Title:
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Electron momentum density studies of the electronic structure of complex systems : measurements and ab initio calculations
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A method for computing electron momentum densities and Compton profiles from
ab initio calculations is presented. This is employed, together with the momentum
density spectroscopy known as Compton scattering to investigate the electronic structure of MgCNi3. A method for computing the positron state within a material is also presented.
In our method for computing the electron momentum density, reciprocal space is
divided into optimally-shaped tetrahedra for interpolation, and the linear tetrahedron
method is used to obtain the momentum density and its projections such as Compton
profiles. Results are presented and evaluated against experimental data, showing good
agreement, and demonstrating the accuracy of our method.
For the intermetallic superconductor MgCNi3 , high-resolution x-ray Compton scattering
experiments were combined with electronic structure calculations to study a
sample with the composition MgCO.93 Ni2.85. Our calculations indicate that the electronic
structure, whilst smeared by disorder, does not drastically change in the presence
of vacancies, and provide an explanation for some of the discrepancies between
measurements of single crystals and polycrystals. Compton scattering measurements
were used to determine a Fermi surface in good agreement with that of our supercell
calculation, establishing the presence of the hole and electron Fermi surface sheets that
are necessary for the proposed two-gap model for the superconductivity. We identify
significant smearing of certain parts of the Fermi surface when C and Ni vacancies are
present.
To calculate the positron state, we have implemented two component density functional
theory in the limit of vanishing positron density. We present calculations of
the positron lifetime, affinity, and of the momentum density of annihilating electron-positron
pairs, for several materials, using a wide variety of electron-positron correlation
and enhancement schemes, finding excellent agreement with previous calculations
and experimental results. Possible limitations of the method are found in describing
positrons localised in vacancies .
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