{"date_updated":"2024-09-26T14:12:52Z","oa_version":"Published Version","citation":{"ieee":"D. W. Savin, P. S. Krsti, Z. Haiman, and P. C. Stancil, “Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications,” <i>The Astrophysical Journal</i>, vol. 606, no. 2. American Astronomical Society, pp. L167–L170, 2004.","ista":"Savin DW, Krsti PS, Haiman Z, Stancil PC. 2004. Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications. The Astrophysical Journal. 606(2), L167–L170.","apa":"Savin, D. W., Krsti, P. S., Haiman, Z., &#38; Stancil, P. C. (2004). Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.1086/421108\">https://doi.org/10.1086/421108</a>","ama":"Savin DW, Krsti PS, Haiman Z, Stancil PC. Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications. <i>The Astrophysical Journal</i>. 2004;606(2):L167-L170. doi:<a href=\"https://doi.org/10.1086/421108\">10.1086/421108</a>","short":"D.W. Savin, P.S. Krsti, Z. Haiman, P.C. Stancil, The Astrophysical Journal 606 (2004) L167–L170.","chicago":"Savin, Daniel Wolf, Predrag S. Krsti, Zoltán Haiman, and Phillip C. Stancil. “Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2004. <a href=\"https://doi.org/10.1086/421108\">https://doi.org/10.1086/421108</a>.","mla":"Savin, Daniel Wolf, et al. “Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications.” <i>The Astrophysical Journal</i>, vol. 606, no. 2, American Astronomical Society, 2004, pp. L167–70, doi:<a href=\"https://doi.org/10.1086/421108\">10.1086/421108</a>."},"type":"journal_article","publisher":"American Astronomical Society","issue":"2","language":[{"iso":"eng"}],"article_type":"original","date_published":"2004-05-10T00:00:00Z","related_material":{"link":[{"url":"https://doi.org/10.1086/421873","relation":"erratum"}]},"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1086/421108"}],"status":"public","day":"10","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_created":"2024-09-06T09:45:29Z","author":[{"first_name":"Daniel Wolf","full_name":"Savin, Daniel Wolf","last_name":"Savin"},{"last_name":"Krsti","full_name":"Krsti, Predrag S.","first_name":"Predrag S."},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"full_name":"Stancil, Phillip C.","first_name":"Phillip C.","last_name":"Stancil"}],"page":"L167-L170","title":"Rate Coefficient for H+ + H2(X1Σg+, ν = 0, J = 0) → H(1s) + H2+ Charge Transfer and Some Cosmological Implications","_id":"17758","extern":"1","volume":606,"article_processing_charge":"No","intvolume":"       606","abstract":[{"text":"Krstic has carried out the first quantum mechanical calculations near threshold for the charge transfer (CT) process H^+ + H_2(X ^1Sigma_g^+, nu=0, J=0) --> H(1s) + H_2^+. These results are relevant for models of primordial galaxy and first star formation that require reliable atomic and molecular data for obtaining the early universe hydrogen chemistry. Using the results of Krstic, we calculate the relevant CT rate coefficient for temperatures between 100 and 30,000 K. We also present a simple fit which can be readily implemented into early universe chemical models. Additionally, we explore how the range of previously published data for this reaction translates into uncertainties in the predicted gas temperature and H_2 relative abundance in a collapsing primordial gas cloud. Our new data significantly reduce these cosmological uncertainties that are due to the uncertainties in the previously published CT rate coefficients.","lang":"eng"}],"publication_status":"published","doi":"10.1086/421108","publication":"The Astrophysical Journal","year":"2004","publication_identifier":{"issn":["0004-637X","1538-4357"]},"scopus_import":"1","month":"05","quality_controlled":"1","oa":1}