Coupled disc-chemistry and N-body simulations identify three classes of giant-planet atmospheres whose elemental ratios (N/O*, C/O*, C/N*, S/N*) trace gas-dominated, planetesimal-dominated, or drift-enhanced accretion in time-dependent discs.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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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Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres
Coupled disc-chemistry and N-body simulations identify three classes of giant-planet atmospheres whose elemental ratios (N/O*, C/O*, C/N*, S/N*) trace gas-dominated, planetesimal-dominated, or drift-enhanced accretion in time-dependent discs.
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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.