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Hubble multi-scalar inflation

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arxiv 1606.05894 v1 pith:775FQ3LC submitted 2016-06-19 gr-qc

classification gr-qc
keywords inflationfieldhubblemodelscurvedderivativesderivedescribe
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abstract

Multiple field models of inflation exhibit new features than single field models. In this work, we study the hierarchy of parameters based on Hubble expansion rate in curved field space and derive the system of flow equations that describe their evolution. Then we focus on obtaining derivatives of number of $e$-folds with respect to scalar fields during inflation and at hypersurface of the end of inflation.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Canonical Scalar Field Inflation with a Woods-Saxon Potential

    gr-qc 2019-08 reject novelty 3.0 of 10

    A Woods-Saxon (logistic) scalar potential is claimed to produce Planck-compatible inflation and reheating, but the supporting slow-roll equations contain sign and algebra errors.

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