pith:AZDAAAMJ
The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
High-eccentricity tidal migration explains the Neptunian ridge as a natural clustering of survivors beyond the tidal disruption limit.
arxiv:2604.16300 v3 · 2026-04-17 · astro-ph.EP
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Claims
High-eccentricity tidal migration thus provides a self-consistent explanation for the ridge and desert boundary geometry.
That a single representative tidal encounter parameter can be chosen to set the overall period offset across the sub-Neptune to super-Neptune regime while the slope is independently reproduced by the survival formalism.
High-eccentricity tidal migration reproduces the Neptunian desert boundary slope and produces the ridge overdensity through density-dependent survival and clustering just beyond the disruption limit.
References
Receipt and verification
| First computed | 2026-05-20T14:03:26.930834Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
06460001892c65fbda2b59caa426904093f9e490717619993dd5d9bc2a9b4e61
Aliases
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/AZDAAAMJFRS7XWRLLHFKIJUQIC \
| 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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