English

Conformal inflation in the metric-affine geometry

High Energy Physics - Theory 2021-02-01 v3 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

Systematic understanding for classes of inflationary models is investigated from the viewpoint of the local conformal symmetry and the slightly broken global symmetry in the framework of the metric-affine geometry. In the metric-affine geometry, which is a generalisation of the Riemannian one adopted in the ordinary General Relativity, the affine connection is an independent variable of the metric rather than given e.g. by the Levi-Civita connection as its function. Thanks to this independency, the metric-affine geometry can preserve the local conformal symmetry in each term of the Lagrangian contrary to the Riemannian geometry, and then the local conformal invariance can be compatible with much more kinds of global symmetries. As simple examples, we consider the two-scalar models with the broken SO(1,1)\mathrm{SO}(1,1) or O(2)\mathrm{O}(2), leading to the well-known α\alpha-attractor or natural inflation, respectively. The inflaton can be understood as their pseudo Nambu-Goldstone boson.

Keywords

Cite

@article{arxiv.2008.00628,
  title  = {Conformal inflation in the metric-affine geometry},
  author = {Yusuke Mikura and Yuichiro Tada and Shuichiro Yokoyama},
  journal= {arXiv preprint arXiv:2008.00628},
  year   = {2021}
}

Comments

6 pages, v2: published version, EPL Editor's Choice, v3: references added