English

Inflation from Broken Scale Invariance

High Energy Physics - Theory 2014-10-22 v1 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We construct a model of inflation based on a low-energy effective theory of spontaneously broken global scale invariance. This provides a shift symmetry that protects the inflaton potential from quantum corrections. Since the underlying scale invariance is non-compact, arbitrarily large inflaton field displacements are readily allowed in the low-energy effective theory. A weak breaking of scale invariance by almost marginal operators provides a non-trivial inflaton minimum, which sets and stabilizes the final low-energy value of the Planck scale. The underlying scale invariance ensures that the slow-roll approximation remains valid over large inflaton displacements, and yields a scale invariant spectrum of perturbations as required by the CMB observations.

Keywords

Cite

@article{arxiv.1406.5192,
  title  = {Inflation from Broken Scale Invariance},
  author = {Csaba Csaki and Nemanja Kaloper and Javi Serra and John Terning},
  journal= {arXiv preprint arXiv:1406.5192},
  year   = {2014}
}

Comments

18 pages, 3 figures

R2 v1 2026-06-22T04:42:45.487Z