pith:7E6EUUIM
How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
Dust traps in protoplanetary discs are leakier than earlier models assumed, so most outer traps sustain oxygen-rich inner discs with gas-phase C/O below 1.
arxiv:2604.11925 v1 · 2026-04-13 · astro-ph.EP
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Claims
dust traps are leakier than previously thought, on a broader parameter space, such that most outer traps (r > 5 au) will result in a long-lived O-rich inner disc with gas-phase C/O < 1
The 1D DustPy model with its coagulation/fragmentation prescriptions and chosen parameter ranges accurately represents real 3D disc physics and that planetesimal formation efficiency can be treated as an independent input.
Broad parameter study with detailed dust evolution code finds most outer dust traps leaky, producing long-lived O-rich inner discs with C/O < 1, while planetesimal formation is needed for strong blocking.
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| First computed | 2026-06-03T14:05:24.495045Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/7E6EUUIMM7DFMMUZ5EBQUHFNVY \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
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Canonical record JSON
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