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chemical thermodynamics of neptunium and plutonium - U.S. ...

chemical thermodynamics of neptunium and plutonium - U.S. ...

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12.1 Neptunium carbon compounds <strong>and</strong> complexes 285ε(12.45, q = 1) =−(0.13 ± 0.10) kg·mol −1 <strong>and</strong> ε(12.45, q = 2) =−(0.56 ±0.19) kg·mol −1 , after increasing the uncertainties by ±0.05 due to the estimation byanalogy. For the 1:3 reaction, we use ε (Np(SCN)+3 ) ≈ ε (AmF + 2 ) = 0.17 kg·mol−1 ,whichresults in ε(12.45, q = 3) =−(0.82 ± 0.13) kg·mol −1 , after increasing the uncertaintyby ±0.05 due to the analogy made. The resulting values at I = 0 are listed inTable 12.8. The values at 25 ◦ C determined with TTA <strong>and</strong> DNNS agree well. We estimatethat the uncertainties <strong>of</strong> these values, taking systematic errors into account, arearound ±0.1 logarithmic units for the formation <strong>of</strong> the 1:1 complex <strong>and</strong> ±0.2 forthe1:2 <strong>and</strong> 1:3 complexes. We select the average <strong>of</strong> these values <strong>and</strong> assign uncertaintiesthat reflect the fact that no independent study is is available on this system.log 10 β1 ◦ (12.45, q = 1, 298.15 K) = 3.0 ± 0.3log 10 β2 ◦ (12.45, q = 2, 298.15 K) = 4.1 ± 0.5log 10 β3 ◦ (12.45, q = 3, 298.15 K) = 4.8 ± 0.5Rao et al. [78RAO/BAG2] performed their measurements at 10, 25 <strong>and</strong> 40 ◦ C, cf.Table 12.8. From the temperature dependence <strong>of</strong> the resulting equilibrium constants,they derived enthalpy values, cf. Appendix A. The values <strong>of</strong> β 2 at different temperaturesshow no steady variation, which gives an indication <strong>of</strong> appreciable uncertainty.Due to lack <strong>of</strong> information, we assume the enthalpies to be independent <strong>of</strong> the ionicstrength <strong>and</strong> assign the uncertainties accordingly. r Hm ◦ (12.45, q = 1, 298.15 K) = −(7 ± 3) kJ·mol−1 r Hm ◦ (12.45, q = 2, 298.15 K) = −(9 ± 9) kJ·mol−1 r Hm ◦ (12.45, q = 3, 298.15 K) = −(13 ± 9) kJ·mol−1The thermodynamic formation data are derived from these constants <strong>and</strong> the selecteddata for Np 4+ <strong>and</strong> SCN − : f G ◦ m (NpSCN3+ , aq, 298.15 K) = −(416 ± 7) kJ·mol −1 f G ◦ m (Np(SCN)2+ 2, aq, 298.15 K) = −(330 ± 10) kJ·mol−1 f G ◦ m (Np(SCN)+ 3, aq, 298.15 K) = −(241 ± 14) kJ·mol−1 f H ◦ m (NpSCN3+ , aq, 298.15 K) = −(487 ± 7) kJ·mol −1 f Hm ◦ (Np(SCN)2+ 2, aq, 298.15 K) = −(412 ± 13) kJ·mol−1 f Hm ◦ (Np(SCN)+ 3, aq, 298.15 K) = −(340 ± 16) kJ·mol−1Sm ◦ (NpSCN3+ , aq, 298.15 K) =−1−(248 ± 25) J·K−1·molSm ◦ (Np(SCN)2+ 2, aq, 298.15 K) =−1−(90 ± 51) J·K−1·molSm ◦ (Np(SCN)+ 3, aq, 298.15 K) =−1(55 ± 66) J·K−1·mol

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