2014
DOI: 10.1007/s11837-014-0882-6
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From Electronic Structure to Thermodynamics of Actinide-Based Alloys

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Cited by 9 publications
(4 citation statements)
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“…Another challenging aspect of these heavy materials is the need to account for all relativistic effects, including spin-orbit interaction. Previous DFT studies on the bcc and fcc phases for actinide alloys have revealed that a fully-relativistic treatment is necessary for an accurate determination of the energetics of all Pu-based alloys [20,32,33,34]. Because relativistic effects cannot be ignored, the exact muffin-tin orbital (EMTO) electronic-structure method has been utilized here that applies a fully relativistic (FR) Green's function technique (based on the improved screened Korringa-Kohn-Rostoker method).…”
Section: Ab Initio Methods and Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Another challenging aspect of these heavy materials is the need to account for all relativistic effects, including spin-orbit interaction. Previous DFT studies on the bcc and fcc phases for actinide alloys have revealed that a fully-relativistic treatment is necessary for an accurate determination of the energetics of all Pu-based alloys [20,32,33,34]. Because relativistic effects cannot be ignored, the exact muffin-tin orbital (EMTO) electronic-structure method has been utilized here that applies a fully relativistic (FR) Green's function technique (based on the improved screened Korringa-Kohn-Rostoker method).…”
Section: Ab Initio Methods and Resultsmentioning
confidence: 99%
“…(a) Heats of formation (symbols, in kJ/mol) of the bcc phase for the Am-U[34], Am-Np[34], Am-Pu[33] and Pu-U[32] alloys and of the fcc phase for Am-U (present study) and Am-Pu [20] systems at T = 0 K, based on the FR-EMTO-CPA method. (b) Metastable miscibility gaps calculated using Eq.…”
mentioning
confidence: 99%
“…4 Liquidus and solidus curves from Bochvar et al [3] , Marples [4] , Taylor [15] , Maeda et al [30] , and Leibowitz et al [31] . Redrawn from Maeda et al [30] and presented by Turchi and Perron in [40] , reproduced here with permission from ANS the composition variation of the heat of formation of the bcc phase (e-Pu, b-Zr) of Pu-Zr obtained from these three assessments [1,32,33] with the one from ab initio electronic structure calculations performed with the fully-relativistic (FR) exact muffin-tin orbital (EMTO) and coherent potential approximation (CPA) methods (FR-EMTO-CPA) at T = 0 K. [34,35] As observed in Fig. 7, there is a common major disagreement: The ab initio results show a change of sign around 46 at.% Zr with a tendency toward phase separation for plutonium-rich alloys and a tendency toward phase formation for zirconium-rich alloys, although the overall magnitude of the heat of formation is small, in contrast with the three thermodynamic assessments, which clearly indicate a tendency toward phase separation in the entire range of alloy composition and much higher values for the heat of formation.…”
Section: Thermodynamic Modelingmentioning
confidence: 99%
“…Despite the demonstrable value of CSP for many classes of materials [21][22][23][24][25][26][27][28][29][30][31][32], and the continuing progress evidenced by a series of blind tests [33][34][35][36][37][38], the success of CSP for molecular crystals has been limited by the inability to routinely predict the relative stability of competing candidate structures [38]. This is largely because the methods used for stability rankings typically ignore or approximate the subtle interplay of several effects, such as intricate inter-molecular interactions [39], the (quantum) statistical mechanics of the nuclei [40] and the unit cell [41], and thermal expansion [42], thereby incurring errors larger than the free energy differences of interest.…”
mentioning
confidence: 99%