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CMB targets after the latest Planck data release
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CMB targets after the latest Planck data release
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We show that a combination of the simplest $\alpha$-attractors and KKLTI models related to Dp-brane inflation covers most of the area in the ($n_{s}$, $r$) space favored by Planck 2018. For $\alpha$-attractor models, there are discrete targets $3\alpha=1,2,...,7$, predicting 7 different values of $r = 12\alpha/N^{2}$ in the range $10^{-2} \gtrsim r \gtrsim 10^{-3}$. In the small $r$ limit, $\alpha$-attractors and Dp-brane inflation models describe vertical $\beta$-stripes in the ($n_{s}$, $r$) space, with $n_{s}=1-\beta/N$, $\beta=2, {5\over 3},{8\over 5}, {3\over 2},{4\over 3}$. A phenomenological description of these models and their generalizations can be achieved in the context of pole inflation. Most of the $1\sigma$ area in the ($n_{s}$, $r$) space favored by Planck 2018 can be covered models with $\beta = 2$ and $\beta = 5/3$. Future precision data on $n_s$ may help to discriminate between these models even if the precision of the measurement of $r$ is insufficient for the discovery of gravitational waves produced during inflation.
Forward citations
Cited by 5 Pith papers
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New Exponential and Polynomial $\xi$-attractors
New family of ξ-attractors yields ns in the interval 1-2/N ≤ ns < 1-1/N with r approaching zero as ξ grows large, plus a supergravity embedding.
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Jordan Frame in Supergravity and Cosmology
New supergravity ξ-attractors built by choosing the Kähler potential first match exponential and polynomial α-attractors with ξ=1/(6α), and Palatini-style supergravity with scalars is shown inconsistent with superconf...
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Jordan Frame in Supergravity and Cosmology
The paper introduces new exponential and polynomial supergravity ξ-attractor models in the Jordan frame with non-minimal coupling and shows that Palatini gravity with independent affine connection has no supergravity ...
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New Exponential and Polynomial $\xi$-attractors
New ξ-attractors with non-minimal coupling and non-canonical kinetics yield Einstein-frame exponential and polynomial potentials whose ns spans 1-2/N to 1-1/N and r can reach zero as ξ grows, fitting Planck, BICEP/Kec...
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Unification of polynomial and exponential cosmological attractors
Embedding polynomial attractor potentials within α-attractor geometry yields a unified model class that interpolates between exponential and polynomial inflationary predictions via a single parameter μ.
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