A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Including the disk buildup phase in protoplanetary disk models produces stronger CO ice enhancement over water in the outer disk but does not yield CO-rich planetesimals without extra mechanisms like pressure traps.
citing papers explorer
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A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks
A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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Dust evolution during protoplanetary disk buildup enhances CO ice relative to water
Including the disk buildup phase in protoplanetary disk models produces stronger CO ice enhancement over water in the outer disk but does not yield CO-rich planetesimals without extra mechanisms like pressure traps.