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Cited article:

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Dust Dynamics in Hall-effected Protoplanetary Disks. I. Background Drift Hall Instability

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Planetesimal gravitational collapse in a gaseous environment: Thermal and dynamic evolution

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A Solution for the Density Dichotomy Problem of Kuiper Belt Objects with Multispecies Streaming Instability and Pebble Accretion

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Thousands of planetesimals: Simulating the streaming instability in very large computational domains

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Compaction during fragmentation and bouncing produces realistic dust grain porosities in protoplanetary discs

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Observing Planetesimal Formation under Streaming Instability in the Rings of HD 163296

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Planetesimal Initial Mass Functions Following Diffusion-regulated Gravitational Collapse

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Planetesimal formation via the streaming instability with multiple grain sizes

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