pith:SFQ6YZ7O
Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends
Sub-Neptune atmospheres produce peak amounts of soot-forming hydrocarbons around 600 K through deep-atmosphere quenching.
arxiv:2604.11919 v2 · 2026-04-13 · astro-ph.EP
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Claims
We find that the predicted abundances of PAHs peak near 600 K, and fall off toward higher and lower Teq, consistent with the observed muted-spectra regime suggested in observational studies by HST and JWST.
That the automated rate-based network generator produces a sufficiently complete reaction set and that deep-atmosphere quenching dominates the observable-layer abundances without photochemistry or other processes substantially altering the PAH levels across the full Teq range.
Deep hydrocarbon chemistry and quenching in sub-Neptunes create PAH abundances peaking at 600 K, providing a first-principles explanation for the muted transmission spectra trend between 500-800 K.
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| First computed | 2026-05-20T00:00:37.871726Z |
|---|---|
| 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/SFQ6YZ7OAN2D35LPLXZGOZEFJW \
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Canonical record JSON
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