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Chemical vapor deposition of low reflective cobalt (II)
oxide films
Eliane Amin-Chalhoub, Thomas Duguet, Diane Samélor, Olivier Debieu,
Elisabeta Ungureanu, Constantin Vahlas
To cite this version:
Eliane Amin-Chalhoub, Thomas Duguet, Diane Samélor, Olivier Debieu, Elisabeta Ungureanu, et al..
Chemical vapor deposition of low reflective cobalt (II) oxide films. Applied Surface Science, Elsevier,
2016, 360, pp.540-546. �10.1016/j.apsusc.2015.10.188�. �hal-01264368�
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Eprints ID : 14628
To link to this article : DOI :
10.1016/j.apsusc.2015.10.188
URL :
http://dx.doi.org/10.1016/j.apsusc.2015.10.188
To cite this version : Amin-Chalhoub, Eliane and Duguet, Thomas and
Samélor, Diane and Debieu, Olivier and Ungureanu, Elisabeta and
Vahlas, Constantin Chemical vapor deposition of low reflective cobalt
(II) oxide films. (2016) Applied Surface Science, vol.360. pp.540-546.
ISSN 0169-4332
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Chemical
vapor
deposition
of
low
reflective
cobalt
(II)
oxide
films
Eliane
Amin-Chalhoub,
Thomas
Duguet
∗,
Diane
Samélor,
Olivier
Debieu,
Elisabeta
Ungureanu,
Constantin
Vahlas
CIRIMAT,CNRS–UniversitédeToulouse,4alléeEmileMonso,BP-44362,31030ToulouseCedex4,France
Keywords:
Opticalreflectivity
MOCVD
Refractiveindexgradient
CoO
Cobaltoxide
a
b
s
t
r
a
c
t
LowreflectiveCoOcoatingsareprocessedbychemicalvapordepositionfromCo2(CO)8attemperatures
between120◦Cand190◦Cwithoutadditionaloxygensource.Theopticalreflectivityinthevisibleand
nearinfraredregionsstemsfrom2to35%dependingondepositiontemperature.Thecombinationof specificmicrostructuralfeaturesofthecoatings,namelyafractal“cauliflower”morphologyandagrain sizedistributionmoreorlesscoveringthenearUVandIRwavelengthrangesenhancelightscattering andgivesrisetoalowreflectivity.Inaddition,thecolumnarmorphologyresultsinadensitygradientin theverticaldirectionthatweinterpretasarefractiveindexgradientloweringreflectivityfurtherdown. Thecoatingformedat180◦Cshowsthelowestaveragereflectivity(2.9%),andpresentsaninteresting
deepblackdiffuseaspect.
1. Introduction
Lowreflectivityfilmsareusedinopticalinstrumentsand sen-sorswiththeaimtoattenuatenoise,namelytoreducetheeffect ofstrayandscatteredlightindifferentspectraldomains[1].Such filmsfindapplicationsinmilitarynightsightforopticalguidance systems[2],in space applications[3] and canalso beused for heatdissipationbetweendifferentcomponentsinmicroelectronic devices[4].Moreover,lightabsorberfilmsareusedinthe renew-ableenergydomaininphotothermalenergyconversion[5–8],in photoelectricenergy conversion[9], and insolar thermophoto-voltaicconversionsystems[10–12].
Blackcoatingsarespread overalargevarietyofmaterialsin thefamilies of metals, alloys, ceramics, and polymers[5,6,13]. Amongthem,thecobalt(II,III)oxideCo3O4 exhibitshighoptical
absorbancewhichisappropriateforsolarabsorbersfor photother-malconversion[14].Indeed,Co3O4 presentsspectrallyselective
surfacesexhibitinghighvaluesofsolarabsorbance(˛)inthe visi-bleandthenearinfra-red(NIR)spectrumandlowvaluesofthermal emittance(ε)intheIRspectrumwhichimprovestheirthermal per-formancebyreducingtheradiativeheatlosscomponent.Moreover, incontrasttochromiumbasedblackcoatings,Co-basedones main-tainacceptablevaluesof˛andεevenafterexposuretoair(1000h at650◦C[15]).
∗ Correspondingauthor.Tel.:+33534323439.
E-mailaddresses:thomas.duguet@ensiacet.fr,doug181@gmail.com(T.Duguet).
Cooxidefilmsareobtainedbywetprocessessuchasthermal decomposition,electrodeposition[14,16,17]andsol–gel[18].Dry processesarealsoemployedsuchasPVD[19,20],ALD[21–24]and
metalorganicCVD(MOCVD)[25–28].SeveralauthorsuseMOCVD
togrowcobalt oxidefilms. Fujiet al.formedCooxidefilmsby
plasmaenhancedMOCVD(PEMOCVD).TheyobtainCoOfilmsat
lowoxygenflowratewithasurfacemorphologyintheformof
packedcolumnargrains.Increasingtheoxygenflowrateleadsto theformationofcolumnarCo3O4filmswithinthesame
temper-aturerange(400◦C)[29].Similarobservationsarementionedby
Tyezkowskietal.whoshowthatfilmcompositionishighly corre-latedtotheO2molarfraction.Filmsarecomposedessentiallyof
Co3O4 withthepresenceofcarbonandamorphousCoOxatlow
O2 flowrate[25].ManeandShivashankar similarlyobtainedby
MOCVDdenseandcontinuousCo3O4 filmswithapackedgrains
morphologywhenusingO2,butporousfilmscomposedofa
mix-tureofCo3O4andCoOwhileusingN2O[30].Co3O4filmsaregrown
aswellbyDirectLiquidInjection(DLI-)MOCVDunderaworking pressureof5Torrbutattemperatureshigherthanours:350–600◦C
[26]. Authors notice that while increasing deposition tempera-ture,thefilmmorphologyvariesdependingonthesubstratetype. FilmroughnessincreasesinthecaseofLaAlO3substratewhileit
decreasesinthecaseofsapphireandMgO;aninterestingwayfor tailoringthemicrostructureofCooxidefilms.
Finally,differentMOCVD precursorscanbeusedin orderto
obtain Co oxide films, suchas tricarbonyl nitrosyl [27], dicar-bonylcyclopentadienylcobalt[31],Cobalt(II)b-diketonateadducts
[26], andCobalt(II) acetylacetonate[30]. In particular,dicobalt octacarbonyl(Co2(CO)8)isusedtoprocessfilmsatlowtemperature
Table1
MOCVDprocessparametersusedforthedepositionofcobaltoxidefilms.
Depositiontemperature(◦C)–Td 120–190
Precursortemperature(◦C) 27
Totalpressure(Torr) 5
SaturationvaporpressureofCo2(CO)8(Torr) 0.0041
N2carriergasflowrate(sccm) 30
N2dilutiongasflowrate(sccm) 170
Co2(CO)8flowrate(sccm) 24.6×10−3
Co2(CO)8molarfraction* 1.23×10−4
Depositionduration(min) 80
*Upperlimitassumingfullefficiencyofprecursorvaporizationandtransport.
(<200◦C),ultimatelyallowingprocessingthermallysensitive
sub-strates[32–36].ThepresentworkrevisitstheuseofCo2(CO)8for
thelowtemperatureMOCVDofcobaltoxides,withfollowingthree peculiarities:(a)itinvestigatesthethermolysisoftheprecursorin theabsenceofreactivegas,e.g.oxygen,(b)itaimsatprocessing pureCoOfilms,(c)itfocusesonthemicrostructureofthefilms.Itis worthnotingthatsuchanapproachhasneverbeeninvestigatedfor theMOCVDofcobaltoxides.Therationaleoftheworkisto
elab-orateaprocessoperatinginaparametricwindowwhichallows
processingfilmswithstablephysicochemicalandmicrostructural characteristicsandthushighperformanceopticalproperties.
The paper is organized as follows. After the experimental
details section, we present and discuss the results
concern-ing the process–structure–properties relationship. Growth rate,
crystallography, composition, and morphology of the coatings
arecorrelatedwithdepositiontemperature(Td).Then, the
opti-cal reflectivity of the films is correlated with chemical and
microstructural characteristics,namelysurfaceroughness, grain sizedistributionandfractaldimension,beforeproviding conclud-ingremarks.
2. Experimentaldetails
CVDexperiments areperformedinaverticalcold-wall
reac-torcomposedofa46mmdiameterquartztube.Siliconsamples
(20×10×1mm3)arecutfrom4′′Si(100)wafersandsonicated
inacetoneandethanolbathsfor5min,driedinanArflow,and
baked at 60◦C for 20min.Theyare weighted and immediately
positionedflatonaninductivelyheatedstainlesssteelsusceptor. DepositiontemperatureTdiscontrolledbyaK-typethermocouple
insertedintothecoreofthesusceptor.Surfacetemperatureis cali-bratedwithanadditionalthermocoupleattachedtothesurfaceofa dummySisample.PureN2(99.9999%,AirProducts)isusedasboth
carrieranddilutiongasandisdeliveredthroughtwogaslines, ther-mallyregulatedat35◦C,andequippedwithmassflowcontrollers.
Avanepumpandpressuregaugesconnectedtotheoutputofthe
quartztubeisusedtoregulatethereactionpressureat5Torr.Tdis
variedfrom120to190◦Cinordertoinvestigateitseffectonthe
filmsmorphology,compositionandopticalabsorptivity.Co2(CO)8
powder(AlfaAesar,stabilizedin5%hexane)isfilledintoaUshaped tube,inagloveboxunder99.9997%pureAr(AirProducts)before beingconnectedunderN2flowwiththeCVDset-up.Theprecursor
isthermallyregulatedat27◦Cresultinginasaturatedvapor
pres-sureof0.0041Torr.ItsvaporiscarriedwithN2leachingthesurface
ofthepowder,andthenmixedwiththedilutiongasN2.Thisgas
mixtureisintroducedfromtheupperpartofthereactorthroughan 8mmtubefacingthesubstrateholder.Theresultinginputprocess conditionsarelistedinTable1.
Surfacemorphologyandroughnessaremeasuredusing
scan-ning electron microscopy (SEM) and atomic force microscopy
(AFM).SEMisperformedonaLEO435VPmicroscope.AFMisused
inambientconditionsonanAgilentTechnologies5500instrument. Scanningisperformedincontactmodewithtipsofspringconstant
Fig.1.Arrhenius-typeplotofthegrowthrateofCoOfilmsfromCo2(CO)8onSi.
ofabout0.292N/m(AppNano). Scanningrateis2mm/s.Images
areprocessedwiththesoftwarePicoImage(AgilentTechnologies). FilmsthicknessesaremeasuredbySEMoncrosssectional micro-graphsatthecenterofeachsample.Crystallographicstructuresare determinedbyX-raydiffraction(XRD)onaSEIFERT-3000TT instru-mentusingaCuKa(1.5418 ˚A)X-raytubeoperatedat40kVand
40mA,aNifilterandsolid-stateLynxeyedetector.EPMAisusedto determinetheelementalcompositionofthefilms(CamecaSXFive instrument).Calibrationisperformedusinghighpuritystandards.
Each measurement is repeatedfive times atdifferent locations
todeterminespatialhomogeneity.Finally,theUV–vis–NIRtotal
reflectivity spectra are measured by a Perkin-Elmer
Lambda-19spectrophotometerequippedwithanintegrationsphere.The
reflectedlightiscollectedinthedirectional-hemispherical geom-etrywithanincidenceangleof8◦.
3. Resultsanddiscussions 3.1. Growthkinetics
Processedfilmssystematicallypresentamataspect.Thecolor changeisvisuallyobservedonthesiliconsubstratesduringthefirst minutesofdeposition,correspondingtotheupperlimitof incuba-tiontime.Visualinspectionofthesurfacefacingthefeedingtube revealsthatfilmsdepositedat160◦Cand180◦Careblack,while
thoseobtainedat120◦C,130◦C,140◦Cand190◦Caregrey.Fig.1
presentsanArrhenius-typeplotoftheglobaldepositionreaction. Linesconnectingpointsareguidetotheeye.Growthratefluctuates asafunctionofTd,increasingfrom120to130◦C,thendecreasing
downto160◦CandfinallyincreasingupagainathigherTd.Growth
ratevaluesvarybetween110nm/minatTd=120◦Cand160◦C,and
225nm/minatTd=130◦C,resultinginfilmswhosethicknessvaries
between9and18mm,asmeasuredoncrosssectionsbySEM.
Then,thegrowthratedoesnotshowanArrhenius-type behav-ior.Itevolvesbetweentwomaximaat130◦Cand190◦Candone
minimumat160◦C.Thisbehaviorhasalreadybeenreportedfor
processesinvolvingCo2(CO)8.Whilescanningarangeof
tempera-turefrom50◦Cto250◦Cataworkingpressureof0.01Torr(which
istwoordersofmagnitudelowerthanours),Yeetal.noticetwo growthratemaximaat120◦Cand220◦C.Theyattributethesharp
increaseofthedepositionratearound120◦Ctoapossibleincrease
of the stickingcoefficient of the precursor at low temperature
[33,37].Then,thegrowthrateislikelytodecreaseasTdisfurther
Fig.2.XRDpatternsoffilmsprocessedatdifferentTd.StarscorrespondtotheSi
substratepeaks.
thesamepressurerange(0.05Torr)andatasubstratetemperature
varyingfrom160◦Cto280◦C,RheeandAhnobtainamaximum
growthrateat200◦C[38],ingoodaccordancewiththe
tempera-turesdeterminedinthepresentstudy(190◦C)andreportedbyYe
etal.’s(220◦C).Similarly,Koetal.observedamaximumat140◦C
(P=0.6Torr)[35],ingoodaccordancewithourlowestmaximum (130◦C)andYeetal.’s(120◦C).
3.2. StructureandmorphologyoftheCoOfilms
Fig.2presentsX-raydiffractogramsofthefilmsprocessedat varioustemperatures. TheX-raypeaksat2 equal36.4◦,42.4◦,
61.5◦,73.7◦and 77.6◦ correspondto(111)(200),(220),(331)
and(222)planesofthecubiccobaltoxide(II)CoOphase.Noother cobaltoxide,namelyCo3O4orCo2O3isrevealedfromthe
diffrac-tograms.Filmspresentnopreferentialorientationandtheaverage crystallitediametercalculatedfromtheSherrerequationis esti-matedbetweenca.100nmand150nm.Itisconcludedthatallfilms arecomposedofCoOwithnoothercrystallinephase.Thisresultis corroboratedwiththeelementalcompositionofthefilms, deter-minedas50±1at.%Co,50±1at.%O(exceptat140◦Cwherethe
compositionis47%at.%Co,53at.%O)withoutcarbon contamina-tion,withinthedetectionlimitofEPMA.Itisinterestingtorecall thatweobtainpureCoOfilmswithoutintroductionofanyreactive gas.Thisprecursorisgenerallyusedforthedepositionofsmooth metalliccobaltfilmsatlow pressure(0.03–0.2Torr)[33–36,39]. Theappliedworkingpressureof5Torrinthisworkleadstothe formationofcobalt(II)oxide.Asimilarresultismentionedinref
[28],whereauthorsobtainedcobaltoxidefilmsunderN2working
pressuresof2.2and45Torr.Whereastheyintentionallyadda par-tialpressureofhydrogenfordecreasingtheamountofCoOinthe films,theyobservedanincreaseoftheamountofCoOfrom43to 76at.%!Thispinpointsthecomplexchemistrytakingplaceatthe surfaceofagrowingtransitionmetaloxidefilminthepresenceof
Fig.3.Topview(left)andcrosssection(right)SEMimagesoffilmsdepositedunder
differenttemperatures.Filmthickness(mm)isshownatcorrespondinglocations.
acarbonylprecursor,bothbeingcatalysts.Thoroughinvestigation ofsuchphenomenonhasbeenattemptedintheliterature(seefor example[40])butitisoutsideofthescopeofthepresentwork.
Fig.3showsSEMimagesoftheCoOfilmsdepositedat
differ-enttemperatures, both in surface viewand cross-section view.
Filmsaredenseandpresentacompactcolumnarstructurewith
acauliflowermorphologywhichisreproducedatdifferentlength scalesfrom0.05mmatthesurfaceofthegrainsto5mmforthe larger features diameter. Films processed at 120◦C and 160◦C
Fig.4.AFMimageofaCoOcoatinggrownat160◦C.
present asurface thatis more accidentaland rougherthanthe
otherfilms,andtheircolumnsarewiderwithalargerconicalangle. Interestingly,theycorrespondtothetwominimumgrowthratesas showninFig.1,andtheyaretheonlysampleswithnovisiblecracks. CrosssectionSEMimagesshowthatfilmthicknessvariesbetween
9mmand19mminagreementwiththoseestimated
experimen-tallybysamplemassdifferencebeforeandaftereachdeposition;a goodhintforalimitedporositywithinthefilms.
Fig.4showsanAFMimageofthe160◦CCoOfilm,withthe
typ-icalcauliflowermorphology.Itexhibitsaroot-meansquare(RMS)
roughnessofca.350nm,whereasfilmsgrownat190◦Cshowa
RMSroughnessof120nm,only.Thedifferencebetweenthe
pro-jectedsurface(400mm2for160◦Cand300mm2for190◦C)andthe scannedsurface(225mm2forboth)showsahigherspecificarea forthesampleprocessedat160◦C.Interestingly,fractal
dimen-sionsdeterminedbytheboxpartitioningmethodare2.35and2.31, at160◦Cand190◦C, respectively;values thatequalthenatural
cauliflowerfractaldimensionof2.33.
Therefore,thepresentCoOfilmsexhibitafractalmorphology. Thecauliflowershape isrepeatedidenticallyat differentscales, fromnano-tomicro-.Intheliterature,onlyafewgroupsreported ontheformationofCoOfilmswithacauliflowerstructure[41,42].
Guptaetal.obtainedthecauliflower morphologyon
electrode-positedfilmsofcobalt–nickeloxide(intheformsofNiOandCo3O4)
withatypicalthicknessofabout10mm[42].Alternatively, differ-entfractalstructuresofcobaltoxide(CoOandCo3O4)thinfilms
havebeensynthesizedbyusinglaserCVDatroomtemperatureand atmosphericpressure.Sizeandmorphologyofthestructurescan betailoredbythelaserirradiationtimeandthegasflowratio[43]. Atwo-stepprocesscanalsobeusedinordertoobtainaporousand fractalsurfacemorphology,wheresmoothmetalliccobaltsurface arefirstformedbyPEMOCVDandthenpost-treatedinanO2plasma
[44].Theabove-mentioneddepositiontechniquesprovideCooxide filmswithtargetedcauliflower microstructure.However,unlike abovewhereonlysomedegreesoffreedomaretechnically avail-able,MOCVDallowstoobtainthefractalcauliflowermorphology
withauniqueprecursorandnoreactivegaswhateverthe
depo-sitiontemperatureis.ButwewillshowbelowthatTdaffectsthe
microstructure,whichinturnimpactsthereflectivityperformance ofthefilms.
Inanattempttoperformastatisticalanalysisofthegrainsize distributionweusethefollowingprocedure.SEMImagesata mag-nificationof×10,000areprocessedateachdepositiontemperature (Gwyddionfreeware[45]).First,amaskisappliedoneachimageby adjustingaslopethreshold,takingadvantageofthefactthatgrains visibleonthesurfaceareseparatedbyvalleys.Thereforethemask
floodsdepressionsbetweengrainsand underlinessurface grain
boundaries.Inordertoassesstheconsistencyofthisanalysis,four slopethresholds(7.5%,10%,12.5%and15%)areused;thetwo max-imabeingdeterminedvisuallybytheoperator.Itshowsthatthe
Fig.5. Grainsizedistribution(Countsvs.Diameter)forsixdifferentdeposition
temperatures.
trenddoesnotvary,meaningthatthetemperaturedependenceof thegrainsizedistributionisconstantwhatevertheslopecriterion.
Oncethemaskhasbeeninverted,anequivalentradiusis
auto-maticallycomputedforeachgrain.Then,weperformafrequency analysistoextractthegrainsizedistributions.
Fig.5showstheresultswithaslopethreshold fixedat10%. Weobserveaclassificationofgrainsizedistributions.The distri-butionforfilmsgrownat160◦Cislargerthanthatat190◦C,180◦C
and120◦C,themselvesbeinglargerthanthat130◦Cand140◦C.
Therefore,withinstatisticalandSEMresolutionlimits,twomain featurescanbeextractedfromthegrainsizedistributionanalysis. First,eachTdleadstotheformationofsurfacegrainswith
diam-etersintherange50nmtoca.200nm(ingoodagreementwith
thebulkSherreranalysisofmeancrystallitessizeof100–150nm). Secondly,thedispersionofthedistributiondependsonTd,andthe
threehighestdepositiontemperaturesproducethelargest distri-butions.Hence,surfacesgrownat160◦C,190◦Cand180◦Cexhibit
arelativelylargersizedistributionoflighttraps,inthe subwave-lengthlightscale,inadditiontocauliflowerswithdiametersupto severalmicrometers.
3.3. Opticalproperties
Fig.6showsthereflectivityspectraoftheCoOfilmsprocessed at different Td. Each spectrum shows a low reflectivity
broad-bandwhichpresentsasignificantevolutionwithvaryingTd.Its
positionisshiftedtolongerwavelengthsanditswidthgradually increaseswithincreasingTduntilitcoversthewholevisible
spec-traldomainat160◦Cand180◦C.The160◦Cand180◦C-CoOfilms
showariseoftheirreflectivityat1050nmwhichcorrespondstothe band-gapenergyoftheSisubstrate.Theyexhibitinterestinglylow [400–800nm]averagereflectivityof4.2and2.9%,respectively.This observationiscomparablewithliteratureresultsbyseveralgroups whodepositedeitherCoO[41]orCo3O4[46]filmsby
electrodepo-sitiontechniquesforsolarabsorberapplications.Interestingly,the electrodepositedCoO(OH)films,thatresultfromsurfacehydration, showaverysimilarsurfacemicrostructure.Thereflectivitytrendof thefilmprocessedat190◦Cisratheroffsetcomparedtotheother
fivefilms.Whileitpresentsalowreflectivitybandaswell,itis nar-rowandlocatedatlowwavelengths(i.e.300nm);similartothatof thefilmprocessedat120◦C.Themeanvalueofthereflectivityof
thisfilminthe400–800nmdomainislargelyhigherthanthoseof theotherfilms.However,itdecreaseswithincreasingwavelength, reachingca.8%at1200nm.Whereasitcouldrepresentthemost
Fig.6. ReflectivityspectraofCoOfilmsonSiwafersforvariousTd.
appropriatesampleforapplicationsintheinfraredpartofthe elec-tromagneticspectrum,weconsideritasanexperimentalartifact regardingthetrendvs.Td.
Inthefollowingwediscusspossiblemechanismsresponsible
forthelowreflectivity,anditsevolutionwithTd.
SincetheCoOfilmsthicknessismuchhigherthanthevisible wavelengths,andsincethesefilmsarenotcomposedofnanoscale multilayersstack,weassumethatinterferencesdonotaffect reflec-tivity.Besides,spectralfeaturescannotbeattributedtointerference fringes.Distinctinterferencefringescouldbeobservedbutonlyfor thinnerfilms(notshownhere).
Althoughseveralstudies onCoO show a bandgapof about
5–6eV (200–250nm) [47,48], othergroups showthat the
indi-rect band gap of CoO ranges from 2.3 to 2.8eV (440–550nm)
[30,49,50].Asa result,interbandtransitions cannot explainthe reflectivityofallthespectra.Especiallythetwolowerreflective samplesdepositedat160◦Cand180◦Cshowariseoftheir
reflec-tivityatnoticeablylowerenergies of1.2–1.3eV(950–1000nm). However,onecannottotallyexcludethattransitionsatenergies
lowerthantheCoObandgapcanoccurinourfilmsasreported
elsewhere[47,49].AndCoOiseffectivelystudiedforitsabsorption propertiesforsolarthermalabsorbers[51],showingthatitisable toabsorbefficientlyinthevisiblerange.Nevertheless,thedistinct riseofthereflectivityattheSiband-gapat1050nmofthe160◦C
and180◦C-CoOfilmsdemonstratesthattheabsorptiondecreases
towardsNIRwavelengths.Theabruptincreaseofreflectivityisdue tothethresholdwheretheextinctioncoefficientofSibecomesnull, andwherethemetallicsampleholdercontributionincreases.
AscanbeennoticedfromSEMobservationinFig.3,thelow reflectivefilmdepositedat160◦Cshowsasurfacewiththehighest
densityofmicrometriccauliflowergrains.Butasimilarfilmsurface isobtainedat120◦Cwhereasitshowstheworsevisible
reflectiv-ityperformance.Then,weassumethattheTd-dependenceofthe
reflectivityisnotduetoscatteringcausedbymm-wide cauliflow-ers:reflectivityismanifestlynotcorrelatedtosurfacedensityand shapeofmm-sizedcauliflowers.However,lightscatteringplaysa significantroleinthereflectivitysincethediffuselightreflectivity spectrumoverlapalmostperfectlywiththetotalreflectivity spec-trum(notshown).Therefore,intheabsenceofastrongcorrelation betweenmicrometricfeaturessurfacedensityandreflectivity,we focusontheevolutionofthefilmstructureatthenanoscale.
Takingintoaccountthecomplexsurfacemicrostructure,wecan consideramodelsurfacelayermadeofsubwavelengthCoOgrains
andvoids(air).Thesurfacecanthenbemacroscopicallyconsidered usingtheeffectivemediumapproximationbyalayerwhose refrac-tiveindexisavolumedensity-weightedaverageofthetwomedia. Althoughtherefractiveindex(n)ofCoOsingle-crystalliesbetween 1.8and2.6(imaginarypart0.03<k<1.37)inthewavelengthrange [200–1200nm][47],therefractiveindexoftheeffectivemediumat thesurfacecanbesignificantlyloweredbecauseofthecontribution ofair(n=1.0).Moreover,thelikelyoccurrenceofmicrostructural changesalongthecolumnarstructurecouldresultinariseofthe densityfromfreesurfacetowardsthebulk.Asaconsequence,the refractiveindexoftheCoOfilmsincreaseswithdepth.Suchfilms havebeenfirstanalyzedbyLordRayleigh[52]whonoticedthat reflectioncanbeconsiderablyreducedwhenthetransitionofthe densitybetweentwomediaisgradual.Foraninfinitelythick non-absorbinglayer,asmoothtransitionbetweentherefractiveindex oftheincidentmediumandtherefractiveindexinthebulkofthe layerresultsinreflectivityclosetozeroaccordingtotheFresnel coefficient[53,54].Foranabsorbinglayerhavingafinitethickness, thatisgreaterthantheskindepthoftheeffectivemedium,the reflectivityisreducedprovidedthattherefractiveindexatthefree surfaceofthelayerisclosefromtheoneoftheairandalsoifno sharpmodificationoftheeffectiverefractiveindexoccursalongthe skindepthofthelayer.
Accordingtothismodel,weconcludethatTdappearsto
influ-encetheeffectiverefractiveindexofthelayerprobablythrough thefilmdensity.Severalauthorsdemonstratethatthewideningof therefractiveindexgradientresultsinasignificantincreaseofthe lowreflectivebroadbandwidth[54,55]similartoourexperimental spectra.Otherparameterscouldalsoinfluencetherefractiveindex suchasthestructuralconfigurationofCoOwhichvaries accord-ingtothedepositionparametersand/orimpuritiesinclusioninthe film.Whateverthecauseleadingtothemodificationofthe effec-tiveindex,itresultsinasignificantreflectanceresponsevariation withTd.
4. Conclusions
We formblackCoO films(ca.50at.% Co,50at.%O) onSiby MOCVDfromCo2(CO)8ataworkingpressureof5Torr.Wefocus
ontheinfluenceofgrowthtemperature(120–190◦C)onthefilm
microstructureandtheresultingopticalreflectivity.Weformthick
(9–18mm)columnarfilmswhichexhibitafractalmorphologyof
cauliflowers,aspecificityofferedbyMOCVDascomparedtoother
depositiontechniques.ThefractaldimensiondeterminedonAFM
surfaceimagesis2.31–2.35;i.e.veryclosetothatofthenatural cauliflower(2.33).Opticswise,filmsareverydiffuseandturnblack fortwopeculiardepositiontemperatures,160and180◦C,forwhich
reflectivityisthelowestonthewholevisiblerange(2–5%). Thelow reflectivityarises fromthe peculiar filmstructures.
Sinceweuseaspectrophotometerequippedwithanintegrating
spherethetotalreflectedlightistakenintoaccountintheanalysis. Hence,thedecreaseoftheintegratedlightintensityisdueto(i) specularreflectivity(arelativelylowrefractiveindexofthe effec-tivesurfacelayermaterial(CoO+voids(air)),(ii)lightdiffusion,(iii) absorptionwithinthelayer,andmostlikely(iv)acombinationof
theabove-mentionedmechanisms.
Thetrendofthereflectivitywithincreasingdeposition temper-atureisassumedtocomefromarisingrefractiveindexgradient fromtheair/surfaceinterfacetowardsthebulkoftheCoOcoating.
Thecoatingsshowacolumnarstructurewithaconicalgeometry
whosesurfaceisassumedtobeaneffectivemediumofCoO+voids (air)(withn«2.2).Hence,weassumethatthereisarefractiveindex gradientfromthesurfacelayertowardsdeepercoordinateswhere thefilmgetsdenser,andconsequentlyclosertonCoO=2.2.This
onthespectra.Itissomehowlinkedtothemicrostructureofthe filmsbutwearenotsuccessfulintheclassificationofthe struc-tureswithTd(mainlybecause190◦Cshowsanunclearreflectivity
behaviormakingthisclassificationtoospeculative). Acknowledgments
TheDIRECCTEMidi-Pyrénéesisacknowledgedforfinancial
sup-port in the framework of the AEROSAT 2012 program, under
contractn◦43186.
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