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Tachyonic Preheating in Plateau Inflation

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arxiv 2108.10767 v2 pith:KBKPXM4H submitted 2021-08-24 astro-ph.CO gr-qchep-phhep-th

classification astro-ph.COgr-qchep-phhep-th
keywords plateauinflationtachyonicpreheatinganalyticinflatonperturbationsanalysis
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Plateau inflation is an experimentally consistent framework in which the scale of inflation can be kept relatively low. Close to the edge of the plateau, scalar perturbations are subject to a strong tachyonic instability. Tachyonic preheating is realized when, after inflation, the oscillating inflaton repeatedly re-enters the plateau. We develop the analytic theory of this process and expand the linear approach by including backreaction between the coherent background and growing perturbations. For a family of plateau models, the analytic predictions are confronted with numerical estimates. Our analysis shows that the inflaton fragments in a fraction of an $e$-fold in all examples supporting tachyonic preheating, generalizing the results of previous similar studies. In these scenarios, the scalar-to-tensor ratio is tiny, $r<10^{-7}$.

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Cited by 2 Pith papers

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

  1. Two-Measure Electroweak Standard Model. Some aspects of cosmological evolution and vacuum stability

    hep-th 2025-01 reject novelty 5.0 of 10

    The paper derives a two-measure version of the electroweak Standard Model in which couplings run classically with the cosmological background, giving small-xi Higgs inflation and a reparameterized fermion mass hierarchy.

  2. Pure Natural Inflation Passes the ACT

    astro-ph.CO 2026-03 unverdicted novelty 4.0 of 10

    Pure natural inflation remains viable against latest ACT+DESI constraints, with a non-trivial fraction of parameter space allowed under standard reheating scenarios.

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