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Conformal inflation in the metric-affine geometry

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arxiv 2008.00628 v3 pith:DTKFM5L3 submitted 2020-08-03 hep-th astro-ph.COgr-qchep-ph

Conformal inflation in the metric-affine geometry

classification hep-th astro-ph.COgr-qchep-ph
keywords geometryconformalmetric-affinelocalsymmetrybrokenconnectionglobal
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 $\mathrm{SO}(1,1)$ or $\mathrm{O}(2)$, leading to the well-known $\alpha$-attractor or natural inflation, respectively. The inflaton can be understood as their pseudo Nambu-Goldstone boson.

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