REVIEW
Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization
classification
astro-ph.CO
keywords
fieldsmagneticamplificationdynamofirstgalaxiesreionizationaddition
read the original abstract
We discuss the amplification of magnetic fields by the small-scale dynamo, a process that could efficiently produce strong magnetic fields in the first galaxies. In addition, we derive constraints on the primordial field strength from the epoch of reionization.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.