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Inflation in string theory: a graceful exit to the real world

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arxiv 1010.0941 v2 pith:RHMEDG5C submitted 2010-10-05 hep-th astro-ph.COhep-ph

Michele Cicoli , Anupam Mazumdar This is my paper · ORCID
classification hep-thastro-ph.COhep-ph
keywords inflationmodelsectorstandardstringanisotropybackgroundbang
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The most important criteria for a successful inflation are to explain the observed temperature anisotropy in the cosmic microwave background radiation, and exiting inflation in a vacuum where it can excite the Standard Model quarks and leptons required for the success of Big Bang Nucleosynthesis. In this paper we provide the first ever closed string model of inflation where the inflaton couplings to hidden sector, moduli sector, and visible sector fields can be computed, showing that inflation can lead to reheating the Standard Model degrees of freedom before the electro-weak scale.

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  1. Preheating Axions in String Cosmology

    hep-th 2024-11 conditional novelty 6.0 of 10

    Preheating of closed-string axions in fibre inflation can overproduce dark matter, yielding new upper bounds on the axion mass and constraints on model parameters.

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