18512 J. Phys. Chem. C 2007, 111, 18512-18519 Structural and Magnetic Properties of Gold and Silica Doubly Coated γ-Fe2O3 Nanoparticles Keeseong Park,† Gan Liang,*,‡ Xiaojun Ji,§ Zhi-Ping Luo,| Chun Li,§ Mark C. Croft,⊥,# and John T. Markert† Department of Physics, UniVersity of Texas at Austin, Austin, Texas 78712, Department of Physics, Sam Houston State UniVersity, HuntsVille, Texas 77341, Department of Experimental Diagnostic Imaging, M. D. Anderson Cancer Center, UniVersity of Texas, Houston, Texas 77030, Microscopy and Imaging Center, Texas A&M UniVersity, College Station, Texas 77843-2257, Department of Physics and Astronomy, Rutgers UniVersity, Piscataway, New Jersey 08854, and National Synchrotron Light Source, BrookhaVen National Laboratory, Upton, New York 11973 ReceiVed: July 22, 2007; In Final Form: September 25, 2007 Extensive structural and magnetic characterization measurements were carried out on gold and silica doubly coated γ-Fe2O3 nanoparticles, which were recently demonstrated to have an efficient photothermal effect and high transverse relaxivities for MRI applications. Powder X-ray diffraction and X-ray absorption spectroscopy show the phase of the uncoated and coated nanoparticles to be that of the γ-Fe2O3 structure. The sizes, structure, and chemical compositions of the nanoparticles were determined by transmission electron microscopy. The magnetization results indicate that coating of the iron oxide nanoparticles by gold/silica decreases the blocking temperature from 160 to 80 K. Such a decrease can be well-explained by spin disorder, causing reduction of the effective volume of the γ-Fe2O3 core. Moreover, it was found that in the temperature (T) range between 100 K and room temperature, the gold/silica coating can cause a slight magnetic change in the γ-Fe2O3 cores from superparamagnetic to almost superparamagnetic. Finally, it was found that the coercivity for both the uncoated and the coated nanoparticles decreases almost linearly with T1/2 with the former decreasing faster than the latter, and this coercivity result confirms that the blocking temperature is decreased by gold/silica coating. These results are valuable for evaluating the future applications of this class of multifunctional, hybrid magnetic nanoparticles in biomedicine. 1. Introduction Superparamagnetic nanoparticles (SPNPs) have great potential for magnetic resonance imaging (MRI), due to their high transverse relaxivity,1,2 and for a wide range of other biomedical applications such as drug delivery.3-6 Indeed, SPNP-enhanced MRI techniques have been under development in recent years for imaging of macrophage activity, atherosclerotic lesions, detection of lymph node metastasis, staging of liver tumors, and monitoring the in vivo distribution of cellular trafficking.1,2,7-11 For in vivo applications, the SPNPs must be coated with a biocompatible and diamagnetic material (such as organic polymers or silica matrixes) to prevent the formation of large aggregates of SPNPs and to facilitate functions such as the attachment of drugs. For example, the dispersion of uncoated γ-Fe2O3 NPs in aqueous solution is stable only in highly acidic or basic media. In recent years, much effort has been devoted to the syntheses and characterization of silica coated superparamagnetic iron oxide (SPIO) nanoparticles (NPs) including γ-Fe2O3 NPs.12-17 It has been proven that silica coated SPIO NPs have an excellent biocompatibility and can homogeneously disperse in * Corresponding author. Tel.: (936) 294-1608; fax: (936) 294-1585; e-mail: [email protected]. † University of Texas at Austin. ‡ Sam Houston State University. § M. D. Anderson Cancer Center, University of Texas. | Texas A&M University. ⊥ Rutgers University. # Brookhaven National Laboratory. aqueous solutions with a wide range of pH values.12-17 Thus, they can be used for the MRI diagnosis of cells or tissues altered by diseases such as cancer. However, to kill the cancer cells or cure the affected tissues by photothermal therapy, the silica coated SPIO NPs need to be coated with particles that have an excellent heat generating ability under controllable conditions. In recent years, nanostructures with highly controlled optical properties have attracted great interest due to their potential diagnostic and therapeutic applications in biological and biomedical systems.18 Among such nanostructures, the gold derived NPs are especially attractive due to their ease of preparation, good biocompatibility, ready bioconjugation, and unique optical properties.19-23 Gold nanoshells have a strong absorbance for the wavelength tunable in the near-infrared (NIR) region of the electromagnetic spectrum. They are, therefore, very promising candidates for localized photothermal therapy because they can mediate strong plasmon-induced surface heat flux upon absorption of the NIR radiation.23-25 Thus, if the Au nanoparticles can be coated on the surface or dispersed into the surface layer of the silica matrix of the silica coated γ-Fe2O3 NPs, then such Au/SiO2 doubly coated γ-Fe2O3 NPs could be made bifunctional (i.e., diagnosis and cure of the cancer cells). Recently, we successfully synthesized Au/SiO2 doubly coated γ-Fe2O3 NPs and found that they can form a stable solution in water and have high transverse relaxivities for MRI applications.26 Furthermore, the broad absorbance between 100 and 900 nm in the UV-vis spectra indicates that these doubly coated particles are suitable for photothermal therapy with light in the 10.1021/jp0757457 CCC: $37.00 © 2007 American Chemical Society Published on Web 11/29/2007 Structural/Magnetic Properties of SPIO Au Nanoshells J. Phys. Chem. C, Vol. 111, No. 50, 2007 18513 NIR region.26 However, in that work, a detailed structural and magnetic characterization of the uncoated and Au/SiO2 doubly coated γ-Fe2O3 NPs was absent. A better understanding of the structural and magnetic properties of this class of doubly coated (bifunctional) NPs is urgently needed for their applications in biomedicine. In this paper, we present detailed results of characterization by temperature- and field-dependent magnetization, transmission electron microscopy (TEM), X-ray diffraction (XRD), and X-ray absorption spectroscopy (XAS) measurements on these Au/SiO2 doubly coated γ-Fe2O3 NPs. 2. Experimental Procedures The synthesis of gold and silica doubly coated γ-Fe2O3 NPs has been described in detail elsewhere.26 The first step is the synthesis of the silica coated γ-Fe2O3 NPs using the well-known Stöber process.27 An aqueous ammonia solution (30 wt %, 7 mL) and 0.5 mL of tetraethylorthosilicate (TEOS) were added to the γ-Fe2O3 (or SPIO) solution at room temperature to form silica NPs. The functional groups at the surface of the silica nanoparticles are primarily silanol (Si-OH) or ethoxy (Si-OEt) groups.28 These silica nanoparticles were then treated with 0.04 mL of 3-minopropyl trimethoxysilane (APTMS) for 6 h to introduce the amino-terminated silica surface. The reaction mixture was refluxed for 30 min to complete the reaction.28 In the second step of the synthesis, 1 mL of γ-Fe2O3-embedded silica solution was added to 5 mL of undiluted tetrakis(hydroxymethyl) phosphonium chloride (THPC) gold solution, causing the THPC gold nanocrystals to attach onto the silica surface. The THPC gold solution was prepared by reduction of chloroauric acid (HAuCl4) with THPC, which produces small gold particles with a net negative interfacial charge.29 Finally, the gold nanoshell was prepared by reduction of the K-Gold solution with formaldehyde (37%). UV-vis absorption spectra of the nanoshells were measured with a Beckman Coutler DU800 UV-vis spectrometer after the reaction to verify the formation of the nanoshell. The spectra are identical to those reported in our previous article.26 The broad absorbance between 100 and 900 nm in the UV-vis spectra indicates that these Au/ SiO2 doubly coated particles are suitable for photothermal therapy with light in the NIR region.26 The water-based Fe2O3 NPs (MEG 304) were purchased from Ferrotech (Nashua, NH). TEOS, APTMS, ammonia solution, THPC, HAuCl4, and formaldehyde were purchased from Sigma-Aldrich (St. Louis, MO). X-ray diffraction (XRD) measurements were performed at room temperature using a Rigaku 2005 X-ray diffractometer with Cu KR radiation. The TEM measurements were carried out using a JEOL 2010 TEM system at a working voltage of 200 kV. All imaging magnifications were calibrated using the standards of SiC lattice fringes30 for high magnifications and commercial cross-line grating replica for low magnifications. To prepare the TEM samples, a small drop of the sample solution was transferred to the top surface of a carbon film supported Cu grid that was previously glow discharged to achieve better dispersion and then dried in air. The average size of the particles was estimated based on a sufficient number of sampling, typically over 50. The EDS measurements were performed using an Oxford Instruments EDS detector with an INCA energy platform. The magnetic properties of the NPs were studied using a Quantum Design MPMS SQUID magnetometer at temperatures ranging from 5 to 300 K and in magnetic fields (H) ranging from 0 to up to 50 kOe. In the magnetization measurement, both the uncoated and the Au/SiO2 coated Fe2O3 NPs were in Figure 1. X-ray diffraction patterns for (a) uncoated γ-Fe2O3 NPs, (b) silica coated γ-Fe2O3, and (c) Au and silica doubly coated γ-Fe2O3 NPs. Figure 2. X-ray absorption spectra at Fe K-edge for γ-Fe2O3 NPs (12 nm) and other reference compounds. the form of dried powders. Gelatin capsules (from Capsuline.com) and water-resistive polycarbonate capsules (from Unipec Inc., Rockville, MD) were used as the sample containers for the uncoated and Au/SiO2 coated Fe2O3 NPs, respectively. Since both the amount of the Au/SiO2 coated Fe2O3 particles (0.6 mg) and the volume fraction of the magnetic Fe2O3 cores in the sample were very small, the magnetic moment of the polycarbonate capsule was measured for background subtraction. The Fe K-edge XAS data were taken in fluorescence mode at room temperature at beamline X-19A at the National Synchrotron Light Source (NSLS) at Brookhaven National Lab. A double-crystal Si (111) monochromator was used for energy selection, which was detuned by reducing the incident photon flux 20% from its maximum value to suppress contamination from harmonics. The energy resolution (∆E/E) of the X-19A beam line was 2 × 10-4, corresponding to about 1.4 eV for the edge energy of the Fe K-edge. The energy calibration of the spectra was made by simultaneously measuring the spectrum of a FeO slide as a reference. The XAS spectra presented in this paper were background subtracted and normalized to unity in the continuum region. 18514 J. Phys. Chem. C, Vol. 111, No. 50, 2007 Park et al. Figure 3. (a) TEM image of the uncoated γ-Fe2O3 NPs. (b) EDS spectrum that confirms that the composition is Fe and O without any other impurities. The signal of Cu is from the Cu grid, and C is from the support film on the Cu grid. (c) Enlargement of the framed area in panel a. 3. Results and Discussion (A) XRD and XAS Results. Figure 1 shows the powder XRD patterns for (a) commercial IONPs, (b) SiO2 coated IONPs, and (c) Au/SiO2 doubly coated IONPs, with each pattern normalized to its maximum intensity. All of the peaks in the patterns of the commercial IONPs can be indexed with the cubic structure corresponding to either γ-Fe2O3 or Fe3O4 phase. Since magnetite (Fe3O4) has a cubic spinel structure and lattice constant similar to maghemite (γ-Fe2O3), it is quite difficult to distinguish γ-Fe2O3 from Fe3O4 using only XRD data. Thus, the existence of Fe3O4 in the commercial IONPs cannot be excluded based only on the XRD data. On the other hand, the X-ray absorption near-edge structure (XANES) of XAS offers a powerful means to distinguish the iron oxide species. Fe lattice sites with different formal valences and local coordination can manifest different chemical shifts and near-edge spectral features in their Fe K-edge spectra. In Figure 2, we compare the Fe K-edge spectra (labeled by γ-Fe2O3, 12 nm) of the commercial IONPs to the powder spectra of four reference compounds: micrometersized γ-Fe2O3, R-Fe2O3, Fe3O4, and FeO. It can be seen that both the shape and the edge energy (defined as the energy at absorption coefficient µ ) 0.5) for the spectrum of the commercial IONPs are very close to those for the micrometer- sized γ-Fe2O3 but very different from the rest of the spectra in Figure 2. This clearly demonstrates that the commercial IONPs used in this study are in the γ-Fe2O3 phase. Figure 1b shows that the XRD pattern of the SiO2 (silica) coated γ-Fe2O3 NPs is very similar to that (Figure 1a) of the uncoated γ-Fe2O3 NPs. This indicates that the coated silica is in an amorphous form before the step of mixing the γ-Fe2O3embedded silica solution with the THPC gold solution during the synthesis process. For the Au and silica doubly coated γ-Fe2O3 particles, the XRD pattern shown in Figure 1c displays three wide peaks that can be identified as the (111), (200), and (220) reflection lines of the Au fcc-cubic phase, indicating that the gold particles are crystallized. In addition, there are four narrow peaks in the pattern that can be attributed to the crystallized SiO2 phase (PDF 31-1233), indicating that a certain portion of the silica is crystallized during the steps of coating Au on the surface of the γ-Fe2O3-embedded silica NPs. At present, while the mechanism of the crystallization of silica due to the coating of the Au particles is unclear, some recent research indicates that Au nanoparticles on silica spheres can induce crystallization of silica at low temperatures.31 The background of this pattern is very similar to the XRD pattern of amorphous SiO2, which decreases rapidly with the increase of 2θ from 23 Structural/Magnetic Properties of SPIO Au Nanoshells J. Phys. Chem. C, Vol. 111, No. 50, 2007 18515 Figure 5. Images of BF (a) and central dark-field image (b) for Au/ SiO2 doubly coated γ-Fe2O3 NPs. In panel b, only the crystalline Fe2O3 and Au particles are highlighted. Larger particles indicated by arrowheads are Fe2O3. Mapping Si and O are shown in panels c and d, respectively. EDS spectrum is shown in panel e. Figure 4. (a) TEM image in lower magnification for Au/SiO2 doubly coated γ-Fe2O3 NPs; large spherical particles, as marked by the black dashed circles for two of them, are the silica spheres, and the small black dots represent Au particles. (b) Enlarged image of several Au particles that clearly show the lattice fringes. (c) Enlarged image from the framed area (enclosed by the dashed loop) in panel a. to 40° and then slowly beyond 40°. Considering the fact that most of these coated particles are spherical (see TEM results) and the observation that usually spherical SiO2 particles are in the amorphous form, we believe that only a small fraction of the silica is crystallized as a minor phase and that most of the silica nanoshells are in the amorphous phase. Interestingly, the Fe2O3 peaks (Figure 1a,b) appearing in the patterns of the SiO2 coated and uncoated Fe2O3 particles are almost unnoticeable in the pattern of the Au/SiO2 coated particles shown in Figure 1c. This very small intensity of the Fe2O3 peaks can be explained by the strong absorption of and scattering from the coated Au particles. Indeed, such a washingout effect was also observed in XRD patterns for some Au passivated Fe NPs.32 (B) TEM and EDS Results. Figure 3a shows a TEM image of the pure or uncoated Fe2O3 particles at low magnification. The average size of the particles is measured to be DFe2O3 ) 12.4 nm with a standard deviation of 4.5 nm, based on the measurements of 412 particles. This value of average size is slightly larger than (but within one standard deviation of) the nominal size of 10 nm given by the vendor (Ferrotech). The EDS data in Figure 3b confirm that the particle composition is Fe and O without any other impurities. The signal of Cu is from the Cu grid, and C is from the support film on the Cu grid. The framed area (enclosed by the dashed rectangular loop) in Figure 3a is enlarged in Figure 3c, where lattice fringes of the crystalline Fe2O3 crystals are visible. A typical TEM image of the Au and silica doubly coated Fe2O3 nanoparticles is shown in Figure 4a. The large spherical particles, two of which are marked by the dashed circles at the left side of the image, are identified as the silica spheres. The average size of these particles is measured to be Dsilica ) 81.5 nm with a standard deviation of 17.0 nm, based on the measurements of 60 particles. The smaller dark particles distributed on the surfaces of these silica spheres are Au nanoparticles. The average diameter of these Au particles is measured to be DAu ) 6.0 nm with a standard deviation of 1.6 nm, based on the measurements of 365 particles. The coated Au only forms dispersed discrete nanoparticles on the surface of silica spheres, rather than a continuous Au layer. An enlarged lattice image of a gold nanoparticle is shown in Figure 4b, where the Au lattice fringes are clearly visible. Figure 4c is an enlargement of a rectangular area (enclosed by the white, rectangular dashed loop) of a silica/Au coated nanoparticle shown in Figure 4a. In the core region of this coated nanoparticle, lattice fringes of the Fe2O3 particle are visible (in phase contrast), as shown by the white dash loop in Figure 4c. The Fe2O3 particles are larger than the Au nanoparticles, with an average size of around 12 nm. These Fe2O3 particles are embedded inside the silica spheres. The silica, as confirmed by either electron diffraction or the imaging as shown in Figure 4c, remains in an amorphous phase. The Au particles exhibit the darkest contrast because of their highest scattering absorption to electrons as compared to other elements. It should be pointed out that since the Au particles (located on the surface of the SiO2 sphere) and the Fe2O3 core are at different heights along the electron beam, they cannot be focused on at the same time to visualize the lattice fringes. However, the fringes for Au and Fe2O3 can be visualized at different defocus values, as taken for Figure 4b,c, respectively. Another view of the Au and silica doubly coated Fe2O3 NPs is presented as a bright field (BF) image in Figure 5a. Figure 5b is a central dark-field (CDF) image from the same area but taken by tilting the incident electron beam to highlight the crystallites inside. As mentioned before, because the mass of Fe2O3 is much lighter than Au, the image contrast (scatteringabsorption contrast) of Fe2O3 is very weak, making it hard to identify in the presence of the strong Au contrast in the BF image taken at low scattering angles. Fe2O3 is only visible in 18516 J. Phys. Chem. C, Vol. 111, No. 50, 2007 Park et al. Figure 6. Temperature-dependent magnetization curves, in both FC and ZFC nodes, measured at (a) 10 Oe and (b) 500 Oe for uncoated γ-Fe2O3 NPs, respectively. Panel c shows the magnetization curves measured at 500 Oe for the SiO2 coated γ-Fe2O3 NPs without Au, and panel d shows the magnetization curves measured at 500 Oe for Au/SiO2 doubly coated γ-Fe2O3 NPs. the previous phase contrast image in Figure 4b. However, in the CDF image in Figure 5b, as the contrast is formed by diffracted beams at high scattering angles (diffraction contrast), both crystalline Fe2O3 and Au particles exhibit high contrast in the CDF image formed from their common diffracted beam positions. It should be pointed out that only those particles that have their diffracted beams along this tilted incident beam direction are imaged (i.e., only selective fractions of the Fe2O3 and Au particles show up in the CDF image in Figure 5b). Importantly, it can be recognized that larger Fe2O3 particles are at the center of the silica spheres, as pointed out by some arrowheads in the Figure 5. The maps of Si (Figure 5c) and O (Figure 5d) are similar, along the silica spheres in the BF image in Figure 5a. The EDS spectrum taken over this entire area (with the background signals of Cu and C removed) is shown in Figure 5e, and it clearly shows the evidence of O, Si, Fe, and Au. A quantitative analysis yields a composition of 62.6% O, 26.4% Si, 1.7% Fe, and 9.3% Au (all in atom percent). The very low concentration of Fe confirms that only small Fe2O3 particles are present inside the silica. (C) Magnetic Properties. Figure 6 presents the field cooled (FC) and zero-field cooled (ZFC) magnetization M(T) curves for the uncoated and Au/SiO2 doubly coated γ-Fe2O3 NPs. The M(T) curves were measured in a temperature range between 5 and 300 K and at two applied fields: 10 and 500 Oe for the uncoated particles and 500 Oe for the coated ones. Figure 6b shows that the 500 Oe ZFC and FC curves for the γ-Fe2O3 NPs (with DFe2O3 ) 12.4 nm) are irreversible below the irreversible temperature Tirr ≈ 300 K, and the blocking temperature TB, defined as the temperature at the maximum of the ZFC curve,33-35 is TB ≈ 160 K. Such observed irreversibility between ZFC and FC curves and a maximum in the ZFC curve are typical for an assembly of SPNP. We note that the values of Tirr and TB observed here for our 12 nm γ-Fe2O3 NPs are higher than Figure 7. Magnetic hysteresis loops for (a) uncoated γ-Fe2O3 NPs and (b) Au/SiO2 coated γ-Fe2O3 NPs, measured at different temperatures in fields between -50 and +50 kOe. the values Tirr ) 175 K and TB ≈ 120 K measured at the same field (500 Oe) by Jeong et al.35 for their γ-Fe2O3 particles with Structural/Magnetic Properties of SPIO Au Nanoshells J. Phys. Chem. C, Vol. 111, No. 50, 2007 18517 Figure 8. Magnetic hysteresis loops of Figure 8 plotted in range of applied fields between -2 and 2 kOe. a smaller particle size of 5-8 nm. This particle size caused a change in TB and can be explained by the theoretical relation34,35 TB ) KV 25kB (1) where V [(1/6)πD3av] is the average volume of the NPs, K is the uniaxial anisotropy constant, and kB the Boltzmann constant. Indeed, such an increase of TB due to the increase of particle size has also been observed previously for γ-Fe2O3 NPs with an average diameter in the range between 5 and 13 nm.35-37 For example, Mukadam et al.36 found that the TB of their γ-Fe2O3 NPs increased from 80 to 160 K with increasing particle size from 8 to 13 nm, when measured at 100 Oe. The 40 K difference in TB observed between our ∼12 nm NPs and the ∼8 nm NPs of Jeong et al.35 appears to be comparable but slightly smaller than the ∆TB/∆Dav rate observed by Mukadam et al.36 A comparison between the curves shown in Figure 6a,b indicates that with the decrease of the applied field H from 500 Oe to a much lower value of 10 Oe, Tirr and TB both increase to above 300 K. Similar high Tirr and TB values (measured at the same field H ) 10 Oe) were also observed by another group34 for γ-Fe2O3 with a similar particle size Dav ) 11.1 nm. The observed increase of TB with decreasing applied field was also previously observed for γ-Fe2O3 NPs of other particle sizes,36,38 and it can be explained by the theoretical relation39,40 ( TB ) TB0 1 - ) CH2 TB0 (2) where TB0 is the blocking temperature at zero-field and C is a field-independent parameter. By comparing the the ZFC curve in Figure 6c with that in Figure 6b, it can be seen that the blocking temperature TB decreases from 160 K to about 80 K with the coating of Au/ 18518 J. Phys. Chem. C, Vol. 111, No. 50, 2007 Park et al. Figure 9. Plots of coercivity (HC) against T1/2 for uncoated γ-Fe2O3 NPs (solid circles) and Au/SiO2 doubly coated γ-Fe2O3 NPs (open circles). Solid lines are the linear fit of the HC data against T1/2 according to eq 6. SiO2 on the γ-Fe2O3 NPs. Comparison between the magnetization curves in Figure 6c,d shows that further coating of Au particles on the surface of the SiO2 spheres does not change TB. We can attribute the 80 K decrease of TB mainly to the reduction of the average effective volume of the γ-Fe2O3 cores, which is caused by the interfacial interaction between the silica and the outer layer of the iron oxide core. Our TEM results have shown that the SiO2 nanoshells (about 35 nm thick) are coated on γ-Fe2O3 cores and that the Au particles (Dav ≈ 6 nm) are only dispersed in a thin layer near the outer surface of the SiO2 nanoshells. This result means that the Fe ions located near the surface of the γ-Fe2O3 cores can only interact with SiO2 (silica) near the γ-Fe2O3/SiO2 interface, not with the Au particles. Such an interaction between Fe ions and SiO2 could produce a thin layer of misaligned or disordered Fe spins near the surface of the spherical γ-Fe2O3 cores. The spins in this magnetically disordered layer should have a negligible contribution to the total magnetization M for the sample and thus can be excluded from the particle volume V in eq 1. Thus, if the average thickness of the spin disordered layers is t, we can define an average effective volume, Veff,41 for the γ-Fe2O3 cores in the Au/SiO2 coated NPs Veff ) π(Dav - 2t)3 6 (3) Then, eq 1 should be replaced by TB ) KVeff 25kB (4) Combining eqs 3 and 4, we have ( TB(t) ) TB(0) 1 - 2t Dav ) 3 (5) where TB(0) is the blocking temperature at t ) 0. Recently, Rosa et al.41 measured the value of t for γ-Fe2O3 NPs embedded in an amorphous SiO2 matrix using a Faraday rotation technique. They found that t was 1.25 ( 0.07 nm and was almost unchanged for all γ-Fe2O3 NPs with the average diameter in the range of 6.2 nm e Dav e 21.8 nm. For our γ-Fe2O3 NPs, Dav (12.4 nm) falls into this range, and thus, t ) 1.25 nm can be used for estimating TB. Using eq 5 and the values TB(0) ) 160 K, Dav ) 12.4 nm, and t ) 1.25 nm, TB for the Au/SiO2 coated γ-Fe2O3 NPs is estimated to be 81 K, which is in excellent agreement with the experimental value of 80 K. Figure 7 shows the magnetic hysteresis M(H) loops of both the uncoated and the coated γ-Fe2O3 NPs, measured in fields up to 50 kOe and at temperatures from 5 to 300 K. In Figure 8, we show these hysteresis loops in the zoomed region between H ) -2 and 2 kOe to demonstrate more clearly the irreversibility in this region. For fields greater than 2 kOe, all the M(H) hysteresis loops for both the uncoated and the coated Fe2O3 particles are reversible at all temperatures. For fields less than 2 kOe, the hysteresis loops of the uncoated particles are completely reversible or superparamagnetic only in the temperature range T g 100 K. For the coated particles, the irreversibility is seen in Figure 8 at all temperatures. Even at 300 K, there is a very small but noticeable irreversibility within (50 Oe. Thus, it seems that the Au/SiO2 coating extends the irreversibility to higher temperatures. Since the irreversibility of the hysteresis loop for the coated particle is extremely small in the temperature range 100 K e T e 300 K, we can say that the Au/SiO2 coated γ-Fe2O3 NPs are almost superparamagnetic in this temperature range. Another effect of Au/SiO2 coating on the M(H) loops is the decrease of Hirr, which is defined as the field at which the irreversibility occurs. For example, from Figure 8, we see that at 5 K, Hirr is about 1 kOe for the Au/ SiO2 coated γ-Fe2O3 NPs but about 2 kOe for the uncoated γ-Fe2O3. From Figure 7, we see that the saturation moment per gram, Msat, is about 73 emu/g at 5 K and 50 kOe for the uncoated γ-Fe2O3 NPs, corresponding to 2.07 µB per formula unit (f.u.) or 1.03 µB/Fe3+. This value is about 83% of the resultant moment (1.25 µB/Fe3+) of the bulk ferrimagnetic maghemite (γ-Fe2O3).42 With the increase of temperature from 5 to 300 K, Msat decreases monotonically from 73 to 61 emu/g. This range in the values of Msat is comparable to that reported by some other groups for their uncoated γ-Fe2O3 NPs of similar sizes.36,38,43 For Au/SiO2 coated γ-Fe2O3 NPs, the Msat value at 300 K and 50 kOe is about 5.6 emu/g, which is about 9.2% of the Msat value (61 emu/g) for the uncoated γ-Fe2O3 NPs. This decrease in Msat is due to the increase of the mass per γ-Fe2O3 NP by coating Au/SiO2 on the γ-Fe2O3 NPs. Even though the Msat (measured in emu/g) value is decreased substantially by Au/SiO2 coating, the low amount of the maghemite phase in the gold and silica doubly coated sample is still sufficient for the T2-weighted MR imaging application, as demonstrated by our previous research.26 A simple calculation using the values of the mass density and the measured Dav for the γ-Fe2O3 core, Au particles, and SiO2 matrix can confirm that such a decrease of Msat requires an average mass density of 0.2 g/cm3 for the Au/SiO2 nanoshells, which corresponds to a 99.53% volume fraction of SiO2 and 0.47% volume fraction of Au with 0.11 g/cm3 for SiO2 and 19.3 g/cm3 for Au. It is well-known that the coercivity, HC, for superparamagnetic systems varies with temperature according to the wellknown expression12,33 () HC T )1HC0 TB 1/2 (6) where HC0 is the coercivity at 0 K. Thus, in Figure 9, we show the HC versus T1/2 plots below the blocking temperature TB for both the coated and the uncoated γ-Fe2O3 NPs, with the values Structural/Magnetic Properties of SPIO Au Nanoshells of HC obtained from the hysteresis loops shown in Figure 8. The data in Figure 9 show that the T1/ 2 dependence of HC is slightly deviated from linearity; such a deviation from linearity has been previously observed for SiO2 coated γ-Fe2O3 NPs.12 A least-squares fit (shown by the straight lines in Figure 8) to the data by eq 6 yields HC0 ) 239 Oe and TB ) 139.3 K for the uncoated γ-Fe2O3 NPs and HC0 ) 263 Oe and TB ) 113.4 K for the Au/SiO2 coated γ-Fe2O3 NPs. This fitting result shows that the Au/SiO2 coating increases HC0 but decreases TB. The decrease of TB by coating is consistent with the TB results obtained from the ZFC M(T) curves in Figure 6. However, the data points in Figure 9 indicate that HC is increased by coating only at low temperatures (i.e., below 50 K). Above 50 K, the values of HC for the coated NPs are actually slightly smaller than that for the uncoated NPs. 4. Conclusion In summary, we have carried out the first extensive structural and magnetic characterization of uncoated and Au/SiO2 doubly coated γ-Fe2O3 NPs by XRD, TEM, EDS, XAS, and magnetization measurements. The XRD and XAS results confirm that the iron oxide NPs before and after coating have the phase of γ-Fe2O3. However, it appears that the coating of Au particles on silica could induce small crystallization of silica even at room temperature. The TEM measurement shows that the gold nannoparticles are dispersed in the outer layer of the silica spheres and that the average diameters of the γ-Fe2O3 cores, Au/SiO2 doubly coated Fe2O3 NPs, and Au NPs are about 12, 82, and 6 nm, respectively. The magnetization results indicate that coating of γ-Fe2O3 by Au/SiO2 decreases the blocking temperature TB from 160 to 80 K and that such a decrease of TB can be well-explained by the spin disorder and reduction of the effective volume of the γ-Fe2O3 core. Thus, this study provides new evidence that silica coating can induce spin disorder in the outer layer of SPIO particles. The hysteresis loops indicate that for T g 100 K, the uncoated γ-Fe2O3 NPs are superparamagnetic and the Au/SiO2 coated γ-Fe2O3 NPs are almost superparamagnetic. The coercivity HC for both the uncoated and the coated nanoparticles decreases almost linearly with T1/2 with the former decreasing faster than the latter. The linear fitting of the HC versus T1/2 data points confirms that TB is decreased by Au/SiO2 coating. All of these new results provide us with a better understanding of the structural and magnetic properties for gold and silica doubly coated SPIO NPs and thus are very valuable for evaluating the future applications of this class of multifunctional NPs in biomedicine. Acknowledgment. The work at Sam Houston State University was supported by the National Science Foundation under Grant CHE-0718482, a grant from the SHSU EGR program, and an award from the Research Corporation. The work at University of Texas at Austin was supported by National Science Foundation under Grant DMR-0605828 and the Welch Foundation under Grant F-1191. The work at the U.T.M.D. Anderson Cancer Center was supported by the National Cancer Institute under Grant R01 CA119387 and by the John S. Dunn Foundation. References and Notes (1) Bulte, J. W.; Kraitchman, D. L. NMR Biomed. 2004, 17, 484. (2) Wang, Y. X.; Hussain, S. M.; Krestin, G. P. Eur. Radiol. 2001, 11, 2319. (3) Tartaj, P.; Morales, M. del P.; Veintemillas-Verdaguer, S.; Gonzalez-Carreno, T.; Serna, C. J. J. Phys. D: Appl. Phys. 2003, 36, 182. J. Phys. Chem. C, Vol. 111, No. 50, 2007 18519 (4) Mondalek, F. G.; Zhang, Y. Y.; Kropp, B.; Kopke, R. D.; Ge, X.; Jackson, R. L.; Dormer, K. J. J. Nanobiotechnol. 2006, 4, 4. (5) Jain, T. K.; Morales, M. A.; Sahoo, S. K.; Leslie-Pelecky, D. L.; Labhasetwar, V. Mol. Pharmaceutics 2005, 2, 194. (6) Morishita, N.; Nakagami, H.; Morishita, R.; Takeda, S.; Mishima, F.; Terazono, B.; Nishijima, S.; Kaneda, Y.; Tanaka, N. Biochem. Biophys. Res. Commun. 2005, 334, 1121. (7) Tanimoto, A.; Kuribayashi, S. Eur. J. Radiol. 2006, 58, 200. (8) Harisinghani, M. G.; Barentsz, J.; Hahn, P. F.; Deserno, W. M.; Tabatabaei, S.; van de Kaa, C. H.; de la Rosette, J.; Weissleder, R. N. Engl. J. Med. 2003, 348, 2491. (9) Schmitz, S. A.; Coupland, S. E.; Gust, R.; Winterhalter, S.; Wagner, S.; Kresse, M.; Semmler, W.; Wolf, K. J. InVest. Radiol. 2000, 35, 460. (10) Schmitz, S. A.; Taupitz, M.; Wagner, S.; Wolf, K. J.; Beyersdorff, D.; Hamm, B. J. Magn. Reson. Imaging 2001, 14, 355. (11) (a) Frank, J. A.; Anderson, S. A.; Kalsih, H.; Jordan, E. K.; Lewis, B. K.; Yocum, G. T.; Arbab, A. S. Cytotherapy 2004, 6, 621. (b) Wickline, S. A.; Lanza, G. M. Circulation 2003, 107, 1092. (12) Tartaj, P.; Gonzalez-Carreno, T.; Serna, C. J. Phys. ReV. B: Condens. Matter Mater. Phys. 2004, 69, 94401. (13) Tartaj, P.; Gonzalez-Carreno, T.; Serna, C. J. J. Phys. Chem. B 2003, 107, 20. (14) Yu, J.; Lee, C.; Im, S.; Lee, J. ReV. AdV. Mater. Sci. 2003, 4, 55. (15) Caizer, C.; Hrianca, I. Ann. Phys. 2003, 12, 115. (16) Taboada, E.; del Real, R. P.; Gich, M.; Roig, A.; Molins, E. J. Magn. Magn. Mater. 2006, 301, 175. (17) Delahaye, E.; Escax, V.; El Hassan, N.; Davidson, A.; Aquino, R.; Dupuis, V.; Perzynski, R.; Raikher, Y. L. J. Phys. Chem. B 2006, 110, 26001. (18) Wickline, S. A.; Lanza, G. M. Circulation 2003, 107, 1092. (19) Schwartzberg, A.; Olson, T.; Talley, C.; Zhang, J. J. Phys. Chem. B 2006, 110, 19935. (20) Schwartzberg, A. M.; Oshiro, T. Y.; Zhang, J. Z.; Huser, T.; Talley, C. E. Anal. Chem. 2006, 78, 4732. (21) Sokolov, K.; Follen, M.; Aaron, J.; Pavlova, I.; Malpica, A.; Lotan, R.; Richards-Kortum, R. Cancer Res. 2003, 63, 1999. (22) El-Sayed, I. H.; Huang, X.; El-Sayed, M. A. Nano Lett. 2005, 5, 829. (23) Loo, C.; Lin, A.; Hirsch, L.; Lee, M. H.; Barton, J.; Halas, N.; West, J.; Drezek, R. Technol. Cancer Res. Treatment 2004, 3, 33. (24) Hirsch, L. R.; Stafford, R. J.; Bankson, J. A.; Sershen, S. R.; Rivera, B.; Price, R. E.; Hazle, J. D.; Halas, N. J.; West, J. L. Proc. Natl. Acad. Sci. U.S.A. 2003, 100, 13549. (25) O’Neal, D. P.; Hirsch, L. R.; Halas, N. J.; Payne, J. D.; West, J. L. Cancer Lett. 2004, 209, 171. (26) Ji, X.; Shao, R.; Elliott, A. M.; Stafford, R. J.; Esparza-Cross, E.; Bankson, J. A.; Liang, G.; Luo, Z. P.; Park, K.; Markert, J. T.; Li, C. J. Phys. Chem. C 2007, 111, 6245. (27) Stöber, W.; Fink, A.; Bohn, E. J. Colloid Interface Sci. 1968, 26, 62. (28) Badley, R. D.; Ford, W. T.; McEnroe, F. J.; Assink, R. A. Langmuir 1990, 6, 792. (29) Grabar, K. C.; Allison, K. J.; Baker, B. E.; Bright, R. M.; Brown, K. R.; Freeman, R. G.; Fox, A. P.; Keating, C. D.; Musick, M. D.; Natan, M. J. Langmuir 1996, 12, 2353. (30) Luo, Z. P. Acta Mater. 2006, 54, 47. (31) Perkas, N.; Pol, V. G.; Pol, S. V.; Gedanken, A. Cryst. Growth Des. 2006, 6, 293. (32) Carpenter, E. E. J. Magn. Magn. Mater. 2001, 115, 17. (33) Sohn, B. H.; Cohen, R. E.; Papaefthymiou, G. C. J. Magn. Magn. Mater. 1998, 182, 216. (34) Banerjee, S.; Roy, S.; Chen, J. W.; Chakravorty, D. J. Magn. Magn. Mater. 2000, 219, 45-52. (35) Jeong, J.; Lee, S.; Kim, J.; Shin, S. Phys. Status Solidi B 2004, 241, 1593. (36) Mukadam, M. D.; Yusuf, S. M.; Sharma, P.; Kulshreshtha, S. K. J. Magn. Magn. Mater. 2004, 272-276, 1401. (37) Martinez-Boubeta, C.; Simeonidis, K.; Angelakeris, M.; PazosPérez, N.; Giersig, M.; Delimitis, A.; Nalbandian, L.; Alexandrakis, V.; Niarchos, D. Phys. ReV. B: Condens. Matter Mater. Phys. 2006, 74, 54430. (38) Datta, P.; Manivannan, A.; Seehra, M. S.; Shah, N.; Seehra, S. Phys. ReV. B: Condens. Matter Mater. Phys. 2004, 70, 174428. (39) El-Hilo, M.; O’Grady, K.; Chantrell, R. W. J. Magn. Magn. Mater. 1992, 114, 307. (40) Dormann, J.; Fiorani, D.; El Yamani, M. Phys. Lett. A 1987, 120, 95. (41) Rosa, G.; Guerrero, H.; Levy, D.; Alvarez-Herrero, A.; del Real, R. P. J. Appl. Phys. 2005, 97, 64314. (42) de Lacheisserie, E. d. T.; Gignoux, D.; Schlenker, M. Magnetism: Fundamentals; Springer, New York, 2005; p 266. (43) Coey, J. M. Phys. ReV. Lett. 1971, 27, 1140.
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