Tatsuya Sakamaki

Dr. Tatsuya Sakamaki


Research Focus & Metrics

Academic Career Length

24Years (2003-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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27 October 2013 in Nature Geoscience
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TSTatsuya Sakamaki
Tatsuya Sakamaki
ASAkio Suzuki
Akio Suzuki
EOEiji Ohtani
Eiji Ohtani
HTHidenori Terasaki
Hidenori Terasaki
SUSatoru Urakawa
Satoru Urakawa
MBMaxim D. Ballmer
Maxim D. Ballmer

30 January 2014 in Nature Communications
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YWYanbin Wang
Yanbin Wang
TSTatsuya Sakamaki
Tatsuya Sakamaki
LSLawrie B. Skinner
Lawrie B. Skinner
ZJZhicheng Jing
Zhicheng Jing
TYTony Yu
Tony Yu
SSStephen R. Sutton
Stephen R. Sutton
A defining characteristic of silicate melts is the degree of polymerization (tetrahedral connectivity), which dictates viscosity and affects compressibility. While viscosity of depolymerized silicate melts increases with pressure consistent with the free-volume theory, isothermal viscosity of polymerized melts decreases with pressure up to ~3–5 GPa, above which it turns over to normal (positive) pressure dependence. Here we show that the viscosity turnover in polymerized liquids corresponds to the tetrahedral packing limit, below which the structure is compressed through tightening of the inter-tetrahedral bond angle, resulting in high compressibility, continual breakup of tetrahedral connectivity and viscosity decrease with increasing pressure. Above the turnover pressure, silicon and aluminium coordination increases to allow further packing, with increasing viscosity and density. These structural responses prescribe the distribution of melt viscosity and density with depth and play an important role in magma transport in terrestrial planetary interiors.

1 January 2006 in Nature
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TSTatsuya Sakamaki
Tatsuya Sakamaki
ASAkio Suzuki
Akio Suzuki
EOEiji Ohtani
Eiji Ohtani

1 June 2014 in Earth and Planetary Science Letters
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ZJZhicheng Jing
Zhicheng Jing
YWYanbin Wang
Yanbin Wang
YKYoshio Kono
Yoshio Kono
TYTony Yu
Tony Yu
TSTatsuya Sakamaki
Tatsuya Sakamaki
GSGUOYIN SHEN
GUOYIN SHEN

5 February 2016 in Science Advances
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TSTatsuya Sakamaki
Tatsuya Sakamaki
EOEiji Ohtani
Eiji Ohtani
HFHiroshi Fukui
Hiroshi Fukui
SKSeiji Kamada
Seiji Kamada
STSuguru Takahashi
Suguru Takahashi
ABAlfred Q. R. Baron
Alfred Q. R. Baron
Experimental determination of V P of hcp-Fe can show potential candidates for major light elements in Earth’s inner core.

13 January 2017 in Scientific Reports
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FMFumiya Maeda
Fumiya Maeda
EOEiji Ohtani
Eiji Ohtani
SKSeiji Kamada
Seiji Kamada
TSTatsuya Sakamaki
Tatsuya Sakamaki
NHNaohisa Hirao
Naohisa Hirao
YOYasuo Ohishi
Yasuo Ohishi
Diamond is an evidence for carbon existing in the deep Earth. Some diamonds are considered to have originated at various depth ranges from the mantle transition zone to the lower mantle. These diamonds are expected to carry significant information about the deep Earth. Here, we determined the phase relations in the MgCO3-SiO2 system up to 152 GPa and 3,100 K using a double sided laser-heated diamond anvil cell combined with in situ synchrotron X-ray diffraction. MgCO3 transforms from magnesite to the high-pressure polymorph of MgCO3, phase II, above 80 GPa. A reaction between MgCO3 phase II and SiO2 (CaCl2-type SiO2 or seifertite) to form diamond and MgSiO3 (bridgmanite or post-perovsktite) was identified in the deep lower mantle conditions. These observations suggested that the reaction of the MgCO3 phase II with SiO2 causes formation of super-deep diamond in cold slabs descending into the deep lower mantle.