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Magnetorheology from surface coverage of spin-coated colloidal lmsMoorthi Pichumaniand Wenceslao Gonz´ alez-Vi ~ nas * In magnetorheological uids, the viscosity usually increases with the eld and the non-Newtonian character of these complex uids may vary signicantly. We provide a new method to measure the relative viscosity of a superparamagnetic colloid, by applying a magnetic eld during a spin-coating process, which involves evaporation of the solvent. We dene the compact equivalent height to take into account the discrete nature of the suspension, and we compare experimental results under dierent conditions. We extend the model of Cregan et al. (J. Colloid Interface Sci., 2007, 314, 324) to turn it into an evaporation rate independent one. The generality of the resulting model facilitates measurement of the magnetic eld dependent viscosity. We also discuss the morphologies of the nal dried colloidal deposits and the possible mechanisms involved in their formation. 1 Introduction Spin-coating of polymer solutions 13 has brought commercial advances in manufacturing devices for electronic applications. Recently, this technique has been extended to colloidal systems 48 to produce colloidal crystals. This technique is recognized for its high reproducibility and robustness with colloids. To understand the spin-coating of colloids and to extend its commercial applicability, it is necessary to charac- terize the ow and uid properties 3,9 as well as the fundamental interactions between the particles and the uid. The interac- tions between the colloidal particles have been studied exten- sively; 10,11 however, the spinning duration is as short as a fraction of a second, and the dynamics lies in fast regimes. Some reports 9,1214 provide insights into the spin-coating systems that combine the ow and the properties of uid. Recently, a report on external electric elds while spin-coating a colloid 15 has shown that hydrodynamic ows are aected via dielectrophoretic connement of the suspension that yields colloidal crystals in a predened direction. In the same period, another report 16 showed the possibility of applying a magnetic eld while a superparamagnetic colloid is spin-coated. Hydrodynamical systems in rotation with magnetic elds are under study in broader areas. For example, this kind of systems may be used as models for astrophysical objects in dierent stages of their existence. Another relevant issue which is under consideration by the scientic community is thin lm prepa- ration using external magnetic elds. However, on the one hand there is no complete agreement about the role played by the solvent of an evaporating suspension during the spin coating. Meyerhofer 2 took the eect of evaporation of the solvent into account for the rst time. Several models have been developed that focus on how the rate of evaporation depends on the angular speed u. This dependency is related to the predominant mechanisms in evaporation, namely the removal of solvent vapor from the airboundary layer, the diusion of the liquid solvent to the surface of the colloid, etc. On the other hand, neither the eect of an applied magnetic eld on volatile suspensions of superparamagnetic colloids nor their interplay with fast rotation of the substrate is known. Our results could be applied to other magnetorheological uids, characteristics of which can be found in a recent review. 17 In this article, we show that it is possible to compare the thickness of the dried deposits of spin coated colloids under very dierent conditions. In this rst result we do not apply any magnetic eld. Other results involve a superparamagnetic colloid with and without applied magnetic eld. The model that we develop allows us to obtain the relative variation of the viscosity of the colloid. In the following, we rst provide some information regarding the experiments, and then we will present the model. Finally, we report the experimental results and discuss them. 2 Experimental set-up The experiments were performed in a customized commercial spin-coater at rotation rates from 2000 to 7000 rpm. Magnetic elds ranging from 0 to 0.066 T were applied using a pair of Helmholtz coils which are placed in such a way that the Dept. of Physics and Appl. Math., University of Navarra, Pamplona, Spain. E-mail: [email protected] Electronic supplementary information (ESI) available: Characterization of superparamagnetic particles and lm thickness proles. See DOI: 10.1039/c2sm27682h Present address: Sri Ramakrishna Engineering College, Vattamalaipalayam, NGGO Colony Post, Coimbatore-641 022, India. Cite this: Soft Matter, 2013, 9, 2506 Received 20th November 2012 Accepted 18th December 2012 DOI: 10.1039/c2sm27682h www.rsc.org/softmatter 2506 | Soft Matter , 2013, 9, 25062511 This journal is ª The Royal Society of Chemistry 2013 Soft Matter PAPER Published on 17 January 2013. Downloaded by University of Zurich on 27/08/2013 20:12:08. View Article Online View Journal | View Issue
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Page 1: Magnetorheology from surface coverage of spin-coated colloidal films

Soft Matter

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Dept. of Physics and Appl. Math., Universi

[email protected]

† Electronic supplementary informationsuperparamagnetic particles and

10.1039/c2sm27682h

‡ Present address: Sri Ramakrishna EngNGGO Colony Post, Coimbatore-641 022,

Cite this: Soft Matter, 2013, 9, 2506

Received 20th November 2012Accepted 18th December 2012

DOI: 10.1039/c2sm27682h

www.rsc.org/softmatter

2506 | Soft Matter, 2013, 9, 2506–25

Magnetorheology from surface coverage of spin-coatedcolloidal films†

Moorthi Pichumani‡ and Wenceslao Gonzalez-Vi~nas*

In magnetorheological fluids, the viscosity usually increases with the field and the non-Newtonian

character of these complex fluids may vary significantly. We provide a new method to measure the

relative viscosity of a superparamagnetic colloid, by applying a magnetic field during a spin-coating

process, which involves evaporation of the solvent. We define the compact equivalent height to take

into account the discrete nature of the suspension, and we compare experimental results under

different conditions. We extend the model of Cregan et al. (J. Colloid Interface Sci., 2007, 314, 324) to

turn it into an evaporation rate independent one. The generality of the resulting model facilitates

measurement of the magnetic field dependent viscosity. We also discuss the morphologies of the final

dried colloidal deposits and the possible mechanisms involved in their formation.

1 Introduction

Spin-coating of polymer solutions1–3 has brought commercialadvances in manufacturing devices for electronic applications.Recently, this technique has been extended to colloidalsystems4–8 to produce colloidal crystals. This technique isrecognized for its high reproducibility and robustness withcolloids. To understand the spin-coating of colloids and toextend its commercial applicability, it is necessary to charac-terize the ow and uid properties3,9 as well as the fundamentalinteractions between the particles and the uid. The interac-tions between the colloidal particles have been studied exten-sively;10,11 however, the spinning duration is as short as afraction of a second, and the dynamics lies in fast regimes.Some reports9,12–14 provide insights into the spin-coatingsystems that combine the ow and the properties of uid.Recently, a report on external electric elds while spin-coating acolloid15 has shown that hydrodynamic ows are affected viadielectrophoretic connement of the suspension that yieldscolloidal crystals in a predened direction. In the same period,another report16 showed the possibility of applying a magneticeld while a superparamagnetic colloid is spin-coated.

Hydrodynamical systems in rotation with magnetic elds areunder study in broader areas. For example, this kind of systemsmay be used as models for astrophysical objects in differentstages of their existence. Another relevant issue which is under

ty of Navarra, Pamplona, Spain. E-mail:

(ESI) available: Characterization oflm thickness proles. See DOI:

ineering College, Vattamalaipalayam,India.

11

consideration by the scientic community is thin lm prepa-ration using external magnetic elds. However, on the one handthere is no complete agreement about the role played by thesolvent of an evaporating suspension during the spin coating.Meyerhofer2 took the effect of evaporation of the solvent intoaccount for the rst time. Several models have been developedthat focus on how the rate of evaporation depends on theangular speed u. This dependency is related to the predominantmechanisms in evaporation, namely the removal of solventvapor from the ‘air’ boundary layer, the diffusion of the liquidsolvent to the surface of the colloid, etc. On the other hand,neither the effect of an applied magnetic eld on volatilesuspensions of superparamagnetic colloids nor their interplaywith fast rotation of the substrate is known. Our results could beapplied to other magnetorheological uids, characteristics ofwhich can be found in a recent review.17

In this article, we show that it is possible to compare thethickness of the dried deposits of spin coated colloids undervery different conditions. In this rst result we do not apply anymagnetic eld. Other results involve a superparamagneticcolloid with and without applied magnetic eld. The model thatwe develop allows us to obtain the relative variation of theviscosity of the colloid. In the following, we rst provide someinformation regarding the experiments, and then we willpresent the model. Finally, we report the experimental resultsand discuss them.

2 Experimental set-up

The experiments were performed in a customized commercialspin-coater at rotation rates from 2000 to 7000 rpm. Magneticelds ranging from 0 to 0.066 T were applied using a pair ofHelmholtz coils which are placed in such a way that the

This journal is ª The Royal Society of Chemistry 2013

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Fig. 2 Micrographs of spin-coated substrate at 8 mm from the center of spin-ning. Scale bars are 50 mm. (A) H ¼ 0 and (B) H ¼ 0.066 T. Spinning rate is 5000rpm. When the magnetic field is applied, the superparamagnetic particles accu-mulate together to form elongated clusters.

Fig. 3 Higher resolution micrographs of the spin-coated substrate. The spinningrate is 5000 rpm and the scale bar is 25 mm. (A and B) H ¼ 0 and (C and D) H ¼0.066 T.

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substrate spins in the region of uniform axial magnetic eld. Asketch of the experimental setup is shown in Fig. 1C andphotographs of the spin-coater with Helmholtz coils are shownin Fig. 1A and B. Applied magnetic elds are varied by adjustingthe current in these coils with an external power supply.

Glass substrates of size 38 � 25 � 1 mm3 are used for allexperiments. They are cleaned with acetone in an ultrasonicbath for een minutes followed by a so basic piranha etchwhich consists of ultra-pure water/ammonia/hydrogen peroxideat the ratio of 5 : 3 : 1 at 67 �C for forty minutes. The substratesare rinsed with ultra-pure water aer each cleaning/etch stage.The cleaned substrates are then dried by nitrogen gas blow.Freshly cleaned substrates are used for each experiment.

The particles are superparamagnetic (see ESI†) and consistof silica coatedmagnetite of diameter 1.51� 0.05 mm (density¼1.6–1.8 g cm�3). They are obtained from microParticles GmbH,Germany. The particles are weighed and homogeneously sus-pended in ultra-pure water to obtain a concentration of 1.44%(v/v). The suspension has an estimated viscosity 3.6% higherthan that of ultra-pure water. Experiments which concern thissuspension are referred as SiO2-MAG. The suspension is ultra-sonicated for een minutes before commencing experiments.The spin-coater is operated at a required rotation rate u and themagnetic eld H is applied. Then, 120 ml of suspension ispipetted onto the spinning substrate. Once the spun suspen-sion is dried, the eld is turned off. Micrographs are taken onthe substrates at 2 mm intervals from the center of spinning.Aer checking that under the same conditions (u, H) all thedeposits are similar, we analyzed one micrograph for each set(u, H, r), where r is the distance to the center of spinning.Typical micrographs, from experiments performed withoutmagnetic eld (Fig. 2A) and with magnetic eld (Fig. 2B) areshown. The images are analyzed through home-made routinesin Octave. As all the deposits from this experiment are sub-monolayers we characterize the amount of deposit by the areaoccupied by clusters of superparamagnetic particles relative to

Fig. 1 (A and B) Photographs of experimental components: (A) a pair ofHelmholtz coil and (B) the same mounted on a spin-coater. (C) Sketch of theexperimental setup and the magnetic field lines (HC: Helmholtz coil; S: substrate).The substrate spins in the region of uniform magnetic field.

This journal is ª The Royal Society of Chemistry 2013

the total area of the region. This value is measured for eachmicrograph and it is called “occupation factor” or surfacecoverage 32. For comparison, representative micrographs withand without applied eld are shown in Fig. 3. Although theelongated clusters clearly appear when a magnetic eld isapplied, in previous similar experiments it has been proved thatthey are not oriented.16

To check the validity of the model (see below) we consider areference experiment, whose results were reported by Giulianiet al.18 They used plain silica particles with a diameter of 458 nmsuspended in Methyl Ethyl Ketone (MEK). The concentrationwas 20% (v/v). They spin-coated the non-magnetic colloidwithout magnetic eld at various spinning rates. Results con-cerning this experiments are referred as SiO2-NM.

3 Model3.1 Previous results

In 1958, Emslie et al.1 reported a model of spin-coating withoutevaporation. That model accounts for (a) the viscous forcescaused by the uid properties and (b) the centrifugal forces ofspinning. When a polymer solution is spun, it leaves a thin layerindicating that the solvent has evaporated. To account forevaporation, Meyerhofer2 included a correction based on the

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assumption that the spin-coating process consists of twodifferent stages: (a) a ow dominated phase followed by (b) anevaporation dominated phase. There are reports19,20 that furthercharacterize the uid ow of non-Newtonian liquids. Later on,Cregan and O'Brien21 considered that the solvent evaporation issimultaneous with the ow dominated phase because thesolvent starts to evaporate once the suspension is pipetted on tothe spinning substrate. Although the Cregan model is moresophisticated, it assumes a constant evaporation rate E. That is,E is not considered to depend on the rotation rate u. In othermodels,2,9 it is assumed that Efu

12 or E f u.

In the Cregan model, the deposited layer thickness (h(s)N),where the s superscript indicates ‘solute’ and ‘N’means at longtimes, i.e. when the colloid is dried on the substrate, is given by:

hðsÞN ¼ hðsÞ0

hðlÞ0

�E

a

�13

; (1)

where h(s)0 and h(l)0 are the initial solute and the solvent thick-ness, respectively. The measurable quantity is the initial lm

thickness h(s)0 + h(l)0 . Also, in eqn (1), a ¼ 2u2

3nwhere u is the

spinning rate and n is the kinematic viscosity of solvent. E, asmentioned above, corresponds to the evaporation rate of thesolvent.

It is assumed that the initial suspension is homogeneous.Then, the thicknesses can be converted into volumes and hence

hðsÞ0

hðlÞ0¼ C

1� C, where C is the initial concentration in v/v. Eqn (1)

thus becomes:

hðsÞN ¼ C

1� C

�3

2nE

�13

u�23 ¼ Au�b; (2)

where A is a constant over the experiment and b ¼ 23.

3.2 Spin-coating of a colloid

We assume that the solvent is volatile enough, such that thecharacteristic time in which appears an appreciable gradient ofconcentration due to the centrifugal force is smaller than theexperiment duration. Consequently, the suspension volumeelements move as a whole and the discrete nature of thedeposited colloidal particles can be taken into account by theuse of a compact equivalent height (CEH). The CEH is denedas the thickness of a homogeneous layer whose volume is thesame as the particles deposited (Fig. 4).

Under this assumption we may use a continuum valid modeljust by substituting the thickness of the deposited homoge-neous layer with the CEH. So, from now on, we are going to useh(s)N as the valid notation in colloidal spin-coating. Of course, the

Fig. 4 Sketch for the meaning of the compact equivalent height (CEH) of adeposit.

2508 | Soft Matter, 2013, 9, 2506–2511

thickness could be dependent on the distance to the center ofrotation r (non-planarization).18 Thus, the denition has to beproperly extended to a local one. Nevertheless, in this section weare going to consider a constant thickness.

In the case of submonolayers formed by 2-D hexagonalstructured clusters, which is a good approximation for non-chained clusters,

hðsÞN ¼ 2p

3ffiffiffi3

p R32; (3)

where R is the radius of the colloidal particles. The coefficient of32 comes from geometric considerations.

In the case of multilayers, the CEH is proportional to thenumber of layers n, as each layer accounts for the number ofparticles per unit area. The coefficient of n is also of geometricnature and depends on the microscopic structure and orienta-tion. It is assumed that the most common structures in spincoating of colloids correspond to the most close packed ones(fcc and hcp).5–8 For the case of fcc100 it can be straightforwardly

proven that hðsÞN ¼ 2p6

Rn ¼ p

3ffiffiffi2

p h� þ ð1� ffiffiffi2

p Þ 2p6

R. For the case

of hcp, hðsÞN ¼ 2p3ffiffiffi3

p Rn ¼ p

3ffiffiffi2

p h� þ 1�

ffiffiffi32

r !2pR3ffiffiffi3

p . In both

cases h* is the dimensional thickness of the deposit.For a large number of layers (n[ 1), in general h(s)N z APF�

h*, where APF is the atomic packing factor for the structure. Inthe case of fcc and hcp:

hðsÞNzp

3ffiffiffi2

p h�: (4)

3.3 Scaling of thicknesses of colloidal deposits underdifferent conditions

To compare two experiments that follow the same continuummodel, but performed under different conditions, it is possibleto compute the ratio between both CEH. In the most complexcase of one being a multilayer-reference and the other being amonolayer:

hðs;refÞN

hðsÞN

¼ 1

2

ffiffiffi3

2

rh�refR32

; (5)

where R is the radius of the particles of the submonolayer. Here,the le hand side of the equation can be substituted by theconsidered model. If we want to compare an experiment whichgives a submonolayer to the height of a reference experimenth*ref in a graph, we should plot also the scaled height for thesubmonolayer hscaled:

hscaled ¼ 2

ffiffiffi2

3

rR32

hðs;refÞN

hðsÞN

; (6)

which in the case of the Cregan model becomes:

hscaled ¼ 2

ffiffiffi2

3

rR32

Aref

A: (7)

This journal is ª The Royal Society of Chemistry 2013

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3.4 Magnetorheology

In this subsection, we generalize eqn (2) by including an evap-oration rate thatmay depend onu, but not on themagneticeld.

Now we compare two experiments performed under the sameconditions except for the appliedmagnetic eld, which both leadto submonolayers. We compare them, as before, by computingthe ratio of the corresponding CEH. In the case of one withoutmagnetic eld and the other with applied magnetic eld:

hðsÞN ðH;uÞhðsÞN ðH ¼ 0;uÞ

¼ 32ðH;uÞ32ðH ¼ 0;uÞ : (8)

If we substitute the le hand side of eqn (8) by the corre-sponding generalized Cregan equation, the only parameter whichremains dependent on the eld is the kinematic viscosity n. Thisleads to:

nðH;uÞnðH ¼ 0;uÞ ¼

�32ðH;uÞ

32ðH ¼ 0;uÞ�3

(9)

4 Results and discussion4.1 Occupation factor and non-planarization

From the spin-coated substrates, micrographs are taken at 2mm increasing intervals from the center of spinning (r).Representative micrographs are shown in Fig. 2. The micro-graphs are thresholded, segmented and then analyzed throughhomemade routines in Octave. For each micrograph we calcu-late the occupation factor 32. Plots of the occupation factor at aspinning rate of 5000 rpm for different magnetic eld strengthsare shown in Fig. 5. In general, it depends on r as the volatilecolloidal suspensions do not planarize.18 Nevertheless, as therotation rate increases, the non-planarization becomes lessevident. For a given spinning rate, mean occupation factors arecalculated for the different applied magnetic elds and they areused for further analysis.

Fig. 5 Occupation factor as a function of increasing radial distance from thecenter of spinning. Spinning rate is 5000 rpm. The estimated error for these data isof the order of 0.02.

This journal is ª The Royal Society of Chemistry 2013

4.2 Film thickness and comparisons with models

Without applied magnetic eld. As has been alreadymentioned, we compare our results to the reference experiment(SiO2-NM) reported by Giuliani et al.18 In order to overcome thenon-planarization, we use a spatial average of the nal depositthickness, which was measured utilizing Atomic Force Micros-copy (Fig. 4a of the reference experiment letter18). This thickness(h*ref) corresponds to a multilayer because the suspension isconcentrated enough, and it is plotted as a function of u, rep-resented by circles in Fig. 6. Using eqn (7), the scaled thicknessfor the deposits of SiO2-MAG experiments is calculated andplotted, with squares, in Fig. 6. The deposits of SiO2-MAGcorrespond to submonolayers because the suspension is diluteenough. Standard deviation in each value characterizes the non-planarization phenomenon. In the ESI,† results correspondingto other conditions are compared to SiO2-NM and SiO2-MAGand show good agreement.

Although particles and solvents have very different charac-teristics (as detailed the experimental set-up section), data fromboth experiments collapse onto a single curve. The commoncurve represents a decreasing tendency for deposit thickness asthe spinning rate is increased. The deviation from the commoncurve at high angular speeds (7000 rpm)may come from the factthat, as the solvent for the SiO2-MAG (water) is more viscous andless volatile, there is shear thickening behavior with respect tothe SiO2-NM case (suspension in MEK).

We compare the correlated experimental data with appro-priate models.2,9,21Our experimental data are in good agreementwith all these models within the experimental error, see squaresand big circles in Fig. 7. As said above, irrespective of the natureand the kind of suspension, the nal deposit thickness dependson the spinning rate u. Power-law t to the non-magneticSiO2-NM reference experiment shows a strong dependency on

the spinning rate, u�34 (Fig. 7 – solid line). The exponent value is

Fig. 6 Comparison of the film thickness profile for different colloids withoutapplied magnetic field. Squares: SiO2-MAG; circles: SiO2-NM. For the latter case,the information is extracted from Fig. 4a of the reported18 reference experimentby doing a spatial average. Data from both experiments seem to collapse onto asingle curve.

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Fig. 7 Comparison of the film thickness profiles for different suspensions withmodels. Squares: SiO2-MAG; big circles: SiO2-NM. For the big circles, the infor-mation is extracted from Fig. 4a of the reported18 reference experiment by doinga spatial average. The data from both experiments collapse onto a single curve.The solid line is the best power-law fit to the SiO2-NM reference experiment. Thedata from experiments are compared with the relevant models.2,9,21 The dottedline corresponds to the model proposed by Cregan and O'Brien.21 Trianglesrepresent the model from Meyerhofer2 and the small circles are obtained usingthe model reported in ref. 9.

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close to the reported one�� 23

�, in the model proposed by

Cregan and O'Brien.21 Nevertheless, the other consideredmodels could also be valid.

With applied magnetic eld. On applying a magnetic eldwhile spin-coating, the scaled thickness for the deposits of SiO2-MAG experiments decreases as the spinning rate is increased. InFig. 8, for clarity, one case corresponding to the eld condition

Fig. 8 Comparison of the film thickness profiles for different colloids withoutand with applied magnetic field. Squares: SiO2-MAG, H ¼ 0 T; diamonds: SiO2-MAG, H ¼ 0.011 T; circles: SiO2-NM. For circles, the information is extracted fromFig. 4a of the reported18 reference experiment by doing a spatial average. Dashedline is a comparison to Cregan model.

2510 | Soft Matter, 2013, 9, 2506–2511

is plotted using diamonds. In this situation too the decreasingtendency of the scaled thickness depends on the spinning rate;however, the thickness value for a given spinning rate is higher(diamonds in Fig. 8) than the ones obtained without magneticeld (squares in Fig. 8). This indicates an increase in meanoccupation factor when a eld is applied. The magnetic dipoleinteractions of the superparamagnetic particles increase theeffective viscosity of the suspension,16 which in turn increasesthe mean occupation factor. The even increase of the meanoccupation factor at low elds indicates that the main effect ofthe magnetic eld is to increase the effective viscosity of thesuperparamagnetic colloid.

4.3 Magnetorheology

Using eqn (9), the relative change in viscosity due to the appliedeld can be calculated. This equation is independent of themodel which assumes the compact equivalent height. As statedabove, we generalize the equation reported by Cregan andO'Brien21 so that the evaporation of solvent may depend on thespinning rate. Information regarding the occupation factor canbe obtained directly from the SiO2-MAG experiments (with andwithout magnetic elds, respectively). We plot the mean andstandard deviation for relative change in viscosity for all u asshown in Fig. 9. The standard deviation in the form of error barappears due to the varying spinning rate and each valueemphasizes the critical role played by u. Nonetheless, one canrelate a larger standard deviation to a more relevant non-New-tonian character5,22,23 as the applied elds are increased. Themean relative viscosity is larger with the eld. This is throughthe magnetic dipole interactions between the super-paramagnetic particles.16 At high magnetic elds, more parti-cles accumulate in elongated clusters. Morphological transitionfrom sparse (without magnetic eld) to sub-monolayer deposits(with magnetic eld) of superparamagnetic particles can beseen in Fig. 2 and 3. Under similar experimental conditions, wedid not observe any preferred direction for these clusters16 andorienting them in a desired direction is challenging.

Fig. 9 Relative change in the viscosity for all spinning rates, in the form of meanvalue and standard deviation, as a function of the applied magnetic fields.

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5 Conclusions

In the absence of a magnetic eld we prove that it is possible tocompare results from experiments under very different condi-tions under a common frame; at least for the thicknesses of thecolloidal deposits. We were able to introduce a CompactEquivalent Height that allows us to extrapolate results fromclassical spin-coating to colloidal spin-coating.

We observe that the main effect of the magnetic eld on asuspension made of superparamagnetic particles and volatilesolvents is the formation of clusters of irregular shapes and ofchain-like shapes. The latter are advected by the strong ows ofthe spin-coating process, which randomize the cluster orienta-tions. Consequently, we can only observe a change of therheological properties of the system.

Our experiments could provide indications on the structureformation mechanisms while using the spin-coating methodwith colloids. To understand these mechanisms, thephenomena occurring at concentrations corresponding to thetransition from submonolayers to multilayers should bestudied; this work is in progress.

We also were able to measure the relative viscosity when amagnetic eld is applied, and the overall change in the non-Newtonian character of the suspension. This technique couldbe applied to other magnetorheological uids, where we mayrecover already known behaviors.24 As the future of magneto-rheological uids is very promising,17 to support the broadapplication of this method independent measurement of theeld-dependent viscosity under shear stresses could be initi-ated. Established methods such as rheological microscopes25–27

can be employed but the presence of external magnetic eldsduring the measurement is challenging.

Acknowledgements

We thank A. Irigoyen Barrio for his help in preparing thecolloidal suspension. We acknowledge C. Gomez-Polo for hergenerous loan of SQUID and fruitful discussions, and J.M.Pastor and M.A. Miranda for the magnetic characterization ofthe superparamagnetic colloidal particles. We thank Claire F.Woodworth for her help in correcting grammar mistakes whilepreparing the manuscript. This work is partly supported by theSpanish Government Contract no. FIS2011-24642. M. P.acknowledges the nancial support from the “Asociacion deAmigos de la Universidad de Navarra” and the Management, SriRamakrishna Engineering College, Coimbatore, India.

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4 P. Jiang and M. McFarland, J. Am. Chem. Soc., 2004, 126,13778–13786.

5 L. Shereda, R. Larson and M. Solomon, Phys. Rev. Lett., 2008,101, 16–19.

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