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A numerical approach to stochastic inflation and primordial black holes

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A numerical approach to stochastic inflation and primordial black holes. / Tomberg, Eemeli.
In: Journal of Physics: Conference Series, Vol. 2156, No. 1, 012010, 21.02.2022.

Research output: Contribution to Journal/Magazine › Conference article › peer-review

Harvard

Tomberg, E 2022, 'A numerical approach to stochastic inflation and primordial black holes', Journal of Physics: Conference Series, vol. 2156, no. 1, 012010. https://doi.org/10.1088/1742-6596/2156/1/012010

APA

Tomberg, E. (2022). A numerical approach to stochastic inflation and primordial black holes. Journal of Physics: Conference Series, 2156(1), Article 012010. https://doi.org/10.1088/1742-6596/2156/1/012010

Vancouver

Tomberg E. A numerical approach to stochastic inflation and primordial black holes. Journal of Physics: Conference Series. 2022 Feb 21;2156(1):012010. doi: 10.1088/1742-6596/2156/1/012010

Author

Tomberg, Eemeli. / A numerical approach to stochastic inflation and primordial black holes. In: Journal of Physics: Conference Series. 2022 ; Vol. 2156, No. 1.

Bibtex

@article{071bfec0f6b945b9a7ba5ba6d3ceed63,
title = "A numerical approach to stochastic inflation and primordial black holes",
abstract = "Certain models of cosmic inflation produce strong cosmological perturbations at short length scales, which may later collapse into primordial black holes. To find the statistics of these strong perturbations and the ensuing black holes, it is necessary to go beyond linear perturbation theory. Stochastic inflation provides a way to take the leading non-linear effects into account. In this contribution, I discuss recent progress in numerical computations of stochastic inflation. A numerical approach can include more of the non-linearities than an analytical calculation, and can be applied to single-field inflationary models with any potential.",
author = "Eemeli Tomberg",
note = "Funding Information: This work was supported by the Estonian Research Council grants PRG803, PRG1055, and MOBTT5 and by the EU through the European Regional Development Fund CoE program TK133 “The Dark Side of the Universe”. The work in [3] was done in collaboration with Daniel Figueroa, Sami Raatikainen, and Syksy R{\"a}s{\"a}nen. Publisher Copyright: {\textcopyright} 2022 Institute of Physics Publishing. All rights reserved.; 17th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2021 ; Conference date: 26-08-2021 Through 03-09-2021",
year = "2022",
month = feb,
day = "21",
doi = "10.1088/1742-6596/2156/1/012010",
language = "English",
volume = "2156",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - A numerical approach to stochastic inflation and primordial black holes

AU - Tomberg, Eemeli

N1 - Funding Information: This work was supported by the Estonian Research Council grants PRG803, PRG1055, and MOBTT5 and by the EU through the European Regional Development Fund CoE program TK133 “The Dark Side of the Universe”. The work in [3] was done in collaboration with Daniel Figueroa, Sami Raatikainen, and Syksy Räsänen. Publisher Copyright: © 2022 Institute of Physics Publishing. All rights reserved.

PY - 2022/2/21

Y1 - 2022/2/21

N2 - Certain models of cosmic inflation produce strong cosmological perturbations at short length scales, which may later collapse into primordial black holes. To find the statistics of these strong perturbations and the ensuing black holes, it is necessary to go beyond linear perturbation theory. Stochastic inflation provides a way to take the leading non-linear effects into account. In this contribution, I discuss recent progress in numerical computations of stochastic inflation. A numerical approach can include more of the non-linearities than an analytical calculation, and can be applied to single-field inflationary models with any potential.

AB - Certain models of cosmic inflation produce strong cosmological perturbations at short length scales, which may later collapse into primordial black holes. To find the statistics of these strong perturbations and the ensuing black holes, it is necessary to go beyond linear perturbation theory. Stochastic inflation provides a way to take the leading non-linear effects into account. In this contribution, I discuss recent progress in numerical computations of stochastic inflation. A numerical approach can include more of the non-linearities than an analytical calculation, and can be applied to single-field inflationary models with any potential.

U2 - 10.1088/1742-6596/2156/1/012010

DO - 10.1088/1742-6596/2156/1/012010

M3 - Conference article

AN - SCOPUS:85131873472

VL - 2156

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012010

T2 - 17th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2021

Y2 - 26 August 2021 through 3 September 2021

ER -