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Diffusion kinetics of proton-induced Ne-21, He-3, and He-4 in quartz

机译:质子诱导的Ne-21,He-3和He-4在石英中的扩散动力学

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摘要

A natural quartz sample free of mineral and fluid inclusions was irradiated with a 200 MeV proton beam to produce spallogenic Ne-21, He-3 and He-4. Temperature-dependent diffusivities of these three nuclides were then determined simultaneously by high precision stepped-heating and noble gas mass spectrometry. The outward mobility of proton-induced nuclides reflects diffusion through the quartz lattice. In the studied range of 70 to 400 degrees C the helium diffusion coefficients exceed those of neon by 5-7 orders of magnitude. The implied diffusion parameters E-a = 153.7 +/- 1.5 (kJ/mol) and ln(D-o/a(2)) = 15.9 +/- 0.3 (ln(s(-1))) and E-a = 84.5 +/- 1.2 (kJ/mol) and ln(D-o/a(2)) 11.1 +/- 0.3 (ln(s(-1))) for proton-induced Ne-21 and He-3, respectively, indicate that cosmogenic neon will be quantitatively retained in inclusion-free quartz at typical Earth surface temperatures whereas cosmogenic helium will not. However, the neon diffusion parameters also indicate that diffusive loss needs to be considered for small (< 1 mm) quartz grains that have experienced elevated temperatures. Since natural quartz often contains fluid inclusions which may enhance noble gas retentivity, these parameters likely represent an end-member case of purely solid-state diffusion. The similar to 70 kJ/mol higher activation energy for neon diffusion compared to helium diffusion likely represents an energy barrier related to its similar to 13% greater diameter and provides a fundamental constraint with which to test theories of solid state diffusion. The diffusion parameters for proton-induced He-4 are indistinguishable from those for He-3, providing no evidence for the commonly expected inverse square root of the mass diffusion relationship between isotopes. We also find preliminary indication that increased exposure to radiation may enhance neon and helium retentivity in quartz at low temperatures. Copyright (c) 2005 Elsevier Ltd.
机译:用200 MeV质子束辐照不含矿物和流体夹杂物的天然石英样品,以产生散裂性Ne-21,He-3和He-4。然后,通过高精度步进加热和稀有气体质谱仪同时测定了这三种核素的温度依赖性扩散系数。质子诱导的核素的向外迁移反映了通过石英晶格的扩散。在70到400摄氏度的研究范围内,氦扩散系数比氖的扩散系数高5-7个数量级。隐含扩散参数Ea = 153.7 +/- 1.5(kJ / mol)和ln(Do / a(2))= 15.9 +/- 0.3(ln(s(-1)))和Ea = 84.5 +/- 1.2 (kJ / mol)和ln(Do / a(2))11.1 +/- 0.3(ln(s(-1)))分别针对质子诱导的Ne-21和He-3,表明宇宙性氖将是在典型的地球表面温度下定量保留在无夹杂的石英中,而宇宙氦则不会。但是,氖扩散参数还表明,对于经历高温的小(<1毫米)石英晶粒,需要考虑其扩散损失。由于天然石英通常包含可提高稀有气体保留性的流体夹杂物,因此这些参数很可能代表纯固态扩散的末端情况。与氦气扩散相比,与氖气扩散相比,类似于70kJ / mol的更高的氖气扩散活化能可能代表了与其约13%的直径相似的能量垒,并提供了测试固态扩散理论的基本约束。质子诱导的He-4的扩散参数与He-3的扩散参数没有区别,因此没有证据表明同位素之间普遍存在的质量扩散关系的平方根反比。我们还发现初步迹象表明,增加辐射暴露可以增强石英在低温下的氖和氦保持性。版权所有(c)2005 Elsevier Ltd.

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