ChemComm
Communication
The authors gratefully acknowledge the Chemical Sciences,
Geosciences, and Biosciences Division, Office of Basic Energy
Sciences, Early Career Research Program of the U.S. Department of
Energy, under Award Nos. DE-SC0006518 and DE-FG02-11ER16239
for support of this work. The University of Pennsylvania and the
Research Corporation for Science Advancement (Cottrell Scholar
Award to E.J.S.) are also acknowledged for financial support. We
thank the U.S. National Science Foundation for support of the
computing cluster (CHE-0131132) used in this work. This work also
Fig. 3 Calculated HOMO and LUMO of complex 1.
DFT calculations on 1 were performed at the B3LYP level of used the Extreme Science and Engineering Discovery Environment
theory, with the ECP28MWB pseudopotential21 for the cerium cation. (XSEDE), which is supported by U.S. National Science Foundation
The geometry optimized bond distances and angles for 1 agree well grant number OCI-1053575.
with the experimental values. The resulting molecular orbital
depiction shows that the HOMO comprises primarily hydroxamate
p* orbital character with an B6% contribution from the cerium
4fz(x2ꢀy2) orbital (Fig. 3). The hydroxamate ligands are oriented at the
Notes and references
1 D. A. Atwood, The rare earth elements: fundamentals and applications,
cerium cation to allow for a symmetry-matched bonding interaction
between the N–O p* orbitals and a 4f orbital of cerium, though the
overlap is small. The LUMO is calculated to be 2.95 eV above the
HOMO and consists of the corresponding antibonding interaction.
Furthermore, the natural population analysis shows a high degree of
charge donation into the central metal cation as indicated by a low
natural charge of the cerium metal centre of 1.41. A similar electronic
structure was observed in the homoleptic Ce[2-(tBuNO)py]4 complex
reported recently by our group,9 providing further evidence that there
is an electronic preference for the pseudo-cubic D2d symmetry
observed in the 8-coordinate k2-nitroxide complexes.
Evidence in support of the calculated electronic structure and
electrochemistry of 1 was determined using UV-visible electronic
absorption spectroscopy (Fig. S9, ESI†). A broad transition at 2.93 eV
was assigned to a LMCT from the hydroxamate ligand field to a
metal 4f orbital. The energy of this transition is in good agreement
with the calculated energy gap between the HOMO and the LUMO
of 2.95 eV. The broadness of this transition can be attributed to
partial mixing of the ligand-based orbitals with the metal-based 4f
orbitals (Fig. 3). A similar spectroscopic interpretation has been
advanced for tetrakis(b-diketonato) cerium complexes.22
John Wiley & Sons Ltd, 2012, 2nd edn.
2 A. Jordens, Y. P. Cheng and K. E. Waters, Miner. Eng., 2013, 41,
97–114.
3 (a) J. Cui, G. A. Hope and A. N. Buckley, Miner. Eng., 2012, 36–38, 91–99;
(b) Pradip and D. W. Fuerstenau, Adv. Sci. Technol. Miner. Benefic. India,
Proc. Symp., 1983, 217–228.
4 Pradip and D. W. Fuerstenau, M&MP, 2013, 30, 1–9.
5 (a) O. Pavez, P. R. G. Brandao and A. E. C. Peres, Miner. Eng., 1996, 9,
357–366; (b) Pradip and D. W. Fuerstenau, Colloids Surf., 1983, 8,
103–119.
6 K. R. Long, G. Van, N. K. Foley and D. Cordier, U. S. Geological
Survey, Scientific Investigations Report, 2010–5220, 1–96.
7 (a) Y. K. Agrawal and H. L. Kapoor, Ann. Chim., 1976, 66, 117–126;
(b) Y. K. Agrawal and H. L. Kapoor, Analusis, 1977, 5, 62–69;
(c) P. C. Verma, P. V. Khadikar and Y. K. Agrawal, Indian J. Chem.,
1976, 14A, 637–638; (d) Y. K. Agrawal, Indian J. Chem., 1976, 14A, 1024;
(e) Y. K. Agrawal, Chem. Anal., 1977, 22, 215–220; ( f ) B. S. Chandravanshi
and V. K. Gupta, Croat. Chem. Acta, 1984, 57, 243–249; (g) Y. K. Agrawal
and J. P. Shukla, J. Indian Chem. Soc., 1974, 51, 373; (h) H. L. Kapoor,
Y. K. Agrawal and P. C. Verma, Talanta, 1975, 22, 193–196; (i) Y. K.
Agrawal and H. L. Kapoor, Talanta, 1976, 23, 235; ( j) S. K. Brahma and
A. K. Chakraburtty, J. Indian Chem. Soc., 1981, 58, 615–617.
8 I. P. Alimarin, I. V. Sokolova and L. I. Ustinova, Russ. Chem. Bull.,
1974, 23, 486–488.
9 J. A. Bogart, A. J. Lewis, S. A. Medling, N. A. Piro, P. J. Carroll,
C. H. Booth and E. J. Schelter, Inorg. Chem., 2013, 52, 11600–11607.
10 (a) J. Cervini-Silva, D. A. Fowle and J. Banfield, Am. J. Sci., 2005, 305,
711–726; (b) J. Cervini-Silva, B. Gilbert, S. Fakra, S. Friedlich and
J. Banfield, Geochim. Cosmochim. Acta, 2008, 72, 2454–2464.
11 S. R. Sofen, S. R. Cooper and K. N. Raymond, Inorg. Chem., 1979, 18,
1611–1616.
In total, our results suggest that the thermodynamics of cerium
hydroxamate complexes strongly favour oxidation to the cerium(IV)
state. Given the typical pKa range for hydroxamic acids of B8.0–8.5,
we expect that the aerated (aerobic) and basic (pH = 9.5) conditions
of froth flotation3b strongly favour binding and oxidation of cerium
12 (a) P. E. Riley, K. Abu-Dari and K. N. Raymond, Inorg. Chem., 1983,
22, 3940–3944; (b) M. Seitz, M. D. Pluth and K. N. Raymond, Inorg.
Chem., 2006, 46, 351–353; (c) A. E. V. Gorden, J. Xu, G. Szigethy,
A. Oliver, D. K. Shuh and K. N. Raymond, J. Am. Chem. Soc., 2007,
129, 6674–6675.
¨
at bastnasite ore surfaces. Mono- and multi-layers of rare earth
complexes proposed to generate hydrophobic foams would be 13 M. P. Neu, J. H. Matonic, C. E. Ruggiero and B. L. Scott, Angew.
Chem., Int. Ed., 2000, 39, 1442–1444.
14 W. L. Smith and K. N. Raymond, J. Am. Chem. Soc., 1981, 103, 3341–3349.
15 M. DelaRosa, K. Bousman, J. Welch and P. Toscano, J. Coord. Chem.,
expected to comprise tetravalent cerium complexes in this con-
text. These observations are consistent with the recently reported
superior performance of alkyl hydroxamic acids over fatty acids
2002, 55, 781–793.
4
´
16 F. Guerard, Y.-S. Lee, R. Tripier, L. P. Szajek, J. R. Deschamps and
¨
in the beneficiation of Mountain Pass bastnasite.
M. W. Brechbiel, Chem. Commun., 2013, 49, 1002–1004.
17 D. Tranqui, J. Laugier, P. Boyer and P. Vulliet, Acta Crystallogr., Sect.
B, 1978, 34, 767–773.
18 R. Shannon, Acta Crystallogr., Sect. A, 1976, 32, 751–767.
19 H. Zheng, S. J. Yoo, E. Muenck and L. Que, Jr., J. Am. Chem. Soc.,
2000, 122, 3789–3790.
The results also suggest that future models of light rare earth metal
ore beneficiation should take into account cerium redox chemistry.
Further, collectors that increase the tendency for the cerium redox
reaction to occur, namely through electron donating groups that
further stabilize the CeIV cation, could further improve hydroxamic 20 M. Matsumoto, H. Kodama, S. Funahashi and H. D. Takagi, Inorg.
acid performance. Exploration of the effect of hydroxamic acid
React. Mech., 2000, 2, 19–31.
21 X. Cao and M. Dolg, THEOCHEM, 2002, 581, 139–147.
22 M. Ciampolini, F. Mani and N. Nardi, J. Chem. Soc., Dalton Trans.,
substituents on the redox properties of the resulting cerium
complexes is currently underway in our laboratories.
1977, 1325–1328.
This journal is ©The Royal Society of Chemistry 2014
Chem. Commun., 2014, 50, 5361--5363 | 5363