SLIDE 15 Introduction
Axion monodromy
Problem: Such a potential requires super-Planckian decay constants f Mp to produce at least 60 e-folds of inflation. This is hard to realize in controlled string compactifications. Possible ways out: axion-alignment [Kim,Nilles,Peloso’05/...], N-flation [Dimopoulos,Kachru,McGreevy,Wacker’05] But: These have come under pressure by arguments based on the ’weak gravity conjecture’ [Arkani-Hamed,Motl,Nicolis,Vafa’06] [Rudelius’15/Montero,Uranga,Valenzuela’15/Brown,Cottrell,Shiu,Soler’15...] Less constrained alternative: ’axion monodromy’ [Silverstein,Westphal ’08]
- ! Break the periodicity of the axion weakly by introducing
’monodromic’ potential: φ ! φ + 2πf ) V ! V + ∆V (2)
Jakob Moritz (DESY) Minimalistic axion monodromy with an ultra-light throat mode July 04, 2017 3 / 16