The drift rate of repeating FRBs implies an emission region size of a few times 10^8 cm, consistent with neutron star magnetospheres, under the radius-to-frequency mapping hypothesis.
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Frequency drifts in FRBs due to radius-to-frequency mapping in magnetospheres of neutron stars
The drift rate of repeating FRBs implies an emission region size of a few times 10^8 cm, consistent with neutron star magnetospheres, under the radius-to-frequency mapping hypothesis.