Theoretical study of the H3− cluster

Abstract
Calculations at the ab initio level with an extended basis set including polarization functions have been performed in order to study the possible existence of ion–induced dipole clusters like H3 in the interstellar medium. Configuration interaction calculations have shown that the interstellar diffuse bands observed by astronomers and not attributed till now can be explained by the presence of such clusters in the ground state and excited states 1Σ0+ and 1Π.

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