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Curvaton Reheating in Non-oscillatory Inflationary Models

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arxiv hep-ph/0212213 v2 pith:J5RLKDRL submitted 2002-12-15 hep-ph astro-ph

classification hep-phastro-ph
keywords mechanismmodelsreheatingcurvatoninflationarynon-oscillatoryconsidercurvature
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abstract

In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitational particle production or the mechanism of instant preheating. In this paper we introduce the curvaton mechanism into NO models to reheat the universe and generate the curvature perturbation. Specifically we consider the Peebles-Vilenkin quintessential inflation model, where the reheating temperature can be extended from 1MeV to $10^{13}$GeV.

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Cited by 3 Pith papers

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

  1. Post-Inflationary Constraints on Nonminimally Coupled Quintessential Inflation

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Gravitational-wave constraints on the reheating temperature rule out single-exponential nonminimally coupled quintessential inflation and require a double-exponential coupling that predicts thawing dark energy with w0...

  2. Dissipative Dark Energy can explain the DESI phantom crossing

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    Weakly dissipative quintessence explains DESI phantom crossing in dark energy without pathological dynamics.

  3. Flipped Rotating Axion Non-minimally Coupled to Gravity: Baryogenesis and Dark Matter

    hep-ph 2025-02 conditional novelty 4.0 of 10

    A rotating axion, kicked into motion by a sign flip in its gravitational effective potential during kination, can co-generate baryon asymmetry and dark matter in a Majoron seesaw model.

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