Magnetic reconnection in neutron stars drives transient axion bursts by exciting mixed Alfvén-axion modes in a non-ideal axion MHD framework.
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PIC simulations show E·B ≠ 0 regions reduce magnetic helicity in sub-ion turbulence, and a new history-dependent helicity density produces time-independent intermediate-scale plateaus consistent with cancellation-dominated 2D decay.
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Axion magnetohydrodynamics and reconnection-driven axion bursts
Magnetic reconnection in neutron stars drives transient axion bursts by exciting mixed Alfvén-axion modes in a non-ideal axion MHD framework.
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Kinetic Route to Helicity-Constrained Decay
PIC simulations show E·B ≠ 0 regions reduce magnetic helicity in sub-ion turbulence, and a new history-dependent helicity density produces time-independent intermediate-scale plateaus consistent with cancellation-dominated 2D decay.