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Ch. Ramesh Kumar et al. / Applied Catalysis A: General 502 (2015) 297–304
Scheme 1. Structure of (a) niobium incorporated Keggin ion (TPANb1 or [PW11Nb1O40
]
4−), (b) niobium salt of tungstophosphoric acid (Nb0.6TPA or Nb0.6PW12O40), and (c)
tungstophosphoric acid supported on niobia (25% TPA/Nb2O5 or 25% H3PW12O40/Nb2O5).
model reaction. The influence of different benzylating agents is also
studied.
and secondary graphite monochromatic. The measurements were
obtained in steps of 0.045◦ with count times of 0.5 s, in the 2ꢀ range
of 2–80◦.
Confocal micro-Raman spectra were recorded at room temper-
2. Experimental
ature in the range of 200–1200 cm−1 using a Horiba Jobin-Yvon
Lab Ram HR spectrometer with
a 17 mW internal He–Ne
2.1. Catalyst preparation
(Helium–Neon) laser source of excitation wavelength of 632.8 nm.
The catalyst samples in powder form (about 5–10 mg) were loosely
spread onto a glass slide below the confocal microscope for mea-
surements.
Nb0.6TPA catalyst was prepared as following. 5 g of TPA was dis-
solved in distilled water and 0.56 g of niobium oxalate dissolved
in 0.1 M oxalic acid solution was added to aqueous solution of TPA
Excess water was evaporated on a water bath and the dried cata-
lyst mass was kept for further drying in an air oven for overnight.
Finally the sample was calcined at 300 ◦C for 2 h.
TPANb1 catalyst was prepared according to the procedure
reported in the literature [7]. In a typical procedure, 10 g of niobium
oxalate was dissolved in 100 ml of 0.1 M oxalic acid solution and 6 g
of Na2HPO4 was dissolved in 100 ml of distilled water. These two
solutions were mixed together. 100 g of Na2WO4·2H2O was dis-
solved in 150 ml of distilled water, and subsequently added to the
solution containing niobium and phosphorous precursors with vig-
orous stirring. After heating the resulting solution to 80 ◦C, 60 ml
of H2SO4 was slowly added to it. The solution was further kept for
reflux at 80 ◦C for 8 h. After cooling the solution to room temper-
ature, the formed TPANb1 was extracted with diethyl ether. The
resulting etherate was maintained at 50 ◦C to obtain solid product,
dried in an oven and calcined at 300 ◦C for 2 h.
The acidity of the catalysts was measured by temperature pro-
grammed desorption (TPD) of ammonia. In a typical experiment,
0.1 g of catalyst was loaded and pre-treated in He gas at 300 ◦C for
2 h. After pre-treatment the temperature was brought to 100 ◦C and
the adsorption of NH3 was carried out by passing a mixture of 10%
NH3 balanced He gas over the catalyst for 1 h. The catalyst surface
was flushed with helium gas at the same temperature for 2 h to flush
off the physisorbed NH3. TPD of NH3 was carried with a tempera-
ture ramp of 10 ◦C/min and the desorbed ammonia was monitored
using thermal conductivity detector (TCD) of a gas chromatograph.
X-ray photo electron spectroscopy (XPS) measurements were
conducted on a KRATOS AXIS 165 with a DUAL anode (Mg and Al)
apparatus using Mg K␣ anode. The non-monochromatized Al K␣
X-ray source (hꢁ = 1486.6 eV) was operated at 12.5 kV and 16 mA.
Before acquisition of the data each sample was out-gassed for about
3 h at 100 ◦C under vacuum of 1.0 × 10−7 T to minimize surface
contamination. The XPS instrument was calibrated using Au as
standard. For energy calibration, the carbon 1s photoelectron line
was used. The carbon 1s binding energy was taken as 285 eV. Charge
neutralization of 2 eV was used to balance the charge up of the
sample. The spectra were deconvoluted using Sun Solaris Vision-
2 curve resolver. The location and the full width at half maximum
(FWHM) value for the species were first determined using the spec-
trum of a pure sample. Symmetric Gaussian shapes were used in
all cases. Binding energies for identical samples were, in general,
reproducible within 0.1 eV.
TPA supported niobium oxide catalyst was prepared by impreg-
nation method. In a typical procedure, required amount of TPA
was dissolved in water and this solution was added to niobium
oxide with continuous stirring. The resultant mixture was allowed
to stand for 3 h and excess water was evaporated on a water bath.
The catalyst was kept overnight for drying in an air oven at 120 ◦C
and finally calcined at 300 ◦C for 2 h. The TPA content on niobia is
kept as 25 wt%. The catalyst is denoted as 25% TPA/Nb2O5.
The X-ray absorptions (XAS) experiments were performed at the
Nb K edge (18.986 KeV) at the BM23 beam line at the European Syn-
chrotron Radiation Facility (ESRF, Grenoble). Monochromatic X-ray
beam was obtained from the white beam by using Si(1 1 1) double
crystal; a harmonic rejection has been performed using Si coated
mirrors. Both the incident (I0) and transmitted (I1) monochromatic
beam intensities were measured by using ionic chambers filled
with 0.65 bar Ar and 2.1 bar Ar, respectively, and eventually I0 filled
up to 2 bar with He. The photon energy was calibrated with the edge
energy obtained from the maxima first derivative of the Nb K-edge
in the Nb foil (18.986 KeV). The reference samples (Nb foil, NbO2)
were measured in transmission mode. Nb2O5 is according to http://
samples measurements were done in fluorescence mode with a
13-element Ge detector (Canberra Industries). The extraction of the
2.2. Characterization of catalysts
The FT-IR spectra were recorded on a Bio-Rad Excalibur series
spectrometer using the KBr disc method.
The nature of the acid sites (Bronsted and Lewis) of the catalyst
samples was determined by FT-IR spectroscopy with chemisorbed
pyridine. The pyridine adsorption studies were carried out in
the diffuse reflectance infrared Fourier transform (DRIFT) mode.
Prior to the pyridine adsorption catalysts samples were degassed
under vacuum at 200 ◦C for 3 h and exposed to dry pyridine.
Then, the excess pyridine was removed by heating the sample at
120 ◦C. After cooling the sample to room temperature, FT-IR spec-
tra of the pyridine-adsorbed samples were recorded. X-ray powder
diffraction (XRD) patterns were recorded on a Rigaku Miniflex
diffractometer using Cu K␣ radiation (1.5406 ◦A) at 40 kV and 30 mA