Ian G. Wood,* Jabraan Ahmed, David P. Dobson and Lidunka Vocˇadlo
Department of Earth Sciences, University College London, Gower Street, London WC1E 6BT,
England. Correspondence e-mail: ian.wood@ucl.ac.uk
Received 27 July 2012 Accepted 15 November 2012
Abstract:
A new high-pressure phase of NiSi has been synthesized in a multi-anvil press by
quenching samples to room temperature from 1223–1310 K at 17.5 GPa and
then recovering them to atmospheric pressure. The crystal structure of this
recovered material has been determined from X-ray powder diffraction data;
the resulting fractional coordinates are in good agreement with those obtained
from an ab initio computer simulation. The structure, in which each atom is sixfold
coordinated by atoms of the other kind, is orthorhombic (space group
Pmmn) with a = 3.27, b = 3.03, c = 4.70 A˚ . This orthorhombic phase of NiSi may
be considered as a ferroelastic distortion of the hypothetical tetragonal (space
group P4/nmm) NiSi structure that was predicted to be the most stable phase (at
0 K) for pressures between 23 and 61 GPa in an earlier ab initio study by
Vocˇadlo, Wood & Dobson [J. Appl. Cryst. (2012), 45, 186–196]. Further ab initio
simulations have now shown that, with increasing pressure (at 0 K), NiSi is
predicted to exist in the following polymorphs: (i) the MnP structure; (ii) the
new orthorhombic structure with space group Pmmn; and (iii) the CsCl
structure. Experimentally, all of these structures have now been observed and, in
addition, a fourth polymorph, an "-FeSi-structured phase of NiSi (never the
most thermodynamically stable phase in athermal ab initio simulations), may be
readily synthesized at high pressure (P) and temperature (T). On the basis of
both experiments and computer simulations it is therefore now clear that the
phase diagram of NiSi at high P and T is complex. The simulated free-energy
differences between different structures are often very small (<10 meV atom1
)
and there is also the possibility of two displacive ferroelastic phase
transformations, the first between structures with Pmmn and P4/nmm symmetry,
and the second from P4/nmm to a different orthorhombic phase of NiSi with
space group Pbma. A complete understanding of the NiSi phase diagram (which
may be of relevance to both planetary cores and the use of thin films of NiSi in
semiconductor technology) can, therefore, only come via in situ experiments at
simultaneous high P and high T.
To download the article click on the link below:
http://www.ucl.ac.uk/EarthSci/people/lidunka/papers/76.pdf

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