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Record W4394005948 · doi:10.1103/physrevd.109.103536

Magnetic fields from small-scale primordial perturbations

2024· preprint· en· W4394005948 on OpenAlexfundno aff
Nanoom Lee, Yacine Ali-Haïmoud

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2024
Typepreprint
Languageen
FieldBiochemistry, Genetics and Molecular Biology
TopicGeomagnetism and Paleomagnetism Studies
Canadian institutionsnot available
FundersYork UniversityCanadian Institute for Advanced ResearchNew York University
KeywordsScale (ratio)PhysicsGeophysicsTheoretical physicsAstrophysicsQuantum mechanics

Abstract

fetched live from OpenAlex

Weak magnetic fields must have existed in the early Universe, as they were sourced by the cross product of electron density and temperature gradients through the Biermann-battery mechanism. In this paper we calculate the magnetic fields generated at cosmic dawn by a variety of small-scale primordial perturbations, carefully computing the evolution of electron density and temperature fluctuations, and consistently accounting for relative velocities between baryons and dark matter. We first compute the magnetic field resulting from standard, nearly scale-invariant primordial adiabatic perturbations, making significant improvements to previous calculations. This ``standard'' primordial field has a root mean square (rms) of a few times ${10}^{\ensuremath{-}15}\text{ }\text{ }\mathrm{nG}$ at $20\ensuremath{\lesssim}z\ensuremath{\lesssim}100$, with fluctuations on $\ensuremath{\sim}\mathrm{kpc}$ comoving scales, and could serve as the seed of present-day magnetic fields observed in galaxies and galaxy clusters. In addition, we consider early Universe magnetic fields as a possible probe of nonstandard initial conditions of the Universe on small scales $k\ensuremath{\sim}1\ensuremath{-}{10}^{3}\text{ }\text{ }{\mathrm{Mpc}}^{\ensuremath{-}1}$. To this end, we compute the maximally allowed magnetic fields within current upper limits on small-scale adiabatic and isocurvature perturbations. Enhanced small-scale adiabatic fluctuations below current cosmic microwave background spectral-distortion constraints could produce magnetic fields as large as $\ensuremath{\sim}5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}11}\text{ }\text{ }\mathrm{nG}$ at $z=20$. Uncorrelated small-scale isocurvature perturbations within current big bang nucleosynthesis bounds could potentially enhance the rms magnetic field to $\ensuremath{\sim}{10}^{\ensuremath{-}14}\ensuremath{-}{10}^{\ensuremath{-}10}\text{ }\text{ }\mathrm{nG}$ at $z=20$, depending on the specific isocurvature mode considered. While these very weak fields remain well below current observational capabilities, our work points out that magnetic fields could potentially provide an interesting window into the poorly constrained small-scale initial conditions of the Universe.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.014
GPT teacher head0.360
Teacher spread0.346 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations1
Published2024
Admission routes1
Has abstractyes

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