CatalysisTodayxxx (2012) xxx–xxx
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Catalysis
Today
j o ur na l ho me p a g e :w w w . e l s e v i e r . c o m / l o c a t e / c a t t o d
In
situ
FT-IR
spectroscopic
investigation
of
gold
supported
on
tungstated
zirconia
as
catalyst
for
CO-SCR
of
NO
x
M.
Kantcheva
∗,
M.
Milanova,
S.
Mametsheripov
DepartmentofChemistry,BilkentUniversity,06800Ankara,Turkey
a
r
t
i
c
l
e
i
n
f
o
Articlehistory: Received27February2012 Accepted23March2012 Available online xxx Keywords: Au/ZrO2–WOxInsituFT-IRspectroscopy NOx+COsurfacereaction
CO-SCRofNOx
a
b
s
t
r
a
c
t
Thepossibilityforapplicationofgold supportedon tungstatedzirconiaascatalystintheselective catalyticreductionofNOxwithCO(CO-SCR)hasbeeninvestigatedbymeansofinsituFT-IR
spec-troscopy.Tungstatedzirconiacontaining18wt%ofWO3 waspreparedbyco-precipitation.Goldwas
depositedonzirconiaandtungstatedzirconiabycationicadsorptionusing[Au(en)2]Cl3 asa
precur-sor(en=ethylenediamine).TheFT-IRspectraobtainedduringtheinteractionofCOwithNOxspecies
adsorbedontheAu/ZrO2–WOx andAu/ZrO2 samplesrevealedtheformationofsurfaceisocyanates
attachedtothegoldparticles.ThegenerationofAu–NCOspeciesoccurredatlowtemperature(25–50◦C). TheW-containingsamplewascharacterizedbyhigheractivityinthead-NOx+COreactionthanthe
W-freeone.ItisshownthatthenitratespeciesoradsorbedNO2areessentialforthegenerationofsurface
isocyanatesandtheoxidationofNObyoxygenisanimportantstep.TheobtainedresultssuggestthatAu catalystssupportedontungstatedzirconiamightbeofinterestfortheselectivereductionofNOxwith
COatlowtemperatures.
© 2012 Elsevier B.V. All rights reserved.
1. Introduction
TheselectivereductionofNOxinthepresenceofoxygenisa
verypromising technologytocontroltheemissionsfromdiesel andlean-burnengines.ReductionofNOxusingeithertheresidual
hydrocarbonsoron-boardfuelwouldbethemostideal technol-ogy.However,thetraditionalmaterialsdevelopedfortheselective reductionofNOxwithhydrocarbons(HC-SCR)donotshow
suffi-cientactivitiesundertheconditionsofleanexhaustespeciallyat lowtemperatures(<150–250◦C)[1–4].Oneofthetypical reduc-tantpresentinthecarexhaustisCO.RecentlyIr/SiO2,Ir/WO3and
Ir/WO3/SiO2catalystshavebeenreportedtobehighlyactiveinthe
selectivereductionofNOwithCO(CO-SCR)[5–11].However,these catalystsshowactivityin the260–400◦C temperaturewindow. Supportedgoldcatalystsareknowntobehighlyactiveinvariety ofreactionsatlowtemperatures[12,13].Inthepresentstudy,we reporttheresultsofFT-IRspectroscopiccharacterizationofgold catalystsupportedontungstatedzirconia.Inordertoevaluatethe potentialofanewmaterialasacatalystinadesiredprocess,itis importanttoinvestigatetheinteractionofthereactantswiththe surface.ForthispurposewestudiedtheadsorptionofCOandits co-adsorptionwithoxygenandNOoverAu-promotedandAu-free tungstatedzirconia.
∗ Correspondingauthor.
E-mailaddress:margi@fen.bilkent.edu.tr(M.Kantcheva).
2. Experimental 2.1. Samplepreparation
Thesamplepreparationisdescribedindetailelsewhere[14]. Inbrief,tungstatedzirconiawassynthesizedbyco-precipitation [15]withnominalcontentof18wt%ofWO3.Goldwasdeposited
ontungstatedzirconiabycationadsorptionfor2hfromaqueous solutionof[Au(en)2]3+complexatpH=9.6androomtemperature.
Afterdryingofthewashedsolidat80◦Cfor48h,thesamplewas calcinedfor1hat400◦C.Thecationicgoldprecursorwasprepared followingtheprocedureofBlockandBailar[16].Thesamplewas labeledasAu/18WZ-CP.
Inordertostudytheeffectoftungsten,goldwasdepositedon tetragonalzirconiaalsobycationadsorptionof[Au(en)2]3+
com-plexusingthesameconditionsappliedtotheW-containingsample.
2.2. Samplecharacterization
The samples were characterized by XRD, DR-UV–vis spec-troscopy,BETmeasurementsandchemicalanalysis,andtheresults werereportedearlier[14].
TheFT-IRspectrawererecordedusinga BomemHartman& BraunMB-102modelFT-IRspectrometerwithaliquid-nitrogen cooledMCTdetector ata resolutionof 4cm−1 (100 scans).The self-supportingdiscs(∼0.01g/cm2)wereactivatedin theIRcell
byheatingfor1hinavacuumat400◦C,andinoxygen(100Torr, 0920-5861/$–seefrontmatter © 2012 Elsevier B.V. All rights reserved.
Physico-chemicalcharacterizationoftheinvestigatedsamples.
Sample SBET(m2/g) WO3(wt%) Auloading(wt%) AverageAuparticle
size(nm)
ZrO2 152 –
Au/ZrO2 143 – 1.43±0.03 8
18WZ-CP 116 18.0 –
Au/18WZ-CP 118 17.6 2.27±0.01 10
passedthroughatrapcooledinliquidnitrogen)atthesame tem-perature,followedbyevacuationfor1hat400◦C.Thespectraof adsorbedgaseswereobtainedbysubtractingthespectraofthe activatedsamplefromthespectrarecorded.Thesamplespectra werealsogas-phasecorrected.
3. Resultsanddiscussion
3.1. Structuralcharacterization
Table1summarizesthechemicalcompositionandBETsurface areasofthesamples.Theresultsofthechemicalanalysis[14]show thatthegolduptakeontungstatedzirconiaishigherthanthaton zirconia.Itiswellknownthattungstatedzirconiacontainsacidic protons[15,17–21]whichinbasicmediumcanundergo deproto-nation.ThiscanleadtotheformationofgreaternumberofM–O− anchoringsites(M=WandZr)forthe[Au(en)2]3+complex
result-inginhighergolduptake.
AccordingtotheXRDdata[14]thematerialshavethestructure oftetragonalzirconia.Theaveragesizeofgoldparticles(Table1)is calculatedbyusingScherrerequationandthemaingolddiffraction lineof2=38.2◦.TheDR-UV–visspectraofgoldcontaining sam-ples[14]exhibitbroadabsorptionwithmaximumat550–590nm characteristicoftheplasmonicoscillationmodeofnanosizedgold particles[22–24].
3.2. AdsorptionofCOatroomtemperature
TheanalysisoftheFT-IRspectraofCOadsorbedatroom tem-peratureonthesamplescanbeveryusefultoobtainqualitative informationonthenatureofsupportedgoldspecies.Fig.1 dis-plays the FT-IR spectra in the carbonyl region of CO (10Torr) adsorbedontheactivatedAu-containingsamples.Theabsorption at2194–2198cm−1 is assigned toCO adsorbed onZr4+ surface
sites[18,21,23,25–27].Thehigh-frequencyshiftexhibitedinthe WOx-containingmaterialisassociatedwiththeincreasedacidity
ofthecoordinativeunsaturatedZr4+sitescausedbythe
electron-withdrawing WOx groups [18,21]. The band corresponding to
theZr4+–COspeciesand thecomposedbandwithmaximumat
2113–2116cm−1areremovedupondynamicevacuationatroom temperature. Accordingto data from the literature [23,25–39], theabsorptionwithmaximumat2113–2116cm−1isassignedto COadsorbedonsmallthree-dimensionalgoldclusters, whereas theshoulderat2125–2130cm−1 couldbeattributedtoAuı+–CO species.Formationofpositivelypolarizedgoldis assumedtobe causedbythepresenceofadsorbedoxygenonthegoldparticles ortheirinteraction withthesupport[23,24,26,28,31,32,35–37]. Hadjiivanovandcoworkers[36,37]proposedthattheabsorption inthe2155–2130cm−1regioncouldbeattributedalsotoAu+–CO
speciesinwhichtheAu+cationresidesonthemetallicgold
parti-cles.Itshouldbenotedthatthelastactivationstepofthesamples consistedofevacuationat400◦Candadsorbedoxygencannotbe expectedundertheseconditions.Moreover,afterthereductionof thesamplesat400◦CwithCO,theabsorptionat2125–2130cm−1 isstillpresentinthespectraofCOadsorbedatroomtemperature. Therefore,itcouldbeproposedthatthefeatureat2125–2130cm−1
couldbeassociatedwiththepresenceofmoredefectivegoldsites locatedmostlikelyattheinterface.Itcannotbeexcludedthatthe absorptionat2125–2130cm−1isassociatedwiththepresenceof largerAuparticles.Thispropositioncouldbesupportedbythefact thatCOadsorbedonsmallgoldparticlesischaracterizedby(CO) modeatlowerwavenumbersandthe(CO)stretchingvibrationis blue-shiftedastheparticlesizeincreases[40].Recently, absorp-tionbandat 2130–2140cm−1 observed upon COadsorption on Au/Nb2O5 hasbeenattributedtoCOcoordinatedtolargergold
nanoparticles[41].
3.3. InsituFT-IRspectroscopicinvestigationoftheNO+O2+CO
reaction
3.3.1. NO+O2surfacereaction
Ingeneral,themechanismofSCRofNOxonvariousoxide
cata-lystsinvolvestheinteractionofstronglyadsorbedNOx−species(x
is2or3)withthereducer[2,42–46].Thereforewestudiedthe ther-malstabilityofNOxspeciesadsorbedonthesurfaceofthe18WZ-CP
andAu/18WZ-CPsamples.
NOxspecies onthesurface oftheAu/18WZ-CPsamplewere
createdby adsorptionof a (10TorrNO+25TorrO2)mixtureat
roomtemperaturefollowedbyevacuationfor20minatthesame temperature(Fig.2A,spectrum(a)).Theabsorptionbandsinthe 1700–1000cm−1 range are typicalof surface nitrates observed ontungstatedzirconia[45–47] and areidentified as monoden-tate(1582and1275cm−1)andbidentate(1629and1219cm−1) NO3− species. The broad absorption centered at 2140cm−1 is
2050 2100 2150 2200 2250 Absorbance Wavenumber (cm-1) Au/ZrO2 Au/18WZ-CP 0.02 2 116 2113 219 4 2198 2130 2125
Fig.1. FT-IRspectraofCO(10Torr)adsorbedatroomtemperatureonthesamples studied.
M.Kantchevaetal./CatalysisTodayxxx (2012) xxx–xxx 3 1000 1250 1500 1750 2000 2250 2500 d c Absorbance Wavenumber (cm-1) a b 0.5 1629 1582 1275 1219 2140
(A)
1500 1750 2000 2250 2500(B)
NO 2 0.05 b c dFig.2.PanelA:FT-IRspectraoftheAu/18WZ-CPsampletakenaftertheadditionofa(10TorrNO+25TorrO2)mixturetotheIRcellfor10minatroomtemperaturefollowed
byevacuationfor20min(a),andafterheatingtheisolatedIRcellfor10minat100◦C(b),200◦C(c)and300◦C(d).PanelB:Gasphasespectracollectedat100◦C(b),200◦C (c)and300◦C(d).
characteristicofNO+species[45–47].HeatingtheisolatedIRcell
inthetemperaturerange100–300◦C,leadstogradualdecreasein theintensitiesofthenitratebands.Thespectraofthegasphase (Fig. 2B) showthat themajor productof decomposition ofthe surfacenitratesisNO2.TheAu-free18WZ-CPsamplecontains
anal-ogoustypeofadsorbedNOxspecieswhichweregeneratedbythe
samewayasdescribedabove(thespectraarenotshown).However, thesurfacenitratesontheAu-containingsampledisplayhigher thermalstability.
Therearereportsintheliterature[35,37],showingthata mix-tureof NO+O2 cancause oxidation of supportedmetallic gold
particlestocationicgoldspeciesandthisprocesscanoccuratroom temperature.Inordertofindtheeffectofco-adsorptionofNO+O2
mixtureontheoxidationstateofgoldintheAu/18WZ-CPsample, weinvestigatedtheadsorptionofCOonthecatalystcontaining pre-adsorbedNOxspecies.Itiswellknownthatthespectral
fea-turesofadsorbedCOcanprovideinformationabouttheoxidation stateoftheadsorptionsite[34].Surfacenitratespecies(absorption bandsbetween1700and1000cm−1)weregeneratedbybringing incontacttheAu/18WZ-CPsamplewithamixtureof10Torrof NOand25TorrofO2for10minatroomtemperaturefollowedby
evacuationatthesametemperaturefor20min(Fig.3,spectrum (a)).Tothesampletreatedinthisway,10TorrofCOwereadded. Thespectrumdetectedatroomtemperatureafter5mincontainsa strongbandwithmaximumat2185cm−1(Fig.3,spectrum(b)).The intensityofthissignalincreasessignificantlyafter10minofcontact withtheCO(Fig.3,spectrum(c)).Weakabsorptionat2130cm−1is observedaswellwhoseintensityincreasesinparallelwiththemain bandat2185cm−1.Thelattersignalfallsintherangeofreported (CO)stretchingvibrationsofAu+–COspecies(2197–2160cm−1
[31–37]).However,theincrease intheintensityof thebandat 2185cm−1 duringthecontactwithCO contradictstheobserved instabilityoftheAu+–COspeciesinCOatmosphere[31–33,35]due
toreductionofAu+adsorptionsitesbyCO.
Inordertoensuremoreefficientoxidationofgold,the cata-lystpelletwastreated witha(10Torr NO+25TorrO2)mixture
at300◦Cfor30min.Thenthetemperaturewasloweredto200◦C andthegasmixturewasremovedfromtheIRcellupondynamic
evacuationwhilecoolingtoroomtemperature.Subsequent adsorp-tionofCO(10Torr)atroomtemperatureresultsintheformation ofweakabsorptionbands at2190and2165cm−1 (Fig.4, spec-trum(a)).Thespectruminthenitrateregion(notshown)displays thesamesetofnitratebandsasshowninFig.2A,althoughwith weakerintensity.Thebandat2190cm−1resiststheevacuationat roomtemperature(Fig.4,spectrum(b))anddisappearsupon out-gassingat100◦C(Fig.4,spectrum(d)).Theobservedbehaviorof theabsorptionat2190cm−1istypicalofAu+–COspecies[34].The
COadsorbedonAu+sitesisstabilizedbythesynergismbetween
the-dativeandback-bondingcomponentsoftheAu+ CObond
[34–37]andthecarbonylcomplexcanbedestroyedat temper-aturehigherthan25◦C.Theabsorptionat2165cm−1 disappears uponevacuationatroomtemperature(Fig.4,spectrum(b))and couldbeattributedtoAuı+–COspeciesorCOadsorbedonlarge
1000 1200 1400 1600 1800 2000 2200 2400 Absorbance Wavenumber (cm-1) a b c 2185 1622 1582 12 75 1227 0. 5 2130
Fig.3. FT-IRspectraoftheAu/18WZ-CPcatalystcollectedaftertheadsorptionof a(10TorrNO+25TorrO2)mixturefor10minatroomtemperaturefollowedby
evacuationfor20minatroomtemperature(a)andadsorptionof10TorrCOatroom temperaturefor5min(b)and10min(c).
2100 2125 2150 2175 2200 2225 2250 2275 Absorbance Wavenumber (cm-1) 21 9 0 216 5 a b c d 0. 02
Fig.4. FT-IRspectraoftheAu/18WZ-CPsamplecollectedaftertheadsorptionofa (10TorrNO+25TorrO2)mixturefor30minat300◦Cfollowedbydynamic
evacu-ationfrom200◦Ctoroomtemperatureandsubsequentadsorptionof10TorrofCO
for10min(a),evacuationfor15minatroomtemperature(b),50◦C(c)and100◦C
(d).
goldparticles.Thisbandisfoundathigherfrequencythanthe cor-respondingbandobservedontheactivatedAu/18WZ-CPsample (seeFig.1)indicatingthateithertheAuı+sitesbearagreater pos-itivechargeorthereisagglomerationofthegoldparticlesafter thehigh-temperaturetreatmentwithNO+O2mixture.Itislikely
thatthespeciesgivingrisetothebandat2165cm−1couldbeAu+
adsorptionsitesdispersedonthesurfaceofmetallicgoldparticles asproposedin[36,37].
Spectrum(a)inFig.4differsfromthespectrumofadsorbed COonthesampletreatedwithNO+O2mixtureatroom
temper-ature(Fig.3,spectrum (c)).It seemsthat theoxidationof gold particlesbytheNO+O2 mixturetakesplaceathigher
tempera-ture(300◦C)andtheabsorptionbandat2185cm−1detectedduring theCOadsorptiononthesampletreatedwithNO+O2mixtureat
roomtemperature(Fig.3,spectra(b)and(c))cannotbeascribedto Au+–COspecies.Thisconclusionissupportedalsobythefactthat
thecoloroftheAu/18WZ-CPsampleafterthepre-treatmentwith NO+O2mixtureatroomtemperatureremainedthesameasthatof
theactivatedsample,i.e.gray-black.However,thetreatmentwith NO+O2mixtureat300◦Ccauseschangesinthecolorofthesample
fromgray-blacktopale-violet.
Takingintoaccountthatthecompoundsadsorbedatroom tem-peratureontheAu/18WZ-CPsampleareCOandNOxspecies,it
couldbeproposedthat thestrongbandat 2185cm−1 in Fig.3 couldbeattributedtoNCOspeciesformedonmetallicgoldsites. Accordingtothe literature[38,48,49] theAu–NCO species give rise to absorption bandat 2180–2190cm−1. In order to verify this assumption we performed13CO adsorption onthe sample
treatedwith NO+O2 mixtureat roomtemperature (Fig. 5).The
bandat2185cm−1isshifteddownby57cm−1andispositionedat 2128cm−1on13Csubstitution.Theobservedvalueisconsistent
withthatreportedbyCelioetal.[50]fortheisotopicshiftdetected onsubstituting13Cfor12CinNCOspeciesadsorbedonCu(100).
Fromtheseresultsitcanbeconcludedthattheweakabsorptionat about2130cm−1inFig.3,spectrum(c)belongstothe13COsatellite
ofthebandat2185cm−1.
Thebehavioroftheabsorptionat2185cm−1 inthepresence ofwatervaporcanbeusedasadditionalevidencesupportingthe assignmentofthisfeaturetoAu–NCOspecies.Itiswellknownthat theNCOspeciescanreactwithwaterproducingammoniaandCO2
throughtheformationofHNCO[11,51].Thespeciescharacterized
2050 2100 2150 2200 2250 Absorbance Wavenumber (cm-1) 2185 2128 a b 0. 5
Fig.5.FT-IRspectraof10TorrofCO(a)and10Torrof13CO(b)adsorbedatroom
temperatureontheAu/18WZ-CPsample.
bytheabsorptionbandat2185cm−1aregeneratedbyadsorption ofCO(10Torr,for10min)onthesampletreatedwithNO+O2
mix-tureatroomtemperatureasdescribedaboveandthenthegaseous COwasevacuatedfor15min(Fig.6A,spectrum(a)).Theaddition of0.1Torrofwatervaporatroomtemperaturecausessignificant decreaseintheintensityofthebandat2185cm−1(Fig.6A, spec-trum(b))andappearanceofCO2andHNCO(as(NCO)at2266cm−1
[51])in thegasphase(Fig.6B, spectrum(b)).The formationof thelattercompoundsconfirmsunambiguouslytheassignmentof thebandat2185cm−1 toAu–NCO species.Increasingthe tem-perature to100◦C resultsin furtherdecreasein theamountof isocyanates(Fig.6A,spectrum(c))andtheydisappearcompletely at200◦C(thespectrumisnotshown).Noammoniawasdetectedin thegasphasemostlikelybecauseofitslowconcentrationand/or adsorptiononthecatalystsurface.ThesamplespectraintheNH stretchingregionarenoisyandarenotrepresentative.The bend-ingmodesofcoordinatedammoniaandNH4+ionfallintheregion
ofstretchingvibrationsof thenitratesand ifformed,they can-notberesolved.ItshouldbenotedthattheadsorptionofCOon theNOx-precoved18WZ-CPsampledoesnotleadtotheformation
ofNCOspecieswhichonoxidessurfacesproduceabsorptionsin the2280–2200cm−1region[38,46,48,49,52].TheabsenceofNCO speciescoordinatedtothesupportinthecaseofAu/18WZ-CP sam-plecanbeexplainedbyunavailabilityofadsorptionsiteswhichare blockedbythenitratespecies.
TheAu–NCOspeciesobservedontheAu/18WZ-CPsampleare characterizedbyhighthermalstabilityandtheyareremovedby dynamicevacuationat350◦C(Fig.7).
3.3.2. NOx+COsurfacereaction
TheaimofthisexperimentistoinvestigatethepossibilityofCO toactasreducingagenttowardtheNOxspeciesadsorbedonthe
M.Kantchevaetal./CatalysisTodayxxx (2012) xxx–xxx 5 2000 2100 2200 2300 2400 Absorbance Wavenumber (cm-1) 0.2 5 2185
(A)
a b c 2000 2100 2200 2300 2400 2500(B)
2266 CO2 0. 05 b c HNCOFig.6.PanelA:FT-IRspectraoftheAu/18WZ-CPcatalystcollectedaftertheadsorptionofa(10TorrNO+25TorrO2)mixturefor10minatroomtemperaturefollowed
byevacuationfor20minatroomtemperature,adsorptionof10TorrCOatroomtemperaturefor10minandevacuationofthegaseousCOfor15min(a),andsubsequent additionof0.1Torrofwatervaporfor10minatroomtemperature(b)and100◦C(c).PanelB:Gasphasespectracorrespondingtothesamplespectra(b)and(c). surfaceoftheAu/18WZ-CPcatalyst.Adsorbednitratespecieswere
createdbyadsorptionofmixtureof10TorrNOand25TorrO2atRT
for10minfollowedbyevacuationfor20minatRT(Fig.8A, spec-trum(a)).ThenCO(10Torr)wasadded(Fig.8A,spectrum(b))and
2100 2120 2140 2160 2180 2200 2220 2240 3500C 3000C 2500C 2000C 1500C 1000C Absorbance Wavenumber (cm-1) RT 0. 25 2185
Fig.7. FT-IRspectraoftheAu/18WZ-CPcatalystcollectedaftertheadsorptionofa (10TorrNO+25TorrO2)mixturefor10minatroomtemperaturefollowedby
evacu-ationfor20minatroomtemperature,adsorptionof10TorrCOatroomtemperature for10minandevacuationofthegaseousCOfor15minatvarioustemperatures (RT=roomtemperature).
theisolatedIRcellwasheatedfor10minatvarioustemperatures. Thesharpbandat2185cm−1assignedtoAu–NCOspeciesincreases inintensityat50◦C(Fig.8A,spectrum(c))anddisappearsat200◦C (Fig.8A,spectrum(f))simultaneouslywiththeNO2observedinthe
gasphase(Fig.8B,spectrum(f)).ItcanbeconcludedthattheNCO speciesreactwiththeNO2leadingtotheformationofCO2andN2.
SomeamountsofN2OandNOaredetectedaswell.Thefactthat
intheabsenceofCO,theNO2ispresentinthegasphase(Fig.2)
supportstheassumptionthattheNO2isreducedbyCOthrough
theintermediacyofAu–NCOspecies.
The spectra shown in Fig. 9 illustrate the reactivity of the Au–NCO species generated ontheAu/18WZ-CP sample toward NO2.TheabsenceofCOinthegasphasepreventstheformation
ofadditionalAu–NCOspeciesat50◦C(seeFig.8A,spectrum(c)) and allowsmonitoringtheonsettemperature oftheNCO+NO2
reaction.TheNCOspecies havebeenobtainedbyadsorptionof 10TorrofCOontheNOx-precoveredAu/18WZ-CPsamplefollowed
byevacuationfor20minatroomtemperature(Fig.9,spectrum (a)).Aftertheadmissionof0.4TorrofNO2 atroomtemperature
(Fig.9,spectrum(b)),theisolatedIRcellwasheatedbetween25 and250◦Cfor 10minateach temperature.Theexposureofthe sampletoNO2atroomtemperature(Fig.9,spectrum(b))causes
strongdecreaseintheintensityofthebandat2185cm−1indicating thattheNCO+NO2reactiontakesplacealreadyat25◦C.The
sur-faceconcentrationoftheNCOspeciesdecreasesrapidlywiththe temperatureandtheydisappearat250◦C(Fig.9,spectrum(g)). Thegasphasespectra(notshown)containCO2andNO2thathas
beentakeninexcess.Asshownabove,theAu–NCOspecieshave highthermalstabilityandleavethesurfaceupondynamic evacu-ationat350◦C(Fig.7).Theseresultsconfirmthehighreactivityof theisocyanatesformedonthegoldparticlesandsuggestthatthe Au/18WZ-CPcatalystmayhavethepotentialforlow-temperature reductionofNOxwithCOinthepresenceofoxygen.
Inordertoobtaininformation abouttheroleofWOxspecies
intheNOx+COsurfacereaction,westudiedtheinteractionofCO
withnitratespeciespre-adsorbedontheAu/ZrO2 catalyst.Also
inthiscase,nitratespecies(bandsbetween1700and1000cm−1) werecreatedbyadsorptionofmixtureof10TorrNOand25Torr O2 at RT for 10min followed by evacuation for 20min at RT
1000 1250 1500 1750 2000 2250 2500
(B)
Absorbance Wavenumber (cm-1) 2185 0. 5 2140 a b c d e f g(A)
1400 1600 1800 2000 2200 2400 CO2 CO NO NO2 0.05 b c d e f g N 2OFig.8. PanelA:FT-IRspectraoftheAu/18WZ-CPcatalystcollectedaftertheadsorptionofa(10TorrNO+25TorrO2)mixturefor10minatroomtemperaturefollowedby
evacuationfor20minatroomtemperature(a),subsequentadsorptionof10TorrCOatroomtemperaturefor10min(b)andheatingtheisolatedIRcellfor10minat50◦C
(c),100◦C(d),150◦C(e),200◦C(f)and250◦C(g).PanelB:Gasphasespectracollectedat25◦C(b),50◦C(c),100◦C(d),150◦C(e),200◦C(f)and250◦C(g).
(Fig.10A,spectrum(a)).Aftertheadditionof10TorrofCOatroom temperature,theisolatedIRcellwasheatedfor10minatvarious temperatures.AswiththeAu/18WZ-CPsample,thesharpbandat 2184cm−1 ischaracteristicof NCOspeciesadsorbedonAu.The
2100 2120 2140 2160 2180 2200 2220 2240 Absorbance Wavenumber (cm-1) a b c d e f g 0. 2 5 2185
Fig.9. FT-IRspectraoftheAu/18WZ-CPcatalystcollectedafterthegenerationofthe Au–NCOspecies(a)(fortheconditionsseeFig.7,spectrum(RT))andsubsequent additionof0.4TorrofNO2for10minat25◦C(b),50◦C(c),100◦C(d),150◦C(e),
200◦C(f)and250◦C(g).
comparisonof thespectrashownin Figs.8and 10leadstothe conclusionthattheWOx-containingcatalystshouldhavehigher
activitybecausetheadsorbedNCOspeciesandNO2 disappearat
200◦Cwhereas inthecase ofAu/ZrO2 sampletheyarepresent
atthistemperature.Despite ofthehigherconcentrationof sur-facenitratesontheAu/ZrO2 sample,theamountofevolvedNO2
islower.Thissuggeststhatthesurfacetungstateslowerthe stabil-ityofthenitrateions.Inaddition,theweakabsorptionsat1450and 1420cm−1observedinthespectrumofAu/ZrO2detectedat250◦C
indicatetheformation of stablepolydentate carbonates [53,54] whichmayhavenegativeeffectonthecatalyticactivity.Nosuch speciesarefoundinthecaseoftheAu/18WZ-CPsample.
Finally,itshouldbenotedthat theAu-free18WZ-CPsample doesnotcatalyzetheinteractionbetweenadsorbedNOxspecies
andCO:theevolvedNO2ispresentinthegasphasebetween25
and350◦C(thedataarenotshown).
3.3.3. Interactionofa(10TorrNO+14TorrCO)mixturewith Au/18WZ-CP
The aim of this experiment is to show the role of NO+O2,
respectivelyNO2,fortheformationofAu–NCOspecies.Thespectra
(Fig.11)arecollectedinthepresenceofNO+COreactionmixtureat varioustemperatures.Thebandat2230cm−1observedinthe spec-trumtakenatroomtemperature(Fig.11A,spectrum(a))istypical ofadsorbedN2OwhichispresentasimpurityinthegaseousNO
(Fig.11B).Theabsorptionat2198cm−1 corresponds toZr4+–CO
whereasthesignalat 2118cm−1 is assignedtoAu0–COspecies
(Fig.11A).ThespectrumrecordedatRTcontainsabsorptionbands whichareattributedtobidentateHCO3−(1606and1222cm−1),
bidentate(1555and1305cm−1)andpolydentatecarbonates(1456 and1420cm−1)[53,54].Theassignmentoftheabsorptionsinthe 1700–1000cm−1regiontocarbonatespeciesisconfirmedbythe FT-IRspectraofadsorbedCOtakeninthe25–250◦Ctemperature range.Thedataarenotshownforthesakeofbrevity.The intensi-tiesofthebandsat2230,2198and2118cm−1decreasewiththe temperatureandtheseabsorptions arenolongerpresentinthe spectrumtakenat150◦C(Fig.11A,spectrum(d)).OnlyZr4+–NO
M.Kantchevaetal./CatalysisTodayxxx (2012) xxx–xxx 7 1000 1250 1500 1750 2000 2250 2500
(B)
Absorbance Wavenumber (cm-1) 0. 5 14 5 0 142 0 2184 b c d e f g a(A)
1400 1600 1800 2000 2200 2400 CO2 CO NO NO2 0.05 b c d e f gFig.10.PanelA:FT-IRspectraoftheAu/ZrO2catalystcollectedaftertheadsorptionofa(10TorrNO+25TorrO2)mixturefor10minatroomtemperaturefollowedby
evacuationfor20minatroomtemperature(a),subsequentadsorptionof10TorrCOatroomtemperaturefor10min(b)andheatingtheisolatedIRcellfor10minat50◦C (c),100◦C(d),150◦C(e),200◦C(f)and250◦C(g).PanelB:Gasphasespectracollectedat25◦C(b),50◦C(c),100◦C(d),150◦C(e),200◦C(f)and250◦C(g).
1000 1200 1400 1600 1800 2000 2200 f e d Absorbance Wavenumber (cm-1) a b c 22 30 2198 2118 0.1 160 6 15 5 5 1305 1222 11 78 1937 14 56 142 0
(A)
1500 1750 2000 2250 2500(B)
f e d c b CO 2 N 2O CO NO 0.0 2 aFig.11.PanelA:FT-IRspectraoftheAu/18WZ-CPcatalystcollectedaftertheadsorptionofa(10TorrNO+14TorrCO)mixturefor10minatroomtemperature(a)and subsequentheatingtheisolatedIRcellfor10minat50◦C(b),100◦C(c),150◦C(d),200◦C(e)and250◦C(f).PanelB:Gasphasespectracollectedat25◦C(a),50◦C(b),100◦C
(c),150◦C(d),200◦C(e)and250◦C(f).
identifiedasNOxspeciesadsorbedatroomtemperature.Nosurface
nitratesandAu–NCOspeciesareformedevenathigher tempera-tures.ThisfactindicatesthatthenitratespeciesoractivatedNO2
areessentialfortheformationofAu–NCOspeciesandthatthe oxi-dationofNObyoxygenisanimportantstep.Thegasphasespectra (Fig.11B)showthattheamountofN2Oincreaseswiththe
tem-peraturebeingthehighestat250◦C(spectrum(f))whentheNO− speciesareremovedcompletelyfromthesurface.TheCO2detected
in thegas phase at 200◦C (Fig.11B, spectrum (e)) most likely appearsasaresultofdecompositionofthesurfacecarbonates.
4. Conclusions
Goldcatalystspreparedbycationicadsorptionofaqueous solu-tionof[Au(en)2]Cl3complexonzirconiaandtungstatedzirconia
havebeeninvestigatedbyinsituFT-IRspectroscopy.The adsorp-tionofCOshowsthepresenceofpositivelycharged(orlargegold clusters)andneutralgoldparticlesonbothsupports.Detailed FT-IRinvestigationoftheinteractionbetweenCOand NOxspecies
pre-adsorbedonAu/ZrO2 andAu/ZrO2–WOx samplesrevealthe
(25–50◦C). The gold isocyanates display highthermal stability. However,theyreactreadilywithNO2atroomtemperature.
Dur-ingthead-NOx+COreactionovertheAu/ZrO2–WOxsample,the
goldisocyanatesdisappearat200◦CsimultaneouslywiththeNO2
thatisgeneratedinthegasphasebydecompositionofthesurface nitrates.ThisprocessontheAu/ZrO2catalysttakesplaceathigher
temperature(250◦C).ItisconcludedthattheincorporationofW tozirconiadecreasesthestabilityoftheadsorbednitrates.The Au-freetungstatedzirconiadoesnotcatalyzetheinteractionbetween adsorbednitratesandCO:theevolvedNO2 ispresentinthegas
phasebetween25and350◦C.
NoformationofsurfacenitratesandAu–NCOspeciesisdetected duringtheNO+CO adsorptiononAu/ZrO2–WOx catalyst inthe
25–250◦Ctemperaturerange.Thisresultimpliesthatthenitrate speciesoradsorbedNO2areessentialforthegenerationofgold
isocyanatesandtheoxidation ofNObyoxygenisanimportant step.IntheabsenceofCO,gaseousNO2overbothAu-containing
catalystsisobservedinthe25–350◦Ctemperaturerange.Thisfact supportstheconclusionthatNO2isreducedbyCOwiththe
inter-mediacyofAu–NCOspeciesleadingtotheformationofN2andCO2.
TheresultsofinsituFT-IRspectroscopicinvestigationpresumethat Ausupportedontungstatedzirconiamightbepotentialcandidate forthedevelopmentoflow-temperaturecatalystfortheselective reductionofNOxwithCO.
Acknowledgments
ThisworkwasfinanciallysupportedbytheScientificand Tech-nologicalResearchCouncilofTurkey(ProjectTBAG-109T854)and BilkentUniversity.ThefinancialsupportofNATOgrantESP.CLG. No.984160isgreatlyappreciated.
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