2009
DOI: 10.1016/j.jnucmat.2009.06.005
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Point defect properties in hcp and bcc Zr with trace solute Nb revealed by ab initio calculations

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Cited by 33 publications
(14 citation statements)
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“…The solution energy for infinite dilution is Ω β mix (x → 0) = 0.312 eV for Zr impurity in β-Nb, and Ω α mix (x → 1) = 0.632 eV for Nb impurity in α-Zr, in agreement with previous ab initio calculations (0.61 eV for Domain [62] and 0.68 eV for Xin et al [51]). Our results are also consistent with the asymmetry observed in the phase diagram, as the high value of Ω α mix explains the very low solubility of niobium in hcp zirconium, whereas the lower value of Ω β mix corresponds to a higher solubility of zirconium in bcc niobium.…”
Section: Solution Energysupporting
confidence: 90%
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“…The solution energy for infinite dilution is Ω β mix (x → 0) = 0.312 eV for Zr impurity in β-Nb, and Ω α mix (x → 1) = 0.632 eV for Nb impurity in α-Zr, in agreement with previous ab initio calculations (0.61 eV for Domain [62] and 0.68 eV for Xin et al [51]). Our results are also consistent with the asymmetry observed in the phase diagram, as the high value of Ω α mix explains the very low solubility of niobium in hcp zirconium, whereas the lower value of Ω β mix corresponds to a higher solubility of zirconium in bcc niobium.…”
Section: Solution Energysupporting
confidence: 90%
“…The obtained values, listed in Table 1, are close to experimental data. The vacancy formation energies also agree with experiments [48][49][50], and with previous ab initio calculations [51,52].…”
Section: Dft Parameterssupporting
confidence: 90%
“…The results will be easily included in the analytical expressions derived in this Letter. These expressions are straightforward to apply in other relevant materials, e.g., transition metals rare earth oxides [60], AlZr [61]), ZrNb [62], FeCr [63], or NiC [64][65][66]. A striking feature highlighted in this Letter which should occur in many systems is the nonlinearities of the effective vacancy formation free enthalpy, within temperature ranges for which it is conventionally admitted that an Arrhenius law is valid.…”
Section: Vxmentioning
confidence: 86%
“…The critical size for the first structural change of the Cu clusters from bcc to 9R is greater than the size of Nb clusters estimated by APT in this study. With respect to the process of precipitation of the bcc Nb phase in the ZreNb alloys, Xin and Liu have speculated that the precipitation of bcc Nb under irradiation occurs in two steps: a domain of the hcp Zr matrix first transforms into bcc Zr and then Nb atoms substitute Zr atoms in the bcc lattice [57]. Their hypothesis is based on the energy consideration of the binding energy between Nb atoms in bcc Zr and hcp Zr, derived from ab initio calculations: the formation of Nb clusters is energetically more favored in bcc Zr rather than in hcp Zr.…”
Section: Discussionmentioning
confidence: 99%