1997
DOI: 10.1029/97jb00395
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Production of nucleogenic neon in the Earth from natural radioactive decay

Abstract: [1980] and Kyser and Rison [1982]. The present study also has shown that the nucleogenic 2•Ne production from the 24Mg(n,00 reaction is only about one-fifth the previous estimate. The contribution of nucleogenic 21Ne from the 24Mg(n,00 reaction is insignificant compared with nucleogenic 2•Ne production from 180(o•,n). Our estimate of the nucleogenic 2•Ne/radiogenic 4He production ratio both in the mantle and in the crust is 4.5 x 10 -8. This production ratio is quite consistent with nucleogenic 21Ne/radiogeni… Show more

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Cited by 174 publications
(118 citation statements)
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“…Our approach is more stringent than that used by Hiinemohr [1989] and Yatsevich and Honda [1997] to calculate the Ne production in mean crust and mantle, since we rely on cross section data instead of thick-target yields. Hence, our approach is applicable to a wide field of target element compounds, since the calculations are independent of limiting assumptions on, e.g., stopping power ratios.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…Our approach is more stringent than that used by Hiinemohr [1989] and Yatsevich and Honda [1997] to calculate the Ne production in mean crust and mantle, since we rely on cross section data instead of thick-target yields. Hence, our approach is applicable to a wide field of target element compounds, since the calculations are independent of limiting assumptions on, e.g., stopping power ratios.…”
Section: Discussionmentioning
confidence: 99%
“…Since the stopping powers for pure elements differ from those for the actual chemical composition considered, a corresponding correction was necessary. This was done by assuming that the ratios of the stopping powers for different elements are independent of energy (for more details see, e.g., West [1979] and Yatsevich and Honda [1997]). In contrast, in our new approach the mass stopping power for the chemical compound is calculated directly and then folded with the excitation functions of the underlying nuclear reactions.…”
Section: Comparison: Thin-target Versus Thick-target Approachmentioning
confidence: 99%
“…[23] The model assumes a uniform initial helium distribution within grains that was determined by Hunt [2000] using the 21 Ne-4 He method [Yatsevich and Honda, 1997] that between 60 and 87% of helium had been lost prior to till emplacement.…”
Section: Transient Modelmentioning
confidence: 99%
“…We provide a comparison of nucleogenic production rates of neutrons, 21 Ne, and 39 Ar calculated in this study to select recent evaluations (Yatsevich and Honda, 1997;Leya and Wieler, 1999;Mei et al, 2010;Yokochi et al, 2012Yokochi et al, , 2014. Similar calculations were previously performed by Fabryka-Martin (1988); Andrews et al (1989Andrews et al ( , 1991; Lehmann et al (1993); Lehmann and Purtschert (1997).…”
Section: Comparison To Previous Resultsmentioning
confidence: 80%
“…In section 6 we present the results, including coefficients for production rate evaluation (6.3) and an estimate of the uncertainty in the calculated results (6.4). A discussion follows in section 7 where we compare our calculations with recent results (Yatsevich and Honda, 1997;Mei et al, 2010;Yokochi et al, 2012Yokochi et al, , 2014.1), calculate the nucleogenic neutron flux out of a rock (7.2), and discuss the geochemical implications (7.3). Concluding remarks follow in section 8.…”
Section: Introductionmentioning
confidence: 99%