Photon
cascade
emission
in
Pr
3+
doped
fluorides
with
CaF
2
structure:
Application
of
a
model
for
its
prediction
Benjamin
Herden
a,
Amador
García-Fuente
a,
Harry
Ramanantoanina
a,
Thomas
Jüstel
b,
Claude
Daul
a,
Werner
Urland
a,∗aDepartmentofChemistry,UniversityofFribourg,CheminduMusée9,1700Fribourg,Switzerland
bDepartmentofChemicalEngineering,MünsterUniversityofAppliedSciences,Stegerwaldstrasse39,48565Steinfurt,Germany
Inthiswork,wepredictandmeasuretheopticalbehaviourofPr3+indifferentbinaryandternaryfluorides.
WeuseavalidatedmodelbasedonLigandFieldTheoryandDensityFunctionalTheorytocalculatethe
multipletenergylevelsarisingfromtheground[Xe]4f2andexcited[Xe]4f15d1electronconfigurations
ofPr3+initschemicalenvironment.Moreover,theluminescencespectraoftheconsideredmaterials
wererecorded.Inoverallthetheoreticaldeterminationcorroboratestotheexperimentalfindings.The
phenomenonofthephotoncascadeemissionisparticularlystressed,beingimportantforthedesignof
modernphosphorswithquantumefficiencieslargerthan100%.
1. Introduction
Divalent and trivalentlanthanideions arewidely appliedin phosphors,lasergainmediaandscintillatorcrystalsorceramics. Especially trivalent praseodymium(Pr3+) shows a largevariety
ofdifferentapplicationsasactivatorion, viz.UVphosphors[1], lasermaterials[2],up-[3]anddown-conversion[4,5]phosphors. Thedown-conversionphosphorsalsocalledquantumcutter sys-temsorphotoncascadeemissionmaterials(PCE),exhibitatwoor morephotonluminescenceprocess,whereatleasttwolowenergy photonsareemittedperonehighenergyphotonabsorbed[6,7]. Therefore,quantumefficiencieslargerthan100%areachievable. PCEmaterialscanbeusefulinplasmadisplaypanelsorHg-free dischargelamps,inwhichthephosphorsareexcitedbyvacuum UVradiationfromtheXeexcimerdischarge[8].
TheobservationofPCEinPr3+phosphorswassimultaneously
describedbySommerdijketal.[4]andbyPiperetal.[5]in1974 forYF3.TherePiperetal.reportedquantumefficienciesofabout
140%, which have also been foundfor -NaLaF4 [9].Aside the
usualfluoridehosts,Pr3+dopedoxidichosts,viz.SrAl
12O19[10],
LaMgB5O10[11],andLaB3O6[12]weredemonstratedtoshowPCE,
whose phenomenon canonlybe observedifthe lowestenergy level oftheexcited[Xe]4f15d1 electronconfiguration ofPr3+ is
locatedabovethe1S
0energyleveloftheground[Xe]4f2electron
∗ Correspondingauthor.
E-mailaddress:[email protected](W.Urland).
configurations[5].Itisofcrucialimportancetodelimitatethe mul-tipletenergylevelsarisingfromtheground[Xe]4f2andtheexcited
[Xe]4f15d1electronconfigurationsofPr3+initschemical
environ-ment.Itturnsoutthatanoverlapbetweenbothmultipletenergy levelsiscontrolledbyabalancebetweentwointeractionssuchas thenephelauxeticeffectandtheligandfieldsplitting[13].
Sincefluorideligandsexhibiting asmallnephelauxeticeffect [13],thepositionofthelowestenergylevelofthe[Xe]4f15d1
con-figurationdependsmainlyontheligandfieldsplittingofthe5d orbitals.Thisligandfieldsplittingismainlydependentonthe coor-dinationsphereofthePr3+ion.
We considerhereinfour differenthostmatrices,(CaF2, SrF2,
BaF2,and ␣-NaYF4)allcrystallizingin thecubic CaF2 structure
type(spacegroupFm−3m).ThePr3+isdopedintheunique
eight-foldcoordinatedcationsitehavingOhsymmetry[14].Thecubic
␣-phaseofNaYF4isthehigh-temperaturepolymorph,unlikethe
lowtemperatureonewhichpossessesthehexagonal(spacegroup P−6)-phase[15].In␣-NaYF4thecationsiteisrandomlyoccupied
by½Na+and½Y3+[16].
The luminescenceof thesePr3+ activatedfluorideshasbeen
experimentallydescribedbyseveralworkinggroups[17–19].The alkalineearthfluorides(CaF2:Pr3+,SrF2:Pr3+,andBaF2:Pr3+)show
inallthecasesbroadbandemissionduetothefactthatthelowest energylevelofthe[Xe]4f15d1configurationislocatedbelowthe1S
0
energylevel[17].Thustheligandfieldsplittingofthe5dorbitalsis expectedtobelarge.Ontheotherhand,the␣-NaYF4:Pr3+shows
lineemissionproperforPCEmaterials[18,19].Heretheligandfield interactionofthe5dorbitals iscertainlyweaker.Thesefindings
Published in &KHPLFDO3K\VLFV/HWWHUV±
which should be cited to refer to this work.
cannotbesolelyexplainedbythedifferentsizesofthereplaced cations,Ca2+:126pm,Sr2+:140pm,Ba2+:156pmandY3+:116pm
incontrasttoPr3+:126.6pm(allgivenforcoordinationnumber
(CN)8[20]),sincethechemicalenvironmentandthesymmetryis inallcasesidentical.Rodnyietal.[21]reportedabouttheenergy shiftofthelowestlevelofthe[Xe]4f15d1configurationasfunction
ofthePr3+concentrationinBaF
2 crystals.Forhigher
concentra-tions(3.0%)PCEwasobservedduetotheformationofPr3+-based
clusters.
Hereweapplyourvalidatedmodel[13]toexplainandpredict theabovementionedPCEphenomenon.Thismodelisalso essen-tialfortailoringphosphorstogeneratewarm-whitelight[22].The structureofthePr3+dopedsystemsisoptimizedusingperiodical
calculationsbasedonDensityFunctionalTheory(DFT)bymeans oftheVASPcode[23,24].ThePBEfunctionalisusedto parame-terizetheexchange-correlationpotential[25].Thestructureofthe dopedsystemisobtainedtakingintoaccountasuper-cellmodel composedbyonePr3+ionin32unit-cellscorrespondingtoadopant
concentrationof3%.ItisimportanttomentionthatthePr3+ionsare
handledasisolatedions.Aselectivecutofthisoptimizedstructure isperformedtakingintoaccountthePr3+centreanditssurrounding
ligands,subjected toa molecularcalculationusingthe Amster-damDensityFunctional (adf2013.01)programpackage [26,27]. WeusethecomputationalmodelnamedLFDFT[13,28,29],whose outputenablesthecomputationsoftheSlater–Condonparameters, spin–orbitcouplingconstantsandligandfieldpotential. Prepara-tionandopticalcharacterizationofCaF2:Pr3+,Na+;SrF2:Pr3+,Na+;
BaF2:Pr3+,Na+;and␣-NaYF4:Pr3+areperformed(seeSection4).The
dopinglevelwasisallcasesadjustedto1.0%toavoidclusteringof Pr3+inthepowdersamples.Thepreparedphosphorswereof
sin-glephaseandluminescencespectrawererecordedfromtheVUV tothenearinfraredregion.
2. Resultsanddiscussion
ThecalculationsforthePr3+dopedalkalineearthfluoridesand
␣-NaYF4 yieldtheparameterslistedinTable1.Inthetabletwo
columnsaredevotedtothe␣-NaYF4systemrelatingthetwo
spe-cialextremesituationswhichareillustratedbytakingthesecond coordinationspherecontainingexclusivelyNa+(hereafterO
h(Na))
Table1
ElectrostaticandligandfieldparametersforallPr3+dopedhostswithO hsite
sym-metry(incm−1).
Host CaF2 SrF2 BaF2 ␣-NaYF4 ␣-NaYF4
Symmetry Oh Oh Oh Oh(Na) Oh(Y)
F2(ff)a 322.8 322.9 322.9 322.9 322.8 F4(ff)a 41.7 41.7 41.7 41.7 41.7 F6(ff)a 4.4 4.4 4.4 4.4 4.4 G1(fd)a 358.9 356.9 351.2 350.2 365.3 F2(fd)a 226.7 225.3 222.7 221.4 229.4 G3(fd)a 30.7 30.5 30.1 29.9 31.2 F4(fd)a 17.4 17.3 17.1 17.0 17.6 G5(fd)a 4.8 4.7 4.7 4.7 4.9 4fb 710 710 710 710 710 5db 945 945 945 945 945 e(f)c 599 538 491 450 673 e(f)c 257 232 213 164 279 e(d)c 14114 13009 12154 11652 16210 e(d)c 4705 4336 4051 3886 5404 AOM(fd)d 15183 17918 20030 21162 9851 aF
k(ff), Fk(fd) and Gk(fd) refer to the interelectronic effect known as
Slater–Condonparameterswidelydescribedintextbooks[30,31].
bSpin–orbitcouplingconstantsforthe4fand5dorbitalswereobtainedusingthe
relativisticZORAapproach[13].
c TheligandfieldinteractionisbetterrepresentedwithrespecttotheAngular
OverlapModel(AOM)parameters[32].InthepresentcasefourAOMparameters areavailableduetotheproblemoftwo-open-shell4fand5delectrons.
d Wereferto[32]anddefine
AOM(fd)accordingly.
Figure1.CalculatedmultipletenergylevelsofPr3+dopedCaF
2,SrF2,andBaF2
correspondingtothe[Xe]4f2(red)andthe[Xe]4f15d1configurations(blue).The
structuresrepresentthecentralPr3+ion(grey)surroundedbyeightF−(green)and
thesecondcoordinationspherecontainingthecorrespondingalkalineearthcations. (Forinterpretationofthereferencestocolourinthisfigurelegend,thereaderis referredtothewebversionofthisarticle.)
orY3+(hereafterO
h(Y))ions.Inbothsituations,Ohsymmetryofthe
coordinationofthePr3+isachieved.
ThetheoreticalresultsaregraphicallyrepresentedinFigure1, wherethemultipletenergylevelsoriginatingfromthe[Xe]4f2and
the[Xe]4f15d1 configurationsaregiveninredand blue,
respec-tively.Anoverlapbetweenbothmultipletenergylevelsisnoticed. ThusPCEisnotobservedasitisconfirmedbyourrelated exper-imental work (see Figure 2) which is also in linewith earlier observationsbyLawsonetal.[17].
Duetotheweakligandfieldinteractionofthe4forbitalsofPr3+
(seeparametersinTable1),inFigure1themultipletenergy lev-elsarisingfromthe[Xe]4f2configurationsseemtobeidenticalin
anysystems.Ontheotherhand,theinfluenceofthechemical sur-roundingonthe5dorbitalsisstrongerwhichresultsinadifferent splittingofthe[Xe]4f15d1configurations.Inthepresentsituation
the5dorbitalsofPr3+splitovere
gandt2girreducible
representa-tionsoftheOhpointgroup.Therefore,themultipletenergylevels
fromthe[Xe]4f15d1configurationsaresplitintwodifferentbands
fullyrecognizedinFigure1butalsointheexperimental character-izationbelow(seeFigure2).
TheionicradiiofCa2+(126pm)andPr3+(126.6pm)forCN8are
almostidentical,whereastheionicradiiofSr2+(140pm)andBa2+
(156pm)aremuchlarger.Thismeans,thatthesizeofthecation whichisreplacedbyPr3+isincreasing(seeTable2)intheseries
ofCaF2,SrF2andBaF2leadingtoadecreaseofthesplittingforthe
5dorbitalsofPr3+.Thetotalsplittingofthecalculatedmultiplet
energylevelsbetweenegandt2gisspecifiedwith20910cm−1for
CaF2:Pr3+,19272cm−1forSrF2:Pr3+,and18006cm−1forBaF2:Pr3+.
TheluminescencespectraofthePr3+dopedalkalineearth
fluo-ridesaremeasured(seeSection4)andgiveninFigure2.Sincewe focusonthelowestenergylevelofthe[Xe]4f15d1 configuration,
excitationspectraweremonitoredintheVUVpartofthespectral range.Theexcitationspectraindicatethattherearetwoseparated bandswhichcanbecomparedtotheegandt2glevelsknownfor
Ohsymmetry.Thesplittingbetweenthesetwobandsisdecreasing
fromabout18230cm−1forCaF2:Pr3+,Na+(1.0%)and14580cm−1
forSrF2:Pr3+,Na+(1.0%)to13260cm−1forBaF2:Pr3+,Na+(1.0%).The
values were derived taking the energy difference between the twomaximaoftheexcitationbands,whereatitis importantto announcethat themeasurementsweredoneatroom tempera-ture(298K).Ourtheoreticalresultsoverestimatethembyabout 20%,althoughthecaseofCaF2:Pr3+areperfectlyinlinewiththe
Figure2.RoomtemperatureluminescencespectraofCaF2:Pr3+,Na+(1.0%),SrF2:Pr3+,Na+(1.0%)andBaF2:Pr3+,Na+(1.0%).VUVexcitationspectraareplottedontheleftand
emissionspectraontheright.Thedashedgreylinerepresentstheenergypositionofthe1S
0energylevel.
observation of Oskam et al. [35]. They reported a ligand field splittingofthe5dorbitalsofabout21000cm−1derivedfrom exper-imentalwork(measuredat6K).Thediscrepancyoriginatesfrom thetemperaturedependenceofthet2g levels,meanwhiletheeg
levelsremainatthesameenergy.Thiswasalready observedby Loh [36] in former investigations of theUV absorption of Pr3+
dopedalkalineearthfluorides.Sincetheeglevelsremainatthe
sameenergy,changesintheemissionspectracannotbeobserved. Thehighestenergylevel1S
0oftheground[Xe]4f2configuration
isexpectedtobelocatedcloseto47000cm−1asitisdetermined theoretically(seeFigure1)andwhichwasalreadydescribedin lit-erature[4,35].Therefore,thelowestenergylevelofthe[Xe]4f15d1
configurationisinallcasesoverlappingwiththehighestenergy level1S
0.PCEforthesephosphorsisnotobservedwhereby the
emissionspectrainFigure2mainlyshowbroadbandemissionfrom thelowestenergylevelofthe[Xe]4f15d1configurationintheUV
partofthespectralrange.IncaseofSrF2:Pr3+,Na+anintermediate
bandbetweentheegandthet2gonesappearswhichisduetoasmall
amountofresidualPrF3[37].However,thisleadstohigher
intensi-tiesofintraconfigurational[Xe]4f2−[Xe]4f2transitionswhichcan
onlybeobservedinthecaseofSrF2:Pr3+,Na+.
Incomparisontothebinaryalkalineearthfluoridestheternary ␣-NaYF4isinvestigated.The␣-polymorphexhibitsthecubicCaF2
structuretypewithNa+andY3+randomlydistributedonthecation
sites.Here,theaveragebondlengthiscomparabletotheoneofCaF2
(seeTable2).
TheresultsofthecalculationsaregiveninFigure3,following thesamerepresentationsasinFigure1.Thetwoabovementioned extremesituationsoftheOhsymmetryarecalculatedseparately.
Anoverlapbetweenbothmultipletenergylevelsisnoticedagain. Thus PCEisnotexpectedin bothsituations whichisin contra-dictiontoourexperimentalresults(seeFigure4)andalsotothe experimentalworkpublishedbySommerdijketal.[18].
Themultipletenergylevelsarisingfromthe[Xe]4f2
configu-rationsinFigure3seemtobeagainnearlyidenticalforthetwo differentOhsituations.Theinfluenceofthechemicalsurrounding
onthe5dorbitalsis muchstrongerwhich resultsina different splittingforthe[Xe]4f15d1configurations.Na+hasalargerionic
radiusthanY3+,leadingtosmallersplittingofthe5dorbitalsof
Pr3+.Therefore,thelowestenergylevelofthe[Xe]4f15d1
config-urationislocatedathigherenergybutstillbelowthe1S 0energy
level.Thetotalsplittingofthecalculatedmultipletenergylevels betweenegandt2gisspecifiedwith17255cm−1forOh(Na)and
24015cm−1fortheOh(Y)symmetry.
Theluminescencespectraof ␣-NaYF4:Pr3+(1.0%)aregivenin
Figure4.Theexcitationspectrumshowsonebroadbandranging from48000to72000cm−1withtwonextneighbouredmaxima. Thehighestenergylevel1S
0oftheground[Xe]4f2configurationis
Table2
Cation–anionbondlengthindifferenthosts(inpm).Literaturevaluesgivethebondlengthoftheundopedhostswhereasthecalculatedonesdisplaythevaluesofthe theoreticalPr–Fbond.Incaseof␣-NaYF4thedistancefromtheliteratureshowstheaveragevalue.
Host CaF2 SrF2 BaF2 ␣-NaYF4 ␣-NaYF4
Symmetry Oh Oh Oh Oh(Na) Oh(Y)
Literature(undoped) 236.6[33] 251.1[33] 268.5[33] 235.7[34] 235.7[34]
Calculated(doped) 237.2 240.9 244.0 245.7 231.8
Figure3.CalculatedmultipletenergylevelsofPr3+doped␣-NaYF
4,corresponding
tothe[Xe]4f2(red)andthe[Xe]4f15d1configurations(blue).Thetwogiven
sym-metriesdifferinthesecondcoordinationspherecontainingjustNa+(O
h(Na))orY3+
(Oh(Y)).ThestructuresrepresentthecentralPr3+ion(grey)surroundedbyeightF−
(green)andthesecondcoordinationspherecontainingNa+(yellow)orY3+(blue).
(Forinterpretationofthereferencestocolourinthisfigurelegend,thereaderis referredtothewebversionofthisarticle.)
stilllocatedatabout47000cm−1(seeFigure1and3).Therefore,the lowestenergylevelofthe[Xe]4f15d1configurationislocatedabove
thehighestenergylevel1S
0whichmeansthatPCEforthisphosphor
ispresent.Theemissionspectrumof␣-NaYF4:Pr3+isdominated
bysharp intraconfigurational[Xe]4f2−[Xe]4f2 transitions which
isingoodagreementwithpreviousresultsofSommerdijketal.
[18].TheemissionlinesintheUVpartofthespectralrange origi-natefromthe1S
0energylevelwiththemaximumat24600cm−1
due to the 1S
0–1I6 transition and representing the first
pho-ton.The emissionlinesin thevisiblepartof thespectral range originate from the 3P
0 energy level and representing the
sec-ond photon. In theUV range at around 43500cm−1 there is a smallamountofbroademissionwhichcannotbeassignedtoany [Xe]4f2–[Xe]4f2transitionknownforPr3+andwhichwasalready
describedelsewhere[19].Thiscouldleadbacktoasmallamountof interconfigurational[Xe]4f15d1–[Xe]4f2emissionoriginatingfrom
thelowestenergylevelofthe[Xe]4f15d1configuration.Incontrary
to LaPO4:Pr3+ where the combination of sharp
intraconfigura-tional[Xe]4f2–[Xe]4f2transitions andbroadinterconfigurational
[Xe]4f15d1–[Xe]4f2 transitions isonlyobservedatlow
tempera-tures[38]herethisisalreadyoccursatroomtemperature. Toexplainthedifferencesbetweentheabovegiven theoreti-calresults(seeFigure3)andtheexperimentalmeasurements(see Figure4),newmodelswereperformedassumingadistortionof theOhsymmetry[39].Thisdistortionoriginatesfromthesecond
coordinationsphereofPr3+whichconsistsof12sitesrandomly
occupiedbyNa+(132pm)andY3+(116pm).Unlikeasmentioned
in[40]thesecondcoordinationsphereisaffectingtheanionswhich arethenresponsibleforthechangeoftheligandfield.Sincethe ionicradiiaswellastheionicchargeofthesetwoionsareso dif-ferentdistortionofthesymmetryisexpected.Takingintoaccount thesecondcoordinationsphere,212=4096differentstructural
con-formationsarepossible,fromwhichonlytwoextremesituations exhibitOhsymmetry.Duetothelargenumberofstructural
con-formations,hereweanalyzeonlythesituationwherethesecond coordinationspherecontainsexactly6Na+and6Y3+ionsbeside
thetwoextremesituationsdiscussedbefore(formoreinformation seeSection4).ThemodelparametersoftheOhcases(seeTable1)
aremodifiedforthedistortedconformationsusingtheAOMforthe angulardistortionandDFTfortheradialpart.Thusthedescentin symmetrygoesfromD3dtoonlyC1.Theresultsofthesecalculations
aregiveninFigure5.
Figure4.Roomtemperatureluminescencespectraof␣-NaYF4:Pr3+(1.0%).VUVexcitationspectrumisgivenontheleftandemissionspectrumontheright.Thedashedgrey
linerepresentstheenergypositionofthe1S
0energylevel.
Figure5.Calculatedmultipletenergylevelsofthe[Xe]4f15d1configurationsofthe
Pr3+doped␣-NaYF
4indifferentsymmetries.Thesolidredlinecharacterizesthe
energyofthe1S
0energyleveloftheground[Xe]4f2configuration.Thestructures
representthecentralPr3+ion(grey)surroundedbyeightF−(green)andthesecond
coordinationspherecontainingNa+(yellow)andY3+(blue).(Forinterpretationof
thereferencestocolourinthisfigurelegend,thereaderisreferredtothewebversion ofthisarticle.)
Themultipletenergylevelsarisingfromthe[Xe]4f2
configura-tionsisnotpresentedinFigure5,sincetheinfluenceofthechemical surroundingisverylow.Theinfluenceofthechemicalsurrounding onthe5dorbitalsforthegivensymmetriesismuchstrongerwhich resultsforeachcaseinadifferentsplitting.Therefore,weachieve symmetrieswherethelowestenergylevelofthe[Xe]4f15d1
con-figuration islocatedbelow thehighestenergy level1S
0 and do
notshowPCElikeD3d.However,forsymmetriesviz.C2h,C2v,Cs,
andC1thelowestenergylevelofthe[Xe]4f15d1configurationis
locatedabovethehighestenergylevel1S
0whichleadstoPCE(see
Figure5).Noticethat lowersymmetrystructureswouldalsobe morecommonamongthe4096differentstructuralconfigurations thanhigherones.ThisexplainsthePCEprocessin␣-NaYF4asan
effectofloweringthesymmetryduetotheeffectofthesecond coordinationsphere,aswellasthesmallamountof interconfigu-rational[Xe]4f15d1–[Xe]4f2emission,whichwouldcomefromPr3+
ionsoccupyinghighersymmetrysites.
3. Conclusions
Insummary,thealkalineearthfluorides,(CaF2,SrF2andBaF2)do
notshowPCEsincethePr3+islocatedatacrystallographicposition
withOhsymmetry.Thesplittingofthe5dorbitalsinthis
symme-tryislarger,insofarasthelowestenergylevelofthe[Xe]4f15d1
configuration is always locatedbelow the highest energy level
1S
0 of theground [Xe]4f2 configuration. Our calculations fit to
theexperimental data,which showmainly interconfigurational [Xe]4f15d1−[Xe]4f2emission.␣-NaYF
4offersaswellOh
symme-tryforthecationposition.Thecalculationofsuchasystemwhere thePr3+ is locatedat a crystallographic positionwithO
h
sym-metrywould leadtoamaterialwithoutshowingPCE. Thisisin contradictionwiththeexperimentaldatawhichshowmainly intra-configurational [Xe]4f2−[Xe]4f2 emission lines.By lowering the
symmetry starting froma highD3d tothe lowC1 this
extraor-dinary finding can be explained. The lower symmetries which describeadistortionofthecrystallographicpositioncanbe eas-ilyexplainedbythesecondcoordinationsphere.Moreover,with thesedifferentsymmetriesitispossibletoexplaintheemission
spectrawhichshowsinadditionasmallpartofinterconfigurational [Xe]4f15d1−[Xe]4f2transitionsintheUVpartofthespectralrange.
4. Experimental
4.1. Computationaldetails
VASPcalculationswereperformedtodeterminethe surround-ingstructureofPr3+inaperiodiclattice.PBEfunctionalwasused
fortheexchange-correlationpotential.TheProjectorAugmented Wavemethod(PAW)wasusedtoreproducetheinteractionofthe valenceelectronswiththenucleiandcoreelectrons.Aplane-wave basissetwithacutoffenergyof400eVwasusedtoreproducethe electronicstates.Theatomicpositionswererelaxeduntilallforces weresmallerthan0.001eV/ ˚A.Fromtherelaxedstructure, molec-ularcalculationswereperformedwithADF2013.01toobtainthe electrostaticandligandfieldparameters.ATZ2P+basissetwasused forPr,andaTZPbasissetwasusedforF.Pointchargesareincluded atthedistanceofthePr3+secondcoordinationspheretoreproduce
theeffectofthelatticepotential.ThedistortedstructuresofNaYF4
areobtainedfrommolecularcalculationsbyfixingthepositionsof theNa+andY3+ionsinthesecondsphere,allowingtorelaxthePr3+
andF−ions.
4.2. Experimentaldetails
Allphosphors were preparedby precipitationfrom aqueous solutionattheDepartmentofChemicalEngineering,Münster Uni-versity ofApplied Sciences. Theconcentrationof Pr3+in theso
preparedphosphorswasadjustedto1%.
Incaseofthealkalineearthfluoridesthealkalineearthnitrates, viz. Ca(NO3)2·4H2O (ProAnalysi, Merck), Sr(NO3)2, (ProAnalysi,
Merck),andBa(NO3)2,(ProAnalysi,Merck),weredissolvedinwater
togetherwithstoichiometricamounts ofPr(NO3)3·6H2O(99.9%,
AlfaAesar)andsubsequentdropwiseadditionofdissolvedNH4HF2
(95%,AlfaAesar)untilprecipitationoccurred.Afterfiltrationand drying1%NaFwasaddedforchargecompensation.Themixtures werethenfilledintoglassy-carboncruciblesandsinteredfor6hat 900◦Cinanitrogenstream.Thenitrogen,whichwasusedtoavoid thereactionofthefluorideswithoxygen,wasfurtherpurifiedby dryingwithmolecularsieveandKOH.
Forthe␣-NaYF4astoichiometricmixtureofYCl3·6H2O(99.9%,
TreibacherIndustrieAG)andPrCl3·6H2O(99.9%,Sigma–Aldrich)
wasdissolvedinwaterandcombinedwithasolutionofatentimes molarexcess ofNaF(ProAnalysi,Merck).Precipitationoccurred immediatelyandafterfiltrationanddryingthemixturewasfilled intoa glassy-carboncrucibleand sinteredfor6hat600◦C ina
nitrogenstream.Thistemperaturewaschosentoavoidthe trans-formationofthecubic␣-phaseofNaYF4tothehexagonal-phase.
4.3. Characterization
Allluminescencemeasurementswereperformedatthe Depart-ment of Chemical Engineering, Münster University of Applied Sciences.
Forallluminescencemeasurementsthepowdersampleswere pressedintoaPTFE-sampleholder,wherebythesurfacewas struc-turedbyusingawhitefleeceafterwards.Allinvestigatedpowder samples were excited at 160nm and the luminescence spec-tra recorded with a VUV spectrometer (Edinburgh Instruments FS920).ThespectrometerwasequippedwithaVUV monochroma-torVM504fromActonResearchCorporation(ARC)andadeuterium lampasanexcitationsource.Thesamplechamberwasflushedwith driedNitrogeninordertopreventabsorptionofVUVradiationby waterandoxygen.Excitationandemissionspectrawererecorded intherangesof120–250nmand200–800nm,respectively.The
emissionspectrawerecorrectedbyusingacorrectionfileobtained from a tungstenincandescent lamp certifiedby NPL. The rela-tiveVUVexcitationintensitiesofthesampleswerecorrectedby dividingthemeasuredexcitationspectraofthesampleswiththe excitationspectrumofsodiumsalicylate(o-C6H4OHCOONa)under
thesameexcitationconditions.Themeasurementswereperformed atambienttemperatureandpressurewithastepsizeof0.5nm.
Acknowledgements
ThisworkissupportedbytheSwissNationalScience Founda-tion(SNF),theSwissStateSecretariatforInnovationandResearch, theEuropeanCooperationinScienceandTechnology(COST)Action EUFEN (CM1006) and the Bundesministerium für Bildung und Forschung(BMBF)project13N9353.Dr.FanicaCimpoesufromthe UniversityofBucharestandDr.JörgNordmannformUniversityof Osnabrückarewarmlyacknowledgedforthefruitfuldiscussionand interestonthistopic.
References
[1]A.Katelnikovas,H.Bettentrup,D.Dutczak,A.Kareiva,T.Jüstel,J.Lumin.131 (2011)2754.
[2]A.Richter,E.Heumann,E.Osiac,G.Huber,W.Seelert,A.Diening,Opt.Lett.29 (2004)2638.
[3]T.Sandrock,E.Heumann,G.Huber,B.H.T.Chai,in:P.Payne(Ed.),Adv.Solid StateLasers,OpticalSocietyofAmerica,SanFrancisco,1996,PM1.
[4]J.L.Sommerdijk,A.Bril,A.W.deJager,J.Lumin.8(1974)341.
[5]W.W.Piper,J.A.DeLuca,F.S.Ham,J.Lumin.8(1974)344.
[6]R.T.Wegh,H.Donker,K.D.Oskam,A.Meijerink,Science283(1999)663.
[7]C.Ronda,J.Lumin.100(2002)301.
[8]T.Jüstel,J.-C.Krupa,D.U.Wiechert,J.Lumin.93(2001)179.
[9]B.Herden,A.Meijerink,F.T.Rabouw,M.Haase,T.Jüstel,J.Lumin.146(2014) 302.
[10]A.M.Srivastava,W.W.Beers,J.Lumin.71(1997)285.
[11]A.M.Srivastava,D.A.Doughty,W.W.Beers,J.Electrochem.Soc.143(1996)4113.
[12]A.M.Srivastava,D.A.Doughty,W.W.Beers,J.Electrochem.Soc.144(1997)L190.
[13]H.Ramanantoanina,W.Urland,A.García-Fuente,F.Cimpoesu,C.Daul,Phys. Chem.Chem.Phys.16(2014)14625.
[14]A.R.West,GrundlagenderFestkörperchemie,Wiley,Weinheim,1992.
[15]C.Renero-Lecuna,R.Martín-Rodríguez,R.Valiente,J.González,F.Rodríguez, K.W.Krämer,H.U.Güdel,Chem.Mater.23(2011)3442.
[16]A.Grzechnik,P.Bouvier,W.A.Crichton,L.Farina,J.Köhler,SolidStateSci.4 (2002)895.
[17]J.K.Lawson,S.A.Payne,Opt.Mater.2(1993)225.
[18]J.L.Sommerdijk,A.Bril,A.W.deJager,J.Lumin.9(1974)288.
[19]B.Herden,J.Nordmann,R.Komban,M.Haase,T.Jüstel,Opt.Mater.35(2013) 2062.
[20]R.D.Shannon,ActaCrystallogr.Sect.A32(1976)751.
[21]P.A.Rodnyi,G.B.Stryganyuk,C.W.E.vanEijk,A.S.Voloshinovskii,Phys.Rev.B 72(2005)195112.
[22]S.Schmiechen,P.Pust,P.J.Schmidt,W.Schnick,NachrichtenAusChem.62 (2014)847.
[23]G.Kresse,J.Hafner,Phys.Rev.B47(1993)558.
[24]G.Kresse,J.Furthmüller,Phys.Rev.B54(1996)11169.
[25]J.P.Perdew,K.Burke,M.Ernzerhof,Phys.Rev.Lett.77(1996)3865.
[26]C.F.Guerra,J.G.Snijders,G.teVelde,E.J.Baerends,Theor.Chem.Acc.99(1998) 391.
[27]G.teVelde,F.M.Bickelhaupt,E.J.Baerends,C.FonsecaGuerra,S.J.A.van Gisber-gen,J.G.Snijders,T.Ziegler,J.Comput.Chem.22(2001)931.
[28]H.Ramanantoanina,W.Urland,F.Cimpoesu,C.Daul,Phys.Chem.Chem.Phys. 15(2013)13902.
[29]H.Ramanantoanina,W.Urland,A.García-Fuente,F.Cimpoesu,C.Daul,Chem. Phys.Lett.588(2013)260.
[30]S.Hüfner,OpticalSpectraofTransparentRareEarthCompounds,Elsevier, NewYork,2012.
[31]R.D. Cowan,The Theory of Atomic Structure and Spectra, University of CaliforniaPress,Berkeley,1981.
[32]H.Ramanantoanina,W.Urland,F.Cimpoesu,C.Daul,Phys.Chem.Chem.Phys. 16(2014)12282.
[33]B.P.Sobolev,E.G.Ippolitov,B.M.Zhigarnovskii,L.S.Garashina,Izv.Akad.Nauk. SSSRNeorg.Mater.1(1965)362.
[34]R.E.Thoma,G.M.Hebert,H.Insley,C.F.Weaver,Inorg.Chem.2(1963)1005.
[35]K.D.Oskam,A.J.Houtepen,A.Meijerink,J.Lumin.97(2002)107.
[36]E.Loh,Phys.Rev.158(1967)273.
[37]S.Kück,I.Sokólska,Appl.Phys.A77(2003)469.
[38]A.M.Srivastava,A.A.Setlur,H.A.Comanzo,W.W.Beers,U.Happek,P.Schmidt, Opt.Mater.33(2011)292.
[39]G.F.Koster,J.O.Dimmock,R.G.Wheeler,H.Statz,ThePropertiesofthe Thirty-TwoPointGroups,MITPress,Cambridge,MA,1963.
[40]D.Tu,Y.Liu,H.Zhu,R.Li,L.Liu,X.Chen,Angew.Chem.125(2013)1166.