7278 J. Phys. Chem. A, Vol. 103, No. 36, 1999
Campbell
of this promotion energy. This model actually assumes the metal
Summary
oxide is described predominantly by the ionic structure M2+O2-
,
We have measured the second-order rate constants as a
function of temperature for the reactions of ground state
lanthanide atoms with oxygen. With the exception of Yb, the
gas-phase lanthanides abstract an oxygen atom to produce the
metal oxide. Energy barriers vary from 3.4 for Ce(1G4) to 11.1
kJ/mol for Tm(2D3/2). The reaction barriers are found to correlate
to the energy required to promote an electron out of the filled
6s subshell. The reaction of Yb(1S0) with O2 proceeds through
a termolecular process with a barrier of 9.5 kJ/mol.
although the correlation between experimental and predicted
values of the bond dissociation energies is quite good if the
free atom values of the promotion energies are used.36 In fact,
Murad indicated that for praseodymium, the Pr+O- structure is
the more important configuration.37 This structure results from
the combination of the 4f36s1 (Pr+) and 2p5 (O-) states. Thus,
the requirement for reaction involves an ionic/covalent curve-
crossing in which the covalent surface asymptotically correlates
to the s1 configuration. Therefore, the smaller the difference
between the asymptotic energies of the lowest s1 and s2 energy
states, the greater the probability of reaction. Murad’s analysis
was only for Pr because the spectroscopic data available was
limited to Pr. However, the observed promotion energy relation
might indicate the M+O- structure is also important for the other
lanthanide monoxides.
Acknowledgment. This research was supported by a Cottrell
College Science Award of Research Corporation.
References and Notes
(1) Plane, J. M. C. In Gas-Phase Metal Reactions; Fontijn, A., Ed.;
Elsevier: Amsterdam, 1992; p. 29.
The reaction of the lanthanide ions with hydrocarbons also
indicates a relationship between the reactivity and electron
configuration. For the reactions of lanthanide ions with
hydrocarbons,38-42 it has been established that large variations
in the activation of C-H and C-C bonds correlate with the
energies required to promote a nonbonding 4f electron to a
reactive 5d or 6s valence orbital. Insertion into a C-H or C-C
bond apparently requires an electronic configuration on the metal
center which is capable of forming two σ bonds. The f orbitals
do not extend far enough spatially to be involved in the bonding;
thus, the promotion of an f electron to a valence orbital is
required to facilitate reaction. Thus, as the energy required to
promote a metal ion electron from an fns1configuration to an
fn-1d1s1 configuration increases, the activation barrier for the
reaction increases. Thus, the rich chemistry of the gas-phase
lanthanide atoms and ions appears to result from the variation
in the electronic energy states in these systems.
(2) Campbell, M. L. Chem. Phys. Lett. 1998, 294, 339 and references
therein.
(3) Brown, C. E.; Mitchell, S. A.; Hackett, P. A. J. Phys. Chem. 1991,
95, 1062.
(4) Campbell, M. L. J. Chem. Soc., Faraday Trans. 1996, 92, 4377
and references therein.
(5) Vinckier, C.; Christiaens, P.; Hendrickx, M. In Gas-Phase Metal
Reactions; Fontijn, A., Ed.; Elsevier: Amsterdam, 1992; p 57.
(6) Campbell, M. L. Laser Chem. 1998, 17, 219.
(7) Helmer, M.; Plane, J. M. C. J. Chem. Soc., Faraday Trans. 1994,
90, 395.
(8) Campbell, M. L. J. Chem. Soc., Faraday Trans. 1998, 94, 353.
(9) Garland, N. L.; Nelson, H. H. Chem. Phys. Lett. 1992, 191, 269.
(10) LePicard, S. D.; Canosa, A.; Travers, D.; Chastaing, D.; Rowe, B.
R.; Stoecklin, T. J. Phys. Chem. 1997, 101, 9988.
(11) Brown, A.; Husain, D. Can. J. Chem. 1976, 54, 4.
(12) Wiesenfeld, J. R.; Yuen, M. J. J. Phys. Chem. 1978, 82, 1225.
(13) Fontijn, A.; Bajaj, P. N. J. Phys. Chem. 1996, 100, 7085.
(14) Granier, C.; Jegou, J. P.; Megie, G. Geophys. Res. Lett. 1989, 16,
243.
(15) Plane, J. M. C. Int. ReV. Phys. Chem. 1991, 10, 55.
(16) Fontijn, A.; Blue, A. S.; Narayan, A. S.; Bajaj, P. N. Combust.
Sci. Technol. 1994, 101, 59.
The pressure dependence of the Yb + O2 reaction indicates
a termolecular addition reaction to produce YbO2 with a barrier
of 9.5 ( 2.8 kJ/mol. It is well-known that third-order reactions
of closed-shell metal atoms with O2 are characterized by an
energy barrier. This barrier is located in the entrance channel
at the crossing of the covalent and ionic potential energy
surfaces.43 With its [Xe]4f146s2 configuration, ytterbium has the
same filled outer s subshell as the alkaline earth metals. In its
reaction with O2, ytterbium is actually more similar to the other
alkaline earths than barium. The abstraction reaction of barium
with O2 is exothermic and proceeds as a bimolecular process
with a barrier of 7.06 ( 0.23 kJ/mol.25 The abstraction reactions
of magnesium, calcium, and strontium with O2 are endothermic
and not thermodynamically feasible at moderate temperatures.
These alkaline earths are observed to undergo termolecular
processes with O2.43-46 In each of these cases, a barrier has
been observed from the temperature dependence of the limiting
low-pressure, third-order rate constant. The barriers for mag-
nesium, calcium, and strontium have been reported by Vinckier
and co-workers as 16.8 ( 0.8, 10.2 ( 0.4, and 8.7 ( 0.6 kJ/
mol, respectively.43-45 Vinckier rationalized the trend in these
barriers based on a model which assumes a partial charge
transfer between the metal atom and oxygen molecule; that is,
there should be a qualitative correlation between the activation
energy and ionization energy. The ionization energies of Mg,
Ca, Sr, and Yb are 7.64, 6.11, 5.69, and 6.25 eV, respec-
tively.22,47 The barrier observed here for ytterbium is similar to
the barriers observed for calcium and strontium. The uncertain-
ties in the activation energies precludes a more definite
conclusion regarding the charge transfer mechanism.
(17) Green, M. L.; Gross, M. E.; Papa, L. E.; Schnoes, K. J.; Brasen,
D. J. Electrochem. Soc. 1985, 132, 2677.
(18) Ouyang, M.; Hiraoka, H. Mater. Res. Bull. 1997, 32, 1099.
(19) Jones, S. L.; Kumar, D.; Singh, R. K.; Holloway, P. H. Appl. Phys.
Lett. 1997, 71, 404.
(20) Campbell, M. L.; McClean, R. E. J. Chem. Soc., Faraday Trans.
1995, 91, 3787.
(21) Meggers, W. F.; Corliss, C. H.; Scribner, B. F. Tables of Spectral-
Line Intensities, Part I Arranged by Elements; NBS Monograph 145; U.S.
Government Printing Office: Washington, DC, 1975.
(22) Martin, W. C.; Zalubas, R.; Hagan, L. Atomic Energy Levelss
The Rare-Earth Elements. Natl. Stand. Ref. Data Ser. (U.S. Natl. Bur. Stand.)
1978, NSRDS-NBS 60.
(23) Wagman, D. D.; Evans, W. H.; Parker, V. B.; Schumm, R. H.;
Halow, I.; Bailey, S. M.; Churney, K. L.; Nuttall, R. L. J. Phys. Chem.
Ref. Data 1982, 11 (Suppl. 2).
(24) Pedley, J. B.; Marshall, E. M. J. Phys. Chem. Ref. Data 1983, 12,
967.
(25) Nien, C.-F.; Plane, J. M. C. J. Phys. Chem. 1991, 94, 7193.
(26) Campbell, M. L. J. Phys. Chem. A 1998, 102, 892.
(27) Linton, C.; Dulick, M.; Field, R. W.; Leyland, P. C.; Barrow, R.
F. J. Mol. Spectrosc. 1983, 102, 441.
(28) Linton, C.; Bujin, G.; Rana, R. S.; Gray, J. A. J. Mol. Spectrosc.
1987, 126, 370.
(29) Carette, P.; Hocquet, A.; Douay, M.; Pinchemel, B. J. Mol.
Spectrosc. 1987, 124, 243.
(30) Linton, C.; Gaudet, D. M.; Schall, H. J. Mol. Spectrosc. 1983, 102,
441.
(31) Liu, Y. C.; Linton, C.; Schall, H.; Field, R. W. J. Mol. Spectrosc.
1984, 104, 72.
(32) Dirscherl, R.; Michel, K. W. Chem. Phys. Lett. 1976, 43, 547.
(33) Campbell, M. L. J. Chem. Phys. 1999, 111, 562.
(34) Ames, L. L.; Walsh, P. N.; White, D. J. Phys. Chem. 1967, 71,
2707.
(35) Hildenbrand, D. L. Chem. Phys. Lett. 1977, 48, 340.
(36) Murad, E.; Hildenbrand, D. L. J. Chem. Phys. 1980, 73, 4005.
(37) Murad, E. Chem. Phys. Lett. 1978, 59, 359.