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

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374 18. Plutonium group 17 (halogen) compounds <strong>and</strong> complexesAppendix A, <strong>and</strong> combination with the enthalpy <strong>of</strong> protonation <strong>of</strong> the fluoride ion, f H ◦ m = (12.2±0.3) kJ·mol−1 , results in the following selected values: r Hm ◦ (18.9, q = 1, 298.15 K) = (9.1 ± 2.2) kJ·mol−1 r Hm ◦ (18.9, q = 2, 298.15 K) = (11 ± 5) kJ·mol−1From this value, we derive the enthalpies <strong>of</strong> formation <strong>and</strong> the entropies <strong>of</strong> PuF 3+<strong>and</strong> PuF 2+2 : f H ◦ m (PuF3+ , aq, 298.15 K) = −(866.1 ± 3.9) kJ·mol −1 f Hm ◦ (PuF2+ 2, aq, 298.15 K) = −(1199.6 ± 6.0) kJ·mol−1S ◦ m (PuF3+ , aq, 298.15 K) = −(229 ± 13) kJ·mol −1Sm ◦ (PuF2+ 2, aq, 298.15 K) = −(105 ± 20) kJ·mol−118.2.1.3 Aqueous Pu(V) fluoridesNo fluoride complexes <strong>of</strong> PuO + 2 have been identified. Values for the NpO+ 2 complexesmay be used as a guideline.18.2.1.4 Aqueous Pu(VI) fluoridesAs in the case <strong>of</strong> <strong>neptunium</strong>(VI), the investigation <strong>of</strong> fluoride complexation <strong>of</strong> <strong>plutonium</strong>(VI)is complicated by the fact that reduction <strong>of</strong> PuO 2+2to Pu(IV) is favouredin acidic medium <strong>and</strong> in the presence <strong>of</strong> fluoride ion. The constants reported in theliterature refer to either <strong>of</strong> the following reaction types,PuO 2+2+ qHF(aq) Å PuO 2 F 2−qq + qH + (18.10)PuO 2+2+ qF − Å PuO 2 F 2−qq , (18.11)depending whether the fluoride ion was protonated or deprotonated under the experimentalconditions. The constants are listed in Table 18.2. As in the case <strong>of</strong> Np(VI),the study published by Krylov, Komarov <strong>and</strong> Pushlenkov [68KRY/KOM2] yields constantsthat are unrealistically high, probably again due to reduction <strong>of</strong> Pu(VI) duringthe experiment (cf. Appendix A). The study <strong>of</strong> Savage [74SAV] is a rather approximateone reporting an even higher formation constant <strong>of</strong> PuO 2 F + , calculated via theformation <strong>of</strong> a hydroxide complex, <strong>and</strong> must be discarded as well. Since the results<strong>of</strong> Patil <strong>and</strong> Ramakrishna [76PAT/RAM] are also discarded (cf. Appendix A), due toa very strong trend in the results, the only remaining data are those <strong>of</strong> Choppin <strong>and</strong>Rao [84CHO/RAO] <strong>and</strong> Sawant et al. [85SAW/CHA] referring to Reaction (18.11).Correction <strong>of</strong> these constants to I = 0byusingε(18.11, q = 1) = −(0.19 ±0.10) kg·mol −1 , as was done for the corresponding <strong>neptunium</strong> system above, yieldsvalues that are not incompatible (cf. Table 18.2). We select the weighted average <strong>of</strong>these constants, but we increase the resulting uncertainty <strong>of</strong> ±0.10 to ±0.20 to reflect

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