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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Mueller, Hans J.
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article
The phase diagram of NiSi under the conditions of small planetary interiors
Abstract
The phase diagram of NiSi has been determined using <em>in situ</em>synchrotron X-ray powder diffraction multi-anvil experiments to 19 GPa,with further preliminary results in the laser-heated diamond cellreported to 60 GPa. The low-pressure MnP-structured phase transforms totwo different high-pressure phases depending on the temperature: theε-FeSi structure is stable at temperatures above ∼1100 K and apreviously reported distorted-CuTi structure (with <em>Pmmn</em>symmetry) is stable at lower temperature. The invariant point is locatedat 12.8 ± 0.2 GPa and 1100 ± 20 K. At higher pressures, ε-FeSi-structured NiSi transforms to the CsCl structure with CsCl-NiSi asthe liquidus phase above 30 GPa. The Clapeyron slope of this transitionis -67 MPa/K. The phase boundary between the ε -FeSi and <em>Pmmn</em>structured phases is nearly pressure independent implying there will be asecond sub-solidus invariant point between CsCl, ε -FeSi and <em>Pmmn</em>structures at higher pressure than attained in this study. In additionto these stable phases, the MnP structure was observed to spontaneouslytransform at room temperature to a new orthorhombic structure (also with<em>Pnma</em> symmetry) which had been detailed in previous <em>ab initio</em> simulations. This new phase of NiSi is shown here to be metastable.