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DOI	10.1016/j.epsl.2021.116825
	Empirical evidence for cosmogenic 3He production by muons
	Larsen I.J.; Farley K.A.; Lamb M.P.; Pritchard C.J.
发表日期	2021
ISSN	0012821X
卷号	562
英文摘要	Cosmic ray muons penetrate deeply into rock where they interact with atoms to produce cosmogenic nuclides. Incorporation of the muon contribution to the production rates of cosmogenic nuclides increases the accuracy of exposure dates, burial ages, and erosion rates inferred from measured nuclide concentrations. In the absence of empirical evidence, it is generally assumed that muons do not produce 3He, a cosmogenic nuclide commonly used for exposure dating. Here we assess whether muons produce 3He by measuring He isotope concentrations in pyroxene and ilmenite from a ∼300 m deep drill core and other subsurface samples of the mid-Miocene Columbia River Basalt in Washington, USA. 3He concentrations in our samples exhibit an exponential decline with depth with an e-folding length of 32.4 m, which corresponds to an attenuation length for 3He production of 8780 g cm−2. The deeply penetrating exponential is diagnostic of 3He production by cosmic ray muons. Assuming no erosion, we constrain the minimum surface muonogenic production rate to be 0.23 atom g−1 pyroxene yr−1, whereas when incorporating erosion the production rate is 0.45 atom g−1 pyroxene yr−1. 3He concentrations in samples deeper than ∼100 meters are consistent with model-based estimates of depth-independent nucleogenic production from the capture by 6Li of neutrons produced by alpha particle reactions on light elements. Measurements in other subsurface samples indicate that muon-produced 3He is prevalent across the Columbia Plateau. The penetration depth of muonogenic 3He production is substantially deeper, and the ratio of muon- to spallation-produced 3He is substantially lower, than found for other cosmogenic nuclides. Our results provide the first definitive empirical evidence for 3He production by muons, which has several implications for quantifying the timing and rates of Earth surface change and interpreting He isotope ratios. Importantly, despite the low production rates, landforms in the Channeled Scablands, which were formed by incision of the Columbia River Basalt by the late-Pleistocene Missoula floods, have high concentrations of 3He inherited from post-Miocene muon exposure. Hence 3He production by muons must be considered, particularly when dating rapid erosional events in old bedrock. Our findings indicate samples with less than several tens of meters of shielding by overlying rock will contain cosmogenic 3He that elevates 3He/4He ratios. Hence caution should be used when using 3He/4He ratios from samples at shallower depths to infer mantle sources of basalt. © 2021 Elsevier B.V.
关键词	3He Columbia River Basalt cosmogenic nuclides exposure dating mantle helium muon
英文关键词	Atoms; Basalt; Core drilling; Cosmic rays; Cosmology; Erosion; Isotopes; Silicate minerals; Attenuation lengths; Columbia Plateau; Columbia river basalts; Cosmic-ray muons; Cosmogenic nuclides; Minimum surfaces; Nuclide concentrations; Production rates; Charged particles; basalt; concentration (composition); cosmic ray; cosmogenic radionuclide; empirical analysis; helium isotope; ilmenite; mantle; pyroxene; United States; Washington [United States]; Columbia
语种	英语
来源期刊	Earth and Planetary Science Letters
文献类型	期刊论文
条目标识符	http://gcip.llas.ac.cn/handle/2XKMVOVA/203178
作者单位	Department of Geosciences, University of Massachusetts, Amherst, MA, United States; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, United States; Department of Geology, Eastern Washington University, Cheney, WA, United States
推荐引用方式 GB/T 7714	Larsen I.J.,Farley K.A.,Lamb M.P.,et al. Empirical evidence for cosmogenic 3He production by muons[J],2021,562.
APA	Larsen I.J.,Farley K.A.,Lamb M.P.,&Pritchard C.J..(2021).Empirical evidence for cosmogenic 3He production by muons.Earth and Planetary Science Letters,562.
MLA	Larsen I.J.,et al."Empirical evidence for cosmogenic 3He production by muons".Earth and Planetary Science Letters 562(2021).