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.
(2023); Wallack et al
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Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends
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.