Possible Role Played by the Fullerene‐like Structures of Interstellar Carbon Dust in the Formation of Molecular Hydrogen in Space

摘要: After a general introduction to the problem of formation molecular hydrogen from atomic in interstellar medium and dense clouds particular, after explanation key role played by surfaces on this process, it is proposed that most suitable carbon surface for (from radiative association process hydrogen) can be represented black rather than graphite. Furthermore, fullerene-like structures present graphene sheets are reaction sites where may formed.