Starting from a Tayler-Spruit dynamo-generated field, simulations yield a weak surface dipole, strong small-scale crustal fields, and crust failures that match low-field magnetar observations.
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From proto-neutron star dynamo to low-field magnetars
Starting from a Tayler-Spruit dynamo-generated field, simulations yield a weak surface dipole, strong small-scale crustal fields, and crust failures that match low-field magnetar observations.