TY - JOUR
T1 - Terrestrial in situ cosmogenic nuclide production rate scaling models
T2 - Theory, progress, and prospects
AU - Zhou, Jie
AU - Zhou, Weijian
AU - Fu, Yunchong
AU - Xian, Feng
AU - Wang, Du
AU - Yang, Xianlin
AU - Dong, Guocheng
AU - Zhang, Li
AU - Tang, Ling
AU - Zhao, Guoqing
AU - Zang, Mengyu
N1 - Publisher Copyright:
© Science China Press 2025.
PY - 2026/1
Y1 - 2026/1
N2 - High-energy cosmic rays bombard target atoms in near-surface minerals, initiating nuclear reactions that produce in situ cosmogenic nuclides such as 10Be and 26Al. Advances in cosmogenic nuclide techniques have been enabled by well-understood production mechanisms, highly sensitive detection at ultra-trace levels, and robust quantitative that describe nuclide production, accumulation, transport, and decay in the near-surface environment. These techniques have advanced Earth science by providing tools for surface exposure dating, sediment burial dating, and quantifying denudation rates of watersheds and bedrocks. This article presents a comprehensive review of the research history of terrestrial in situ cosmogenic nuclide production rates, the theoretical frameworks and computational methodologies used to construct production rate scaling models, with particular attention to key controlling factors, and evaluates the differences among various production rate scaling models and their underlying causes. To improve the accuracy and precision of future production rate scaling models, we recommend the following four research priorities: (1) Enhance quantitative comparison and data assimilation between measured and simulated cosmic-ray spectra to refine particle-transport simulation algorithms and reduce uncertainties in secondary cosmic-ray energy spectra. (2) Reconstruct temporal variations in geomagnetic field intensity and solar activity since the Pleistocene to provide more robust constraints on time-dependent cosmic-ray energy spectra. (3) Systematically measure and theoretically evaluate proton- and neutron-induced cross sections on main target atoms (O, Si, Al, Fe, Mg, etc.) across energy ranges relevant to TCN production and compile the results into a comprehensive evaluated database. (4) Strengthen geological calibrations of production rates across multi-nuclide (3He, 10Be, 14C, 21Ne, 26Al, 36Cl, etc.) and multi-mineral (quartz, calcite, etc.) systems to develop a globally applicable, internally consistent production rate model.
AB - High-energy cosmic rays bombard target atoms in near-surface minerals, initiating nuclear reactions that produce in situ cosmogenic nuclides such as 10Be and 26Al. Advances in cosmogenic nuclide techniques have been enabled by well-understood production mechanisms, highly sensitive detection at ultra-trace levels, and robust quantitative that describe nuclide production, accumulation, transport, and decay in the near-surface environment. These techniques have advanced Earth science by providing tools for surface exposure dating, sediment burial dating, and quantifying denudation rates of watersheds and bedrocks. This article presents a comprehensive review of the research history of terrestrial in situ cosmogenic nuclide production rates, the theoretical frameworks and computational methodologies used to construct production rate scaling models, with particular attention to key controlling factors, and evaluates the differences among various production rate scaling models and their underlying causes. To improve the accuracy and precision of future production rate scaling models, we recommend the following four research priorities: (1) Enhance quantitative comparison and data assimilation between measured and simulated cosmic-ray spectra to refine particle-transport simulation algorithms and reduce uncertainties in secondary cosmic-ray energy spectra. (2) Reconstruct temporal variations in geomagnetic field intensity and solar activity since the Pleistocene to provide more robust constraints on time-dependent cosmic-ray energy spectra. (3) Systematically measure and theoretically evaluate proton- and neutron-induced cross sections on main target atoms (O, Si, Al, Fe, Mg, etc.) across energy ranges relevant to TCN production and compile the results into a comprehensive evaluated database. (4) Strengthen geological calibrations of production rates across multi-nuclide (3He, 10Be, 14C, 21Ne, 26Al, 36Cl, etc.) and multi-mineral (quartz, calcite, etc.) systems to develop a globally applicable, internally consistent production rate model.
KW - Cosmic rays
KW - In situ cosmogenic nuclide
KW - Nuclear reaction cross-section
KW - Production rate scaling models
KW - Spallation reaction
UR - https://www.scopus.com/pages/publications/105022274179
U2 - 10.1007/s11430-025-1731-y
DO - 10.1007/s11430-025-1731-y
M3 - 文献综述
AN - SCOPUS:105022274179
SN - 1674-7313
VL - 69
SP - 27
EP - 47
JO - Science China Earth Sciences
JF - Science China Earth Sciences
IS - 1
ER -