Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe

We propose a novel dust battery mechanism for generating seed magnetic fields in the early Universe, in which charged dust grains are radiatively accelerated, inducing strong electric currents that subsequently generate magnetic fields. Our analysis demonstrates that this process is effective even a...

Full description

Saved in:
Bibliographic Details
Main Authors: Nadine H. Soliman, Philip F. Hopkins, Jonathan Squire
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adcb39
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1849322153573351424
author Nadine H. Soliman
Philip F. Hopkins
Jonathan Squire
author_facet Nadine H. Soliman
Philip F. Hopkins
Jonathan Squire
author_sort Nadine H. Soliman
collection DOAJ
description We propose a novel dust battery mechanism for generating seed magnetic fields in the early Universe, in which charged dust grains are radiatively accelerated, inducing strong electric currents that subsequently generate magnetic fields. Our analysis demonstrates that this process is effective even at very low metallicities (approximately ∼10 ^−5 Z _⊙ ), and capable of producing seed fields with significant amplitudes of B ∼ μ G around luminous sources over timescales of years to Myr and across spatial scales ranging from au to kpc. Crucially, we find that this mechanism is generically ∼10 ^8 times more effective than the radiatively driven electron battery or Biermann battery in relatively cool gas (≪10 ^5 K), including both neutral and ionized gas. Furthermore, our results suggest that, to first order, dissipation effects do not appear to significantly impede this process, and that it can feasibly generate coherent seed fields on macroscopically large interstellar medium (ISM) scales (much larger than turbulent dissipation scales or electron mean-free-paths in the ISM). These seed fields could then be amplified by subsequent dynamo actions to the observed magnetic fields in galaxies. Additionally, we propose a subgrid model for integration into cosmological simulations, and the required electric-field expressions for magnetohydrodynamic-particle-in-a-cell simulations that explicitly model dust dynamics. Finally, we explore the broad applicability of this mechanism across different scales and conditions, emphasizing its robustness compared to other known battery mechanisms.
format Article
id doaj-art-7879c661e5fa463e845c53bfdf7f3f7c
institution Kabale University
issn 1538-4357
language English
publishDate 2025-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal
spelling doaj-art-7879c661e5fa463e845c53bfdf7f3f7c2025-08-20T03:49:31ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198515510.3847/1538-4357/adcb39Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early UniverseNadine H. Soliman0https://orcid.org/0000-0002-6810-1110Philip F. Hopkins1https://orcid.org/0000-0003-3729-1684Jonathan Squire2https://orcid.org/0000-0001-8479-962XTAPIR, Mailcode 350-17, California Institute of Technology , Pasadena, CA 91125, USA ; nsoliman@caltech.eduTAPIR, Mailcode 350-17, California Institute of Technology , Pasadena, CA 91125, USA ; nsoliman@caltech.eduPhysics Department, University of Otago , 730 Cumberland Street, Dunedin 9016, New ZealandWe propose a novel dust battery mechanism for generating seed magnetic fields in the early Universe, in which charged dust grains are radiatively accelerated, inducing strong electric currents that subsequently generate magnetic fields. Our analysis demonstrates that this process is effective even at very low metallicities (approximately ∼10 ^−5 Z _⊙ ), and capable of producing seed fields with significant amplitudes of B ∼ μ G around luminous sources over timescales of years to Myr and across spatial scales ranging from au to kpc. Crucially, we find that this mechanism is generically ∼10 ^8 times more effective than the radiatively driven electron battery or Biermann battery in relatively cool gas (≪10 ^5 K), including both neutral and ionized gas. Furthermore, our results suggest that, to first order, dissipation effects do not appear to significantly impede this process, and that it can feasibly generate coherent seed fields on macroscopically large interstellar medium (ISM) scales (much larger than turbulent dissipation scales or electron mean-free-paths in the ISM). These seed fields could then be amplified by subsequent dynamo actions to the observed magnetic fields in galaxies. Additionally, we propose a subgrid model for integration into cosmological simulations, and the required electric-field expressions for magnetohydrodynamic-particle-in-a-cell simulations that explicitly model dust dynamics. Finally, we explore the broad applicability of this mechanism across different scales and conditions, emphasizing its robustness compared to other known battery mechanisms.https://doi.org/10.3847/1538-4357/adcb39CosmologyGalaxy formationCosmic magnetic fields theoryMagnetic fieldsAstrophysical dust processesComputational methods
spellingShingle Nadine H. Soliman
Philip F. Hopkins
Jonathan Squire
Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
The Astrophysical Journal
Cosmology
Galaxy formation
Cosmic magnetic fields theory
Magnetic fields
Astrophysical dust processes
Computational methods
title Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
title_full Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
title_fullStr Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
title_full_unstemmed Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
title_short Dust Battery: A Novel Mechanism for Seed Magnetic Field Generation in the Early Universe
title_sort dust battery a novel mechanism for seed magnetic field generation in the early universe
topic Cosmology
Galaxy formation
Cosmic magnetic fields theory
Magnetic fields
Astrophysical dust processes
Computational methods
url https://doi.org/10.3847/1538-4357/adcb39
work_keys_str_mv AT nadinehsoliman dustbatteryanovelmechanismforseedmagneticfieldgenerationintheearlyuniverse
AT philipfhopkins dustbatteryanovelmechanismforseedmagneticfieldgenerationintheearlyuniverse
AT jonathansquire dustbatteryanovelmechanismforseedmagneticfieldgenerationintheearlyuniverse