Elsevier

Calphad

Volume 64, March 2019, Pages 43-54
Calphad

Experimental investigations and thermodynamic modelling of the Cr–Nb–Sn–Zr system

https://doi.org/10.1016/j.calphad.2018.11.002Get rights and content

Abstract

This work reports the Calphad modelling of the Cr–Nb–Sn–Zr quaternary system. In a previous paper, the thermodynamic modelling of the Cr–Nb–Sn system was presented. Since no experimental data were available for the Cr–Sn–Zr ternary system, new experimental data are provided, within this study, on the isothermal section at 900 °C. A ternary C14 phase has been identified on the Sn-poor side of the phase diagram. In addition to these experimental data, Density Functional Theory (DFT) calculations are carried out in order to determine formation enthalpies of the stable and metastable compounds. At last, the Special Quasirandom Structures (SQS) method is jointly used with DFT calculations in order to estimate the mixing enthalpies of the A2 and A3 binary solid solutions. Finally, these experimental and calculated data in addition to those from the literature, are used as input data for the Calphad modelling of the Cr–Zr, Nb–Zr and Sn–Zr binary systems and the Cr–Nb–Zr, Cr–Sn–Zr and Nb–Sn–Zr ternary systems. A complete database for the Cr–Nb–Sn–Zr quaternary system is provided.

Introduction

Zirconium alloys are mainly used as fuel cladding and structural materials in Light Water Reactors (LWR) because of their very low thermal neutron absorption coefficient, their excellent mechanical properties and corrosion resistance and the relative stability of their properties under irradiation [1], [2]. In order to improve significantly the behaviour of the claddings, both in nominal and accidental conditions, it appears useful to have a better control of the microstructure and phase transformations occurring in these alloys, as a function of temperature and composition. In this frame, a new thermodynamic database dedicated to Zirconium alloys is being developed using the Calphad approach, considering the five following elements Zr, Cr, Fe, Nb, Sn. These elements allow the stabilization of Zr(Cr,Fe)2 precipitates (Zircaloy-4) or β-Nb solid solution (M5®) which improve the mechanical strength as well as the corrosion resistance of the alloys [3], [4]. The novelty of this work relies on the systematic use of the Density Functional Theory (DFT) calculations for the reassessment of the individual binary and ternary subsystems.

This paper presents the Calphad modelling of the Cr–Nb–Sn–Zr quaternary system. In a previous paper [5], we have already presented the thermodynamic modelling of the Cr–Nb–Sn ternary system based on new experimental and calculated data, reassessing the Cr–Nb, Cr–Sn and Nb–Sn binary systems. The Calphad modelling of the Cr–Nb–Sn ternary system and of the Cr–Nb and Nb–Sn binary systems is adopted from Ref. [5] but a new description of the Cr–Sn system is given in the present paper. Moreover, in the present study, a partial isothermal section of the Cr–Sn–Zr system was determined at 1173 K. Note that, to our knowledge, no experimental data had been previously determined for this ternary system before the present work. This isothermal section exhibits a ternary C14 phase on the Sn-poor region. In addition to the new experimental determination, we provide new DFT calculations of the formation enthalpies of all the quaternary end-members of the C14, C15 and C36 phases, of all the end-members of the A15 phase in the Nb–Sn–Zr system, and of η and ZrSn2 in the Sn-Zr system. DFT calculations on Special Quasirandom Structures (SQS) were performed to determine the mixing enthalpies of the A2 and A3 binary solid solutions. As it will be discussed in Section 4.3.2, a recent publication dedicated to the Calphad modelling of the Sn–Zr system [6] is available in the literature. Unfortunately, Perez et al. [6] used the formation enthalpies measured by Meschel et al. [7] that exhibit very large deviations from publications [8], [9], [10] and from our own DFT calculations. For the Nb–Zr system, a very thorough description is available in the literature [11]. Nevertheless, their authors have rejected some measurements of the monotectoid reaction which appear to be reliable due to a lower oxygen contamination of the samples. Moreover, a recent measurement of the monotectoid reaction temperature [12] shows important gap with the optimized one. At last, many researchers have performed thermodynamic modelling of the Cr–Zr system [13], [14], [15], [16] but the assessments were obtained without DFT calculations and the resulting formation enthalpies exhibit large deviations from the DFT ones. A very careful and recent publication dedicated to the Calphad modelling of the Cr–Zr system [17] is available in the literature. Unfortunately, Lu et al. [17] used a two-sublattice model for the description of the C14 and C36 Laves phases that is not compatible with our database.

Thus, the Cr–Zr, Nb–Zr and Sn–Zr binary systems have been reassessed.

The first part of this paper is dedicated to the literature survey of the binary systems, the second part is dedicated to the methodology of our approach and the third part to our results and the Calphad modelling of the different sub-systems of the quaternary system.

Section snippets

Experimental data

The Cr–Zr system has been studied by many researchers [17], [18], [19], [20], [21], [22], [23], [24], [25], [26], [27], [28], [29], [30]. This system includes three intermetallic phases, the C15, C36 and C14 Laves phases, ordered at Cr2Zr stoichiometry. This system presents two eutectic reactions, one eutectoid reaction and two metatectic reactions.

Domagala et al. [20], Gebhardt et al. [21] and Rumball et al. [24] determined the solubility of the terminal solid solutions on the Zr–rich side. In

Experimental details

The samples were prepared from high purity metals (Cr from Alfa Aesar (99.99%), Sn from Alfa Aesar (99.8%) and Zr “Van Arkel” (55 ppm of oxygen) from LTMEX-CEA) by arc melting under argon atmosphere. The alloys were melted five times and turned upside down between each melting. The weight losses were not significant. The samples were then wrapped in molybdenum sheets (less reactive than Ta with the possible presence of liquid Sn) and placed in a silica tube sealed under argon. After annealing,

Calphad assessment

The thermodynamic assessment of Cr–Sn system published in Ref [5] has been revised to avoid excessively large excess entropic parameters for the liquid and the bcc phases. This could be achieved only by introducing third order non-temperature dependent parameters for this phase. The list of updated parameters can be found in Table 2.

DFT results

Fig. 1 shows the 0 K calculated formation enthalpies of the end-members of the C14, C15 and C36 Laves phase as a function of the mole fraction of zirconium,

Conclusions

The thermodynamic modelling of the Cr–Nb–Sn–Zr quaternary system has been performed using the Calphad approach according to our new experimental and calculated data and the combination of the assessed ternary sub-systems. Note that the thermodynamic modelling of the Cr–Nb–Sn system was presented in a previous paper [5] and the assessment of the Cr–Sn has since been slightly modified.

The experimental study has been carried out in order to determine several phase equilibria in the isothermal

Acknowledgements

Eric Bouaravong and Didier Hamon are acknowledged for the synthesis and EPMA measurements, respectively. SQS and DFT calculations were performed using HPC resources from GENCI–CINES (Grant 2017-096175 and den0006). The authors wish to thank the GDR CNRS no 3584 TherMatHT for fruitful discussions and collaborative work on the present project. This work was conducted and funded within the framework of the French Tripartite Institute CEA/EDF/Framatome [Projet Gaine].

Data statement

All data generated or analysed during this study are included in this published article

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