Due to the attractor mechanism, the entropy of an extremal black hole does not vary continuously as we vary the asymptotic values of various moduli fields. Using this fact we argue that the entropy of an extremal black hole in string theory, calculated for a range of values of the asymptotic moduli for which the microscopic theory is strongly coupled, should match the statistical entropy of the same system calculated for a range of values of the asymptotic moduli for which the microscopic theory is weakly coupled. This argument does not rely on supersymmetry and applies equally well to nonsupersymmetric extremal black holes. We discuss several examples which support this argument and also several caveats which could invalidate this argument
We consider theories with gravity, gauge fields and scalars in four-dimensional asymptotically flat ...
We reconsider entropy of black holes which do not have finite area horizon. It is suggested that som...
The product of the areas of the event horizon and the Cauchy horizon of a non-extremal black hole eq...
Due to the attractor mechanism, the entropy of an extremal black hole does not vary continuously as ...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with ...
A five-dimensional dyonic black hole in Type-I theory is considered that is extremal but non-supersy...
After summarizing the development of black hole thermodynamics in the seventies, we describe a recen...
A five-dimensional dyonic black hole in Type-I theory is considered that is extremal but non-supersy...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with...
The supersymmetric flow equations describing the flow of moduli from infinity to the black hole hori...
In these lecture notes we describe recent progress in our understanding of attractor mechanism and e...
Non-extremal black holes in (Formula presented.) supergravity have two horizons, the geometric mean ...
At the horizon, a static extremal black hole solution in N=2 supergravity in four dimensions is dete...
We give several pieces of evidence to show that extremal black holes cannot be obtained as limits of...
The statistical entropy of a five-dimensional black hole in Type II string theory was recently deriv...
We consider theories with gravity, gauge fields and scalars in four-dimensional asymptotically flat ...
We reconsider entropy of black holes which do not have finite area horizon. It is suggested that som...
The product of the areas of the event horizon and the Cauchy horizon of a non-extremal black hole eq...
Due to the attractor mechanism, the entropy of an extremal black hole does not vary continuously as ...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with ...
A five-dimensional dyonic black hole in Type-I theory is considered that is extremal but non-supersy...
After summarizing the development of black hole thermodynamics in the seventies, we describe a recen...
A five-dimensional dyonic black hole in Type-I theory is considered that is extremal but non-supersy...
We investigate four-dimensional spherically symmetric black hole solutions in gravity theories with...
The supersymmetric flow equations describing the flow of moduli from infinity to the black hole hori...
In these lecture notes we describe recent progress in our understanding of attractor mechanism and e...
Non-extremal black holes in (Formula presented.) supergravity have two horizons, the geometric mean ...
At the horizon, a static extremal black hole solution in N=2 supergravity in four dimensions is dete...
We give several pieces of evidence to show that extremal black holes cannot be obtained as limits of...
The statistical entropy of a five-dimensional black hole in Type II string theory was recently deriv...
We consider theories with gravity, gauge fields and scalars in four-dimensional asymptotically flat ...
We reconsider entropy of black holes which do not have finite area horizon. It is suggested that som...
The product of the areas of the event horizon and the Cauchy horizon of a non-extremal black hole eq...