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We acknowledge GSECARS, APS, and ANL for the use of the synchrotron and laser facilities and the High Pressure Collaborative Access Team for the use of the ruby system. We thank F. de Groot, J.-P. Rueff, W. Sturhahn, T. Tsuchiya, and W. J. Evans for helpful discussions and G. Shen, M. Hu, and K. Visbeck for their assistance in the experiments. Use of the APS was supported by U.S. Department of Energy (DOE, Office of Science, Basic Energy Sciences, under contract DE-AC02-06CH11357. GSECARS is supported by NSF Earth Sciences (EAR-0622171) and DOE Geosciences (DE-FG02-94ER14466, This work at LLNL was performed under the auspices of the U.S. DOE by University of California and LLNL under contract W-7405-Eng-48. J.-F.L. is also supported by the Lawrence Livermore Fellowship. S.D.J. acknowledges financial support from NSF/EAR 0721449, and V.V.S. acknowledges financial support from DOE. Science 317, 1743-1745 2007
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We acknowledge GSECARS, APS, and ANL for the use of the synchrotron and laser facilities and the High Pressure Collaborative Access Team for the use of the ruby system. We thank F. de Groot, J.-P. Rueff, W. Sturhahn, T. Tsuchiya, and W. J. Evans for helpful discussions and G. Shen, M. Hu, and K. Visbeck for their assistance in the experiments. Use of the APS was supported by U.S. Department of Energy (DOE), Office of Science, Basic Energy Sciences, under contract DE-AC02-06CH11357. GSECARS is supported by NSF Earth Sciences (EAR-0622171) and DOE Geosciences (DE-FG02-94ER14466). This work at LLNL was performed under the auspices of the U.S. DOE by University of California and LLNL under contract W-7405-Eng-48. J.-F.L. is also supported by the Lawrence Livermore Fellowship. S.D.J. acknowledges financial support from NSF/EAR 0721449, and V.V.S. acknowledges financial support from DOE. Science 317, 1743-1745 (2007)
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