Dynamical Tadpoles and Weak Gravity Constraints
arXiv:2011.00051 · doi:10.1007/JHEP05(2021)177
Abstract
Non-supersymmetric string models are plagued with tadpoles for dynamical fields, which signal uncanceled forces sourced by the vacuum. We argue that in certain cases, uncanceled dynamical tadpoles can lead to inconsistencies with quantum gravity, via violation of swampland constraints. We describe an explicit realization in a supersymmetric toroidal orientifold with D7-branes, where the dynamical tadpole generated by displacement of the D7-branes off its minimum leads to violation of the axion Weak Gravity Conjecture. In these examples, cancellation of dynamical tadpoles provides consistency conditions for the configuration, of dynamical nature (as opposed to the topological conditions of topological tadpoles, such as RR tadpole cancellation in compact spaces). We show that this approach provides a re-derivation of the Z-minimization criterion for AdS vacua giving the gravitational dual of a-maximization in 4d toric quiver SCFTs.
v3, added references, JHEP accepted, 34 pages + 1 appendix, 3 figures
References in corpus (17)
- On the Geometry of the String Landscape and the Swampland
- Monodromy in the CMB: Gravity Waves and String Inflation
- The Swampland: Introduction and Review
- The String Landscape and the Swampland
- Spacetime Instanton Corrections in 4D String Vacua - The Seesaw Mechanism for D-Brane Models
- A Natural Framework for Chaotic Inflation
- Sasaki-Einstein Manifolds and Volume Minimisation
- Stringy Instantons and Quiver Gauge Theories
- F-term Axion Monodromy Inflation
- Instanton Induced Neutrino Majorana Masses in CFT Orientifolds with MSSM-like spectra
- D7-Brane Chaotic Inflation
- Swampland Conjectures for Strings and Membranes
- Higgs-otic Inflation and String Theory
- The Inflaton as a MSSM Higgs and Open String Modulus Monodromy Inflation
- Chiral 4d String Vacua with D-branes and Moduli Stabilization
- Pair Production and Gravity as the Weakest Force
- A Note on Membrane Interactions and the Scalar potential