Abstract
In this study, we have determined the combined effect of pressure and temperature on the compressional-wave velocity (VP) of Ne up to 53 GPa and 1100 K using Brillouin scattering in externally heated diamond-anvil cells. The phase transition from the supercritical fluid to solid phase was observed to cause a 10.5–11% jump in VP, and the magnitude in the VP contrast across the phase transition increases with temperature. In addition, we have observed an abnormal reduced increase rate of VP with pressure in the supercritical Ne fluid at both 800 and 1100 K before the transition to the solid phase. VP of the solid Ne exhibits a nonlinear increase with pressure at all the investigated temperatures. The elevating temperature was noted to cause an apparent reduction in VP, yet the reduction in VP caused by increasing temperature dramatically decreases at higher pressures. At 20 GPa, increasing temperature by 100 K can lower the VP of Ne by 2.4%. Yet elevating temperature by 100 K can only reduce the VP by 0.4% at 50 GPa. We further compare VP of Ne to that of other rare gases, including Ar, Kr, and Xe. At 300 K, VP of Ne shows a stronger dependence on pressure than both Kr and Xe. Moreover, increasing temperature can produce a greater reduction in VP of Ne than that of Ar below 50 GPa. Our measured VP of Ne is also useful for understanding the velocity structure of giant planets, such as Jupiter.
Funding
Z. Mao acknowledges supports from the National Key R&D Program of China (2018YFA0702703), and the Strategic Priority Research Program of the Chinese Academy of Sciences (XDB18000000). This work was performed at GeoSoil-EnviroCARS, Advanced Photon Source, Argonne National Laboratory, supported by the National Science Foundation (EAR-1634415) and Department of Energy (DE-FG02-94ER14466). Use of the COMPRES-GSECARS gas loading system was supported by COM-PRES under NSF Cooperative Agreement EAR-1606856.
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Articles in the same Issue
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- Computer modeling of apparently straight bond angles: The intriguing case of all-silica ferrierite
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Articles in the same Issue
- Crossroads in Earth and Planetary Materials
- Computer modeling of apparently straight bond angles: The intriguing case of all-silica ferrierite
- Composite materials based on zeolite stilbite from Faroe Islands for the removal of fluoride from drinking water
- The Italian Solfatara as an analog for Mars fumarolic alteration
- Change of crackling noise in granite by thermal damage: Monitoring nuclear waste deposits
- Constraining the timing and character of crustal melting in the Adirondack Mountains using multi-scale compositional mapping and in-situ monazite geochronology
- Melting in the Fe-FeO system to 204 GPa: Implications for oxygen in Earth’s core
- Controls on tetrahedral Fe(III) abundance in 2:1 phyllosilicates
- Stability, composition, and crystal structure of Fe-bearing Phase E in the transition zone
- Enrichment of manganese to spessartine saturation in granite-pegmatite systems
- Al and Si diffusion in rutile
- Sound velocity of neon at high pressures and temperatures by Brillouin scattering
- A Cr3+ luminescence study of natural topaz Al2SiO4(F,OH)2 up to 60 GPa
- Two generations of exsolution lamellae in pyroxene from Asuka 09545: Clues to the thermal evolution of silicates in mesosiderite
- Crystallographic and fluid compositional effects on the halogen (Cl, F, Br, I) incorporation in pyromorphite-group minerals
- Diffusion of F and Cl in dry rhyodacitic melt