Laser Induced Breakdown Spectrometry of Vanadium in Titania Supported Silica Catalysts

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    Talanta 47 (1998) 143151

    Laser induced breakdown spectrometry of vanadium in titania

    supported silica catalysts

    P. Lucena a, L.M. Cabaln a, E. Pardo b, F. Martn b, L.J. Alemany b, J.J. Laserna a,*a Department of Analytical Chemistry, Faculty of Sciences, Uniersity of M alaga, E-29071, Malaga, Spainb Department of Chemical Engineering, Faculty of Sciences, Uniersity of Malaga, E-29071, Malaga,Spain

    Received 17 September 1997; received in revised form 4 February 1998; accepted 10 February 1998

    Abstract

    The capability of laser induced breakdown spectrometry (LIBS) for vanadium determination in a x V2TiO2SiO2catalyst is presented. The microplasma was generated onto the sample surface using a pulsed Nd:YAG laser operating

    in the second harmonic (532 nm). Laser produced plasmas were collected and detected using a charge-coupled device

    (CCD). In order to minimize the complex spectral interferences of emission lines and matrix effects a wide spectral

    range (210 660 nm) was studied. The focusing of the laser beam on the surface was optimized to improve the

    signal-to-background ratio, and consequently the limit of detection. The analytical lines selected were used to evaluate

    the calibration curve. The detection limit for V was estimated to be 38 g g1 in 2TiO2 SiO2. The method precision

    expressed as relative standard deviation (RSD) was better than 6% in the concentration range 2001000 g g1.

    1998 Elsevier Science B.V. All rights reserved.

    Keywords: LIBS; Vanadium analysis; Catalysts; Quantitative determination

    1. Introduction

    TiO2-supported vanadium oxides have been ex-

    tensively studied and used due to their high cata-

    lytic activity and selectivity in many chemical

    reactions [17]. For instance, V/TiO2is one of the

    most effective catalysts in the selective catalytic

    reduction (SCR) of NOx

    by NH3 [7,8]. Industri-

    ally, in these catalysts the anatase, a polymorph

    form of TiO2, is used as support for vanadium

    oxide. Titania is the support more widely used for

    this purpose, although alumina, and to a lesser

    extent silica are also used. In spite of its wide use,

    titania suffers several drawbacks, including lim-

    ited surface area, poor mechanical strength and a

    low sintering resistance. On the other hand, the

    interaction of vanadia with silica is weak and,

    consequently it results in a higher tendency to

    thermally induced aggregation with a poor disper-

    sion of the active phase, while alumina-supported

    vanadia catalysts are susceptible to sulfation. The

    binary TiO2 SiO2 system, in principle, seems an

    ideal candidate to overcome the above disadvan-

    tages [9].* Corresponding author. Tel.: +34 5 2131881; fax: +34 5

    2132000; e-mail: [email protected]

    0039-9140/98/$19.00 1998 Elsevier Science B.V. All rights reserved.

    PIIS0039-9140(98)00063-0

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    P. Lucena et al./Talanta 47 (1998) 143151144

    It is envisaged that ternary V Ti Si systems

    display similar characteristics to those of binary

    V Ti catalysts. In addition to the economic

    benefits, the presence of silica grants much better

    mechanical properties to the system, which may

    allow its application in fluidized bed reactors or

    extrusion into monolith reactors. The bulk, the

    surface physico-chemical properties and the reac-tivity of VTiSi systems are strongly dependent

    on the method used for their preparation and the

    precursors used in the vanadia distribution. Vana-

    dium loading determines the nature and distribu-

    tion of vanadia species on the titania support.

    Therefore the structure and morphology of the

    TiO2 SiO2 substrate will determine to a large

    extent the dispersion of vanadia. In contrast to

    binary systems, ternary catalysts are still not fully

    understood.

    For VTiSi systems, it is very interesting to

    evaluate the dispersion and possible diffusion of

    vanadium into the support. Knowledge of thequantitative microstructure and composition are

    of great importance in understanding the possible

    correlations of distribution and composition with

    catalytic properties. Consequently, the develop-

    ment of analytical methods for these materials is

    of great practical interest.

    The capability of laser induced breakdown

    spectrometry (LIBS) for materials characteriza-

    tion has been widely demonstrated [10 14]. Re-

    cent analytical applications of LIBS include the

    determination of aluminum in zinc alloy [15], the

    simultaneous determination of aluminum, copper,

    iron, nickel, and zinc in alloys [16], the determina-tion of copper in steel [17], and the detection of

    lead in concrete [18]. Surface analysis of photonic-

    grade silicon has been demonstrated [19,20]. How-

    ever, no applications of LIBS for vanadium

    determination in catalysts have been previously

    reported. For this purpose, other surface analysis

    techniques (such as secondary ion mass spec-

    trometry; X-ray photoelectron spectroscopy) can

    be used [21]. In comparison with those techniques,

    LIBS presents a number of advantages including

    the need for little or no sample preparation, the

    minute sample quantities needed, the possibility

    of work without controlled atmospheres and the

    rapid analysis time. In this paper, LIBS has been

    evaluated for the quantitative determination of

    vanadium in xV2TiO2 SiO2 catalysts.

    2. Experimental section

    2.1. Apparatus

    The LIBS system has been described in previ-

    ous works [22,23]. Briefly, it consisted of a pulsed

    Nd:YAG laser operating in the second harmonic

    (Continuum, model Surelite SLI-20, =532 nm,

    pulse width 5 ns), which was used to generate the

    microplasma. The laser energy at the sample was

    4 mJ pulse1. The laser beam was focused at

    normal incidence onto the sample surface using a

    planoconvex glass lens with a focal length of 100

    mm and f-number of 4. The plasma image was

    collected by a planoconvex quartz lens with focal

    length of 100 mm and dispersed by an imaging

    spectrograph (Chromex, model 500 IS, fitted withthree indexable gratings of 300, 1200 and 2400

    grooves mm1). Two of the three gratings (300

    and 2400 grooves mm1) were employed in this

    study. The reciprocal linear dispersion was 20 and

    2.5 nm mm1, respectively. These values gave

    spectral coverages of 120 nm for the 300 grooves

    mm1 grating and 15 nm for the 2400 grooves

    mm1 grating with the detector used. The en-

    trance slit width was 10 m and the height was 10

    mm.

    The spectrally resolved light was detected with

    a solid-state two-dimensional charge-coupled

    device (CCD) system (Stanford Computer Optics,model 4 Quik 05). The CCD consists of 752(h)

    582(v) elements. The photoactive area is 64.5

    mm2. The spectral resolution of the system was

    0.16 and 0.02 nm pixel1 using the 300 grooves

    mm1 and the 2400 grooves mm1 gratings,

    respectively. The CCD is equipped with an S 20 Q

    photocatode (spectral response from 180 to 820

    nm) and an intensifier system (microchannel plate,

    MCP). Operation of the detector was controlled

    by 4 Spec 1.20 software. Shutter and delay times

    can be selected in 50 ns steps. A fast photodiode

    was used as external trigger for exact synchroniza-

    tion of the incident laser pulse and opening of the

    camera shutter. The emission signal was corrected

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    P. Lucena et al./Talanta 47 (1998) 143151 145

    by subtraction of the dark current of the detector,

    which was separately measured for the same expo-

    sure time. Calibration of the detector system was

    conducted by using a mercury emission lamp and

    several lines emitted from a laser induced titanium

    plasma. Samples were placed on a manual XY

    Z translation stage to be moved with respect to

    the laser beam.

    2.2. Samples

    Catalysts were prepared using 2TiO2 SiO2 as a

    carrier for the ternary systems xV2TiO2 SiO2.

    Silica microspheres (Aerosil 200 from Degussa)

    with size ca. 13 nm diameter and surface area of

    200 m2 g1 were used as starting material. The

    resulting xV2TiO2 SiO2 material was obtained

    by co-deposition of titania and vanadia on the

    silica surface by incipient wetness impregnation,

    as described by Geuss et al. [24] and others [25

    28]. The impregnation was made by adding amethanolic solution containing variable amounts

    of titanium tetraisopropoxide and vanadium

    acetil-acetonate to the support particles. The sus-

    pension was ultrasonically dispersed to ensure a

    good homogeneity. The superficial precipitation

    on silica occurs in a few minutes at room temper-

    ature. Powders were then washed and dried in air

    at 373 K overnight, and afterwards they were

    calcined at 773 K in air for 2 h. This procedure

    allows deposition of oxo-hydrated titanium

    vanadium, which yields dispersed TiO2, with

    vanadium incorporated into the TiO2 crystal lat-

    tice. Several samples with different vanadiumloads were prepared, and they are labelled as

    xV2TiO2 SiO2, where x denotes the theoreti-

    cal vanadium loading in g g1 and 2TiO2, two

    theoretical monolayers incorporated onto the sil-

    ica surface. A monolayer was considered as the

    loading of titania for completed covering of silica

    surface by a 0.38 nm thick [26] film of TiO2,

    which corresponds to the longest axis of the rutile

    unit cell. The titanium oxide incorporated on

    silica remains as small crystals of anatase covering

    the silica surface, as previously reported by

    Galan-Fereres et al. [26].

    A set of six sample pellets were grounded with

    a mortar and pelletized at a pressure of 7.5 Ton

    cm2 for 15 min. Approximately 0.15 g of mix-

    ture was pressed leading to samples of 13 mm in

    diameter and about 0.5 mm thick. Concentration

    of the calibration standards was in the range

    20010000 g g1 vanadium in the 2TiO2 SiO2support. In addition, for qualitative analysis other

    series of three pellets was prepared: one pellet

    with a 2TiO2 SiO2 support, the second one withvanadium in form of V2O5 and the third one with

    a 1:1 (w/w) V2O5 TiO2 mixture. As precision and

    accuracy of LIBS are highly dependent on sample

    composition, homogeneity, and surface condition,

    samples were carefully prepared according to the

    described methodology.

    3. Results and discussion

    3.1. Spectral analysis

    In the analysis of solid samples by LIBS, theresulting plasma includes lines corresponding to

    the sample elements and matrix constituents.

    Thus, the goal in the quantitative determination

    of an element by LIBS is to find a well-resolved

    line for the element of interest, free of matrix

    interferences. In the determination of V in xV

    2TiO2 SiO2 samples, silica can be easily iden-

    tified. A simple study of spectral range permits the

    choice of the optimal region for observing vana-

    dium without spectral interferences of Si and O

    emission lines. The main problem in this kind of

    sample is the presence of TiO2. The large number

    of Ti lines along the UV-VIS region and theirhigh intensities can complicate the qualitative and

    quantitative analysis. Five different spectral re-

    gions were studied for the most important emis-

    sion lines of Ti and V in the range 210660 nm.

    The spectral window covering the range 404418

    nm was chosen since it contains the most intense

    vanadium peak (411.18 nm) free from interference

    of neighbouring spectral lines. Fig. 1(ac) shows,

    respectively, the LIBS spectra corresponding to

    the 2TiO2 SiO2 matrix, to neat V2O5 and to a 1:1

    (w/w) V2O5 TiO2 mixture. As shown in Fig. 1(c),

    the main peaks for Ti and V are clearly distin-

    guished. In these figures, only the most intense

    emission lines were labelled [29]. Spectra were

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    P. Lucena et al./Talanta 47 (1998) 143151146

    obtained using a single laser shot. Integration

    time and delay time were 1 s and 300 ns,

    respectively.

    3.2. Effect of laser beam focusing on the

    signal-to-background ratio

    It is well-known that performance of LIBS for

    quantitative analysis is related among other fac-

    tors to the signal-to-background ratio (S/B) [30].

    Since the background in LIBS depends on the

    laser fluence used, a study on the effect of laser

    focusing conditions on the S/B was performed.

    Fig. 2 shows the variation of the average signal-

    to-background values and their precision (in

    terms of relative standard deviation, RSD) as a

    function of the relative lens-target distance. The

    values were calculated taking the background as

    the mean background signal along 30 pixels in an

    interference free region and close to the peak of

    interest. In Fig. 2, the distance 0 indicates that

    the sample was placed at the lens focal length.

    Positive values of the relative focusing lens-target

    distance refer to the beam focused at a distance

    above the sample surface, while negative values

    refer to the beam focal position placed inside the

    material.From this figure, it is interesting to note that

    the S/B precision appeared approximately con-

    stant for relative lens-target distances from 2 to

    +4 mm. However, the S/B reached a maximum

    when the focal point was placed 12 mm above

    the target surface. This value decreases drastically

    when the laser beam was defocused a few millime-

    ters onto the sample surface because the laser

    fluence decreases. Scanning electron micrographs

    of the craters produced by laser ablation in the

    10000V2TiO2 SiO2 pellet surface at two differ-

    Fig. 1. Single-shot LIB spectra corresponding to (a) 2TiO2SiO2support, (b) V2O5and (c) 1:1 (w/w) V2O5TiO2mixture. The delay

    time was 300 ns. Acquisition time was of 1 s. MCP gain: 700 V.

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    P. Lucena et al./Talanta 47 (1998) 143151 147

    Fig. 1. (Continued)

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    P. Lucena et al./Talanta 47 (1998) 143151148

    Fig. 2. Signal-to-background ratio and its RSD (%) vs relative focusing lens-target distance. The V(I) line at 411.18 nm was used

    for the measurements and the results were obtained using the pellet 10000V2TiO 2SiO2 support. Other conditions as in Fig. 1.

    ent focusing distances are shown in Fig. 3. Micro-

    graphs A and B were taken respectively at the

    focal point and at a relative lens-target distance of

    +2 mm, respectively. Two cumulative laser shots

    were used. Micrographs confirm that the 0 posi-

    tion presents the smallest irradiated surface. How-

    ever, the efficiency in ablating the sample, and

    consequently the S/B, can be increased when the

    laser beam is focused above the focal point (+2

    mm) because the laser energy is still enough to

    allow ablation and the beam has a larger area ofcontact with the target surface. When further

    defocused, the laser fluence becomes lower and it

    is less efficient in ablating the sample. Conse-

    quently, the optimum focal condition for both

    maximum ablation and higher signal-to-back-

    ground ratio is at a focusing lens-target distance

    of+2 mm.

    The irradiated areas and the laser fluences for

    each focusing distance are summarized in Table 1.

    The ablated areas were calculated assuming an

    elliptical shape of the crater. As shown, a fluence

    of 2.6 J cm2 with ablated area of 18.6102

    mm2 were found for the optimum focusing condi-

    tions. It should be to noted that although the

    plasma is formed at atmospheric pressure and

    above the focal point, the laser fluence used is

    below the threshold fluence for breakdown of air,

    and hence no lines corresponding to its several

    components are observed.

    3.3. Quantitatie analysis

    It is well known that at early times following

    plasma formation, the LIBS spectrum is domi-

    nated by an intense radiation continuum andionic emissions. Emission lines are broadened by

    the Stark effect. Temporal resolution was found

    to improve both linearity and signal reproducibil-

    ity of the catalyst analysis. In this case, to com-

    pensate for the decreased signal at delayed

    integration, ten laser shots were accumulated. The

    optimal delay was estimated to be 1.3 s after the

    laser shot. The use of internal standardization was

    necessary to compensate for the pulse-to-pulse

    variability and to minimize matrix effects. At

    delayed integration, continuum emission was re-

    duced, but the intensity of the lines of the internal

    standard were also affected. For instance, the

    ionic Ti (II) line intensity at 416.37 nm decreased

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    P. Lucena et al./Talanta 47 (1998) 143151 149

    Fig. 3. Scanning electron micrographs of 10000V2TiO2SiO2 sample, showning the craters produced after two cummulative laser

    shots. (A) Sample placed at the focusing lens focal position. (B) Sample placed 2 mm below the focusing lens focal position.

    significantly, while the intensity of the neutral Ti

    line at 407.85 nm increased. For this reason, the

    atomic emission line of Ti was then chosen for

    internal standardization. In addition, this line sa-

    tisfies the regular requirements of an internal stan-

    dard, i.e. proximity to the analyte line and

    freedom from interference with the neighbouring

    spectral lines.

    Several lines of V were evaluated to construct

    the calibration graph. The V(I) line at 411.18 nm

    was finally selected as it provides the largest sensi-tivity with the smallest standard deviation, thus

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    P. Lucena et al./Talanta 47 (1998) 143151150

    Table 1

    Irradiated areas and laser fluences at different focusing lens-to-

    sample distances

    Focusing lens-target Fluence (J cm2)Crater area

    (mm2, 102)distance (mm)

    3 42.1 1.0

    2.615.72

    6.5 6.215.0 8.00

    +1 15.6 2.7

    +2 18.6 2.6

    +3 30.8 1.3

    The sample was 10 000 g g1 V in a TiO2SiO2 support.

    presents good linearity, with correlation coeffi-

    cient R2=0.9966. Deviation from linearity was

    found at concentrations above 1000g g1, prob-

    ably due to self-absorption [31,32].

    The detection limit (CL) was calculated from

    the formula:

    CL=3s/S

    where s is the standard deviation of the V to Tisignal ratio at low concentration andS represents

    the method sensitivity calculated from the slope of

    the linear section of the calibration curve. The

    LOD from the time-resolved calibration graph

    using thes value at 200 g g1 V was 38 g g1

    V. This value is well below the V level expected in

    xV2TiO2 SiO2 catalysts. The method precision

    was better than 6% RSD in the concentrate range

    2001000 g g1.

    To check for the accuracy of the proposed

    method, a recovery experiment was performed.

    The results are summarized in Table 2. As shown,

    recovery values are satisfactory, better than 90%

    leading to the best limit of detection. Fig. 4 shows

    the calibration graph for V in the 2TiO2 SiO2support. This figure presents the ratio between the

    net line intensities of vanadium and internal stan-

    dard as a function of V concentration. The net

    peak signal was obtained by subtraction of the

    background signal. As shown in Fig. 4, the curve

    Fig. 4. Time-resolved calibration curve of V in a 2TiO2SiO2 support. The intensity of the 411.18 nm V(I) line was ratioed to that

    of the 407.85 nm Ti(I) line. For construction of the calibration curve, mean values were calculated from six repeated measurements,each measurement representing an average of ten shots, from different target locations. The Inset shows the linear portion of

    calibration curve where each point represents the mean value.

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