Weak cosmic-ray heating events barely change the predicted H2 ice abundance because H2 desorption is already capped by the grain strike frequency, so they cannot fix the H2 freeze-out problem for 0.1 μm grains.
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The Effect of Weak Cosmic Ray Heating Events on the Desorption of $\rm H_2$
Weak cosmic-ray heating events barely change the predicted H2 ice abundance because H2 desorption is already capped by the grain strike frequency, so they cannot fix the H2 freeze-out problem for 0.1 μm grains.