Fully resolved Keplerian turbulence concentrates pebbles into clumps and reduces their radial drift, potentially bypassing the drift and fragmentation barriers to planetesimal formation at canonical dust-to-gas ratios.
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A unique solution to overcome the barriers to planetesimal formation at low dust-to-gas ratio
Fully resolved Keplerian turbulence concentrates pebbles into clumps and reduces their radial drift, potentially bypassing the drift and fragmentation barriers to planetesimal formation at canonical dust-to-gas ratios.