THERMAL EQUATION OF STATE OF FE3P BY X-RAY DIFFRACTION: IMPLICATIONS FOR PHOSPHORUS IN THE PLANETARY CORES

2017 ◽  
Author(s):  
Xiaojing Lai ◽  
◽  
Bin Chen ◽  
Bin Chen ◽  
Feng Zhu ◽  
...  
2005 ◽  
Vol 66 (5) ◽  
pp. 706-710 ◽  
Author(s):  
G.A. Voronin ◽  
C. Pantea ◽  
T.W. Zerda ◽  
L. Wang ◽  
Y. Zhao

2018 ◽  
Vol 45 (10) ◽  
pp. 995-1001 ◽  
Author(s):  
Masayuki Nishi ◽  
Jun Tsuchiya ◽  
Takeshi Arimoto ◽  
Sho Kakizawa ◽  
Takehiro Kunimoto ◽  
...  

2014 ◽  
Vol 140 (16) ◽  
pp. 164508 ◽  
Author(s):  
Anna Y. Likhacheva ◽  
Sergey V. Rashchenko ◽  
Artem D. Chanyshev ◽  
Talgat M. Inerbaev ◽  
Konstantin D. Litasov ◽  
...  

2009 ◽  
Vol 94 (7) ◽  
pp. 071904 ◽  
Author(s):  
Yuejian Wang ◽  
Jianzhong Zhang ◽  
Hongwu Xu ◽  
Zhijun Lin ◽  
Luke L. Daemen ◽  
...  

2010 ◽  
Vol 95 (11-12) ◽  
pp. 1708-1716 ◽  
Author(s):  
E. J. Tronche ◽  
M. van Kan Parker ◽  
J. de Vries ◽  
Y. Wang ◽  
T. Sanehira ◽  
...  

2010 ◽  
Vol 107 (11) ◽  
pp. 113517 ◽  
Author(s):  
Xiaohui Yu ◽  
Zhijun Lin ◽  
Jianzhong Zhang ◽  
Liping Wang ◽  
Zejun Ding ◽  
...  

Minerals ◽  
2020 ◽  
Vol 10 (3) ◽  
pp. 212
Author(s):  
Richard L. Rowland ◽  
Barbara Lavina ◽  
Kathleen E. Vander Kaaden ◽  
Lisa R. Danielson ◽  
Pamela C. Burnley

Understanding basic material properties of rare earth element (REE) bearing minerals such as their phase stability and equations of state can assist in understanding how economically viable deposits might form. Bastnäsite is the most commonly mined REE bearing mineral. We synthesized the lanthanum-fluoride end member, bastnäsite-(La) (LaCO3F), and investigated its thermal behavior and decomposition products from 298 K to 1173 K under ambient pressure conditions through thermogravimetric analysis, differential scanning calorimetry, evolved gas analysis, and high temperature powder X-ray diffraction. We also investigated the compressibility of bastnäsite-(La) via single crystal X-ray diffraction in diamond anvil cells at an ambient temperature up to 11.3 GPa and from 4.9 GPa to 7.7 GPa up to 673 K. At ambient pressure, bastnäsite-(La) was stable up to 598 K in air, where it decomposed into CO2 and tetragonal γ-LaOF. Above 948 K, cubic α-LaOF is stable. High temperature X-ray diffraction data were used to fit the Fei thermal equation of state and the thermal expansion coefficient α298 for all three materials. Bastnäsite-(La) was fit from 298 K to 723 K with V0 = 439.82 Å3, α298 = 4.32 × 10−5 K−1, a0 = −1.68 × 10−5 K−1, a1 = 8.34 × 10−8 K−1, and a2 = 3.126 K−1. Tetragonal γ-LaOF was fit from 723 K to 948 K with V0 = 96.51 Å3, α298 = 2.95×10−4 K−1, a0 = −2.41×10−5 K−1, a1 = 2.42×10−7 K−1, and a2 = 41.147 K−1. Cubic α-LaOF was fit from 973 K to 1123 K with V0 = 190.71 Å3, α298 = −1.12×10−5 K−1, a0 = 2.36×10−4 K−1, a1 = −1.73 × 10−7 K−1, and a2 = −17.362 K−1. An ambient temperature third order Birch–Murnaghan equation of state was fit with V0 = 439.82 Å3, K0 = 105 GPa, and K’ = 5.58.


Minerals ◽  
2020 ◽  
Vol 10 (2) ◽  
pp. 98
Author(s):  
Eric Edmund ◽  
Francesca Miozzi ◽  
Guillaume Morard ◽  
Eglantine Boulard ◽  
Alisha Clark ◽  
...  

Knowledge of the elastic properties and equations of state of iron and iron alloys are of fundamental interest in Earth and planetary sciences as they are the main constituents of telluric planetary cores. Here, we present results of X-ray diffraction measurements on a ternary Fe–Ni–Si alloy with 5 wt% Ni and 5 wt% Si, quasi-hydrostatically compressed at ambient temperature up to 56 GPa, and under simultaneous high pressure and high temperature conditions, up to 74 GPa and 1750 K. The established pressure dependence of the c/a axial ratio at ambient temperature and the pressure–volume–temperature (P–V–T) equation of state are compared with previous work and literature studies. Our results show that Ni addition does not affect the compressibility and axial compressibility of Fe–Si alloys at ambient temperature, but we suggest that ternary Fe–Ni–Si alloys might have a reduced thermal expansion in respect to pure Fe and binary Fe–Si alloys. In particular, once the thermal equations of state are considered together with velocity measurements, we conclude that elements other than Si and Ni have to be present in the Earth’s inner core to account for both density and seismic velocities.


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