Formation of H2 on an olivine surface: a computational study

The formation of H₂ on a pristine olivine surface forsterite (010)] is investigated computationally. Calculations show that the forsterite surface catalyzes H₂ formation by providing chemisorption sites for H atoms. The chemisorption route allows for stepwise release of the reaction exothermicity and stronger coupling to the surface, which increases the efficiency of energy dissipation. This suggests that H₂ formed on a pristine olivine surface should be much less rovibrationally excited than H₂ formed on a graphite surface. Gas-phase H atoms impinging on the surface will first physisorb relatively strongly  ( E _phys= 1240 K)  . The H atom can then migrate via desorption and re-adsorption, with a barrier equal to the adsorption energy. The barrier for a physisorbed H atom to become chemisorbed is equal to the physisorption energy, therefore there is almost no gas-phase barrier to chemisorption. An impinging gas-phase H atom can easily chemisorb  ( E _chem= 12 200 K)  , creating a defect where a silicate O atom is protonated and a single electron resides on the surface above the adjacent magnesium ion. This defect directs any subsequent impinging H atoms to chemisorb strongly (39 800 K) on the surface electron site. The two adjacent chemisorbed atoms can subsequently recombine to form H₂ via a barrier (5610 K) that is lower than the chemisorption energy of the second H atom. Alternatively, the adsorbed surface species can react with another incoming H atom to yield H₂ and regenerate the surface electron site. This double chemisorption 'relay mechanism' catalyzes H₂ formation on the olivine surface and is expected to attenuate the rovibrational excitation of H₂ thus formed.