9 research outputs found
Plateau Inflation from Random Non-Minimal Coupling
A generic non-minimal coupling can push any higher-order terms of the scalar
potential sufficiently far out in field space to yield observationally viable
plateau inflation. We provide analytic and numerical evidence that this
generically happens for a non-minimal coupling strength of the order
. In this regime, the non-minimally coupled field is sub-Planckian
during inflation and is thus protected from most higher-order terms. For larger
values of , the inflationary predictions converge towards the sweet spot
of PLANCK. The latter includes obtained from CMB normalization
arguments, thus providing a natural explanation for the inflationary
observables measured.Comment: 9 pages, twocolumn, some figures; v2: 1 figure and appendix added,
jcap layou
Pole Inflation - Shift Symmetry and Universal Corrections
An appealing explanation for the Planck data is provided by inflationary
models with a singular non-canonical kinetic term: a Laurent expansion of the
kinetic function translates into a potential with a nearly shift-symmetric
plateau in canonical fields. The shift symmetry can be broken at large field
values by including higher-order poles, which need to be hierarchically
suppressed in order not to spoil the inflationary plateau. The herefrom
resulting corrections to the inflationary dynamics and predictions are shown to
be universal at lowest order and possibly to induce power loss at large angular
scales. At lowest order there are no corrections from a pole of just one order
higher and we argue that this phenomenon is related to the well-known extended
no-scale structure arising in string theory scenarios. Finally, we outline
which other corrections may arise from string loop effects.Comment: twocolumn, 9 pages, 1 figure; v2: clarifications and refs added, JHEP
layout, 19 page
Starobinsky-Type Inflation from -Corrections
Working in the Large Volume Scenario (LVS) of IIB Calabi-Yau flux
compactifications, we construct inflationary models from recently computed
higher derivative -corrections. Inflation is driven by a Kaehler
modulus whose potential arises from the aforementioned corrections, while we
use the inclusion of string loop effects just to ensure the existence of a
graceful exit when necessary. The effective inflaton potential takes a
Starobinsky-type form , where we obtain one set-up
with and one with corresponding to inflation
occurring for increasing or decreasing respectively. The inflationary
observables are thus in perfect agreement with PLANCK, while the two scenarios
remain observationally distinguishable via slightly varying predictions for the
tensor-to-scalar ratio . Both set-ups yield . They hence realise inflation with moderately large fields
without saturating the Lyth
bound. Control over higher corrections relies in part on tuning underlying
microscopic parameters, and in part on intrinsic suppressions. The intrinsic
part of control arises as a leftover from an approximate effective shift
symmetry at parametrically large volume.Comment: 29 pages, 6 figures; v2: clarifications and refs adde
Power Spectrum of Inflationary Attractors
Inflationary attractors predict the spectral index and tensor-to-scalar ratio
to take specific values that are consistent with Planck. An example is the
universal attractor for models with a generalised non-minimal coupling, leading
to Starobinsky inflation. In this paper we demonstrate that it also predicts a
specific relation between the amplitude of the power spectrum and the number of
e-folds. The length and height of the inflationary plateau are related via the
non-minimal coupling: in a wide variety of examples, the observed power
normalisation leads to at least 55 flat e-foldings. Prior to this phase, the
inflationary predictions vary and can account for the observational indications
of power loss at large angular scales.Comment: 5 pages, 1 figure; v2: added refs; to appear in PR
Disentangling the - Duality
Motivated by UV realisations of Starobinsky-like inflation models, we study
generic exponential plateau-like potentials to understand whether an exact
-formulation may still be obtained when the asymptotic shift-symmetry of
the potential is broken for larger field values. Potentials which break the
shift symmetry with rising exponentials at large field values only allow for
corresponding -descriptions with a leading order term with
, regardless of whether the duality is exact or approximate. The
-term survives as part of a series expansion of the function and
thus cannot maintain a plateau for all field values. We further find a lean and
instructive way to obtain a function describing -inflation
which breaks the shift symmetry with a monomial, and corresponds to effectively
logarithmic corrections to an model. These examples emphasise that
higher order terms in -theory may not be neglected if they are present at
all. Additionally, we relate the function corresponding to chaotic
inflation to a more general Jordan frame set-up. In addition, we consider
-duals of two given UV examples, both from supergravity and string
theory. Finally, we outline the CMB phenomenology of these models which show
effects of power suppression at low-.Comment: 30 pages, 2 figures; v2: added refs, 1 figure, and minor
clarifications; to appear in JCA
The Power Spectrum of Inflationary Attractors
Inflationary attractors predict the spectral index and tensor-to-scalar ratio to take specific values that are consistent with Planck. An example is the universal attractor for models with a generalized nonminimal coupling, leading to Starobinsky inflation. In this paper we demonstrate that it also predicts a specific relation between the amplitude of the power spectrum and the number of -folds. The length and height of the inflationary plateau are related via the nonminimal coupling: in a wide variety of examples, the observed power normalization leads to at least 55 flat -foldings. Prior to this phase, the inflationary predictions vary and can account for the observational indications of power loss at large angular scales