{ "id": "1407.3135", "version": "v1", "published": "2014-07-11T12:42:13.000Z", "updated": "2014-07-11T12:42:13.000Z", "title": "H$_{2}$O Maser Pumping: The Effect of Quasi-Resonance Energy Transfer in Collisions between H$_2$ and H$_2$O Molecules", "authors": [ "A. V. Nesterenok", "D. A. Varshalovich" ], "comment": "arXiv admin note: text overlap with arXiv:1309.7547", "journal": "Published in Astronomy Letters, 2014, Vol. 40, No.7, pp. 425-434", "doi": "10.1134/S1063773714070068", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "The effect of quasi-resonance energy transfer in collisions between H$_2$ and H$_2$O molecules in H$_2$O maser sources is investigated. New data on the state-to-state rate coefficients for collisional transitions for H$_2$O and H$_2$ molecules are used in the calculations. The results of ortho-H$_2$O level population inversion calculations for the 22.2-, 380-, 439-, and 621-GHz transitions are presented. The ortho-H$_2$O level population inversion is shown to depend significantly on the population distribution of the para-H$_2$ $J = 0$ and $2$ rotational levels. The possibility of quasi-resonance energy transfer in collisions between H$_2$ molecules at highly excited rotational-vibrational levels and H$_2$O molecules is considered. The quasi-resonance energy transfer effect can play a significant role in pumping H$_2$O masers in the central regions of active galactic nuclei and in star-forming regions.", "revisions": [ { "version": "v1", "updated": "2014-07-11T12:42:13.000Z" } ], "analyses": { "keywords": [ "collisions", "maser pumping", "quasi-resonance energy transfer effect", "level population inversion calculations", "state-to-state rate coefficients" ], "tags": [ "journal article" ], "publication": { "journal": "Astronomy Letters", "year": 2014, "month": "Jul", "volume": 40, "number": 7, "pages": 425 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1305876, "adsabs": "2014AstL...40..425N" } } }