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Curvaton with Polynomial Potential

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arxiv 0808.1793 v2 pith:HLPYQ4EI submitted 2008-08-13 hep-th astro-phgr-qchep-ph

classification hep-thastro-phgr-qchep-ph
keywords curvatonpotentialfieldpolynomialcalculatecurvaturedeltadominated
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abstract

In general a weakly self-interacting curvaton field is expected and the curvaton potential takes the polynomial form. The curvaton potential can be dominated by the self-interaction term during the period of inflation if the curvaton field stays at a large vacuum expectation value. We use the $\delta {\cal N}$ formalism to calculate the primordial curvature perturbation in the various possible scenarios which make the curvaton model much richer.

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Cited by 1 Pith paper

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    astro-ph.CO 2025-01 conditional novelty 6.0 of 10

    Soliton isocurvature perturbations produce gravitational waves whose sky anisotropies are enhanced by non-Gaussianity, offering a new probe of the early universe.

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