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J. Chem. Phys., Vol. 110, No. 18, 8 May 1999
Communications
FIG. 4. Left side: 1D single pulse 31P MAS spectra of
bulk undoped InP and two TOPO/oxide passivated InP
clusters of different diameters; 60 s delay between ex-
periments; masϭ10 kHz. Right side: Plot of the ex-
tracted 31P chemical shift values ͑circles͒ vs. inverse
energy. The nanoparticle UV/vis absorption curves
͑300 K toluene͒ are also displayed for comparison. The
chemical shift data is correlated with the inverse aver-
age band gap energy of the InP particles given by the
point of inflection of the absorption curves ͑vertical
dashed lines͒.
´ ´
tance from the origin and the azimuthal angle that define the
position of electron l in a spherical coordinate system cen-
tered at the nuclear spin with the z axis collinear with B0 .
Summing explicitly over all states n with electronic excita-
tion energies ⌬En is necessary for a rigorous calculation of
p . Qualitatively, Eq. ͑1͒ explains the experimental obser-
vation: With decreasing particle size, the electronic excita-
tion energies ⌬En increase and thereby reduce the downfield
paramagnetic chemical shift. The graph in Fig. 4 implies the
crude approximation that ⌬E1Ӷ⌬EnÞ1 . In this limit, the
fairly linear relationship between the 31P shift and the aver-
age inverse lattice band gap energy, extrapolated from the
bulk, suggests that a change from ⌬E1 towards a limiting
energy separation, more suitable for molecular systems, is
not yet reached for an InP cluster with dӍ25 Å.
The results in this study are based upon the sensitivity of
NMR to the local structure and electronic surroundings of
the nuclear spins. A variety of surface components are iden-
tified and characterized using multinuclear polarization
transfer and two-dimensional correlation techniques. We ex-
pect that the application of recent developments in ab initio
and density functional methods for the calculation of mag-
netic resonance parameters25 will complement and further
elucidate our experimental observations in this new class of
materials.
͑1996͒; O. I. Micic, H. M. Cheong, H. Fu, A. Zunger, J. R. Sprague, A.
Mascarenhas, and A. J. Nozik, J. Phys. Chem. 101, 4904 ͑1997͒.
5 H. Fu and A. Zunger, Phys. Rev. B 56, 1496 ͑1997͒.
6 D. L. Klein, P. L. McEuen, J. E. B. Katari, R. Roth, and A. P. Alivisatos,
Appl. Phys. Lett. 68, 2574 ͑1996͒.
7 C.-C. Chen, A. B. Herold, C. S. Johnson, and A. P. Alivisatos, Science
276, 398 ͑1997͒.
8 A. A. Guzelian, J. E. B. Katari, A. V. Kadavanich, U. Banin, K. Hamad,
E. Juban, P. Alivisatos, R. H. Wolters, C. C. Arnold, and J. R. Heath, J.
Phys. Chem. 100, 7212 ͑1996͒.
9 M. Mehring, Principles of High Resolution NMR in Solids ͑Springer, Ber-
lin, 1983͒.
10 M. Tomaselli, D. deGraw, J. L. Yarger, M. P. Augustine, and A. Pines,
Phys. Rev. B 58, 8627 ͑1998͒.
11 D. L. VanderHart, H. S. Gutowsky, and T. C. Farrar, J. Am. Chem. Soc.
89, 5056 ͑1967͒.
12 The 115In NMR signals of the investigated particles were broadened be-
yond detectability due to quadrupolar couplings, possibly caused by slight
bond strains and electric field gradients at or near the surface. Decoupling
at the bulk 115InP resonance frequency ͑Ref. 10͒ had no detectable nar-
rowing effect on the 31P lineshape.
13 A. Pines, M. G. Gibby, and J. S. Waugh, J. Chem. Phys. 59, 569 ͑1973͒.
14 T. S. Lobana, in The Chemistry of Organophosphorous Compounds Vol.
2, edited by F. R. Hartley ͑Wiley, New York, 1992͒.
15 J. R. Sachleben, E. W. Wooten, L. Emsley, A. Pines, V. L. Colvin, and A.
P. Alivisatos, Chem. Phys. Lett. 198, 431 ͑1992͒; L. R. Becerra, C. B.
Murray, R. G. Griffin, and M. G. Bawendi, J. Chem. Phys. 100, 3297
͑1994͒.
16 Since
exceeds the strongest 31P–31P dipolar coupling frequency, the
mas
homonuclear 31P polarization transfer is negligible during the CP period.
17 B. H. Meier, Adv. Magn. Opt. Reson. 18, 1 ͑1994͒; S. M. De Paul, M.
Tomaselli, A. Pines, M. Ernst, and B. H. Meier, J. Chem. Phys. 108, 826
͑1998͒.
ACKNOWLEDGMENTS
18 U. Haeberlen, High Resolution NMR in Solids, Selective Averaging ͑Aca-
demic, New York, 1976͒.
This work was supported by the Director, Office of En-
ergy Research, Office of Basic Energy Sciences, Materials
Sciences Division, U.S. Department of Energy, under con-
tract No. DE-AC03-76SF00098. J.L.Y., M.B., and R.H.H.
acknowledge support from NSF research fellowships. M.T.
acknowledges support from the Swiss National Science
Foundation.
19 Z. Gan, D. M. Grant, and R. R. Ernst, Chem. Phys. Lett. 254, 349 ͑1996͒.
20 TOPO/oxide passivated InP particles showed an additional 31PO4-surface
resonance at 5 ppm (␦m1/2asϭ15 ppm). The assignment is based on
1H→ C→ P double cross-polarization experiments.
21 D. K. Sodickson, M. H. Levitt, S. Vega, and R. G. Griffin, J. Chem. Phys.
98, 6742 ͑1993͒.
13
13
22 M. Baldus, M. Tomaselli, B. H. Meier, and R. R. Ernst, Chem. Phys. Lett.
230, 329 ͑1994͒.
1 L. E. Brus, J. Phys. Chem. 90, 2555 ͑1986͒; A. P. Alivisatos, ibid. 100,
13226 ͑1996͒.
23 A. M. Thayer, M. L. Steigerwald, T. M. Duncan, and D. C. Douglass,
Phys. Rev. Lett. 60, 2673 ͑1988͒.
2 C. B. Murray, D. J. Norris, and M. G. Bawendi, J. Am. Chem. Soc. 115,
8706 ͑1993͒.
24 N. F. Ramsey, Phys. Rev. 78, 699 ͑1950͒.
25 M. Schindler and W. Kutzelnigg, J. Chem. Phys. 76, 1919 ͑1982͒; V. G.
Malkin, O. L. Malkina, and D. R. Salahub, Chem. Phys. Lett. 204, 80
͑1993͒; F. Mauri, B. G. Pfrommer, and S. G. Louie, Phys. Rev. Lett. 77,
5300 ͑1996͒.
3 V. L. Colvin, A. P. Alivisatos, and J. G. Tobin, Phys. Rev. Lett. 66, 2786
͑1991͒; M. G. Bawendi, P. J. Carroll, W. L. Wilson, and L. E. Brus, J.
Chem. Phys. 96, 946 ͑1992͒.
4 S.-H. Kim, R. H. Wolters, and J. R. Heath, J. Chem. Phys. 105, 7957
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