Laser-shock compression of diamond and evidence of a negative-slope melting curve

2007 ◽  
Vol 6 (4) ◽  
pp. 274-277 ◽  
Author(s):  
Stéphanie Brygoo ◽  
Emeric Henry ◽  
Paul Loubeyre ◽  
Jon Eggert ◽  
Michel Koenig ◽  
...  
2013 ◽  
Vol 67 (7) ◽  
Author(s):  
Stefano Paleari ◽  
Dimitri Batani ◽  
Tommaso Vinci ◽  
Roberto Benocci ◽  
Keisuke Shigemori ◽  
...  

2018 ◽  
Vol 124 (3) ◽  
pp. 035904 ◽  
Author(s):  
Alex W. Bryant ◽  
David Scripka ◽  
Faisal M. Alamgir ◽  
Naresh N. Thadhani

2012 ◽  
Vol 26 (07) ◽  
pp. 1250050 ◽  
Author(s):  
VU VAN HUNG ◽  
LE DAI THANH

The high-pressure melting curve of semiconductors with defects has been studied using statistical moment method (SMM). In agreement with experiments and with DFT calculations we obtain a negative slope for the high-pressure melting curve. We have derived a new equation for the melting curve of the defect semiconductors. The melting was investigated at different high pressures, and the SMM calculated melting temperature of Si, AlP, AlAs and GaP crystals with defects being in good agreement with previous experiments.


2016 ◽  
Vol 2 (8) ◽  
pp. e1600157 ◽  
Author(s):  
Toshimori Sekine ◽  
Norimasa Ozaki ◽  
Kohei Miyanishi ◽  
Yuto Asaumi ◽  
Tomoaki Kimura ◽  
...  

Forsterite (Mg2SiO4) is one of the major planetary materials, and its behavior under extreme conditions is important to understand the interior structure of large planets, such as super-Earths, and large-scale planetary impact events. Previous shock compression measurements of forsterite indicate that it may melt below 200 GPa, but these measurements did not go beyond 200 GPa. We report the shock response of forsterite above ~250 GPa, obtained using the laser shock wave technique. We simultaneously measured the Hugoniot and temperature of shocked forsterite and interpreted the results to suggest the following: (i) incongruent crystallization of MgO at 271 to 285 GPa, (ii) phase transition of MgO at 285 to 344 GPa, and (iii) remelting above ~470 to 500 GPa. These exothermic and endothermic reactions are seen to occur under extreme conditions of pressure and temperature. They indicate complex structural and chemical changes in the system MgO-SiO2 at extreme pressures and temperatures and will affect the way we understand the interior processes of large rocky planets as well as material transformation by impacts in the formation of planetary systems.


2011 ◽  
Vol 59 (13) ◽  
pp. 5276-5287 ◽  
Author(s):  
C.T. Wei ◽  
B.R. Maddox ◽  
A.K. Stover ◽  
T.P. Weihs ◽  
V.F. Nesterenko ◽  
...  

2015 ◽  
Vol 92 (2) ◽  
Author(s):  
K. Miyanishi ◽  
Y. Tange ◽  
N. Ozaki ◽  
T. Kimura ◽  
T. Sano ◽  
...  

2003 ◽  
Vol 110 ◽  
pp. 851-856 ◽  
Author(s):  
M. A. Meyers ◽  
M. S. Schneider ◽  
B. K. Kad ◽  
V. A. Lubarda ◽  
F. Gregori ◽  
...  

2019 ◽  
Vol 33 ◽  
pp. 100703
Author(s):  
S. Morioka ◽  
N. Ozaki ◽  
M. Hosomi ◽  
K. Katagiri ◽  
T. Matsuoka ◽  
...  

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