Weak Gravity Conjecture for the Effective Field Theories with N Species

Abstract

We conjecture an intrinsic UV cutoff for the validity of the effective field theory with a large number of species coupled to gravity. In four dimensions such a UV cutoff takes the form $\Lambda =\sqrt{\lambda /N}{M}_p$ for $N$ scalar fields with the same potential $\lambda {\varphi }_i^4$, $i=1,...,N$. This conjecture implies that the assisted chaotic inflation or N-flation might be in the swampland, not in the landscape. Similarly a UV cutoff $\Lambda =g{M}_p/\sqrt{N}$ is conjectured for the U(1) gauge theory with $N$ species.

12 pages; refs added and some statements clarified

References in corpus (4)

• The String Landscape and the Swampland
• Black Hole Bound on the Number of Species and Quantum Gravity at LHC
• Random Polynomials and the Friendly Landscape
• Theoretic Limits on the Equation of State Parameter of Quintessence

Cited by in corpus (4)

• Simple Bounds from the Perturbative Regime of Inflation
• Large Non-Gaussianity Implication for Curvaton Scenario
• N-vaton
• Spectral Index in Curvaton Scenario