Hybrid cosmological attractors
Renata Kallosh, Andrei Linde

TL;DR
This paper develops hybrid inflation models with $ extit{ extbf{α}}$-attractor properties, showing how parameters influence spectral index predictions and providing flexible models adaptable to precise cosmological data.
Contribution
It introduces $ extit{ extbf{α}}$-attractor hybrid inflation models with adjustable predictions, applicable to a broad class of uplifted inflationary scenarios.
Findings
In the large $N$ limit, models reproduce universal $ extit{ extbf{α}}$-attractor predictions.
Adjusting parameters $V_{up}$ and $ extphi_c$ interpolates between different spectral index predictions.
Models offer flexibility to match evolving cosmological observational constraints.
Abstract
We construct -attractor versions of hybrid inflation models. In these models, the potential of the inflaton field is uplifted by the potential of the second field . This uplifting ends due to a tachyonic instability with respect to the field , which appears when becomes smaller than some critical value . In the large limit, these models have the standard universal -attractor predictions. In particular, for the exponential attractors. However, in some special cases the large limit is reached only beyond the horizon, for . This may change predictions for the cosmological observations. For any fixed , in the limit of large uplift , or in the limit of large , we find another attractor prediction, . By changing the parameters and…
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