Inflationary quasi-scale invariant attractors
arXiv:1505.03386 · doi:10.1103/PhysRevD.93.024040
Abstract
In a series of recent papers Kallosh, Linde, and collaborators have provided a unified description of single-field inflation with several types of potentials, ranging from power law to supergravity, in terms of just one parameter . These so-called -attractors predict a spectral index and a tensor-to-scalar ratio , which are fully compatible with the latest Planck data. The only common feature of all -attractors is a non-canonical kinetic term with a pole, and a potential analytic around the pole. In this paper, starting from the same Einstein frame with a non-canonical scalar kinetic energy, we explore the case of non-analytic potentials. We find the functional form that corresponds to quasi-scale invariant gravitational models in the Jordan frame, characterised by a universal relation between and that fits the observational data but is clearly distinct from the one of the -attractors. It is known that the breaking of the exact classical scale-invariance in the Jordan frame can be attributed to one-loop corrections. Therefore we conclude that there exists a class of non-analytic potentials in the non-canonical Einstein frame that are physically equivalent to a class of models in the Jordan frame, with scale-invariance softly broken by one-loop quantum corrections.
Version accepted for publication in Phys. Rev. D
References in corpus (17)
- The Standard Model Higgs boson as the inflaton
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- The Unity of Cosmological Attractors
- Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data
- Large Field Inflation and Double -Attractors
- Dynamically Induced Planck Scale and Inflation
- Planck, LHC, and -attractors
- Escher in the Sky
- Does the first chaotic inflation model in supergravity provide the best fit to the Planck data?
- Inflation in scale-invariant theories of gravity
- Reconstructing the inflationary from observations
- Dark Energy, Induced Gravity and Broken Scale Invariance
- Thermodynamics of topological black holes in gravity
- Disentangling the - Duality
- Inflationary cosmology from quantum Conformal Gravity
- Scale-invariant rotating black holes in quadratic gravity
- Inflation and Dark Energy with a Single Superfield
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- New universal attractor in nonmininally coupled gravity: Linear inflation
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- Quartic inflation and radiative corrections with non-minimal coupling
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