First experimental determination of the40Ar((Formula presented) )39Ar reaction cross section and39Ar production in Earth’s atmosphere

  • S. Bhattacharya
  • , M. Paul*
  • , R. N. Sahoo
  • , R. Purtschert
  • , H. F.R. Hoffmann
  • , M. Pichotta
  • , K. Zuber
  • , D. Bemmerer
  • , T. Döring
  • , R. Schwengner
  • , M. L. Avila
  • , E. Lopez-Saavedra
  • , J. C. Dickerson
  • , C. Fougères
  • , J. McLain
  • , R. C. Pardo
  • , K. E. Rehm
  • , R. Scott
  • , I. Tolstukhin
  • , R. Vondrasek
  • T. Bailey, L. Callahan, A. M. Clark, P. Collon, Y. Kashiv, A. Nelson, D. Robertson, D. Neto, C. Ugalde, M. Tessler, S. Vaintraub
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

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 languageEnglish
JournalGeochimica et Cosmochimica Acta
DOIs
StateAccepted/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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