Abstract
The cosmogenic39Ar(t1/2 = 268 years) isotope of argon is used for geophysical dating and tracing of underground and ocean water, as well as ice owing to its appropriate half-life and chemical inertness as a noble gas;39Ar serves also in nuclear weapon test monitoring. We measured for the first time the total cross section of the main39Ar cosmogenic production reaction in the atmosphere, namely40Ar(n,2n)39[jls-end-space/]Ar, using 14.8 ± 0.3 MeV neutrons. The neutrons, produced by a deuterium-tritium generator, impinged on a stainless steel sphere filled with Ar gas highly enriched in the40Ar isotope and were monitored by a stack of fast-neutron activation foils. The reaction yield was measured by atom counting of long-lived39Ar with noble gas accelerator mass spectrometry and, independently, by decay counting relative to atmospheric argon (39Ar/Ar= (Formula presented) ). A total40Ar(n,2n)39[jls-end-space/]Ar cross section of 610 ± 100 mb was determined at 14.8 ± 0.3 MeV incident neutron energy. This result serves as a benchmark for recent theoretical calculations and evaluations, found to reproduce well the experimental total cross section. We use these energy-dependent theoretical cross sections together with experimental spectra of cosmogenic neutrons at different altitudes to calculate the global average rate of neutron-induced39Ar atmospheric production, resulting in (Formula presented)39Ar atoms/cm2[jls-end-space/]/day. The secular equilibrium between the39Ar calculated production rate and radioactive decay rate leads to a partial isotopic abundance39Ar/Ar(Formula presented), showing that ≈[jls-end-space/]73% of atmospheric39Ar is produced by cosmogenic neutrons, the remaining part believed to be induced by muons and high-energy γ rays. The40Ar((Formula presented) )39Ar cross section at 14 MeV is also a key parameter for quantifying the anthropogenic contribution to atmospheric39Ar produced during the thermonuclear tests of the 1960s. We estimate that anthropogenic39Ar accounts for roughly 20% of the present atmospheric inventory.
| Original language | English |
|---|---|
| Journal | Geochimica et Cosmochimica Acta |
| DOIs | |
| State | Accepted/In press - 2025 |
Bibliographical note
Publisher Copyright:© 2025 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND license. http://creativecommons.org/licenses/by-nc-nd/4.0/
Keywords
- Accelerator mass spectrometry
- Ar atmospheric production
- Ar(n,2n)Ar reaction
- Low-level counting
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