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Lu et al. J Mater Inf 2022;2:11  I http://dx.doi.org/10.20517/jmi.2022.15         Page 5 of 18


                                Table 2. Crystallographic and model information of stable phases in Ni-Mo-Re system
                                Phase    Pearson symbol  Prototype  Model
                                Liquid   -             -         (Ni,Mo,Re) 1
                                fcc_A1   cF4           Cu        (Ni,Mo,Re) 1(VA) 1
                                bcc_A2   cI2           W         (Ni,Mo,Re) 1(VA) 3
                                hcp_A3   hP2           Mg        (Ni,Mo,Re) 1(VA) 0.5
                                         oP56          NiMo      (Ni) 24(Ni,Mo,Re) 20(Mo) 12
                                Ni 3Mo   oP8           Cu 3Ti    (Ni,Mo) 3(Ni,Mo) 1
                                Ni 4Mo   tI10          Ni 4Mo    (Ni) 4(Mo) 1
                                         tP30          CrFe      (Ni,Mo,Re) 2(Ni,Mo,Re) 4(Ni,Mo,Re) 8
                                                                 (Ni,Mo,Re) 8(Ni,Mo,Re) 8
                                         cI58            -Mn     (Ni,Mo,Re) 2(Ni,Mo,Re) 8(Ni,Mo,Re) 24
                                                                 (Ni,Mo,Re) 24
                                bct      tI56          Mo 3CoSi  (Mo,Re) 9(Ni,Re) 4(Ni) 1


               cell volume only, then to volume and cell shape, and finally simultaneously to volume, cell shape and atomic
               position (i.e., full relaxation) in the present work. On this basis, a fast convergence speed can be achieved. To
               check the symmetry preservation, the radial distribution functions were analyzed [64] .

               In addition, VASP calculations were also performed to obtain the formation energies of all the end-members
               of the    and    phases. The k-point meshes were 12 × 12 × 12 and 8 × 8 × 15, respectively. To facilitate
               the calculations, the ZenGen script-tool [65]  was adopted to conveniently generate input files for the VASP
               calculations.



               THERMODYNAMIC MODELS
               In the Ni-Mo-Re system, the stable phases included in this assessment are liquid, fcc, bcc, hcp,   , Ni 3Mo,
               Ni 4Mo,   ,    and the bct phase with a Mo 3CoSi structural prototype. Their crystal structure information and
               the thermodynamic models are summarized in Table 2. The thermodynamic descriptions of the pure elements
               Ni, Mo and Re were taken from the Scientific Group Thermodata Europe (SGTE) unary database (Version
               5.0) [66] . All the phases were described by the sublattice model within CEF. Detailed mathematical expressions
               are available in our previous work [67] .

               Solution phases
               The solution phases (including liquid, fcc, bcc and hcp) were treated as substitutional solutions and described
               by a substitutional solution model with the Redlich-Kister polynomials [68] .

                                                                                                       
                                                                                            
                                                                                                 
               Normally, for the interaction parameter, a linear temperature dependence is sufficient, i.e.,         ,    +      ,   +      ,     .
               In the present work, the measured excess heat capacity for the fcc phase of the Ni-Mo system is available, so a
                     (  ) term was introduced to produce a constant excess heat capacity.
               Intermetallic phases
               In the present work, three intermetallic phases, i.e.,   , Ni 3Mo and Ni 4Mo, were considered for the Ni-Mo
               system. The solubility of Re was ignored in both Ni 3Mo and Ni 4Mo due to the lack of experimental data.

               The molar Gibbs energy of each intermetallic phase    is described as:
                                                           (              )
                                             ∑             ∑     ∑
                                                                                     
                                             =            +              ln        +       ;           (1)
                                                                       
                                                      
                                                                    
                                                                       
                                                                    
                        
               where    is the site fraction of component i in the sublattice s,    is the Gibbs free energy of the end member
                        
                                                                       
                                                                               
                                      
               I, R is the gas constant,    as is the number of sites of sublattice s and             corresponds to the molar excess
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