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The heaviest chemical elements are naturally produced by the rapid neutron-capture process (r-process) during neutron star mergers or supernovae. Ther-process production of elements heavier than uranium (transuranic nuclei) is poorly understood and inaccessible to experiments so must be extrapolated by using nucleosynthesis models. We examined element abundances in a sample of stars that are enhanced inr-process elements. The abundances of elements ruthenium, rhodium, palladium, and silver (atomic numbersZ= 44 to 47; mass numbersA= 99 to 110) correlate with those of heavier elements (63 ≤Z≤ 78,A> 150). There is no correlation for neighboring elements (34 ≤Z≤ 42 and 48 ≤Z≤ 62). We interpret this as evidence that fission fragments of transuranic nuclei contribute to the abundances. Our results indicate that neutron-rich nuclei with mass numbers >260 are produced inr-process events.
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An Improved Average Atomic Number Calculation for Estimating Backscatter and Continuum Production in Compounds
Abstract It is often assumed that electron backscatter and continuum (bremsstrahlung) productions emitted from electron-solid interactions during X-ray microanalysis in compounds can be extrapolated from pure element observations by means of the assumption of average atomic number, or Z-bar (Z¯). For pure elements the average Z is equal to the atomic number, but this direct approach fails for compounds. The use of simple atomic fractions yields completely spurious results, and while the commonly used mass fraction Z averaging produces fairly reasonable results, we know from physical considerations that the mass of the neutron plays only a negligible role in such interactions below ∼1 MeV. Therefore, including the mass or atomic weight in such calculations can only introduce further errors in these models. We present an expression utilizing atomic fractions of the atomic numbers of the elements in the compound (Z fraction), with an exponent to account for the variation in nuclear screening as a function of the element Z value.
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- Award ID(s):
- 2012191
- PAR ID:
- 10466397
- Date Published:
- Journal Name:
- Microscopy and Microanalysis
- Volume:
- 29
- Issue:
- 4
- ISSN:
- 1431-9276
- Page Range / eLocation ID:
- 1436 to 1449
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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- Free Publicly Accessible Full Text
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Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.1093/micmic/ozad069
