Continuous ablation during engulfment dissolves Jupiter-like planets completely inside stellar convective envelopes, enabling observable lithium enrichment.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
Fully kinetic simulations show collisionless Kelvin-Helmholtz instability produces localized plasma mixing mediated by vortex advection and reconnection, with ions mixing more effectively than electrons.
citing papers explorer
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Continuous mass ablation of planets engulfed in stellar envelopes
Continuous ablation during engulfment dissolves Jupiter-like planets completely inside stellar convective envelopes, enabling observable lithium enrichment.
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The azimuthal structure of magnetically arrested disks during flux eruption events
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
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Plasma Mixing Driven by the Collisionless Kelvin-Helmholtz Instability: Insights from fully kinetic simulation and density-based diagnostics
Fully kinetic simulations show collisionless Kelvin-Helmholtz instability produces localized plasma mixing mediated by vortex advection and reconnection, with ions mixing more effectively than electrons.