2011
DOI: 10.1016/j.gca.2011.08.023
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Xenon and Argon: A contrasting behavior in olivine at depth

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Cited by 26 publications
(26 citation statements)
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“…On the other hand, if noble gases were to have higher silicate solid/liquid partition coefficients at high pressure (e.g., Xe: Sanloup et al . []), they could be stored in silicate phases rather than Fe‐Ni‐S liquids. In this scenario, the droplet occurrence would only have acted as a physical mechanism to isolate the LLSVP from whole mantle convection (through a density increase) but not as the host of the noble gases (especially Xe).…”
Section: Consistency With Geochemical Observationsmentioning
confidence: 99%
See 1 more Smart Citation
“…On the other hand, if noble gases were to have higher silicate solid/liquid partition coefficients at high pressure (e.g., Xe: Sanloup et al . []), they could be stored in silicate phases rather than Fe‐Ni‐S liquids. In this scenario, the droplet occurrence would only have acted as a physical mechanism to isolate the LLSVP from whole mantle convection (through a density increase) but not as the host of the noble gases (especially Xe).…”
Section: Consistency With Geochemical Observationsmentioning
confidence: 99%
“…On the one hand, if helium is preferentially partitioned into Fe-Ni-S liquid, the Fe-Ni-S liquid could potentially store significant primordial noble gases compared with silicate crystals [Heber et al, 2007;Bouhifd et al, 2013;Huang et al, 2014]. On the other hand, if noble gases were to have higher silicate solid/liquid partition coefficients at high pressure (e.g., Xe: Sanloup et al [2011]), they could be stored in silicate phases rather than Fe-Ni-S liquids. In this scenario, the droplet occurrence would only have acted as a physical mechanism to isolate the LLSVP from whole mantle convection (through a density increase) but not as the host of the noble gases (especially Xe).…”
Section: Consistency With Geochemical Observationsmentioning
confidence: 99%
“…Ren e Bès, 1,2,a) Philippe Martin, 1,b) Emerson Vathonne, 1 R emy Delorme, 1 Catherine Sabathier, 1 Michel Freyss,1 We report here the direct experimental observation of the preferential xenon incorporation site in uranium dioxide and analyse how its incorporation evolves with the annealing temperature. We show that High Energy Resolution Fluorescence Detection X-ray Absorption Near Edge Structure in combination with first-principles calculations enable a precise determination of the Xe incorporation site.…”
Section: Experimental Evidence Of Xe Incorporation In Schottky Defectmentioning
confidence: 99%
“…Assuming equal degassing efficiencies for all noble gases means that the atmospheric inventories of 36+38 Ar, Kr, and Xe may be only 50% of the total BSE inventories. Sanloup et al (2005Sanloup et al ( , 2011 suggested that at high pressure XeO 2 can substitute for SiO 2 in quartz and to lesser extent into olivine. Their proposals remain speculative although Brock and Schrobilgen (2011) synthesized XeO 2 .…”
Section: Secondary Origin Of Earth's Atmospherementioning
confidence: 99%