Coupled Lorentz-tide simulations show cores with dynamic viscosity above ~10^24 Pa s can survive over 1 Gyr in kilogauss magnetic fields around white dwarfs.
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Survivability of radio-loud planetary cores orbiting white dwarfs
Coupled Lorentz-tide simulations show cores with dynamic viscosity above ~10^24 Pa s can survive over 1 Gyr in kilogauss magnetic fields around white dwarfs.