20–22 Dec 2017
University of Padova, Scuola Galileiana
Europe/Rome timezone

Session

Weak Gravity and Swampland Conjectures in String Inflation

20 Dec 2017, 09:00
Aula Magna (University of Padova, Scuola Galileiana)

Aula Magna

University of Padova, Scuola Galileiana

via San Massimo 33, 35121 Padova

Conveners

Weak Gravity and Swampland Conjectures in String Inflation

  • Fabrizio Rompineve (IFAE Barcelona)
  • Gianluca Zoccarato (Hong Kong IAS and UW Madison)

Weak Gravity and Swampland Conjectures in String Inflation: discussion session

  • There are no conveners in this block

Description

The amount of gravitational waves produced during inflation is crucially linked to the distances in field space traversed by the inflaton field. In particular, large primordial tensor modes require field displacements larger than the Planck scale. This is the scenario of Large Field Inflation (LFI). As we await the final observational verdict on this class of realizations, it is important to understand whether transplanckian field values violate general properties of Quantum Gravity. The Weak Gravity Conjecture (WGC) aims at capturing implications of Quantum Gravity for Effective Field Theory (EFT), thus represents a promising tool to address the theoretical consistency of LFI.

In the first part we will give an introduction to the swampland program which tries to identify the criteria that low energy effective field theories ought to satisfy in order to couple consistently with quantum gravity. We will enumerate the known swampland conjectures offering arguments to support them as well as some examples drawn from string theory where these conjectures are satisfied. A lot of attention will be devoted to the Weak Gravity Conjecture and its various formulations.

In the second part we focus on the consequences of the WGC for models of Large Field Inflation. We start by introducing the basic problems of Large Field Inflation in EFT and thus motivate axions as inflaton candidates. We then review general constraints on axion inflation based on an appropriately generalized WGC. We also discuss constraints on setups based on string compactifications. We then specify to two subclasses of string-motivated models: Axion Alignement and Axion Monodromy. We focus on stringy realizations and discuss interpretations of the WGC in terms of the geometry of the extra dimensions and moduli stabilization.

Presentation materials

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