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Surface Plasmons on Metal Nanoparticles - UNAM

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3808 J. Phys. Chem. C, Vol. 111, No. 10, 2007 Noguezrepresentati<strong>on</strong>, finite differences methods, etc. 46 Once a numericalmethod is chosen, it is important to select a “realistic”dielectric functi<strong>on</strong> that better resembles the material propertiesof the system, in this case, particles of nanometric sizes. Here,we show the main characteristics that a realistic dielectricfuncti<strong>on</strong> should have to calculate the light extincti<strong>on</strong> of NPs.A. Nanoparticle Dielectric Functi<strong>on</strong>. As starting point, wecan employ dielectric functi<strong>on</strong>s measured experimentally forbulk metals, ɛ exp (ω). These dielectric functi<strong>on</strong>s have c<strong>on</strong>tributi<strong>on</strong>sfrom interband (inter) and intraband (intra) electr<strong>on</strong>transiti<strong>on</strong>s, which we can assume are additiveɛ exp (ω) ) ɛ inter (ω) + ɛ intra (ω) (2)Interband c<strong>on</strong>tributi<strong>on</strong>s are due to electr<strong>on</strong> transiti<strong>on</strong>s fromoccupied to empty bulk bands separated by an energy gap. Theelectr<strong>on</strong>s are bound by a restoring force given by the energydifference between ground and excited electr<strong>on</strong>ic states inmetals, usually at the ultra violet (UV) regi<strong>on</strong>. 41 Intrabandc<strong>on</strong>tributi<strong>on</strong>s come from electr<strong>on</strong> transiti<strong>on</strong>s at the Fermi levelin incompletely filled bands, or when a filled band overlaps inenergy with an empty band. These transiti<strong>on</strong>s also provide anabsorpti<strong>on</strong> mechanism but at lower energies. Electr<strong>on</strong>s at theFermi level in metals are excited by phot<strong>on</strong>s of very smallenergies, such that, they are essentially “free’’ electr<strong>on</strong>s. Thec<strong>on</strong>tributi<strong>on</strong>s from free electr<strong>on</strong>s to ɛ exp (ω) can be describedby the Drude model 41ω p2ɛ intra (ω) ) 1 -ω(ω + i/τ)where ω p is the plasma frequency and 1/τ the damping c<strong>on</strong>stantdue to the dispersi<strong>on</strong> of the electr<strong>on</strong>s. For most metals at roomtemperature, 1/τ is much less than ω p , and the plasma frequencyfor metals is usually in the visible and UV regi<strong>on</strong>s, with energiespω p from 3 to 20 eV. The theoretical values of ω p can disagreefrom those obtained experimentally, since the c<strong>on</strong>tributi<strong>on</strong> fromthe b<strong>on</strong>d electr<strong>on</strong>s or interband transiti<strong>on</strong>s is not c<strong>on</strong>sidered inthe Drude model. In fact, the b<strong>on</strong>d electr<strong>on</strong>s create a positivebackground that screens the free electr<strong>on</strong>s and ω p is usuallypulled down. For instance, the Drude model predicts for silvera plasma frequency to be 9.2 eV, 41 but the measured <strong>on</strong>e isactually 3.9 eV. 49The collisi<strong>on</strong> time τ determines a characteristic distance λ τ ,which plays a fundamental role in the theory of electr<strong>on</strong>c<strong>on</strong>ducti<strong>on</strong>. An electr<strong>on</strong> picked at random at a given momentwill, <strong>on</strong> average, travel a distance λ τ before its next collisi<strong>on</strong>.This distance λ τ is also known as the mean free path of electr<strong>on</strong>s,and at room temperatures is of the order of few nanometers.Here, we are interested in small NPs mostly at room temperature;hence, we have to c<strong>on</strong>sider that electr<strong>on</strong>s can be alsodispersed by the NP surface, because the free electr<strong>on</strong>’s meanfree path is now comparable or larger than the dimensi<strong>on</strong> ofthe particle. Therefore, it is necessary to include an extradamping term τ(a) toɛ exp (ω), due to the surface scattering ofthe “free’’ electr<strong>on</strong>s. The surface dispersi<strong>on</strong> not <strong>on</strong>ly depends<strong>on</strong> the particle size, but also <strong>on</strong> its shape. 50To include surface dispersi<strong>on</strong> we need modify the intrabandc<strong>on</strong>tributi<strong>on</strong>s by changing the damping term. From eq 2, weobtain the input of the bound charges by subtracting the freeelectr<strong>on</strong> c<strong>on</strong>tributi<strong>on</strong> from the bulk dielectric functi<strong>on</strong>. The freeelectr<strong>on</strong> c<strong>on</strong>tributi<strong>on</strong>s are calculated with Drude and using thetheoretical values of ω p . Now, we include the surface dampingby adding the extra damping term τ(a) to the Drude model.Finally, we obtain a dielectric functi<strong>on</strong>, which also depends <strong>on</strong>(3)Figure 1. Interband c<strong>on</strong>tributi<strong>on</strong>s to the dielectric functi<strong>on</strong> of bulksilver.the NP size, and includes the c<strong>on</strong>tributi<strong>on</strong>s of (i) the freeelectr<strong>on</strong>s, (ii) surface damping, and (iii) interband transiti<strong>on</strong>sor bound electr<strong>on</strong>s, given byɛ(ω, a) ) ɛ inter (ω) + ɛ NP intra (ω, a)) {ɛ exp (ω) - ɛ intra (ω)} +{2ω p1 -ω(ω + i/τ + i/τ(a))} (4)In this work, we will c<strong>on</strong>sider for all the cases the surfacedispersi<strong>on</strong> of a sphere of radius a given by 1/τ(a) )V f /a, 51 whereV f is the Fermi velocity of the electr<strong>on</strong> cloud. The smaller theparticle, the more important is the surface dispersi<strong>on</strong> effect. Laterwe will show that surface dispersi<strong>on</strong> effects do not change thelocati<strong>on</strong> of the surface modes, but they affect the coupling ofsuch proper modes with the applied field, making the res<strong>on</strong>ancepeaks wider and less intense. 18In Figure 1, we show the interband or bound electr<strong>on</strong>s inputto the bulk dielectric functi<strong>on</strong> of silver as measured by Johns<strong>on</strong>and Christy, 49 according to eq 2, and using Drude to model theintraband input. The main c<strong>on</strong>tributi<strong>on</strong> to the imaginary part ofɛ inter (ω) is at wavelengths below 325 nm, whereas for largerwavelengths, the input is almost nil. On the other hand, thec<strong>on</strong>tributi<strong>on</strong>s to the real part are always different from zero,being the most significant at about 315 nm, while between 350and 700 nm the real part is almost c<strong>on</strong>stant. We should keep inmind that interband electr<strong>on</strong> transiti<strong>on</strong>s will absorb energy, butnot c<strong>on</strong>tribute to SPRs.Once the NP’s dielectric functi<strong>on</strong> is determined, we have tochoose a method to find the SPRs. In this work, we employ thespectral representati<strong>on</strong> formalism and the discrete dipole approximati<strong>on</strong>(DDA). In secti<strong>on</strong> III, we introduce the mainc<strong>on</strong>cepts of the spectral representati<strong>on</strong> formalism, and in secti<strong>on</strong>sIV and VI, we employ it to study the SPRs of ellipsoidal NPs,as well as supported NPs and 1D chains. For the case ofsuspended polyhedral NPs, we employ DDA, which is a wellsuited technique for studying scattering and absorpti<strong>on</strong> ofelectromagnetic radiati<strong>on</strong> by particles of arbitrary shapes withsizes of the order or less than the wavelength of the incidentlight. 52 For a more complete descripti<strong>on</strong> of DDA and itsnumerical implementati<strong>on</strong>, DDSCAT, the reader can c<strong>on</strong>sultrefs 17 and 53-56.B. Large <strong>Nanoparticles</strong> versus Small <strong>Nanoparticles</strong>. Theimportance of the absorpti<strong>on</strong> and scattering process as a functi<strong>on</strong>of the particle size can be studied for spherical particles usingthe Mie theory, see for example ref 18. It was found that for


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 3809NPs of less than 40 nm of diameter the radiati<strong>on</strong> processes arenegligible, and the particle <strong>on</strong>ly absorbs energy. On the otherhand, the scattering effects dominate the resp<strong>on</strong>se of NPs of100 nm and larger.1. Small Particles (40 nm). When the size of the particleincreases, the radiati<strong>on</strong> effects become more and more important.The displacement of the electr<strong>on</strong>ic cloud is no l<strong>on</strong>ger homogeneouseven for spherical particles, and <strong>on</strong>ce more, highmultipolar charge distributi<strong>on</strong>s are induced. This fact can beseen from the Mie theory, where the extincti<strong>on</strong> and scatteringcross secti<strong>on</strong>s are expressed in series expansi<strong>on</strong> of the involvedfields, which are described in terms of spherical harm<strong>on</strong>icfuncti<strong>on</strong>s, such that, the different multipolar excitati<strong>on</strong>s and theirc<strong>on</strong>tributi<strong>on</strong> can be easily identified. 43 For instance, in a recentexperiment, up to hexa-multipolar charge distributi<strong>on</strong>s have beenobserved in large spherical NPs. 57 Furthermore, the acceleratedelectr<strong>on</strong>s produce an additi<strong>on</strong>al polarizati<strong>on</strong> field that depends<strong>on</strong> the ratio between the size of the particle and the wavelengthof the incident light. 58 Because of this sec<strong>on</strong>dary radiati<strong>on</strong>, theelectr<strong>on</strong>s lose energy experiencing a damping effect, whichmakes wider the SPRs. 18 This field reacts against the quasistaticpolarizati<strong>on</strong> field and shifts the positi<strong>on</strong> of the modes to largerwavelengths. Thus, the radiati<strong>on</strong> damping reduces the intensityand makes broader and asymmetric the SPR peaks, which arered-shifted.In summary, the optical signature of small particles is givenby the SPRs that depend <strong>on</strong> the NPs shape, which are associatedto different surface charge distributi<strong>on</strong>s that are explained interms of different multipolar moments. The SPRs are influencedby the NP size, such that, for particles of few nanometers theres<strong>on</strong>ances do not change their positi<strong>on</strong> or frequency, but theybecome wider because of surface dispersi<strong>on</strong> effects. When thesize increases the SPRs are now affected by the sec<strong>on</strong>daryradiati<strong>on</strong>, which moves their positi<strong>on</strong> to smaller frequencies andmakes broader the peaks. Besides, light scattering is also present,which induces the excitati<strong>on</strong> of new SPRs of higher multipolarorder.In c<strong>on</strong>clusi<strong>on</strong>, to describe the optical resp<strong>on</strong>se of NPs, it iscrucial to understand the number, positi<strong>on</strong>, and width of theSPRs as a functi<strong>on</strong> of the NP shape, size, and envir<strong>on</strong>ment.III. <str<strong>on</strong>g>Surface</str<strong>on</strong>g> <str<strong>on</strong>g>Plasm<strong>on</strong>s</str<strong>on</strong>g>: General TheoryWhen c<strong>on</strong>ducti<strong>on</strong> electr<strong>on</strong>s oscillate coherently, they displacea electr<strong>on</strong> cloud from the nuclei giving rise to a surface chargedistributi<strong>on</strong>. The Coulomb attracti<strong>on</strong> between positive andnegative charges results in restoring forces, characterized byoscillati<strong>on</strong> frequencies of the electr<strong>on</strong> cloud with respect to thepositive background, which are different from those of theincident EM wave. Each collective oscillati<strong>on</strong> with differentsurface charge distributi<strong>on</strong> is known as surface plasm<strong>on</strong>res<strong>on</strong>ance (SPR). The number of such modes as well as theirfrequency and width are determined by the electr<strong>on</strong> density,effective mass, particle’s shape, size, dielectric functi<strong>on</strong>, andits envir<strong>on</strong>ment. In this work, we are interested in the surfaceplasm<strong>on</strong> resp<strong>on</strong>se of metal NPs; therefore, we c<strong>on</strong>sider particleswhose sizes are much smaller than the wavelength of theincident light, where the quasi-static limit is still valid.A. <str<strong>on</strong>g>Surface</str<strong>on</strong>g> <str<strong>on</strong>g>Plasm<strong>on</strong>s</str<strong>on</strong>g>. Let us c<strong>on</strong>sider a NP composed of ahomogeneous, isotropic, and n<strong>on</strong>magnetic material with dielectricfuncti<strong>on</strong> ɛ(ω). The NP is embedded in a n<strong>on</strong>magnetic hostwith dielectric c<strong>on</strong>stant ɛ h . Under the acti<strong>on</strong> of an incident EMwave, the free charges are displaced producing a polarizati<strong>on</strong>field PB. The light absorpti<strong>on</strong> is given by the proper modes ofthe NP, which are specified by PB. The proper modes resp<strong>on</strong>siblefor the optical absorpti<strong>on</strong> satisfy ∇ ‚PB )∇×PB )0, inside theparticle, but ∇ ‚PB*0, <strong>on</strong> the surface. These surface modes areevanescent electromagnetic waves, which are not necessarilylocalized near the surface, but they are accompanied by apolarizati<strong>on</strong> charge ∇ ‚PB <strong>on</strong> it. We should recall that boundelectr<strong>on</strong>s do not participate in the collective moti<strong>on</strong> of theelectr<strong>on</strong> cloud, thus, SPRs are quite independent of the interbandc<strong>on</strong>tributi<strong>on</strong>s to the dielectric functi<strong>on</strong>, except that they can actas a positive background changing in some way the envir<strong>on</strong>mentof the free electr<strong>on</strong>s.In the existing theories, the frequencies of the res<strong>on</strong>ant propermodes and their coupling strength to the applied field cannotbe immediately calculated, because they involve a procedurethat usually requires taking the n<strong>on</strong>dissipati<strong>on</strong> limit, which callsfor a vast amount of numerical effort. However, we can c<strong>on</strong>structa theory that yields both the frequencies of the proper modesand the size of their coupling strength to the applied field bybuilding a spectral representati<strong>on</strong> of the effective polarizabilityof the system. In this representati<strong>on</strong>, the effective polarizabilityis expressed as a sum of terms with single poles, such that, thelocati<strong>on</strong> of the poles is associated with the frequencies of thenormal modes through a spectral variable, and their strengthwith the coupling of these modes to the applied field. Thespectral representati<strong>on</strong> has advantages over other theories,because it separates the c<strong>on</strong>tributi<strong>on</strong> of the dielectric propertiesfrom the geometrical <strong>on</strong>es. The latter allows us to perform asystematic study of the optical resp<strong>on</strong>se of NPs: <strong>on</strong>ce a shapeis chosen, the frequencies of the plasm<strong>on</strong> res<strong>on</strong>ance of particlesof different size and dielectric properties can be calculated witha minimum numerical effort. Next we present a brief introducti<strong>on</strong>to the spectral representati<strong>on</strong> formalism.


3810 J. Phys. Chem. C, Vol. 111, No. 10, 2007 NoguezB. Spectral Representati<strong>on</strong> Formalism. The spectral representati<strong>on</strong>formalism was first introduced by Fuchs to studythe optical properties of i<strong>on</strong>ic crystal cubes. 37 In this seminalpaper, Fuchs showed that the particle’s polarizability can bewritten as a sum over normal modes. Later, Bergman 38 andMilt<strong>on</strong> 39 showed that the effective local dielectric functi<strong>on</strong> ofany two-phase composite in 3D can always be written in termsof a spectral representati<strong>on</strong>. The main advantage of thisrepresentati<strong>on</strong> is that the proper modes do not depend <strong>on</strong> thedielectric properties of the comp<strong>on</strong>ents but <strong>on</strong>ly <strong>on</strong> the geometryof the system. Moreover, from the explicit expressi<strong>on</strong>s of thespectral representati<strong>on</strong>, we can easily obtain the strength of thecoupling of different optically active modes with the appliedfield, whose frequency is determined by the poles of thepolarizability.Within the spectral representati<strong>on</strong>, the NP’s polarizability R-(ω) is expressed as a sum of terms with single poles 374πV R(ω) )- ∑nC(n)s(ω) - s n(5)where C(n) is the spectral functi<strong>on</strong>, which gives the strength ofeach eigenvalue s n , and V is the NP volume. The spectral variables(ω) is defined in terms of the dielectric properties of thecomp<strong>on</strong>ents as 371s(ω) )(6)1 - ɛ(ω)/ɛ hThe nth SPR given by the nth pole of eq 5 has a complexfrequency Ω n ) ω n + iγ n , which satisfies s(Ω n ) ) s n , wherethe real frequency, ω n , gives the locati<strong>on</strong> of the proper mode,and γ n gives its relaxati<strong>on</strong> rate. Furthermore, it has been shown 38that the eigenvalues are real numbers between 0 es n e1, andthe spectral functi<strong>on</strong> satisfies the sum rule 37∑C(n) ) 1nwhich means that the total strength of all modes is c<strong>on</strong>served.Now, substituting the dielectric functi<strong>on</strong> from eq 4 into thespectral variable expressi<strong>on</strong> in eq 6, the frequency Ω n of thenth eigenmode is given byΩ n ) ω n + iγ n )-iΓ + -Γ 2 + ω p 2 s n A n (7)with A n ) [s n (ɛ inter + 1 - ɛ h ) + ɛ h ] -1 and 2Γ ) 1/τ + 1/τ(a).From here, we can infer some general behavior of the SPRs.For instance, if the relaxati<strong>on</strong> time decreases (Γ increases), thefrequency of the SPR is always red-shifted. However, this shiftis very small since for typical metals Γ , ω p . Now, when theparticle is immersed in vacuum ɛ h ) 1, and assuming that thereare not c<strong>on</strong>tributi<strong>on</strong>s from interband transiti<strong>on</strong>s (ɛ inter ) 0), weobtain that A n ) 1, such that, ω n ) ω p s n . For a homogeneoussphere, it has being found that there is a single mode with s n )1/3 and C(n) ) 1, such that, by substituting in eq 5, <strong>on</strong>e obtainsthe well-known expressi<strong>on</strong> of the sphere polarizability.Otherwise A n < 1, such that, the SPRs are always red-shiftedwith respect to vacuum. Furthermore, we find that the shift isnot just by a c<strong>on</strong>stant because it depends <strong>on</strong> the proper modeitself: the smaller the eigenvalue s n is, the larger the red shiftis. Therefore, we found that the locati<strong>on</strong> of the surface plasm<strong>on</strong>res<strong>on</strong>ances is sensitive to the dielectric envir<strong>on</strong>ment, and as therefracti<strong>on</strong> index increases, the spectrum suffers a red shift andbecomes wider. This is because the red-shift is larger forres<strong>on</strong>ances at greater wavelength. However, the number ofres<strong>on</strong>ances is still the same independently of the refracti<strong>on</strong> indexof the host medium.The main advantage of the spectral representati<strong>on</strong> is that thelocati<strong>on</strong> of the poles and their strength are independent of thesize and dielectric properties of the particle and depend <strong>on</strong>ly<strong>on</strong> its shape. To show the capabilities of the spectral representati<strong>on</strong>formalism, we will study in detail the case of ellipticalparticles, where an explicit expressi<strong>on</strong> of the spectral representati<strong>on</strong>of the polarizability is easily found. This case is useful toillustrate how the eigenvalues s n depend <strong>on</strong> the geometricalparameters, and how the frequencies of these proper modes canbe easily obtained. Although the proper modes and their strengthare independent of the NPs size and dielectric properties, explicitvalues of these are difficult to obtain. Until now, the spectralrepresentati<strong>on</strong>s of different NPs have been found <strong>on</strong>ly forspherical, ellipsoidal, and cubic geometries, as well as forcolloidal suspensi<strong>on</strong>s of spherical particles, and supportedellipsoidal NPs, which we will employ in secti<strong>on</strong> VI.IV. El<strong>on</strong>gated <strong>Nanoparticles</strong><strong>Metal</strong> nanoellipsoids possess three plasm<strong>on</strong> res<strong>on</strong>ances corresp<strong>on</strong>dingto the oscillati<strong>on</strong> of electr<strong>on</strong>s al<strong>on</strong>g the three axesof the NP. The res<strong>on</strong>ance wavelength depends <strong>on</strong> the orientati<strong>on</strong>of the electric field relative to the particle. By changing theaxes length, the plasm<strong>on</strong> res<strong>on</strong>ance frequencies of the nanoellipsoidcan be tuned systematically. The possibility of tuningthe optical resp<strong>on</strong>se of NPs has attracted the attenti<strong>on</strong> ofscientists, and a large variety of new synthesis methods havebeen developed to fabricate el<strong>on</strong>gated NPs. 59-71 When theseNPs are dispersed in a matrix (solid or liquid), the randomorientati<strong>on</strong> leads to an average absorpti<strong>on</strong> spectrum c<strong>on</strong>tainingthe three plasm<strong>on</strong> res<strong>on</strong>ances. On the other hand, when the axesof the nanoellipsoids are oriented in the same directi<strong>on</strong>, it ispossible to distinguish between the different res<strong>on</strong>ances by usingpolarized light. 70,71In this secti<strong>on</strong>, we employ the spectral representati<strong>on</strong> to obtainthe SPR of nanoellipsoids as a functi<strong>on</strong> of their geometricalparameters and independent of the dielectric properties. Thisallows us to do a systematic study of the SPRs of gold andsilver el<strong>on</strong>gated NPs with different aspect ratios and immersedin different media. Finally, we study the case of alignedspheroids and the dependence of the SPRs <strong>on</strong> light polarizati<strong>on</strong>.The reader can c<strong>on</strong>sult recent reviews by Murphy et al. 72 andPérez-Juste et al., 73 which provide a nice overview of thesynthesis and properties of el<strong>on</strong>gated NPs.A. Spectral Representati<strong>on</strong> of Ellipsoidal <strong>Nanoparticles</strong>.Let us c<strong>on</strong>sider an ellipsoidal NP under the acti<strong>on</strong> of an uniformexternal electric field. The ellipsoid has a volume V e )(4π/3)abc, where a, b, and c are its semiaxes. The comp<strong>on</strong>entsof the ellipsoid’s dipolar polarizability is 74R γ (ω) ) V e ɛ(ω) - ɛ h4π ɛ h + L γ [ɛ(ω) - ɛ h ]where γ denotes x, y, orz and L γ are functi<strong>on</strong>s of a, b, c, andthe eccentricity e. Notice that L γ are independent of the materialproperties of the ellipsoid and depend <strong>on</strong>ly <strong>on</strong> the geometricalparameters. Using the definiti<strong>on</strong> of the spectral variable in eq6, we can rewrite each comp<strong>on</strong>ent γ of the ellipsoid’s polarizability,as(8)4π1RV γ (ω) )-(9)e s(ω) - L γ


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 38111:101:20TABLE 1: Eigenvalues of the SPRs of Prolates and Oblates Spheroids of Different Aspect Ratiosa:c1:21:41:61:8s n L x,L z L x,L z L x,L z L x,L z L x,L z L x,L zprolate 0.1735, 0.4132 0.0754, 0.4623 0.0432, 0.4784 0.0284, 0.4858 0.0203, 0.4898 0.0067, 0.4966oblate 0.2363, 0.5272 0.1482, 0.7036 0.1077, 0.7846 0.0845, 0.8308 0.0695, 0.8608 0.0369, 0.9262In this case, we can easily identify the geometrical factors withthe eigenvalues of the surface proper modes of the spheroid, s n) L γ , and their strength are C γ ) 1/3. Thus, the eigenvaluesare independent of the material properties of the ellipsoid, andthe SPRs are given by the poles of eq 9. Taking into accountthe definiti<strong>on</strong> of the spectral variable, we find that these SPRsfulfill the c<strong>on</strong>diti<strong>on</strong> ɛ(ω)L γ + ɛ h (1 - L γ ) ) 0. Now, it isnecessary to calculate the depolarizati<strong>on</strong> factors L γ .For simplicity, let us c<strong>on</strong>sider ellipsoids generated by therotati<strong>on</strong> of an ellipse around its major or minor axes, whichproduce prolate or oblate spheroids, corresp<strong>on</strong>dingly. Sinceprolate and oblate NPs have a symmetry axis, they have threeproper modes, where two of them are degenerated. Thegeometrical factors L γ for prolate spheroids (a > b ) c) are 74L x ) 1 - e22e 3 (log 1 + e1 - e - 2e )L y ) L z ) 1/2(1 - L x ) and e ) 1 - b 2 /a 2 (10)Whereas for oblate spheroids (a ) b > c), they areL z ) 1 + e2e 3 (e - tan -1 e)L x ) L y ) 1/2(1 - L z ) and e ) a 2 /c 2 - 1 (11)For a sphere (a ) b ) c), it is evident that the depolarizati<strong>on</strong>factors are all degenerated, and to satisfy the sum rule c<strong>on</strong>diti<strong>on</strong>,they must be equal to L x ) L y ) L z ) 1/3, and the SPR fulfillsthe well-known expressi<strong>on</strong> ɛ(ω)L γ + ɛ h (1 - L γ ) ) ɛ(ω) + 2ɛ h) 0.In the previous secti<strong>on</strong>, we found a general behavior of theSPRs, where a red shift of the modes is found when the particleis immersed in a host media, and when interband electr<strong>on</strong>stransiti<strong>on</strong>s are present. To make a closer analysis of the SPRsof el<strong>on</strong>gated NPs and without loss of generality, let us assumethat the NP is immersed in vacuum and its dielectric functi<strong>on</strong>does not c<strong>on</strong>tain c<strong>on</strong>tributi<strong>on</strong>s from interband transiti<strong>on</strong>s, andΓ , ω p , such that ω n ) ω p s n . In this case, the frequency ofthe res<strong>on</strong>ance for the sphere is given by the well-knownexpressi<strong>on</strong> ω n)1 ) ω p 3. Now, let us analyze the case forprolate particles when the semi-axis a goes to ∞, and a cylinderor needle with its axis al<strong>on</strong>g x is obtained. Then, the depolarizati<strong>on</strong>factors are L x f 0, L y ) L z f 1/2, such that, as aincreases, the mode al<strong>on</strong>g the symmetry axis is red-shifted untilit ceases to be visible (zero frequency), while the two perpendicularmodes c<strong>on</strong>verge to ω n ) ω p 2. The other limit case isfor oblates when a and b f ∞ that corresp<strong>on</strong>ds to a flat plateor disk, and the depolarizati<strong>on</strong> factors L x ) L y f 0 and L z f1. Here, the two identical modes al<strong>on</strong>g the symmetry axis cease,since their res<strong>on</strong>ances go to zero as a and b f ∞ while theperpendicular <strong>on</strong>e ω n f ω p . In Table 1, we show the depolarizati<strong>on</strong>factors for prolate and oblates spheroids as a functi<strong>on</strong>of the aspect ratio a:c. We observe that for an aspect ratio a:c) 6:1 (1:6) for prolates (oblates), the limit cases menti<strong>on</strong>edpreviously have been already attained within a 10%.B. Applicati<strong>on</strong> to Gold and Silver NPs. To exhibit thepotentiality of the spectral representati<strong>on</strong>, here, we perform asystematic study of the SPRs of ellipsoidal gold and silver NPsthat are immersed in different media. In the following, we definethe aspect ratio of the NP as the length of the major axis dividedby the width of the minor axis. We will also label the modes asl<strong>on</strong>gitudinal (LM) when they are al<strong>on</strong>g the symmetry axis ofthe particle, whereas transversal modes (TM) are those excitedin the perpendicular directi<strong>on</strong>. Let us c<strong>on</strong>sider gold (Au), andsilver (Ag) NPs with theoretical pω p ) 8.55 and 9.2 eV,respectively. The NPs are embedded in a medium with refracti<strong>on</strong>index n ) ɛ h . For visible wavelengths, the c<strong>on</strong>tributi<strong>on</strong>s ofinterband transiti<strong>on</strong>s can be approximated by a c<strong>on</strong>stant, ɛ inter= 9.9 for Au and ɛ inter = 3.9 for Ag. With these parameters,we calculate the dielectric functi<strong>on</strong> according to eq 4, and usingthe eigenvalues n s from Table 1, and substituting in eq 7, thefrequency of the LM and TM modes of prolate and oblates NPscan be obtained with minimum numerical effort.In Figure 2, we plot the positi<strong>on</strong> of the res<strong>on</strong>ance as a functi<strong>on</strong>of the aspect ratio for gold prolate (left side) and silver oblate(right side) NPs, embedded in vacuum with n ) 1, water/glycerol with n ) 1.3, dimethyl sulfoxide or silica glass with n) 1.47, sapphire with n ) 1.77 or TiO 2 with n ) 2.79. Ingeneral, we c<strong>on</strong>firm that, as the refracti<strong>on</strong> index of the hostmedia increases, all of the modes are always red-shifted. TheLM of prolate particles behaves as the TM of oblate NPs, wherethe positi<strong>on</strong> of the modes is displaced to larger wavelengths asthe aspect ratio increases, although the shift is smaller for oblatesthan for prolates. In the same way, the TM of prolates behavessimilarly to that of the LM of oblates, but now, the modes areshifted to smaller wavelengths when the aspect ratio increases,and this shift is larger for oblates than for prolates. We observethat the LMs and TMs of prolates and oblates, respectively,show a linear behavior independently of the refracti<strong>on</strong> index n,where the slope is modified by n as well as by the particularshape. For instance, the slope of the LMs of prolates is largerthan that of the TMs of oblates. On the other hand, the TM(LM) of prolates (oblates) shows a behavior inversely proporti<strong>on</strong>alto the aspect ratio. The TMs of prolates are always blueshifted,and for aspect ratios between 1 and 3, it occurs rapidly,whereas from 4.5 and larger the limit value is almost reached.Furthermore, the limit value of LMs of oblates is slightly shiftedto large wavelengths as n increases, whereas for prolates thelimit value of TMs is more susceptible to the value of n.The linear behavior of the modes of el<strong>on</strong>gated NPs has beenobserved experimentally and theoretically in nanorods andnanodisks. 59-67 In some of these works, phenomenologicalequati<strong>on</strong>s to determine the positi<strong>on</strong> of the res<strong>on</strong>ances have beenproposed. However, these empirical models can be applied <strong>on</strong>lyto a specific system, where the slope of the linear equati<strong>on</strong>depends <strong>on</strong> the soluti<strong>on</strong> where the particles are dispersed. Onthe other hand, using the expressi<strong>on</strong>s for the eigenvalues givenin eqs 10 and 11, we find an exact dependence of the SPRpositi<strong>on</strong> as a functi<strong>on</strong> of the aspect ratio. For instance, let usc<strong>on</strong>sider the case when the spheroid is nearly spherical (e ,1), such that, the l<strong>on</strong>gitudinal eigenvalues of prolates and oblatesNPs are approximately 74


3812 J. Phys. Chem. C, Vol. 111, No. 10, 2007 Noguezs prolate LM ) 1 3 - 215 e2 , and s oblate TM ) 1 3 + 215 e2respectively. Since e 2 is inversely proporti<strong>on</strong>al to the aspect ratiofor prolates, and proporti<strong>on</strong>al for oblates, we find from eq 7that the frequencies of LMs for prolates are inversely proporti<strong>on</strong>alto the aspect ratio, whereas they are proporti<strong>on</strong>al to it foroblates. Also from eq 7, we find that all modes are inverselyproporti<strong>on</strong>al to ɛ h . Now, c<strong>on</strong>sidering that the wavelength isinversely proporti<strong>on</strong>al to the frequency, λ ) c/ω, we obtain thatthe positi<strong>on</strong> of the LMs of prolates is proporti<strong>on</strong>al to the aspectratio, while for oblates is inversely proporti<strong>on</strong>al. Additi<strong>on</strong>ally,the modes are proporti<strong>on</strong>al to the refracti<strong>on</strong> index n in all cases.These explain the behavior of the res<strong>on</strong>ances in Figure 2, aswell as the observati<strong>on</strong>s of experimental and theoreticalworks. 59-67 Notice that deviati<strong>on</strong>s from a prolate ellipsoidalshape have effects <strong>on</strong> the optical properties of nanorods. 64,67C. Aligned El<strong>on</strong>gated <strong>Nanoparticles</strong>. To show the sensitivityof anisotropic NPs to polarized light, we simulate the opticalabsorbance of prolate spheroids with a small aspect ratio of 1.6and a major axis of 8 nm, which are embedded in silica (n )1.47). The optical absorbance of the nanocomposites has beencalculated by c<strong>on</strong>trolling the angle θ of the wavevector kB ofthe incident electromagnetic field with respect to the major axisof the NP. The polarizati<strong>on</strong> of the incident electric field wasvaried at different angles φ with respect to the minor axis andperpendicular to kB. In Figure 3, panels a and b, the simulatedabsorbance spectra are shown for the incident electromagneticfield at θ )-45° and 90°, respectively, and different angles ofpolarizati<strong>on</strong>. When θ )-45° in Figure 3a, it is observed thatfor φ ) 0° the electric field is al<strong>on</strong>g the minor axis exciting<strong>on</strong>ly the surface plasm<strong>on</strong> at 375 nm. C<strong>on</strong>versely, when the angleof polarizati<strong>on</strong> is φ ) 72° , both res<strong>on</strong>ances are excited, butthe <strong>on</strong>e at 375 nm is weaker than the res<strong>on</strong>ance at 470 nm.Similarly, when θ ) 90° in Figure 3b, the wavevector kB isalmost aligned to <strong>on</strong>e of the minor axes, and as a c<strong>on</strong>sequence,the electric field is polarized al<strong>on</strong>g the other minor axis at φ )0° and almost al<strong>on</strong>g the major axis at φ ) 72°. Finally, if wec<strong>on</strong>sider that θ ) 0° (not shown in the figure), the wavevectorkB is al<strong>on</strong>g the major axis, in such a way that the electric fieldmostly excites the res<strong>on</strong>ance at 375 nm for any polarizati<strong>on</strong>.Similar c<strong>on</strong>clusi<strong>on</strong>s have been found recently for metal nanorods.71Recently, the shape and alignment of metallic NPs embeddedin insulator matrices have been c<strong>on</strong>trolled using MeV i<strong>on</strong> beamirradiati<strong>on</strong>. 69,70 Symmetric NPs were transformed into anisotropicparticles whose larger axis is al<strong>on</strong>g the i<strong>on</strong> beam. Up<strong>on</strong>irradiati<strong>on</strong>, the surface plasm<strong>on</strong> res<strong>on</strong>ance of symmetric particlessplit into two res<strong>on</strong>ances whose separati<strong>on</strong> depends <strong>on</strong> thefluence of the i<strong>on</strong> irradiati<strong>on</strong>. 70 Simulati<strong>on</strong>s of the opticalabsorbance showed that the anisotropy is caused by thedeformati<strong>on</strong> and alignment of the nanoparticles and that bothproperties can be c<strong>on</strong>trolled with the irradiati<strong>on</strong> fluence. 70V. Shape Influence <strong>on</strong> the <str<strong>on</strong>g>Surface</str<strong>on</strong>g> <str<strong>on</strong>g>Plasm<strong>on</strong>s</str<strong>on</strong>g>In the case of metal NPs, many results indicate the presenceof polyhedral shapes with well-defined facets and vertices, likeicosahedral (IH) and decahedral (DH) NPs, as well as fcc relatedmorphologies like cubes and truncated cubes (TC). 28,29,57,75-79To understand the influence of morphology, the SPRs forpolyhedral NPs have been recently studied. 80 A general relati<strong>on</strong>shipbetween the SPRs and the morphology of each NP wasestablished in terms of their vertices and faces. The opticalresp<strong>on</strong>se was investigated for cubes and DHs, as well as fordifferent truncati<strong>on</strong>s of them. 80 Here, we show results for cubicand DH silver NPs whose volume is equal to that of a spherewith a radius of 2.2 nm, which are immersed in a media witha refracti<strong>on</strong> index n ) 1.47. The extincti<strong>on</strong> efficiencies, Q ext ,were calculated using DDA with the order of 10 5 polarizableentities, which ensure the c<strong>on</strong>vergence of the optical resp<strong>on</strong>sefor each NP. We employ the measured bulk dielectric functi<strong>on</strong>for silver by Johns<strong>on</strong> and Christy, 49 which is modified accordingto eq 4 to incorporate the surface dispersi<strong>on</strong> effects.A. Cubic Morphology. We first study Q ext for a nanocube,and then, we compare it to those obtained for different TCs,the IH, and the sphere. In Figure 4, we show Q ext for a silvernanocube immersed in a medium with n ) 1.47 (solid line)and in vacuum (dashed line). In both spectra, we observe thatthe optical resp<strong>on</strong>se below 325 nm follows the same behaviorindependently of the dielectric properties of the surroundingmedia, since at those wavelengths and smaller the mainabsorpti<strong>on</strong> mechanism is due to the interband transiti<strong>on</strong>s.Therefore, this structure should also be independent of themorphology of the NP, as we will show later when we compareQ ext for different TCs. At larger wavelengths, both spectra showFigure 2. Positi<strong>on</strong>s of LM and TM surface plasm<strong>on</strong> res<strong>on</strong>ances of gold prolate (left side) and silver oblate (right side) NPs with different aspectratios and embedded in various media. The lines are just for guidance.


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 3813Figure 3. Simulated optical absorbance for linear-polarized light from 0° to 90°. The polarizati<strong>on</strong> indicated in the sec<strong>on</strong>d plot is the same for all.The wavevector of the incident electromagnetic field respect to the major axis is depicted.Figure 4. Extincti<strong>on</strong> efficiency of a silver cube nanoparticle as afuncti<strong>on</strong> of the wavelength of the incident light, and immersed invacuum and in silica. The main six surface plasm<strong>on</strong> res<strong>on</strong>ances areindicated.a rich structure of peaks, which is better observed when n )1.47. We menti<strong>on</strong>ed in secti<strong>on</strong> III that, for media with n > 1,the spectrum is red-shifted with respect to vacuum. Furthermore,this shift is not just by a c<strong>on</strong>stant, because it depends <strong>on</strong> theproper mode itself. It is clear from Figure 4 that the SPRs arespread out as n > 1, and the red shift is larger for SPRs atgreater wavelengths. For instance, when n ) 1.47, we canidentify six SPRs more easily than when n ) 1. These sixres<strong>on</strong>ances were found by Fuchs, 37 who calculated nine SPRswhere <strong>on</strong>ly six of them account for more than the 96% of thespectrum. The SPRs 1 and 2 corresp<strong>on</strong>d to the dipolar andquadrupolar charge distributi<strong>on</strong>s and are located at 506 and 466nm, respectively, and their amplitude is particularly high at thecorners. The modes 3-6 are at smaller wavelengths and showhigher multipolar charge distributi<strong>on</strong>s. The amplitude of modes5 and 6 is high at the center of the faces, whose normal pointsal<strong>on</strong>g the electric field. 37Now, let us compare Q ext of a nanocube to those for differentTCs, the IH and the sphere. The TCs are obtained by truncatingthe eight corners of the cube by l × r, where l is the length ofthe cube’s side and 0 < r E 1/2. We label the differenttruncati<strong>on</strong>s with the number r. When r ) 1/2 a cuboctahedr<strong>on</strong>(CO) is obtained. Six octag<strong>on</strong>s and eight triangles compose allof the TCs, except the CO that is composed by six planar squaresand eight triangles. All of the TCs have 14 faces. Finally, if weperformed a symmetric truncati<strong>on</strong> of the cube with a largernumber of planes, <strong>on</strong>e could arrive to the IH, and with an infinitenumber of planes to the sphere. In Figure 5, the extincti<strong>on</strong>efficiencies of TCs with r from 1/8 to 1/2 are shown. The opticalresp<strong>on</strong>se below 325 nm is the same independently of themorphology, as expected. It is observed that, even for theFigure 5. Extincti<strong>on</strong> efficiencies as a functi<strong>on</strong> of the wavelength ofthe incident light of a silver cube, different truncated cubes, and aspherical nanoparticle.smallest truncati<strong>on</strong> (r ) 1/8), the SPRs are very sensitive tothe morphology. In this case, the dipolar SPR is blue-shiftedabout 30 nm. The locati<strong>on</strong> of the dipolar and quadrupolar SPRsare now very close, such that, <strong>on</strong>ly <strong>on</strong>e wide peak is observedaround 474 nm, which is more intense. The SPR 3 has vanished,and the others show a slightly blue shift. The same trend isobserved for larger truncati<strong>on</strong>s, and when the CO is obtainedwith r ) 1/2, the spectrum becomes wider. For the IH, thespectrum does not show the individual peaks, is narrower thanthe <strong>on</strong>e for the CO, but is wider than the sphere that shows asingle peak, which corresp<strong>on</strong>ds to the dipolar SPR.In summary, it was found that as the truncati<strong>on</strong> r increases(i) the main res<strong>on</strong>ance is always blue-shifted, (ii) the SPRs atsmaller wavelength are closer to the dominant mode, so theycan be hidden, and (iii) the width of the main SPRs increases.For instance, the full width at the half-maximum (fwhm) of theTC with 1/8 is about 70 nm, whereas the <strong>on</strong>e with r ) 1/2(CO) is about 115 nm. This means that the sec<strong>on</strong>dary res<strong>on</strong>ancesdo not disappear but are closer to the dominant SPR, producingwider spectra at larger truncati<strong>on</strong>s. For the IH and the sphere,the fwhm are about 60 and 20 nm, respectively. This indicatesthat the SPRs vanish as the number of faces increases or whenthe symmetry of the NP is greater. The res<strong>on</strong>ance of the sphereis always at the smallest wavelength, whereas the main SPR ofthe IH is blue-shifted with respect of the cubes but at a largerwavelength of the sphere. Then, as the number of faces of theNP increases (i) there are fewer SPRs, (ii) the main res<strong>on</strong>anceis blue-shifted, and (iii) the fwhm of the spectra decreases.B. Decahedral Morphology. Another important morphologypresent in metal NPs is the DH or pentag<strong>on</strong>al bipyramid, whichis obtained by different synthesis methods. 21-26 The regular DH,


3814 J. Phys. Chem. C, Vol. 111, No. 10, 2007 NoguezFigure 6. Extincti<strong>on</strong> efficiency as a functi<strong>on</strong> of the wavelength of theincident light for the regular decahedr<strong>on</strong> and its truncated morphologiesfor parallel light polarizati<strong>on</strong>.shown in Figure 6, is composed of 10 planar triangular faces,which resemble two pentag<strong>on</strong>s. However, when the NP’s sizeis in the range between 1 and 5 nm, the regular DH is rarelyobserved, and the most comm<strong>on</strong> shapes are the truncated <strong>on</strong>es:the Marks and rounded DHs. The first structure was introducedby Marks 81 and is remarkably stable. In very clean growthc<strong>on</strong>diti<strong>on</strong>s, or with weak interacti<strong>on</strong>s with substrates, this is <strong>on</strong>eof the predominant shapes for the discussed size interval. Away to describe the Marks DH is as a regular DH, which hastruncati<strong>on</strong>s <strong>on</strong> its facets, as shown in Figure 6. When thetruncati<strong>on</strong> reaches a maximum value, a morphology with theshape of a star DH is formed. Another type of DH NP, whichis often observed, corresp<strong>on</strong>ds to the rounded pentag<strong>on</strong>al NP,in which the truncati<strong>on</strong> has a minimum possible value producinga c<strong>on</strong>trast reducti<strong>on</strong> in the borders. This type of particle isfrequently formed when colloidal growth methods are used. 22Here, we briefly discuss the SPRs of the rounded dh with atruncati<strong>on</strong> of r ) 1/8, the Marks dh with r ) 1/6, the star, andthe regular DH. A more detailed discussi<strong>on</strong> can be found inrefs 27 and 80.Due to the symmetry of the DH NP, two different polarizati<strong>on</strong>sof the incident electromagnetic field are present: when EBis parallel or perpendicular to the pentag<strong>on</strong>al motif. When theelectric field is perpendicular to the pentag<strong>on</strong> of the regular DH,the spectrum shows a peak with its maximum at about 358 nmand has a fwhm of 90 nm. It was found that SPRs present atthe perpendicular polarizati<strong>on</strong> are not affected with any truncati<strong>on</strong>,except for the star DH, 80 where the main SPR is red-shiftedby 100 nm and is 5.5 times more intense, and its fwhm isnarrowed to 40 nm. 80 On the other hand, the parallel polarizati<strong>on</strong>is more sensitive to the different truncati<strong>on</strong>s. In Figure 6, Q extof the regular, rounded, Marks, and star DHs, when EB is parallel,are shown. The resp<strong>on</strong>se of the star decahedral is totally differentsince it shows res<strong>on</strong>ances in a very wide range of wavelengths.For the parallel polarizati<strong>on</strong>, the rounded decahedra show thesame effect as a functi<strong>on</strong> of the truncati<strong>on</strong> as observed in thecase of truncated cubes. The main res<strong>on</strong>ance is blue-shifted,and becomes the most intense peak after truncati<strong>on</strong>.VI. Influence of Physical Envir<strong>on</strong>ment <strong>on</strong> <str<strong>on</strong>g>Surface</str<strong>on</strong>g><str<strong>on</strong>g>Plasm<strong>on</strong>s</str<strong>on</strong>g> Res<strong>on</strong>ancesWe showed that with small changes of the morphology it ispossible to tune the SPRs of NPs. Here, we want to study howthese SPRs are influenced if the physical envir<strong>on</strong>ment ismodified. In this directi<strong>on</strong>, we have already shown how theSPRs are shifted if the dielectric properties of the surroundingmedia are changed. In particular, we showed that the SPRs ina medium with refracti<strong>on</strong> index n > 1 are red-shifted withrespect to those in vacuum. Furthermore, this shift depends <strong>on</strong>the proper mode itself: the larger the wavelength of theeigenmode, the greater the red shift, and the more spread outthe SPRs. However, we are interested not <strong>on</strong>ly in the case whenthe dielectric properties are changed but also when the physicalenvir<strong>on</strong>ment of the NP becomes different. We w<strong>on</strong>der whathappens to the SPRs when the particles lie <strong>on</strong> a substrate orwhen they are close enough that the dilute limit is not l<strong>on</strong>gervalid, and the electromagnetic interacti<strong>on</strong>s am<strong>on</strong>g NPs shouldbe c<strong>on</strong>sidered.These two situati<strong>on</strong>s are of great importance in a large varietyof problems that have promising technological applicati<strong>on</strong>s, likesurface-enhanced Raman scattering (SERS), 82-84 catalytic processes,85,86 plasm<strong>on</strong>ic devices, 87,88 and others. For instance, inthe case of the electromagnetic effect in SERS, the anomalousenhancement of the optical resp<strong>on</strong>se has been examined byadsorbing molecules at n<strong>on</strong>-flat metallic surfaces and at NPsof different shapes. Although the optical spectra of adsorbedmolecules might carry informati<strong>on</strong> about specific features ofthe molecular electr<strong>on</strong>ic structure or charge-transfer mechanisms,the informati<strong>on</strong> sought in the optical resp<strong>on</strong>se ofsupported particles is related more to their shape, substrateinducedmultipolar coupling, or local field effects. The calculati<strong>on</strong>of the field at the surface of these NPs requires the fullsoluti<strong>on</strong> of the optical resp<strong>on</strong>se problem.In this secti<strong>on</strong>, we study two important systems where thephysical envir<strong>on</strong>ment of the isolated or suspended NPs ischanged. First, we analyze the SPRs when the particle is placedabove a substrate. Sec<strong>on</strong>d, we examine the SPRs for a linearchain of NPs, which are close enough that they interact becauseof the local electromagnetic field.A. Supported <strong>Nanoparticles</strong>. The optical resp<strong>on</strong>se ofmetallic NPs deposited <strong>on</strong> a substrate is also characterized bythe presence of SPRs. The locati<strong>on</strong> and broadening of theseres<strong>on</strong>ances depend <strong>on</strong> the geometrical and dielectric propertiesof the system. When the system is under the acti<strong>on</strong> of an externalEM field, it induces a charge polarizati<strong>on</strong> <strong>on</strong> the particle thatcauses a charge distributi<strong>on</strong> <strong>on</strong> the substrate, which in turnsalso affects the NP. In the quasistatic limit, this chargedistributi<strong>on</strong> can be seen as the image charge distributi<strong>on</strong> of theNP, as shown in Figure 7. Although the dipolar approximati<strong>on</strong>might be sufficient for describing the optical resp<strong>on</strong>se of anisolated sphere, the substrate-induced field acting <strong>on</strong> the amplevolume of the NP is no l<strong>on</strong>ger homogeneous in space, andmultipolar modes of very high order might excite in additi<strong>on</strong>to the dipole (see Figure 7b). The interacti<strong>on</strong> between the NPsis also important, especially in the case of a high c<strong>on</strong>centrati<strong>on</strong>of them. However, the study of a single supported particle canbe also performed in the dilute regime. 89-93Different authors have included the multipolar interacti<strong>on</strong>sc<strong>on</strong>sidering particles of different shapes; 91-97 however, thenumerical complexity of the problem restricts the number ofmultipolar modes taken to describe the system. A powerfultheoretical method was developed to calculate the opticalresp<strong>on</strong>se of a particle-substrate system using the spectralrepresentati<strong>on</strong>. 91 With this method, <strong>on</strong>e is also able to includea larger number of multipoles, allowing the treatment of particlescloser to the substrate. The inclusi<strong>on</strong> of multipolar interacti<strong>on</strong>sbetween the particle and its image gives rise to res<strong>on</strong>ancesadditi<strong>on</strong>al to the dipolar <strong>on</strong>e. The structure of these res<strong>on</strong>ancesis more evident when the c<strong>on</strong>trast between the dielectric


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 3815Figure 7. (a and b) Electromagnetic interacti<strong>on</strong> between the NP and substrate as a functi<strong>on</strong> of the separati<strong>on</strong>, modeled using the image method.Induced local field for an applied field (c) normal and (d) parallel to the interface.Figure 8. Extincti<strong>on</strong> efficiency of silver spherical NPs located above the substrate by a distance d, for an external field (a) normal and (b) parallelto the substrate.resp<strong>on</strong>ses of the ambient and substrate increases. 91 For example,when a particle is in close c<strong>on</strong>tact with the substrate, smoothspectra are obtained. On the c<strong>on</strong>trary, when the particle islocated at a certain distance above the substrate, a well-definedstructure of res<strong>on</strong>ances is found.Let us first analyze the optical resp<strong>on</strong>se of a silver sphericalNP of radius of 10 nm lying above a substrate of Al 2 O 3 withdielectric c<strong>on</strong>stant ɛ sub ) 3.132 and embedded in air. Due tothe presence of the substrate, the symmetry of the system isbroken and different proper modes can be found for lightpolarized parallel and normal to the interface. In Figure 8, weshow Q ext for light polarized (a) parallel and (b) normal to thesubstrate surface, where a spherical NP is located at differentdistances d. Atd ) 100 nm, the interacti<strong>on</strong> between NP andsubstrate is null, and the optical resp<strong>on</strong>se corresp<strong>on</strong>ds to thatof an isolated sphere, being the SPR the same for bothpolarizati<strong>on</strong>s. As the particle approaches the substrate, themultipolar excitati<strong>on</strong>s are evident since the spectra become widerand several peaks are observed. For instance, at d ) 1nmandnormal polarizati<strong>on</strong>, the dipolar SPR is red-shifted about 10 nm,and a sec<strong>on</strong>dary SPR at 346 nm with quadrupolar character isexcited, giving rise to the shoulder shown in the inset. Whenthe NP is touching the substrate, d ) 0 nm, we have taken 2000multipolar interacti<strong>on</strong>s, where c<strong>on</strong>vergence has been partlyreached. 91 For illustrati<strong>on</strong> purposes, we also show the case whend ) 0.01 nm that shows how sensitive the optical resp<strong>on</strong>se ofthe normal modes is. When the particle is touching the substrate,the SPR with dipolar character shifts to larger wavelengths, andthe coupling between multipolar modes become important; thus,more modes are excited and their individual character identitystarts to disappear, such that, the spectra is twice as wide as the<strong>on</strong>e of the isolated sphere, and the individual SPRs are not l<strong>on</strong>gerobserved. Note that as the radius of the sphere diminishes, theimaginary part of the NP dielectric functi<strong>on</strong> increases, such that,the broadening effects wash out the details of the res<strong>on</strong>antstructure. 92 Thus, different spectra could be obtained c<strong>on</strong>sideringparticles of different material even if the geometry of the systemis the same. 93Although the influence of the substrate is the same for bothpolarizati<strong>on</strong>s, the optical resp<strong>on</strong>se to the applied field parallelto the substrate seems to be less sensitive to its presence. It hasbeen found that the excited SPRs cover a more extended regi<strong>on</strong>of values when the applied field is normal to the surface thanwhen it is parallel, and they are distributed more symmetricallyin the first case. 91 Independently of the directi<strong>on</strong> of the appliedfield, the spectra is always red-shifted as the particle approachesthe substrate. This can be explained using the simple modeldepicted in Figure 7, panels c and d. When the external field isapplied normal to the interface, shown in Figure 7c, it polarizesboth particle and substrate in the same directi<strong>on</strong>, such that, theinduced local field acting <strong>on</strong> the particle is al<strong>on</strong>g the appliedfield and against the restoring forces, thus decreasing thefrequency of the SPRs. When the field is applied parallel tothe interface, Figure 7d, it polarizes the particle in the oppositedirecti<strong>on</strong> to the substrate polarizati<strong>on</strong>, but the induced local fieldacting <strong>on</strong> the particle is also al<strong>on</strong>g the applied field and againstthe restoring forces, again decreasing the frequency of the SPRs.Now, let us c<strong>on</strong>sider spheroidal NPs with their symmetry axisnormal to the interface, located at a minimum distance d, andimmersed in air. The same type of behavior of the mode spectrawas found as for the case of the sphere, as the distance fromthe substrate is varied. Let us study the case when the NP is ata fixed distance, but its aspect ratio a/b varies. In Figure 9, weshow Q ext of a silver prolate at d ) 0.01 nm from a TiO 2


3816 J. Phys. Chem. C, Vol. 111, No. 10, 2007 NoguezFigure 9. Extincti<strong>on</strong> efficiency of silver prolates located at a distance d ) 0.01 nm, and different aspect ratios a/b, for an external field (a) normaland (b) parallel to the substrate.Figure 10. Extincti<strong>on</strong> efficiency of silver oblates located at a distance d ) 0.1 nm, and different aspect ratios a/b, for an external field (a) normaland (b) parallel to the substrate.substrate with dielectric c<strong>on</strong>stant ɛ sub ) 7.8. In this particulargeometry, the normal polarizati<strong>on</strong> excites the l<strong>on</strong>gitudinal modes(LMs), whereas the parallel polarizati<strong>on</strong> excites the transversalmodes (TMs) of prolates, as defined in secti<strong>on</strong> IV. We observethat the LMs are red-shifted as the aspect ratio a/b increases,whereas the TMs are blue-shifted, corroborating our previousfindings for the suspended prolates. One can see that, as theratio a/b increases, a dominant mode appears, which turns outto lie very close to the dipolar mode of the suspended spheroid.This means that as a/b increases the spheroid actually decouplesfrom the substrate. In c<strong>on</strong>trast, as a/b f 1, the dominant modemerges down and the mode-strength distributi<strong>on</strong> becomesbroader and equal to that found for the sphere. In c<strong>on</strong>clusi<strong>on</strong>,we observe that multipolar effects become more important asa/b tends to unity, that is, when the actual shape tends to bespherical.The dependence of the spectra with the distance betweenparticle and substrate is similar for oblate spheroids as forspheres and prolates. This means that the multipolar effects dueto the substrate acting <strong>on</strong> the particle are more important whenparticle and substrate are in c<strong>on</strong>tact, and their importancedecreases as the particle recedes from the substrate. In Figure10, we show Q ext of silver oblates at a fixed distance d ) 0.1nm from a substrate with dielectric c<strong>on</strong>stant ɛ sub ) 4.7. Now,the normal polarizati<strong>on</strong> excites the transversal modes (TMs),whereas the parallel polarizati<strong>on</strong> excites the l<strong>on</strong>gitudinal modes(LMs). One can see that as a/b increases the spectra centroidfor the normal (parallel) field shifts toward larger (smaller)wavelengths, and as the eccentricity increases, a tendency towardthe appearance of a dominant mode is str<strong>on</strong>ger for the fieldparallel to the substrate than for the normal <strong>on</strong>e.In c<strong>on</strong>clusi<strong>on</strong>, it was found that the multipolar effects <strong>on</strong> theoptical properties of a NP due to the presence of a substratedepend <strong>on</strong> the directi<strong>on</strong> of the applied external field. We havefound that, for oblate and prolate particles with aspect ratio a/b> 3, the multipolar effects are reduced and the dipolarapproximati<strong>on</strong> gives a good descripti<strong>on</strong> of the behavior of thesystem. Since multipolar effects become more important forsystems where the substrate has a large dielectric c<strong>on</strong>stant, inthis case, the dipolar approximati<strong>on</strong> is not good enough. Wehave also shown that very different spectra could be obtainedc<strong>on</strong>sidering particles of different material even if the geometryof the system (i.e., the semiaxes and the distance) is the same.Finally, it was also found that the interpretati<strong>on</strong> of the opticalspectra could be helpful to elucidate the shape, size and distanceof the NPs. Recent experiments in supported silver NPs havereproduced our results discussed in this secti<strong>on</strong>. 97-100B. One-Dimensi<strong>on</strong>al (1D) Nanostructures. There is intenseand growing interest in <strong>on</strong>e-dimensi<strong>on</strong>al (1D) nanostructuresfrom the perspective of their synthesis and unique properties,especially with respect to their excellent optical resp<strong>on</strong>se.C<strong>on</strong>trolled patterning and alignment of nanostructures is criticalfor studying fundamental collective properties and for incorporatingthese promising materials into nanoelectr<strong>on</strong>ic, sensing,optoelectr<strong>on</strong>ic, and plasm<strong>on</strong>ic devices. Several methods havebeen employed to align 1D structures, either from soluti<strong>on</strong>s/suspensi<strong>on</strong>s of the materials postsynthesis, in substrates, as wellas using more sophisticated methods as i<strong>on</strong> beam implantati<strong>on</strong>in solid matrices. In these systems, <strong>on</strong>e crucial questi<strong>on</strong> is howimportant is the interacti<strong>on</strong> am<strong>on</strong>g particles.Here, the effective dielectric resp<strong>on</strong>se for a 1D chain ofinteracting identical NPs is studied. We do this within the


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 3817Figure 11. Model of the induced local field for an applied field (a)parallel and (b) transversal to the NPs chain.quasistatic limit, and we perform a systematic study for differenttypes of disorder and for filling fracti<strong>on</strong>s covering the wholerange, from the extreme-dilute to the closed-packed limits. Ourobjective is twofold, (i) we want to study the properties of an1D system due to the intrinsic interest that exists in the behaviorof low-dimensi<strong>on</strong>al systems and (ii) we want to shed some lightinto the possible dependence of the effective dielectric resp<strong>on</strong>se<strong>on</strong> the type of disorder. This allows us to analyze fluctuati<strong>on</strong>sinduced in the local field by the positi<strong>on</strong>al disorder of the NPs.We employed the spectral representati<strong>on</strong> to calculate the modes,and the details can be found elsewhere. 102,103When spherical NPs are aligned al<strong>on</strong>g a particular directi<strong>on</strong>,the symmetry of the system is broken, and different propermodes can be found for light polarized parallel and perpendicularto the chain. When the external field is parallel, it polarizes theparticles, such that, the induced local field is in the samedirecti<strong>on</strong> as the applied field, see Figure 11a, and against therestoring forces, thus decreasing the frequency of the SPRs.When the field is perpendicular to the chain, shown in Figure11b, it polarizes the induced local field against the applied field,but in the same directi<strong>on</strong> of the restoring forces, thus increasingthe frequency of the SPRs.To understand the influence of the physical envir<strong>on</strong>ment,results are presented for the extincti<strong>on</strong> efficiency Q ext as afuncti<strong>on</strong> of wavelength, for the ordered case and two differentkinds of disorder (A and B), and for different filling fracti<strong>on</strong>s.In disorder A, we randomly move the NPs within an interval2δ from the positi<strong>on</strong>s of a periodic chain. The parameter 0 eδ e 1/2 serves as a measure of the disorder, for example, δ )0 corresp<strong>on</strong>ds to the ordered case and δ ) 1/2 to the maximumallowed disorder of this type. The disorder type B corresp<strong>on</strong>dsto random positi<strong>on</strong>s with the <strong>on</strong>ly restricti<strong>on</strong> that NPs do notoverlap. The choice of these types of disorder has nothing inparticular; the idea is simply to illustrate the sensitivity of theoptical resp<strong>on</strong>se to a specific type of disorder algorithm,although some similar behaviors can be found. For example,(i) when a periodic 1D crystal is heated up, such that, the atomsmove randomly around their ordered positi<strong>on</strong>s, or (ii) when thesystem is heated up and suddenly cooled down, such that,random positi<strong>on</strong>s without any correlati<strong>on</strong> can be found.In Figure 12, the influence of disorder is shown at differentfilling fracti<strong>on</strong>s. The nanospheres of 20 nm of radii are madeof silver and embedded in air, and we have set δ ) 1/2 fordisorder A. We c<strong>on</strong>sider an external field parallel to the chain.The case when the external field lies transversal to the chainwill not be reported in this work; nevertheless, our study showedthat in this case the corresp<strong>on</strong>ding disorder and multipolar effectsare similar but less pr<strong>on</strong>ounced. In Figure 12a, the extincti<strong>on</strong>for an ordered NP chain for three different filling fracti<strong>on</strong>s isshown. In the ordered case and dilute limit (f f 0), the propermodes of the system become equal to the multipolar res<strong>on</strong>ancesof the isolated sphere, where for small and medium fillingfracti<strong>on</strong>s the dipolar mode is dominant. For a finite f, theeigenmodes are shifted due to the coupling of the spheresthrough fields of the same multipolar order. Up<strong>on</strong> interacti<strong>on</strong>,the individual multipolar character is lost. One should noticethat, due to the symmetry of the ordered chain, the interactingfields of multipoles of even order are canceled. Therefore, at f) 0.8 also the octupolar fields are important. As f increases,the proper modes have a m<strong>on</strong>ot<strong>on</strong>ic red (blue) shift when thefield is parallel (transversal) to the chain. In Figure 12, weappreciate that the larger the disorder, the larger the shift, andthe multipolar fluctuati<strong>on</strong>s, instead of few res<strong>on</strong>ances, excite ac<strong>on</strong>tinuum distributi<strong>on</strong> of them. This makes the multipolarcoupling more efficient. In Figure 12b for disorder A moreFigure 12. Extincti<strong>on</strong> efficiency of a 1D chain of metal NPs at different filling fracti<strong>on</strong>s, for an external field parallel to the chain axis. The upperpanels a-c corresp<strong>on</strong>d to the ordered chain and disorders A and B, respectively. The lower panels d-f corresp<strong>on</strong>ds to filling fracti<strong>on</strong>s f ) 0.3, 0.5,and 0.8, respectively.


3818 J. Phys. Chem. C, Vol. 111, No. 10, 2007 Noguezres<strong>on</strong>ances are observed <strong>on</strong>ly at f ) 0.8, whereas for disorderB, shown in Figure 12c, the multipolar character is evident atany filling fracti<strong>on</strong>. Notice that for larger filling fracti<strong>on</strong>s andgreater disorder the dipolar character of the res<strong>on</strong>ant mode islost.In c<strong>on</strong>clusi<strong>on</strong>, we found that as the filling fracti<strong>on</strong> increases,more multipolar interacti<strong>on</strong>s are present, for all the positi<strong>on</strong>alarrangements. As the positi<strong>on</strong>al disorder increases, it alsoinduces the excitati<strong>on</strong> of new multipolar c<strong>on</strong>tributi<strong>on</strong>s. It seemsthat the spectrum becomes wider as there is more “room’’ fordisorder. As a c<strong>on</strong>sequence, the inclusi<strong>on</strong> of these multipolarmodes shifts the main peak to higher (lower) wavelengths andincreases the extensi<strong>on</strong> of the tail in the low (high)-wavelengthside, for an external field parallel (transversal) to the chain. Butthe most interesting thing is that there is not <strong>on</strong>ly a red shift ofthe peaks but also a drastic change in the profile. Furthermore,it was found that, due to the symmetry of the system, there isno coupling between the directi<strong>on</strong>s parallel and transversal tothe chain. This means that an external field parallel to the chainwill induce multipoles in each sphere, with an axis of symmetryalso parallel to the chain, but they will fluctuate in magnitudeand phase. These fluctuati<strong>on</strong>s cause the existence of a manifoldof collective modes with a c<strong>on</strong>tinue range of res<strong>on</strong>ant frequencies.VII. Summary and Future TrendsWe have studied the general behavior of the surface plasm<strong>on</strong>res<strong>on</strong>ances <strong>on</strong> small metal NPs in terms of their shape andphysical envir<strong>on</strong>ment. For instance, the locati<strong>on</strong> of theseres<strong>on</strong>ances <strong>on</strong> NPs of different shapes has been studied andhas been found that NPs with fewer faces and sharper verticesshow res<strong>on</strong>ances in a wider range of wavelengths. We alsoshowed that, when a NP is truncated, the main res<strong>on</strong>ance isblue-shifted, overlapping sec<strong>on</strong>dary res<strong>on</strong>ances and, therefore,increasing the full width at half-maximum. However, fordecahedral particles, the truncati<strong>on</strong> to Marks and roundeddecahedra shows the same blue shift effect, but the full widthat half-maximum decreases, perhaps because the sec<strong>on</strong>daryres<strong>on</strong>ances no l<strong>on</strong>ger exist as the number of faces increases.We also explained in detail the optical anisotropy of el<strong>on</strong>gatedNPs, such as, ellipsoids, decahedra, etc., where the dependenceof the positi<strong>on</strong> of the res<strong>on</strong>ances is analytically explained interms of their aspect ratio.We have analyzed the case where n<strong>on</strong>interacting el<strong>on</strong>gatedNPs are aligned in a given directi<strong>on</strong>, such that, the opticalresp<strong>on</strong>se can be tuned using polarized light and changing theaspect ratio. We also studied the case of a linear chain ofinteracting NPs, where again, the surface plasm<strong>on</strong> res<strong>on</strong>ancesare sensitive to the light polarizati<strong>on</strong>, and their dependence withthe positi<strong>on</strong>al disorder of the particles. This 1D nanostructurescan be the starting point for more complex structures. Finally,the case of supported NPs was also studied. In this case, theline-shape of the spectra, and its relati<strong>on</strong> with high-multipolarexcitati<strong>on</strong>, is studied in detailed for ellipsoidal NPs. The opticalresp<strong>on</strong>se is studied for different physical situati<strong>on</strong>s: as a functi<strong>on</strong>of the distance between the particle and substrate, as well as interms of the anisotropy of the particle.This informati<strong>on</strong> would be useful to motivate the developmentof more complex nanostructures with tunable surface plasm<strong>on</strong>res<strong>on</strong>ances. For this, it would be desirable to develop a simpletheory capable of predicting the positi<strong>on</strong> and strength of theSPRs of an ample variety of NPs shapes and physical envir<strong>on</strong>ments.We have already menti<strong>on</strong>ed that the spectral representati<strong>on</strong>formalism completes with these characteristics, because itseparates the c<strong>on</strong>tributi<strong>on</strong> of the dielectric properties from thegeometrical <strong>on</strong>es. We have shown the potentiality of this theory,that allows us to perform a systematic study of the opticalresp<strong>on</strong>se of NPs, <strong>on</strong>ce a shape is chosen. However, explicitexpressi<strong>on</strong>s of the spectral representati<strong>on</strong> are difficult to obtain,but alternative forms could be found.Acknowledgment. I am in debt to my many colleagues andstudents that have c<strong>on</strong>tributed al<strong>on</strong>g these years to the study ofthe optical resp<strong>on</strong>se <strong>on</strong> nanoparticles. In particular, I would liketo acknowledge Professor Rubén G. Barrera and Dr. Carlos E.Román for their illuminating c<strong>on</strong>tributi<strong>on</strong>s in spectral representati<strong>on</strong>formalism and substrate effects. I also want toacknowledge the c<strong>on</strong>tributi<strong>on</strong> of Ana Lilia G<strong>on</strong>zález in the studyof the polyhedral particles. Partial financial support fromCONACyT Grant Nos. 48521-F and 44306-F and DGAPA-<strong>UNAM</strong> Grant No. IN101605 is also acknowledged.References and Notes(1) Noguez, C.; Román-Velázquez, C. E. Phys. ReV. B 2004, 70,195412.(2) Intravaia, F.; Lambrecht, A. Phys. ReV. Lett. 2005, 94, 110404.(3) Xu, H.; Käll, M. Phys. ReV. Lett. 2002, 89, 2468021.(4) Ozbay, E. Science 2006, 331, 189.(5) Maier, S. A.; Kik, P. G.; Atwater, H. A.; Meltzer, S.; Harel, E.;Koel, B. E.; Requicha, A. A. G. Nat. Mat. 2003, 2, 229.(6) Maier, S. A.; Atwater, H. A. J. Appl. Phys. 2005, 98, 011101.(7) Zhang, Y.; Gu, C.; Schwartzberg, A.; Chen, S.; Zhang, J. Z. Phys.ReV. B2006, 73, 1654051.(8) Haynes, C. L.; McFarland, A. D.; Van Duyne, R. P. Anal. Chem.2005, 77, 338A.(9) Jin, R.; Cao, Y.; Mirkin, C. A.; Kelly, K. L.; Schatz, G. C.; Zheng,J.-G. Science 2001, 294, 1901.(10) Jin, R.; Cao, Y. C.; Hao, E.; Métraux, G. S.; Schatz, G. C.; Mirkin,C. A. Nature 2003, 425, 487.(11) Sönnichsen, C.; Reinhard, B. M.; Liphardt, J.; Alivisatos, A. P.Nat. Biotechnol. 2005, 33, 741.(12) Hibbins, A. P.; Evans, B. R.; Sambles, J. R. Science 2005, 308,670.(13) Liz-Marzán,L.M.Langmuir 2006, 22, 32.(14) Barnes, W. L.; Dereux, A.; Ebbesen, T. W. Nature 2003, 424, 824.(15) Huang, X.; El-Sayed, I. H.; Qian, W.; El-Sayed, M. A. J. Am. Chem.Soc. 2006, 128, 2115.(16) Kelly, K. L.; Cor<strong>on</strong>ado, E.; Zhao, L. L.; Schatz, G. C. J. Phys.Chem. B 2003, 107, 668.(17) Sosa, I. O.; Noguez, C.; Barrera, R. G. J. Phys. Chem. B 2003,107, 6269.(18) Noguez, C. Opt. Mat. 2005, 27, 1204.(19) Payne, E. K.; Shuford, K. L.; Park, S.; Schatz, G. C.; Mirkin, C.A. J. Phys. Chem. B 2006, 110, 2150.(20) Lee, K.-S.; El-Sayed, M. A. J. Phys. Chem. B 2005, 109, 20331.(21) Wang, Z. L. J. Phys. Chem. B 2000, 104, 1153.(22) Yacamán, M. J.; Ascencio, J. A.; Liu, H. B.; Gardea-Torresdey, J.J. Vac. Sci. Technol. B 2001, 19, 1091.(23) Yang, C. Y. J. Cryst. Growth 1979, 47, 274.(24) Kuo, C.-H.; Chiang, T.-F.; Chen, L.-J.; Huang, M. H. Langmuir2004, 20, 7820.(25) Wei, G.; Zhou, H.; Liu, Z.; S<strong>on</strong>g, Y.; Wang, L.; Sun, L.; Li, Z. J.Phys. Chem. B 2005, 109, 8738.(26) Nilius, N.; Ernst, N.; Freund, H.-J. Phys. ReV. Lett. 2000, 84, 3994.(27) G<strong>on</strong>zalez, A. L.; Noguez, C.; Ortiz, G. P.; Rodriguez-Gattorno, G.J. Phys. Chem. B 2005, 109, 17512.(28) Tao, A.; Sinsermsuksakul, P.; Yang, P. Angew. Chem., Int. Ed.2006, 45, 4597.(29) Baletto, F.; Ferrando, R. ReV. Mod. Phys. 2005, 77, 371.(30) Barnard, A. S.; Lin, X. M.; Curtiss, L. A. J. Phys. Chem. B 2005,109, 24465.(31) Román-Velázquez, C. E.; Noguez, C.; Garzón,I.L.J. Phys. Chem.B 2003, 107, 12035.(32) Sánchez-Castillo, A.; Román, Velázquez, C. E.; Noguez, C. Phys.ReV. B2006, 73, 045401.(33) Yao, H.; Miki, K.; Nishida, N.; Sasaki, A.; Kimura, K. J. Am. Chem.Soc. 2005, 127, 15536.(34) Negishi, Y.; Nobusada, K.; Tsukuda, T. J. Am. Chem. Soc. 2005,127, 5261.(35) Nobusada, K. J. Phys. Chem. B 2004, 108, 11904.


Feature Article J. Phys. Chem. C, Vol. 111, No. 10, 2007 3819(36) Negishi, Y.; Takasugi, Y.; Sato, S.; Yao, H.; Kimura, K.; Tsukuda,T. J. Am. Chem. Soc. 2004, 126, 6518.(37) Fuchs, R. Phys. ReV. B1975, 11, 1732.(38) Bergman, D. Phys. Rep. 1978, 43, 377.(39) Milt<strong>on</strong>, G. W. Appl. Phys. Lett. 1980, 37, 300.(40) Barrera, R. G.; Noguez, C.; Anda, E. V. J. Chem. Phys. 1992, 96,1574.(41) Bohren, C. F.; Human, D. R. Absorpti<strong>on</strong> and Scattering of Lightby Small Particles; John Wiley & S<strong>on</strong>s: New York, 1983.(42) Mie, G. Ann. Phys. 1908, 25, 377.(43) Kreibig, U.; Vollmer, M. Optical properties of metal clusters;Springer-Verlag: Berlin, 1995.(44) Asano, S.; Yamamoto, G. Appl. Opt. 1980, 14, 29.(45) Lind, A. C.; Greenberg, J. M. J. Appl. Phys. 1966, 37, 3195.(46) Mishchenko, M. I.; Hovenier, J. W.; Travis L. D. Light Scatteringby N<strong>on</strong>spherical Particles; Academic Press: San Diego, 2000.(47) Gans, R. Ann. Physik 1912, 37, 881; 1915, 47, 270.(48) Van de Hulst, H. C. Light Scattering by Small Particles; John Wiley& S<strong>on</strong>s: New York, 1957.(49) Johns<strong>on</strong>, P. B.; Christy, R. W. Phys. ReV. B1972, 6, 4370.(50) Cor<strong>on</strong>ado, E. A.; Schatz, G. C. J. Chem. Phys. 2003, 119, 3926.(51) Kreibig, U. J. Phys. F: Met. Phys. 1974, 4, 999.(52) Purcell, E. M.; Pennypacker, C. R. Astrophys. J. 1973, 186, 705.(53) Draine, B. T. Astrophys. J. 1988, 333, 848.(54) Draine, B. T.; Goodman, J. Astrophys. J. 1993, 405, 685.(55) Draine, B. T.; Flatau, P. J. J. Opt. Am. A 1994, 11, 1491.(56) Draine, B. T; Flatau, P. T. Source code DDSCAT 6.0, http://www.astro.princet<strong>on</strong>.edu/∼draine/DDSCAT.html.(57) Kumbhar, A. S.; Kinnan, M. K.; Chumanov, G. J. Am. Chem. Soc.2005, 127, 12444.(58) Meier, M.; Wokaun, A. Opt. Lett. 1983, 8, 581.(59) Al-Sayed, A.-M.; Majied, A.-S. Colloids Surf. A 2004, 246, 61.(60) Lee, K.-S.; Al-Sayed, A.-M. J. Phys. Chem. B 2005, 109, 20331.(61) Perez-Juste, J.; Liz-Marzan, L. M.; Carnie, S.; Chan, D. Y. C.;Mulvaney, P. AdV. Funct. Mater. 2004, 14, 571.(62) Gou, L.; Murphy, C. J. Chem. Mater. 2005, 17, 3668.(63) Murphy, C. J.; Jana, N. R. AdV. Mater. 2002, 14, 80.(64) Brioude, A.; Jiang, X. C.; Pileni, M. P. J. Phys. Chem. B 2005,109, 13138.(65) Jiang, X. C.; Brioude, A.; Pileni, M. P. Colloids Surf. A 2006, 277,201.(66) Brioude, A.; Pileni, M. P. J. Phys. Chem. B 2005, 109, 23371.(67) Xu, X.; Cortie, M. B. AdV. Funct. Mater. 2006, 6, 2170.(68) Orendorff, C. J.; Murphy, C. J. J. Phys. Chem. B 2006, 110, 3990.(69) Penninkhof, J. J.; van Dillen, T.; Roorda, S.; Graf, C.; vanBlaaderen, A.; Vredenberg, A. M.; Polman, A. Nucl. Instrum. Methods B2006, 242, 523.(70) Oliver, A.; Reyes-Esqueda, J. A.; Cheang-W<strong>on</strong>g, J. C.; Román-Velázquez, C. E.; Crespo-Sosa, A.; Rodríguez-Fernández, L.; Seman, J.A.; Noguez, C. Phys. ReV. B2006, 74, 245425.(71) Cortie, M. B.; Xu, X.; Ford, M. J. Phys. Chem. Chem. Phys. 2006,8, 3520.(72) Murphy, C. J.; Sau, T. K.; Gole, A. M.; Orendorff, C. J.; Gao, J.;Gou, L.; Hunyadi, S. E.; Li, T. J. Phys. Chem. B 2005, 109, 13857.(73) Peréz-Juste, J.; Pastoriza-Santos, I.; Liz-Marzan, L. M.; Mulvaney,P. Coord. Chem. ReV. 2005, 249, 1870.(74) Lifshitz, E. M.; Landau, L. D.; Pitaevskii, L. P. Electrodynamicsof C<strong>on</strong>tinuous Media, 2nd ed.; Butterworth-Heinemann: Burlingt<strong>on</strong>, MA,1984.(75) Sun, Y.; Xia, Y. Science 2002, 298, 2176.(76) Zhou, M.; Chen, S.; Zhao, S. J. Phys. Chem. B 2006, 110, 4510.(77) Chen, Y.; Gu, X.; Nie, C.-G.; Jiang, Z.-Y.; Xie, Z.-X.; Lin, C.-J.Chem. Comm. 2006, 33, 4181.(78) Salzemann, C.; Brioude, A.; Pileni, M.-P. J. Phys. Chem. B 2006,110, 7208.(79) Banerjee, I. A.; Yu, L.; Matsui, H. Proc. Natl. Acad. Sci. 2003,100, 14678.(80) G<strong>on</strong>zález, A. L.; Noguez, C. J. Comp. Theor. Nanosci. 2007, 4,273.(81) Marks, L. D. Rep. Prog. Phys. 1994, 57, 603.(82) Haes, A. J.; Haynes, C. L.; McFarland, A. D.; Zou, S.; Schatz, G.C.; Van, Duyne, R. P. MRS Bull. 2005, 30, 368.(83) Schatz, G. C.; Young, M. A.; Van Duyne, R. P. <str<strong>on</strong>g>Surface</str<strong>on</strong>g> EnhancedRaman Scattering Physics and Applicati<strong>on</strong>s. In Topics in Applied Physics;Kneipp, K., Moskovits M., Kneipp, H., Eds.; Springer: New York, 2006;Vol. 103, pp 19-46.(84) Dieringer, J. A.; Lyandres, O.; McFarland, A. D.; Shah, N. C.;Stuart, D. A.; Whitney, A. V.; Y<strong>on</strong>z<strong>on</strong>, C. R.; Young, M. A.; Yuen, J.;Zhang, X.; Van, Duyne, R. P. Faraday Discuss. 2006, 132, 9.(85) Haruta, M.; Kageyama, H.; Kamijo, N.; Kobayashi, T.; Delannay,F. Stud. Surf. Sci. Catal. 1988, 44, 33.(86) Haruta, M.; Kobayashi, T.; Sano, H.; Yamada, N. Chem. Lett. 1987,2, 405.(87) Li, K.; Stockman, M. I.; Bergman, D. J. Phys. ReV. Lett. 2005, 72,153401.(88) Cvitkovic, A.; Ocelic, N.; Aizpurua, J.; Guckenberger, R.; Hillenbrand,R. Phys. ReV. Lett. 2006, 97, 060801.(89) Beitia, C.; Borensztein, Y.; Lazzari, R.; Nieto, J.; Barrera, R. G.Phys. ReV. B1999, 60, 6018.(90) Beitia, C.; Borensztein, Y.; Barrera, R. G.; Román, C. E.; Noguez,C. Physica B 2000, 279, 25.(91) Román-Velázquez, C. E.; Noguez, C.; Barrera, R. G. Phys. ReV. B2000, 61, 10427.(92) Román-Velazquez, C. E.; Noguez, C.; Barrera, R. G. Phys. StatusSolidi (a) 1999, 175, 393.(93) Román, C. E.; Noguez, C.; Barrera, R. G. MRS Symp. Proc. 2000,581, 485.(94) Wind, M. M.; Vlieger, J.; Bedeaux, D. Physica A 1987, 141, 33.Wind, M. M.; Bobbert, P. A.; Vlieger J.; Bedeaux, D. Physica A 1987,143, 164.(95) Ruppin, R. Phys. ReV. B1992, 45, 11209.(96) Bobbert, P. A.; Vlieger, J. Physica A 1986, 137, 243.(97) Bedeaux, D.; Vlieger, J. Optical properties of surfaces; ImperialCollege Press: L<strong>on</strong>d<strong>on</strong>, 2004.(98) Lazzari, R.; Roux, S.; Sim<strong>on</strong>sen, I.; Jupille, J.; Bedeaux, D.; Vlieger,J. Phys. ReV. B2002, 65, 235424.(99) Lazzari, R.; Sim<strong>on</strong>sen, I.; Jupille, J. Europhys. Lett. 2003, 61, 541.(100) Lazzari, R.; Jupille, J.; Layet, J. M. Phys. ReV.B2003, 68, 045428.(101) Xu, G.; Tazawa, M.; Jin, P.; Nakao, S. Appl. Phys. A 2005, 80,1535.(102) Noguez, C.; Barrera, R. G. Phys. ReV. B1998, 57, 302.(103) Noguez, C.; Barrera, R. G. Physica A 1994, 211 399.

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