Attractors at weak gravity
arXiv:hep-th/9812049 · doi:10.1016/S0550-3213(99)00096-6
Abstract
We study the attractor mechanism in low energy effective D=4, N=2 Yang-Mills theory weakly coupled to gravity, obtained from the effective action of type IIB string theory compactified on a Calabi-Yau manifold. Using special Kähler geometry, the general form of the leading gravitational correction is derived, and from this the attractor equations in the weak gravity limit. The effective Newton constant turns out to be spacetime-dependent due to QFT loop and nonperturbative effects. We discuss some properties of the attractor solutions, which are gravitationally corrected dyons, and their relation with the BPS spectrum of quantum Yang-Mills theory. Along the way, we obtain a satisfying description of Strominger's massless black holes, moving at the speed of light, free of pathologies encountered in some earlier proposals.
21 pages, Latex, no figures, references added
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Cited by in corpus (20)
- Orientifolds of K3 and Calabi-Yau Manifolds with Intersecting D-branes
- Wall-Crossing from Boltzmann Black Hole Halos
- Merging the Weak Gravity and Distance Conjectures Using BPS Extremal Black Holes
- Finiteness and the Swampland
- Supergravity Instantons for N=2 Hypermultiplets
- Four ways across the wall
- The 0-brane action in a general D=4 supergravity background
- Small Black Hole Explosions
- BPS Soliton Solutions of a D3-brane Action
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- Black Holes as Probes of Moduli Space Geometry
- Excision of Singularities by Stringy Domain Walls
- The Kahler Cone as Cosmic Censor
- Quiver indices and Abelianization from Jeffrey-Kirwan residues
- The many symmetries of Calabi-Yau compactifications
- BPS Dendroscopy on Local
- Threebranes in F-theory
- Gauge Theories on the Coulomb branch
- Towards the Core of the Quantum Monopole