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arxiv: 1406.5192 · v1 · pith:6PTCUVCFnew · submitted 2014-06-19 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph

Inflation from Broken Scale Invariance

classification ✦ hep-th astro-ph.COgr-qchep-ph
keywords scaleinvarianceinflatonlow-energybrokendisplacementseffectiveinflation
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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.

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