A new explicit symmetric splitting scheme for charged-particle dynamics achieves uniform second-order error bounds for position and parallel velocity in strong magnetic fields with maximal ordering.
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Synchrotron cooling produces an energy-dependent loss cone and a cooled-loss-cone plasma distribution in neutron star outer magnetospheres, with losses localized at a few hundred to a thousand stellar radii.
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Improved error estimates of a new splitting scheme for charged-particle dynamics in strong magnetic field with maximal ordering
A new explicit symmetric splitting scheme for charged-particle dynamics achieves uniform second-order error bounds for position and parallel velocity in strong magnetic fields with maximal ordering.
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Synchrotron-cooled plasma distribution in the outer magnetosphere of a neutron star
Synchrotron cooling produces an energy-dependent loss cone and a cooled-loss-cone plasma distribution in neutron star outer magnetospheres, with losses localized at a few hundred to a thousand stellar radii.