Lectures on the Swampland Program in String Compactifications
Marieke van Beest, José Calderón-Infante, Delaram Mirfendereski, Irene Valenzuela
TL;DR
The paper introduces the Swampland program as a framework to distinguish EFTs that can be UV completed within quantum gravity from those that cannot, using string theory as a testbed. It presents the core conjectures—No Global Symmetries, Completeness, Weak Gravity, Swampland Distance, Emergence, AdS/non-SUSY AdS Instability, and de Sitter—along with motivations, evidence from string compactifications, and interrelations (e.g., WGC with SDC and Emergence). The notes emphasize how these conjectures constrain low-energy physics, inflation, and cosmology, and discuss strong versions and open questions, highlighting a coherent, interconnected structure that governs quantum gravity consistency. The discussed connections suggest a roadmap toward understanding why certain IR phenomena (like approximate symmetries, light towers, and field-range limitations) arise from UV quantum gravity principles and dualities in string theory.
Abstract
The Swampland program aims to determine the constraints that an effective field theory must satisfy to be consistent with a UV embedding in a quantum gravity theory. Different proposals have been formulated in the form of Swampland conjectures. In these lecture notes, we provide a pedagogical introduction to the most important Swampland conjectures, their connections and their realization in string theory compactifications. The notes are based on the series of lectures given by Irene Valenzuela at the online QFT and Geometry summer school in July 2020.
