In the unscreened-field case, Schwinger pair creation supplies charges far exceeding the Goldreich-Julian rate and removes ~90% of rotational energy within 30 ms for B_p=10^14 G and P_0=1 ms, suppressing gravitational-wave losses and linking millisecond magnetars to the observed population.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
2026 2representative citing papers
A centered swept-back multipolar magnetic field up to octupole order reproduces the bolometric thermal X-ray light curve of MSP J0030+0451.
citing papers explorer
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Energy Loss of Newborn Magnetars by Schwinger Process
In the unscreened-field case, Schwinger pair creation supplies charges far exceeding the Goldreich-Julian rate and removes ~90% of rotational energy within 30 ms for B_p=10^14 G and P_0=1 ms, suppressing gravitational-wave losses and linking millisecond magnetars to the observed population.
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The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451
A centered swept-back multipolar magnetic field up to octupole order reproduces the bolometric thermal X-ray light curve of MSP J0030+0451.