Chiral dynamos grow too slowly and are suppressed by flipping when chirality is pumped gradually, rendering them inefficient in protoneutron stars and barely viable near the electroweak transition.
Woltjer, A theorem on force free magnetic fields, PNAS44, 489 (1958)
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Inefficiency of chiral dynamos in protoneutron stars and the early universe
Chiral dynamos grow too slowly and are suppressed by flipping when chirality is pumped gradually, rendering them inefficient in protoneutron stars and barely viable near the electroweak transition.