Evidence presented: The authors model saturated porous seep flow as either (i) buoyancy/thermal–solutal convection or (ii) methane adsorption-driven osmosis (“osmotic pump”). For a seep scenario with permeability k≈10⁻¹² m² extended over k≈10⁻¹³–10⁻¹¹ m² and dilution≈20, they predict osmotic seep downward velocities ≈3.1 m/yr and methane efflux ≈0.025 mol m⁻² yr⁻¹, versus buoyant seep downward ≈0.38 m/yr and methane efflux ≈0.0031 mol m⁻² yr⁻¹, concluding osmosis can amplify deep seawater recirculation by ~10× relative to buoyancy/heat alone. They further argue this recirculation can reduce hydrate destabilization timescales from millennia to ~decades (as short as ~30 years) under warming in their framework.
The most discriminating test would be to seek independent constraints on deep methane-driven osmotic pressure differences and correlated downward seawater velocities (not just surface seep rates) at sites where methane concentrations are high and permeability is low—checking whether measured downward flows track the paper’s osmotic scaling better than buoyancy-only alternatives.
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