English

Effective Field Theory for Inflation

Cosmology and Nongalactic Astrophysics 2011-06-14 v1 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

This is a version of the author's Ph.D. thesis. The methods of effective field theory are used to study generic theories of inflation with a single inflaton field and to perform a general analysis of the associated non-Gaussianities. We investigate the amplitudes and shapes of the various three and four-point correlators which are generated by different classes of single-field inflationary models. Besides the well-known results for the so called P(X,\phi) model and the ghost inflationary theories, which we recover, we point out that extrinsic curvature-generated interactions may give rise to large non-Gaussianities with distinctive features in the form of specific shape-functions (e.g. flat, orthogonal etc..) for the correlators.

Keywords

Cite

@article{arxiv.1106.2189,
  title  = {Effective Field Theory for Inflation},
  author = {Matteo Fasiello},
  journal= {arXiv preprint arXiv:1106.2189},
  year   = {2011}
}

Comments

Ph.D. thesis

R2 v1 2026-06-21T18:20:50.046Z