1959
DOI: 10.1103/physrev.116.1516
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Total Neutron Cross Section of Xenon and Krypton

Abstract: and the elements in the Fe peak need temperatures well above 2X1G 9 °K for their formation. It is reasonable to suppose that the elements Na to Ca are produced at intermediate temperatures. We have shown that the carbon burning reactions at temperatures between 5X10 8 and 10X10 8 °K produce large amounts of Na 23 and of the Mg isotopes plus decreasing amounts of Al 27 and Si, but very little of heavier nuclei. One striking feature of our results is the relatively large ratio of Na 23 to Mg 24 produced, 1:2 to … Show more

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Cited by 29 publications
(1 citation statement)
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“…We have chosen 84 Kr because it is an inert gas with the highest isotopic abundance of natural krypton (nearly 57%), making it easier to ionize and separate. Additionally, the E CM r = 519 eV (E LAB r = 43.6 keV) resonance in 84 Kr(n,γ) 85m Kr has a cross section of σ r = 363 b [5], which is energetically beneficial from a beam production, transport, and implantation perspective. Furthermore, the isomeric state at 305 keV in 85m Kr β decays to the ground state of 85 Rb, while emitting a strong 151-keV γ-ray line [6].…”
Section: Ion Species Selection and The Ntd High-intensity Low-energy ...mentioning
confidence: 99%
“…We have chosen 84 Kr because it is an inert gas with the highest isotopic abundance of natural krypton (nearly 57%), making it easier to ionize and separate. Additionally, the E CM r = 519 eV (E LAB r = 43.6 keV) resonance in 84 Kr(n,γ) 85m Kr has a cross section of σ r = 363 b [5], which is energetically beneficial from a beam production, transport, and implantation perspective. Furthermore, the isomeric state at 305 keV in 85m Kr β decays to the ground state of 85 Rb, while emitting a strong 151-keV γ-ray line [6].…”
Section: Ion Species Selection and The Ntd High-intensity Low-energy ...mentioning
confidence: 99%