Observational analysis reveals how the chiral magnetic effect shapes magnetar fields in neutron stars, suggesting new dynamics in magnetic energy redistribution.
The chiral magnetic effect (CME)—a macroscopic manifestation of the quantum chiral anomaly—induces currents along magnetic field lines, facilitating mutual conversion between chiral asymmetry and magnetic helicity. Although the finite electron mass suppresses chiral asymmetry through spin-flip processes, we demonstrate that the CME effectively shapes magnetar field evolution. Magnetic helicity acts as a persistent internal source of chiral asymmetry, which mediates the redistribution of magnetic energy across spatial scales, without requiring an external energy source. Our three-dimensional magnetothermal simulations of the neutron star crust reveal a mechanism that significantly reconfigures the magnetic field inherited at birth, amplifying both toroidal and poloidal large-scale dipolar components (crucial for spin-down) to strengths of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML"><a:mrow><a:mo>></a:mo><a:msup><a:mn>10</a:mn><a:mn>14</a:mn></a:msup></a:mrow></a:math> G within just a century, at the expense of small-scale structures. This astrophysical application of the CME, distinct and complementary to conventional hydrodynamic dynamo models, offers an innovative framework for understanding magnetar field dynamics and provides a transformative solution to the origin of their exceptionally strong, large-scale fields.
No takes yet. Share an insight, caveat, or question.
Dehman et al. (2025) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: