{"paper":{"title":"OH+ in astrophysical media: state-to-state formation rates, Einstein coefficients and inelastic collision rates with He","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.chem-ph"],"primary_cat":"astro-ph.SR","authors_text":"A. Aguado, B. Godard, F. J. Aoiz, F. Lique, J. Cernicharo, J. F. Castillo, J. Klos, J. R. Goicoechea, M. Etxaluze, N. Bulut, O. Roncero, S. Gomez-Carrasco","submitted_at":"2014-05-16T14:16:29Z","abstract_excerpt":"The rate constants required to model the OH$^+$ observations in different regions of the interstellar medium have been determined using state of the art quantum methods.\n  First, state-to-state rate constants for the H$_2(v=0,J=0,1)$+ O$^+$($^4S$) $\\rightarrow$ H + OH$^+(X ^3\\Sigma^-, v', N)$ reaction have been obtained using a quantum wave packet method. The calculations have been compared with time-independent results to asses the accuracy of reaction probabilities at collision energies of about 1 meV. The good agreement between the simulations and the existing experimental cross sections in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.4173","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}