A comment on no-force conditions for black holes and branes
arXiv:2010.11590 · doi:10.1088/1361-6382/abe01a
Abstract
In the context of the Weak Gravity Conjecture the notion of quasi-extremality for black holes and branes was recently defined as the property of having either vanishing horizon size or surface gravity. It was derived that such objects obey a no-force condition. In this short note I present a simplified derivation that is essentially present in the formalism of timelike reduction pioneered by Breitenlohner, Gibbons and Maison. This formalism also provides the natural definition of quasi-extremality for gravitational instantons (and wormholes) sourced by axion fluxes and strengthens the argument that macroscopic axion wormholes do not contribute in the path integral since they are self-repulsive in a Euclidean sense.
arXiv comment9 pages incl references: v2 typos corrected, few refs added: v3 few paragraphs added, version to be published in Class.Quant.Grav
References in corpus (20)
- The String Landscape, Black Holes and Gravity as the Weakest Force
- The Swampland: Introduction and Review
- The String Landscape and the Swampland
- The Weak Gravity Conjecture and Scalar Fields
- Sharpening the Weak Gravity Conjecture with Dimensional Reduction
- Euclidean Wormholes in String Theory
- Euclidean wormholes, baby universes, and their impact on particle physics and cosmology
- Non-Supersymmetric Attractor Flow in Symmetric Spaces
- Universal BPS structure of stationary supergravity solutions
- Generating Geodesic Flows and Supergravity Solutions
- Merging the Weak Gravity and Distance Conjectures Using BPS Extremal Black Holes
- Repulsive Forces and the Weak Gravity Conjecture
- The String Landscape, the Swampland, and the Missing Corner
- Scalar Fields, Hierarchical UV/IR Mixing and The Weak Gravity Conjecture
- Erice Lectures on Black Holes and Attractors
- Baby Universes, Holography, and the Swampland
- Duality and Axionic Weak Gravity
- Euclidean axion wormholes have multiple negative modes
- The Hesse potential, the c-map and black hole solutions
- The holographic dual to supergravity instantons in