Multifield Dynamics in Higgs-otic Inflation
S. Bielleman, L.E. Ibanez, F.G. Pedro, I. Valenzuela

TL;DR
This paper analyzes the full two-field dynamics of Higgs-otic inflation, revealing that isocurvature perturbations are damped and the model's predictions align with current observational data.
Contribution
It provides a comprehensive analysis of adiabatic and isocurvature perturbations in Higgs-otic inflation, improving the understanding of its observational signatures.
Findings
Isocurvature perturbations are exponentially damped by the end of inflation.
Tensor-to-scalar ratio is in the range 0.08-0.12, consistent with Planck/BICEP.
Full two-field analysis increases the model's predictivity.
Abstract
In Higgs-otic inflation a complex neutral scalar combination of the and MSSM Higgs fields plays the role of inflaton in a chaotic fashion. The potential is protected from large trans-Planckian corrections at large inflaton if the system is embedded in string theory so that the Higgs fields parametrize a D-brane position. The inflaton potential is then given by a DBI+CS D-brane action yielding an approximate linear behaviour at large field. The inflaton scalar potential is a 2-field model with specific non-canonical kinetic terms. Previous computations of the cosmological parameters (i.e. scalar and tensor perturbations) did not take into account the full 2-field character of the model, ignoring in particular the presence of isocurvature perturbations and their coupling to the adiabatic modes. It is well known that for generic 2-field potentials such effects may significantly…
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