11406 J. Phys. Chem. B, Vol. 103, No. 51, 1999
Sandrock and Foss
(19) Kreibig, U.; Vollmer, M. Optical Properties of Metal Clusters,
Springer-Verlag: Berlin, 1995.
(20) Schmitt, J.; Machtle, P.; Eck, D.; Mohwald, H.; Helm, C. A.
Langmuir 1999, 15, 3256.
(21) Furneaux, R. C.; Rigby, W. R.; Davidson, A. P. Nature 1989, 337,
147.
(22) Shumilova, N. A.; Zutaeva, E. V. In Encyclopedia of Electrochem-
istry of the Elements; Bard, A. J., Ed.; Marcel-Dekker: New York, 1978,
M.L.S also acknowledges the financial support of the ARCS
Foundation. The authors are grateful to Prof. George Schatz
and Lance Kelley for useful discussion and advice regarding
the DDA theory and execution of the DDSCAT Program. The
DDSCAT program was obtained from B. T. Draine and P. J.
tron microscopy support was provided by the Lombardi Cancer
Center Microscopy and Imaging Shared Resource (U.S. Public
Health Service Grant 2P30-CA-51008).
8.
(23) The dimensions of the particles were determined from TEM images.
The average length, diameter, spacing distance, and standard deviations
were determined from measurements of thirteen to twenty individual
structures.
References and Notes
(24) Johnson, P. B.; Christy, R. W. Phys. ReV. B 1972, 6, 4370.
(1) Lam, D. M. K.; Rossiter, B. W. Sci. Am. 1991, NoVember, 80.
(2) Chumanov, G.; Sokolov, K.; Gregory, B. W.; Cotton, T. M. J. Phys.
Chem. 1995, 99, 9466.
(3) Moskovits, M. ReV. Mod. Phys. 1985, 57, 783.
(4) Hache, F.; Klein, R. D.; Flytzanis, C. J. Opt. Soc. Am. B 1986, 3,
1647.
(5) Flytzanis C.; Hache, F.; Klein, M. C.; Richard, D.; Roussingnol,
P. In Progress in Optics; Wolf, E., Ed., North-Holland: Amsterdam, 1991,
29, 323.
(6) Sandrock, M. L.; Pibel, C. D.; Geiger, F. M.; Foss, C. A., Jr. J.
Phys. Chem. B. 1999, 103, 2668.
(7) Storhoff, J. J.; Elghanian, R.; Mucic, R. C.; Mirkin, C. A.; Letsinger,
R. L. J. Am. Chem. Soc. 1998, 120, 1959.
(8) Liao, P. F. In Surface Enhanced Raman Scattering; Chang, R. K.,
Furtak, T. E., Eds.; Plenum Press: New York, 1982.
(9) Hulteen, J. C.; van Duyne, R. P. J. Vac. Sci. Technol. 1995, 13,
1553.
(10) Preston, C. K.; Moskovits, M. J. Phys. Chem. 1988, 92, 2957.
(11) Preston, C. K.; Moskovits, M. J. Phys. Chem. 1993, 97, 8405.
(12) Tierney, M. J.; Martin, C. R. J. Phys. Chem. 1989, 93, 2878.
(13) Foss, C. A., Jr.; Hornyak, G. L.; Stockert, J. A.; Martin, C. R. J.
Phys. Chem. 1994, 98, 2963.
(14) Yu, Y.; Chang, S.; Lee, C.; Wang, C. R. C. J. Phys. Chem. B 1997,
101, 6661.
(25) (a) Meier, M.; Wokaun, A. Opt. Lett. 1983, 8, 851. (b) Zeman, E.
J.; Schatz, G. C. In Proceedings of the 17th Jerusalem Symposium; Pullman,
B., Jortner, J., Nitzan, A., Gerber, B., Eds.; Reidel: Dordrecht, Holland,
1984; p 413.
(26) For all MLWA and DDA simulations, Cext or Qext values were
calculated at 4 nm intervals from 350 to 800 nm and plotted as continuous
curves using Excel software.
(27) Granqvist, C. G.; Hunderi, O. Phys. ReV. B 1977, 16, 1353.
(28) Purcell, G. M.; Pennypacker, C. R. Astrophys. J. 1973, 186, 705.
(29) Draine, B. T.; Flatau, P. J. J. Opt. Soc. Am. A 1994, 11, 1491.
(30) Jensen, T.; Kelly, L.; Lazarides, A.; Schatz, G. C. J. Cluster Sci.
1999, 10, 295.
(31) In the computation of extinction spectra using the DDSCAT
program, the selection of an insufficient number of polarizable elements
results in spectral oscillations on the long wavelength side of the plasmon
resonance maximum. For each of the spectra in Figure 8, the number of
polarizable elements was increased until the oscillations disappeared. We
find that the number of polarizable elements required to prevent such
oscillations increases as the interparticle spacing decreases.
(32) In the study reported in ref 15, porous aluminum oxide films
containing Au rods were impregnated with polyethylene and then exposed
to base to dissolve all of the alumina. The Au rods were then mechanically
oriented in the plane of the polyethylene film surface. Normal incidence
plasmon resonance spectra were obtained at various polarization angles
relative to the direction of rod orientation. Significantly, under conditions
of parallel polarization, the spectra of the Au rod systems indicated long
wavelength resonance bands arising from the particles’ long axes. Short
wavelength resonances were either absent or present only at very low
intensity (consistent with either imperfect orientation of the rod-like particles,
or a very small number of spherical Au impurity particles).
(15) Al-Rawashdeh, N. R.; Sandrock, M. L.; Seugling, C. J.; Foss, C.
A., Jr. J. Phys. Chem. B 1998, 102, 361.
(16) El-Kouedi, M.; Sandrock, M. L.; Seugling, C. J.; Foss, C. A., Jr.
Chem Mater. 1998, 10, 3287.
(17) Van de Hulst, H. C. Light Scattering by Small Particles; Dover:
New York, 1981.
(18) Bohren, C. F.; Huffman, D. R. Absorption and Scattering of Light
by Small Particles; Wiley: New York, 1983.