3D evolution of neutron star magnetic fields from a realistic core-collapse turbulent topology

Published in MNRAS 523, 5198, 2023

Recommended citation: C. Dehman, D. Viganò, S. Ascenzi, J.A. Pons & N. Rea (2023). 3D evolution of neutron star magnetic fields from a realistic core-collapse turbulent topology. MNRAS 523, 5198. (arXiv, ADS, DOI)
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