Local structure of molten AuGa2 under pressure: Evidence for coordination change and planetary implications
Abstract
In situ x-ray diffraction measurements and inverse Monte Carlo simulations of pair distribution functions were used to characterize the local structure of molten AuGa2 up to 16 GPa and 940 K. Our results document systematic changes in liquid structure due to a combination of bond compression and coordination increase. Empirical potential structure refinement shows the first-neighbor coordination of Ga around Au and of Au around Ga to increase from about 8 to 10 and 4 to 5, respectively between 0 and 16 GPa, and the inferred changes in liquid structure can explain the observed melting-point depression of AuGa2 up to 5 GPa. As intermetallic AuGa2 is an analogue for metallic SiO2 at much higher pressures, our results imply that structural changes documented for non-metallic silicate melts below 100 GPa are followed by additional coordination changes in the metallic state at pressures in the 0.2-1 TPa range achieved inside large planets.
- Authors:
-
- Hacettepe Univ, Ankara (Turkey); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of California, Berkeley, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC), Basic Energy Sciences (BES)
- OSTI Identifier:
- 1436513
- Alternate Identifier(s):
- OSTI ID: 1462006
- Grant/Contract Number:
- NA0002198; AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Scientific Reports
- Additional Journal Information:
- Journal Volume: 8; Journal Issue: 1; Journal ID: ISSN 2045-2322
- Publisher:
- Nature Publishing Group
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 36 MATERIALS SCIENCE; 79 ASTRONOMY AND ASTROPHYSICS; 75 CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY
Citation Formats
Kalkan, Bora, Godwal, Budhiram, Raju, Selva Vennila, and Jeanloz, Raymond. Local structure of molten AuGa2 under pressure: Evidence for coordination change and planetary implications. United States: N. p., 2018.
Web. doi:10.1038/s41598-018-25297-9.
Kalkan, Bora, Godwal, Budhiram, Raju, Selva Vennila, & Jeanloz, Raymond. Local structure of molten AuGa2 under pressure: Evidence for coordination change and planetary implications. United States. https://doi.org/10.1038/s41598-018-25297-9
Kalkan, Bora, Godwal, Budhiram, Raju, Selva Vennila, and Jeanloz, Raymond. Tue .
"Local structure of molten AuGa2 under pressure: Evidence for coordination change and planetary implications". United States. https://doi.org/10.1038/s41598-018-25297-9. https://www.osti.gov/servlets/purl/1436513.
@article{osti_1436513,
title = {Local structure of molten AuGa2 under pressure: Evidence for coordination change and planetary implications},
author = {Kalkan, Bora and Godwal, Budhiram and Raju, Selva Vennila and Jeanloz, Raymond},
abstractNote = {In situ x-ray diffraction measurements and inverse Monte Carlo simulations of pair distribution functions were used to characterize the local structure of molten AuGa2 up to 16 GPa and 940 K. Our results document systematic changes in liquid structure due to a combination of bond compression and coordination increase. Empirical potential structure refinement shows the first-neighbor coordination of Ga around Au and of Au around Ga to increase from about 8 to 10 and 4 to 5, respectively between 0 and 16 GPa, and the inferred changes in liquid structure can explain the observed melting-point depression of AuGa2 up to 5 GPa. As intermetallic AuGa2 is an analogue for metallic SiO2 at much higher pressures, our results imply that structural changes documented for non-metallic silicate melts below 100 GPa are followed by additional coordination changes in the metallic state at pressures in the 0.2-1 TPa range achieved inside large planets.},
doi = {10.1038/s41598-018-25297-9},
journal = {Scientific Reports},
number = 1,
volume = 8,
place = {United States},
year = {2018},
month = {5}
}
Web of Science
Figures / Tables:

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