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.
Seismicity on Tidally Active Solid-Surface Worlds
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abstract
Tidal interactions between planets or stars and the bodies that orbit them dissipate energy in their interiors. The energy dissipated drives internal heating and a fraction of that energy will be released as seismic energy. Here we formalize a model to describe the tidally-driven seismic activity on planetary bodies based on tidal dissipation.
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astro-ph.EP 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
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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.