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Numerical stochastic inflation constrained by frozen noise

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Numerical stochastic inflation constrained by frozen noise. / Tomberg, Eemeli.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2023, No. 4, 042, 14.04.2023.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Tomberg, E 2023, 'Numerical stochastic inflation constrained by frozen noise', Journal of Cosmology and Astroparticle Physics, vol. 2023, no. 4, 042. https://doi.org/10.1088/1475-7516/2023/04/042

APA

Tomberg, E. (2023). Numerical stochastic inflation constrained by frozen noise. Journal of Cosmology and Astroparticle Physics, 2023(4), Article 042. https://doi.org/10.1088/1475-7516/2023/04/042

Vancouver

Tomberg E. Numerical stochastic inflation constrained by frozen noise. Journal of Cosmology and Astroparticle Physics. 2023 Apr 14;2023(4):042. doi: 10.1088/1475-7516/2023/04/042

Author

Tomberg, Eemeli. / Numerical stochastic inflation constrained by frozen noise. In: Journal of Cosmology and Astroparticle Physics. 2023 ; Vol. 2023, No. 4.

Bibtex

@article{73f334feaa414bc39ad5f29dc7c42306,
title = "Numerical stochastic inflation constrained by frozen noise",
abstract = "Stochastic inflation can resolve strong inflationary perturbations, which seed primordial black holes. I present a fast and accurate way to compute these perturbations in typical black hole producing single-field models, treating the short-wavelength Fourier modes beyond the de Sitter approximation. The squeezing and freezing of the modes reduces the problem to one dimension, and the resulting new form of the stochastic equations, dubbed 'constrained stochastic inflation,' can be solved efficiently with semi-analytical techniques and numerical importance sampling. In an example case, the perturbation distribution is resolved in seconds deep into its non-Gaussian tail, a speed-up of factor 109 compared to a previous study. Along the way, I comment on the role of the momentum constraint in stochastic inflation.",
keywords = "cosmological perturbation theory, inflation, primordial black holes, quantum field theory on curved space",
author = "Eemeli Tomberg",
note = "Publisher Copyright: {\textcopyright} 2023 IOP Publishing Ltd and Sissa Medialab.",
year = "2023",
month = apr,
day = "14",
doi = "10.1088/1475-7516/2023/04/042",
language = "English",
volume = "2023",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "4",

}

RIS

TY - JOUR

T1 - Numerical stochastic inflation constrained by frozen noise

AU - Tomberg, Eemeli

N1 - Publisher Copyright: © 2023 IOP Publishing Ltd and Sissa Medialab.

PY - 2023/4/14

Y1 - 2023/4/14

N2 - Stochastic inflation can resolve strong inflationary perturbations, which seed primordial black holes. I present a fast and accurate way to compute these perturbations in typical black hole producing single-field models, treating the short-wavelength Fourier modes beyond the de Sitter approximation. The squeezing and freezing of the modes reduces the problem to one dimension, and the resulting new form of the stochastic equations, dubbed 'constrained stochastic inflation,' can be solved efficiently with semi-analytical techniques and numerical importance sampling. In an example case, the perturbation distribution is resolved in seconds deep into its non-Gaussian tail, a speed-up of factor 109 compared to a previous study. Along the way, I comment on the role of the momentum constraint in stochastic inflation.

AB - Stochastic inflation can resolve strong inflationary perturbations, which seed primordial black holes. I present a fast and accurate way to compute these perturbations in typical black hole producing single-field models, treating the short-wavelength Fourier modes beyond the de Sitter approximation. The squeezing and freezing of the modes reduces the problem to one dimension, and the resulting new form of the stochastic equations, dubbed 'constrained stochastic inflation,' can be solved efficiently with semi-analytical techniques and numerical importance sampling. In an example case, the perturbation distribution is resolved in seconds deep into its non-Gaussian tail, a speed-up of factor 109 compared to a previous study. Along the way, I comment on the role of the momentum constraint in stochastic inflation.

KW - cosmological perturbation theory

KW - inflation

KW - primordial black holes

KW - quantum field theory on curved space

U2 - 10.1088/1475-7516/2023/04/042

DO - 10.1088/1475-7516/2023/04/042

M3 - Journal article

AN - SCOPUS:85153187725

VL - 2023

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 4

M1 - 042

ER -