Numerically modeling stochastic inflation in slow-roll and beyond
Abstract
In this work, we present a complete numerical treatment of inflationary dynamics under the influence of stochastic corrections from sub-Hubble modes. We discuss how to exactly model the stochastic noise terms arising from the sub-Hubble quantum modes that give rise to the coarse-grained inflaton dynamics in the form of stochastic differential equations. The stochastic differential equations are solved event by event on a discrete time grid. We then compute the power spectrum of curvature perturbations that can be compared with the power spectrum computed in the traditional fashion using the Mukhanov-Sasaki equation by canonically quantizing the inflaton fluctuations. Our numerical procedure helps us to easily extend the formalism to ultra slow-roll inflation and study the possibility of primordial black hole formation.
- Authors:
-
- Univ. of Minnesota, Minneapolis, MN (United States)
- Publication Date:
- Research Org.:
- Univ. of Minnesota, Minneapolis, MN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1849955
- Grant/Contract Number:
- FG02-87ER40328
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 102; Journal Issue: 12; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Evolution of the universe; Inflation
Citation Formats
De, Aritra, and Mahbub, Rafid. Numerically modeling stochastic inflation in slow-roll and beyond. United States: N. p., 2020.
Web. doi:10.1103/physrevd.102.123509.
De, Aritra, & Mahbub, Rafid. Numerically modeling stochastic inflation in slow-roll and beyond. United States. https://doi.org/10.1103/physrevd.102.123509
De, Aritra, and Mahbub, Rafid. Tue .
"Numerically modeling stochastic inflation in slow-roll and beyond". United States. https://doi.org/10.1103/physrevd.102.123509. https://www.osti.gov/servlets/purl/1849955.
@article{osti_1849955,
title = {Numerically modeling stochastic inflation in slow-roll and beyond},
author = {De, Aritra and Mahbub, Rafid},
abstractNote = {In this work, we present a complete numerical treatment of inflationary dynamics under the influence of stochastic corrections from sub-Hubble modes. We discuss how to exactly model the stochastic noise terms arising from the sub-Hubble quantum modes that give rise to the coarse-grained inflaton dynamics in the form of stochastic differential equations. The stochastic differential equations are solved event by event on a discrete time grid. We then compute the power spectrum of curvature perturbations that can be compared with the power spectrum computed in the traditional fashion using the Mukhanov-Sasaki equation by canonically quantizing the inflaton fluctuations. Our numerical procedure helps us to easily extend the formalism to ultra slow-roll inflation and study the possibility of primordial black hole formation.},
doi = {10.1103/physrevd.102.123509},
journal = {Physical Review. D.},
number = 12,
volume = 102,
place = {United States},
year = {Tue Dec 01 00:00:00 EST 2020},
month = {Tue Dec 01 00:00:00 EST 2020}
}
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