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• W2006079601 abstract "The H3+ is a key ion in the interstellar chemistry. The rate of recombination of H3+ with electrons, α, plays a pivotal role in the level of ionization of interstellar plasmas. Over the past 50 years a number of studies of this recombination have been carried out, yet they did not lead to an unambiguous value of α. We report observation of the rate of de-ionization of H3+ as low as αeff ~ 3×10-9 cm3 s-1 at hydrogen density decreasing down to 5×1010 cm-3. This implies that the dissociative recombination of H3+ under interstellar conditions is very slow with αDR<<10-8 cm3 s-1. This value is in agreement with theoretical predictions and astronomical observations, and provides an explanation of the `enigma of H3+'." @default.
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• W2006079601 date "2001-07-20" @default.
• W2006079601 modified "2023-10-18" @default.
• W2006079601 title "Experimental study of recombination of H₃⁺ions with electrons relevant for interstellar and planetary plasmas" @default.
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• W2006079601 doi "https://doi.org/10.1088/0953-4075/34/15/104" @default.
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