and Witten Index of Dilaton Black Holes

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          Abstract

          We have found that for extreme dilaton black holes an inner boundary must be introduced in addition to the outer boundary to give an integer value to the Euler number. The resulting manifolds have (if one identifies imaginary time) topology \(S^1 \times R \times S^2 \) and Euler number \(\chi = 0\) in contrast to the non-extreme case with \(\chi=2\). The entropy of extreme \(U(1)\) dilaton black holes is already known to be zero. We include a review of some recent ideas due to Hawking on the Reissner-Nordstr\"om case. By regarding all extreme black holes as having an inner boundary, we conclude that the entropy of {\sl all} extreme black holes, including \([U(1)]^2\) black holes, vanishes. We discuss the relevance of this to the vanishing of quantum corrections and the idea that the functional integral for extreme holes gives a Witten Index. We have studied also the topology of ``moduli space'' of multi black holes. The quantum mechanics on black hole moduli spaces is expected to be supersymmetric despite the fact that they are not HyperK\"ahler since the corresponding geometry has torsion unlike the BPS monopole case. Finally, we describe the possibility of extreme black hole fission for states with an energy gap. The energy released, as a proportion of the initial rest mass, during the decay of an electro-magnetic black hole is 300 times greater than that released by the fission of an \({}^{235} U\) nucleus.

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          Supersymmetry as a Cosmic Censor

          In supersymmetric theories the mass of any state is bounded below by the values of some of its charges. The corresponding bounds in case of Schwarzschild and Reissner-Nordstr\"om black holes are known to coincide with the requirement that naked singularities be absent. Here we investigate charged dilaton black holes in this context. We show that the extreme solutions saturate the supersymmetry bound of \(N=4\ d=4\) supergravity, or dimensionally reduced superstring theory. Specifically, we have shown that extreme dilaton black holes, with electric and magnetic charges, admit super-covariantly constant spinors. The supersymmetric positivity bound for dilaton black holes, \(M \geq \frac{1}{\sqrt 2}(|Q|+|P|)\), takes care of the absence of naked singularities of the dilaton black holes and is, in this sense, equivalent to the cosmic censorship condition. The temperature, entropy and singularity are discussed. The Euclidean action (entropy) of the extreme black hole is given by \(2\pi |PQ|\). We argue that this result, as well as the one for Lorentzian signature, is not altered by higher order corrections in the supersymmetric theory. When a black hole reaches its extreme limit, it cannot continue to evaporate by emitting elementary particles, since this would violate the supersymmetric positivity bound. We speculate on the possibility that an extreme black hole may ``evaporate" by emitting smaller extreme black holes.
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            Black Holes in Thermal Equilibrium

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              Charge Quantization of Axion-Dilaton Black Holes

              We present axion-dilaton black-hole and multi-black-hole solutions of the low-energy string effective action. Under \(SL(2,R)\) electric-magnetic duality rotations only the ``hair" (charges and asymptotic values of the fields) of our solutions is transformed. The functional form of the solutions is duality-invariant. Axion-dilaton black holes with zero entropy and zero area of the horizon form a family of stable particle-like objects, which we call {\it holons}. We study the quantization of the charges of these objects and its compatibility with duality symmetry. In general the spectrum of black-hole solutions with quantized charges is not invariant under \(SL(2,R)\) but only under \(SL(2,Z)\) or one of its subgroups \(\Gamma_{l}\). Because of their transformation properties, the asymptotic value of the axion-dilaton field of a black hole may be associated with the modular parameter \(\tau\) of some complex torus and the integer numbers \((n,m)\) that label its quantized electric and magnetic charges may be associated with winding numbers.
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                Author and article information

                Journal
                20 July 1994
                1994-11-17
                Article
                10.1103/PhysRevD.51.2839
                hep-th/9407118
                ecd5e844-ed75-47f3-8d75-f04572a06007
                History
                Custom metadata
                NI94003 and SU-ITP-94-9
                Phys.Rev.D51:2839-2862,1995
                51 pages, 4 figures, LaTeX. Considerably extended version. New sections include discussion of the Witten index, topology of the moduli space, black hole sigma model, and black hole fission with huge energy release
                hep-th gr-qc

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