Published April 23, 2020 | Version v1
Journal article Open

Effective field theory of degenerate higher-order inflation

  • 1. Kyoto University
  • 2. University of Chicago

Description

We extend the effective field theory of inflation to a general Lagrangian constructed from Arnowitt-Deser-Misner variables that encompasses the most general interactions with up to second derivatives of the scalar field whose background breaks temporal diffeomorphism invariance. Degeneracy conditions, corresponding to 8 distinct types-only one of which corresponds to known degenerate higher-order scalar-tensor models-provide necessary conditions for eliminating the Ostrogradsky ghost in a covariant theory at the level of the quadratic action in unitary gauge. Novel implications of the degenerate higher-order system for the Cauchy problem are illustrated with the phase space portrait of an explicit inflationary example: Not all field configurations lead to physical solutions for the metric even for positive potentials; solutions are unique for a given configuration only up to a branch choice; solutions on one branch can apparently end at nonsingular points of the metric and their continuation on alternate branches lead to nonsingular bouncing solutions; unitary gauge perturbations can go unstable even when degenerate terms in the Lagrangian are infinitesimal. The attractor solution leads to an inflationary scenario where slow-roll parameters vary and running of the tilt can be large even with no explicit features in the potential far from the end of inflation, requiring the optimized slow-roll approach for predicting observables.

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PhysRevD.101.083531.pdf

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Additional details

Identifiers

DOI
10.1103/PhysRevD.101.083531
Other
oai:uchicago.tind.io:12184

Funding

U.S. Department of Energy
DE-FG02-13ER41958
Simons Foundation
Japan Society for the Promotion of Science
JP17H06359
Japan Society for the Promotion of Science
JP18K13565

UChicago Information

Division(s)
Physical Sciences Division
Department(s)
Astronomy and Astrophysics
Center(s) or Institute(s)
Kavli Institute for Cosmological Physics