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Primordial turbulence from inflation: a new inflaton-driven turbulent regime
Abstract
For the first time, we establish a direct connection between inflationary dynamics and the subsequent magnetohydrodynamic evolution. Starting from vacuum fluctuations, we self-consistently evolve the coupled inflaton-plasma system through inflation, reheating, and into the radiation-dominated era. We find an inflaton-driven inverse cascade followed by freely decaying turbulence, with kinetic energy dominating over magnetic energy and driving dynamo amplification. The inflaton-driven turbulence causes steeper magnetic energy decay than helical turbulence and should therefore be accounted for subsequent evolution of primordial fields and their present-day observables.
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BibTeX
@misc{iarygina2026primordial,
title = {{Primordial turbulence from inflation: a new inflaton-driven turbulent regime}},
author = {Oksana Iarygina and Axel Brandenburg},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.10326},
eprint = {2609.10326},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.10326},
}
RIS
TY - UNPB
TI - Primordial turbulence from inflation: a new inflaton-driven turbulent regime
AU - Oksana Iarygina
AU - Axel Brandenburg
PY - 2026
DA - 2026/09/09
PB - arXiv
DO - 10.48550/arxiv.2609.10326
UR - https://arxiv.org/abs/2609.10326
AB - For the first time, we establish a direct connection between inflationary dynamics and the subsequent magnetohydrodynamic evolution. Starting from vacuum fluctuations, we self-consistently evolve the coupled inflaton-plasma system through inflation, reheating, and into the radiation-dominated era. We find an inflaton-driven inverse cascade followed by freely decaying turbulence, with kinetic energy dominating over magnetic energy and driving dynamo amplification. The inflaton-driven turbulence causes steeper magnetic energy decay than helical turbulence and should therefore be accounted for subsequent evolution of primordial fields and their present-day observables.
ER -