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Tachyonic preheating in plateau inflation

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Tachyonic preheating in plateau inflation. / Tomberg, Eemeli; Veermae, Hardi.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2021, No. 12, 035, 16.12.2021.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Tomberg, E & Veermae, H 2021, 'Tachyonic preheating in plateau inflation', Journal of Cosmology and Astroparticle Physics, vol. 2021, no. 12, 035. https://doi.org/10.1088/1475-7516/2021/12/035

APA

Tomberg, E., & Veermae, H. (2021). Tachyonic preheating in plateau inflation. Journal of Cosmology and Astroparticle Physics, 2021(12), Article 035. https://doi.org/10.1088/1475-7516/2021/12/035

Vancouver

Tomberg E, Veermae H. Tachyonic preheating in plateau inflation. Journal of Cosmology and Astroparticle Physics. 2021 Dec 16;2021(12):035. doi: 10.1088/1475-7516/2021/12/035

Author

Tomberg, Eemeli ; Veermae, Hardi. / Tachyonic preheating in plateau inflation. In: Journal of Cosmology and Astroparticle Physics. 2021 ; Vol. 2021, No. 12.

Bibtex

@article{7fbd07b83816481094d31f19a406f696,
title = "Tachyonic preheating in plateau inflation",
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.",
keywords = "cosmological perturbation theory, inflation, quantum field theory on curved space",
author = "Eemeli Tomberg and Hardi Veermae",
year = "2021",
month = dec,
day = "16",
doi = "10.1088/1475-7516/2021/12/035",
language = "English",
volume = "2021",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "12",

}

RIS

TY - JOUR

T1 - Tachyonic preheating in plateau inflation

AU - Tomberg, Eemeli

AU - Veermae, Hardi

PY - 2021/12/16

Y1 - 2021/12/16

N2 - 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.

AB - 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.

KW - cosmological perturbation theory

KW - inflation

KW - quantum field theory on curved space

U2 - 10.1088/1475-7516/2021/12/035

DO - 10.1088/1475-7516/2021/12/035

M3 - Journal article

AN - SCOPUS:85122859506

VL - 2021

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 12

M1 - 035

ER -