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Electronic structure of stoichiometric and Ar+-bombarded ZrO2 determined by resonant photoemission

Morant, C.; Fernández, A.; Rodríguez González-Elipe, Agustín; Soriano, L.; Stampfi, A.; Bradshaw, A.M.; Sanz, J.M.

Abstract

The electronic properties of thermally grown ZrO2 thin films before and after Ar+ bombardment have been studied with resonant photoemission spectroscopy using synchrotron radiation. For stoichiometric ZrO2 thin films the experimental valence-band spectra are in good agreement with the calculated density of states for bulk ZrO2. For both stoichiometric and Ar+-bombarded ZrO2 thin films, resonant photoemission from the valence band was observed when the photon energy was swept through the Zr 4p→4d transition energy. The resonant profile was found to exhibit a maximum at hν=39 eV, followed by a second well-resolved broad maximum around 50 eV. The feature at 39 eV is consistent with resonant enhancement of the Zr 4d states and has been used to identify those regions of the valence band with an important Zr 4d admixture. The results are in good agreement with the calculated Zr 4d partial density of states. The intensity increase observed at hν∼45-50 eV is found to be associated with the nonbonding region of the valence band, although a proper interpretation is needed. In addition, it was found that Ar+ bombardment induces electronic states in the band-gap region and changes in the O 2p valence band. Three distinct emission bands were identified in the band gap as a function of the Ar+ dose. They are associated with the formation of oxygen vacancies and mixed oxidation states due to preferential sputtering of the oxygen atoms. Resonant photoemission of these Ar+-bombarded films demonstrates both the cationic character of the band-gap states and the increase of the cationic contribution to the O 2p valence band.

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PHYSICAL REVIEW BVOLUME S2, NUMBER 16 1S OCTOBER 1995-II Elec onic s uc u e o s oichiome ic and A +-bomba ded Z O2 de e mined by esonan pho oemission C. Mo an Can oblanco, E-28049 Mad id, Spain A. Fe nandez and A. R. Gonzalez-Elipe Ins i u o Ciencia de Ma e iales de Se illa, Consejo Supe io de In es igaciones Cien igcas, Uni e sidad de Se illa, Depa amen o de Quimica Ino ga'nica, P.O. Box 1115,E41071 -Se illa, Spain L. So iano Can oblanco, E-28049 Mad id, Spain A. S amp i and A. M. B adshaw F i z Habe I-ns i u -de Max Planck G-esellscha- , Fa aday eg 4-6, 14195Be lin, Ge many J.M. Sanz* Can oblanco, E-28049 Mad id, Spain (Recei ed 2May 1995; e ised manusc ip ecei ed 10July 1995) The elec onic p ope ies o he mally g own Z O& hin ilms be o e and a e A + bomba dmen ha e been s udied wi h esonan pho oemission spec oscopy using synch o on adia ion. Fo s oichiome ic Z 02 hin ilms he expe imen al alence-band spec a a e in good ag eemen wi h he calcula ed densi y o s a es o bulk Z 02. Fo bo h s oichiome ic and A +-bomba ded Z 02 hin ilms, esonan pho o- emission om he alence band was obse ed when he pho on ene gy was swep h ough he Z 4p ~4d ansi ion ene gy. The esonan p o ile was ound o exhibi amaximum a h =39 eV, ollowed by a second well- esol ed b oad maximum a ound 50 eV. The ea u e a 39 eV is consis en wi h esonan enhancemen o he Z 4d s a es and has been used o iden i y hose egions o he alence band wi h an impo an Z 4d admix u e. The esul s a e in good ag eemen wi h he calcula ed Z 4d pa ial densi y o s a es. The in ensi y inc ease obse ed a h -45 — 50 eV is ound o be associa ed wi h he nonbond- ing egion o he alence band, al hough ap ope in e p e a ion is needed. In addi ion, i was ound ha A + bomba dmen induces elec onic s a es in he band-gap egion and changes in he 02p alence band. Th ee dis inc emission bands we e iden i ied in he band gap as a unc ion o he A + dose. They a e associa ed wi h he o ma ion o oxygen acancies and mixed oxida ion s a es due o p e e en ial spu e ing o he oxygen a oms. Resonan pho oemission o hese A +-bomba ded ilms demons a es bo h he ca ionic cha ac e o he band-gap s a es and he inc ease o he ca ionic con ibu ion o he 0 2p alence band. I. INTRODUCTION The main pu pose o his pape is o in es iga e he elec onic s uc u e o he mally g own Z 02 hin ilms as well as he e ec s induced by A + bomba dmen using esonan pho oemission spec oscopy (RPES). The elec- onic band s uc u e o Z 02, a e ac o y ansi ion- me al oxide (TMO), is o g ea in e es om bo h he echnological and undamen al poin s o iew. I s wide use as ahigh-pe o mance ce amic o nuclea and high- empe a u e applica ions, as well as in gas sensing, elec o-op ical, hin- ilm, and ca alysis applica ions makes band s uc u e in o ma ion e y impo an o un- de s anding i s physical and chemical p ope ies. Pas in- es iga ions seem o ha e been o ien ed mainly owa ds p ac ical aspec s, ' a he han owa ds hese mo e un- damen al aspec s. 'Only a ew expe imen s ha e p obed he elec onic s uc u e o Z 02, 'and hei in- e p e a ion has elied on alimi ed numbe o band s uc- u e calcula ions. Mo eo e , he elec onic s uc u e o de ec s on ansi ion-me al oxides has also become a subjec o ex ensi e s udy. 'Low-ene gy ion bo n- ba dmen is o en used o c ea e de ec s in TMO's, bu , because o he di icul y o cha ac e iza ion, i s e ec on elec onic p ope ies has no ye been su Ficien ly s udied. Many spec oscopic s udies ha e shown ha oxygen a- cancies cause localized ene gy le els in he band gap. In mos cases i has p o en di icul , howe e , o ela e he obse ed elec onic s a es o speci ic de ec s, e en hough his has been a emp ed ecen ly in some heo e ical ap- p oaches. ''To ou knowledge only Sobole e al. ,using asel -consis en sca e ed-wa e me hod, 0163-1829/95/52(16)/11711(10)/$06.00 11 711 1995 The Ame ican Physical Socie y 11 712 C. MORANT e al. ha e ied o s udy he inAuence o oxygen acancies on he elec onic s uc u e o Z 02. The changes in compo- si ion and elec onic s uc u e induced in Z 02 by 3keV A + bomba dmen ha e been s udied by co e and alence-band x- ay pho oelec on spec oscopy (XPS) as epo ed in a ecen pape . The esul s showed ha he elec onic s uc u e was ai ly sensi i e o A + spu e - ing, a ea men ha p oduces emission ea u es in he band gap and o he changes in he O2p egion o he alence band (VB), which in u n we e asc ibed o he o ma ion o oxygen acancies and suboxides (i.e., educ- ion). Howe e , he ela i ely low pho oemission c oss sec ion o he VB p e en ed any de ini i e conclusions om being d awn as o he elec onic s uc u e o he s oichiome ic and A +-bomba ded solid and o he A +-modi ied su ace. The phenomenon o RPES in ansi ion me als and hei compounds has been he subjec o many ecen in- es iga ions. Ala ge esonance in he dpho oion- iza ion c oss sec ion is known o occu a pho on ene gies close o he h eshold o ap~d ansi ion. The eso- nance p ocess is usually explained as being due o he in- e e ence be ween he di ec pho oemission p ocess and au oioniza ion o ahighly localized exci ed s a e c ea ed by pho oabso p ion. Simila e ec s a e ound o he alence bands o TMO's e en when hose ha e a o mal dcon igu a ion: I is assumed ha he esonance is due o hyb idiza ion be ween he 02p and ca ion do bi als. In ac , RPES is used ex ensi ely as ame hod o isola e he d-s a e con ibu ion and o unde s and he VB s uc- u e o ansi ion-me al compounds and o he complex hyb idized sys ems. Fo ade ailed discussion he eade is e e ed o he e iew by Da is and he book by Hen ich and Cox. S udies o he esonan phenomenon i sel a e also in e es ing since he de ails o he esonance in some compounds a e no ully unde - s ood. Fo example, ex a esonances no di ec ly ela ed o he me al ds a es ha e been ecen ly obse ed in Ti02 (Re . 37) and MoS2, bu asa is ac o y explana ion has no ye been pu o wa d. In his pape we desc ibe aPES and RPES s udy o Z 02 hin ilms be o e and a e A + bomba dmen aimed a ob aining abe e unde s anding o i s alence- band s uc u e and o he changes induced by A + bom- ba dmen . In Sec. II we desc ibe some expe imen al de- ails and he sample p epa a ion. In Sec. IIIAwe p esen acompa ison o he expe imen al da a wi h he calcula ed densi y o s a es (DOS) o ob ain a eliable pic- u e o he alence-band s uc u e. The RPES s udy o he Z Q& alence band is p esen ed in Sec. IIIB. Ap e- limina y accoun o some o hese esul s appea ed else- whe e. 'Sec ion IIICis dedica ed o he e ec s induced by A + bomba dmen . In Sec. IIIDwe p esen and dis- cuss he RPES da a om ahighly educed su ace (i.e., Z O„) ob ained by A + bomba dmen o he o iginal su - ace. Asumma y and he conclusions a e p esen ed in Sec. IV. II. EXPERIMENTAL DETAILS Apolyc ys alline Z oil o 99.98%%uo pu i y om Good- ellow Me als has been used h oughou his wo k. The oil was subjec ed o he usual cleaning p ocedu es by insing in ace one, e hanol, and dis illed wa e be o e i was in oduced in o he UHV chambe . The su ace was hen cleaned by A + spu e ing and annealed unde he condi ions p e iously desc ibed in o de o a oid seg e- ga ion o impu i ies which hinde he oxida ion. The mally g own Z 02 hin ilms we e ob ained by hea - ing he oil a -450 K o longe han 30 min in an oxy- gen a mosphe e (I'o — 10 To ). In some cases, a e long pe iods o subsequen exposu e o he esidual gas some OH adso p ion was obse ed, bu could be easily e- mo ed by hea ing a 373 K o sho pe iods. In o de o induce su ace de ec s and changes in s oichiome y he sample was bomba ded wi h A + ions using an ion gun ope a ed a 0.5and 2keV and cu en densi ies o — 1pA cm The pho oemission expe imen s we e pe o med on he TGM3 monoch oma o a he Be lin synch o on adia- ion sou ce (BESSY) using pho on ene gies be ween 30 and 70 eV. A hese ene gies he escape dep h o he pho oelec ons is expec ed o be less han 10 A. The angle o incidence o he p-pola ized ligh was 45 wi h espec o he sample no mal. The spec a we e eco ded a no mal emission wi h an ADES-400 elec on ene gy analyze . The o e all esolu ion (monoch oma o + spec ome e ) was ypically 600 meV. O e iew spec a we e measu ed in he cons an - e a ding- a io mode, whe eas he alence-band spec a in he 0~E~ ~14 eV binding-ene gy ange we e aken in he cons an - analysis-ene gy mode wi h apass ene gy o 20 eV. Fo a mo e de ailed desc ip ion o he monoch oma o he eade is e e ed o he BESSYuse 's handbook. All he alence-band spec a p esen ed in his pape ha e been no malized o he pho on Aux as measu ed a a gold mi o a he en ance o he spec ome e chambe . In mos cases abackg ound has been sub ac ed om he spec a using s anda d me hods. III. RESULTS AND DISCUSSION A. Elec onic s uc u e o Z O& Figu e 1shows an o e iew spec um o he mally g own Z Oz eco ded a h =50 eV. The spec um shows he Z 4p double a 30.6eV, he b oad 02s peak a 21.7eV, and he alence band peaked a 5.3eV wi h a clea ly dis inguishable shoulde a highe ene gies. The binding ene gy is e e ed o he Fe mi le el o me allic zi conium. Figu e 2shows he 0— 14 eV binding-ene gy (E~) ange measu ed wi h h =35 eV. Fo compa ison we ha e in- cluded he o al densi y o s a es, as well as he pa ial ox- ygen and zi conium densi ies o s a es, calcula ed by So i- ano e aI. o cubic zi conia using he LSW me hod. The calcula ed DOS was ob ained in e ms o he Z and 02p pa ial DOS's weigh ed acco ding o hei espec- i e c oss sec ions. Fo amo e de ailed desc ip ion o his p ocedu e see Re . 8. The o e all shape o he expe - imen al cu e is well explained by he calcula ed bulk DOS. The alence band exhibi s wo dis inc s uc u es a -9and -6eV binding ene gy, which acco ding o he 52 EI.ECTRONIC STRUCTURE OF STOICHIOMETRIC AND A +-. . . 11 713 I) 12 10- Z 02, hu=508V EF 8- I— (0 Z4- LLI I— Z2- 0- I 50 IIIII 40 30 20 10 BINDING ENERGY (eV) FIG. 1. Pho oemission spec um measu ed a h =50 eV om s oichiome ic Z 02. ES os 0- I— GO Z UJ I— Z band s uc u e calcula ion co espond o he bonding O 2pc and nonbonding 02pm. o bi als, espec i ely, and con ain an impo an zi conium con ibu ion. The Z con ibu ion is mo e signi ican in he highe -binding- ene gy egion, whe e he bonding 02p o bi als a e ex- pec ed o ha e ala ge admix u e o Z o bi als, and il- lus a es he impo ance o he co alen in e ac ion (es- ima ed o be abou 24%) in he bonding o Z 02. The wid h o he alence band is es ima ed o be -4.8eV om he ene gy sepa a ion o he poin s o maximum slope on each side o he band. The alence-band max- imum (VBM) is loca ed a — 3.8eV below he Fe mi le el as de e mined by ex apola ion o he angen on he low-binding-ene gy side o he 02p band. This alue is in good ag eemen wi h ha de e mined by o he elec- on spec oscopies" and op ical gaps epo ed in he li e a u e. ''" Apa om he almos classic calcula ion o Mo inaga, Adachi, and Tsukuda based on adisc e e a ia ional (DV) Xa clus e me hod, a ious o he a emp s ha e been made o s udy he elec onic s uc u e o Z O2. Us- ing he linea -mu in- in-o bi als (LMTO) me hod Med ede a e QI. ha e de e mined he ene gy band s uc u es o Z 02 and o he TMO's in o de o in es i- ga e ends in he band gap and cohesi e ene gy. The band s uc u e o cubic and e agonal zi conia ha e been calcula ed by Jansen using densi y- unc ional heo y. The s uc u al and elec onic p ope ies o cubic and e agonal zi conia we e also explo ed by O lando e al. using ape iodic ab ini io Ha ee-Fock me hod. Zan- diehnadem, Mu ay, and Ching pe o med calcula ions o he h ee s able phases o Z 02 (i.e.,monoclinic, cu- bic, and e agonal) using he o hogonalized linea com- bina ion o a omic o bi als (OLCAO) me hod, and con- cluded ha he bonding is e y simila o he h ee c ys- al s uc u es wi h only mino di e ences in he wid h o he band and he band gap. In addi ion o he gene al good ag eemen a esul common o all hese calcula ions is he exis ence o an impo an co alen bonding con i- bu ion, which has been con i med expe imen ally wi h 0 ls x- ay abso p ion spec oscopy' (XAS) and esonan pho oemission. '" Ade ailed discussion o hese calcula- ions and hei compa ison wi h o he app oaches as well as wi h expe imen al pho oemission (PES) and b emss ahlung isoch oma (BIS) spec a can be ound in Re s. 8and 13. We no e ha he pho oemission in ensi y o he PES spec a epo ed he e does no all o ze o wi hin he band gap e en o he eshly p epa ed su ace. Weak emission in he band gap ex ends om he op o he alence band up o he Fe mi le el, showing amaximum a Ez =2.5eV. An expanded iew o hei con ibu ion is shown in Fig. 2. Usually, such bands a e asc ibed o apped elec ons in oxygen acancies and o he su ace de ec s' caused by he p epa a ion me hod used (i.e., hea ing a low oxygen p essu es). Howe e , by means o asel -consis en sca e ed-wa e me hod, Sobole e al. ha e p edic ed ha oxygen acancies in pe ec Z 02 c ys als a e expec ed o cause apped elec ons in local s a es wi hin he gap a binding ene gies be ween 1.5and 2eV, in good ag eemen wi h he band obse ed in his s udy. Ap e ious XPS s udy has quan i ied his e ec gi ing an elec on su ace densi y o 6X 10' cm which is equi alen o amonolaye o oxygen acancies. I will be shown below ha he in ensi y o his ea u e can be subs an ially inc eased by ion bomba dmen . B. Resonan pho oemission in Z IO2 Dos os 14 12 10 86420 BINDING ENERGY (eV) FIG. 2. Calcula ed bulk DOS (solid line) (see ex and Re . 8 o de ails) and expe imen al alence-band pho oemission spec- um (poin s) a h =35 eV o s oichiome ic Z O2. Lowe cu es: Calcula ed Z and 0pa ial densi ies o s a es (Re . 8). The p ocess o esonan pho oemission has been ex en- si ely used as ame hod o isola ing he ca ionic con i- bu ion o he alence band o ansi ion-me al com- pounds. The ene gy dis ibu ion cu es (EDC's) om he alence band o Z 02 we e hus measu ed a pho on ene - gies be ween 30 and 70 eV as shown in Fig. 3. They indi- ca e ha he ela i e in ensi ies o he wo ea u es ob- se ed in he alence band a e e y sensi i e o he pho- on ene gy due o a esonance p ocess associa ed wi h he Z 4p h eshold. Al hough he esonance mani es s i sel C. MORANT e al. III'LII'III'I'II Z 02 Eh(eV) F70 10- a) Z 02 EF 60 50 5- 45 42 40 39 38 36 33 30 ~iIII l 14 12 10 86420-2 BINDING ENERGY (eV) FIG. 3. Valence-band pho oemission spec a o Z 02 as a unc ion o he pho on ene gy. o e he whole alence band a pho on ene gies be ween 36 and 50 eV, he 02p bonding egion on he high- binding-ene gy side o he alence band is enhanced a pho on ene gies a ound 39 eV. In he case o he spec- um aken a h = 30 eV he unusually high in ensi y o he gap s a es is due o he con ibu ion o he Z 4p co e le els exci ed wi h second-o de ligh . In o de o s udy sepa a ely he beha io o he bond- ing and nonbonding con ibu ions o he alence band, we ollowed ap ocedu e p e iously used by Zhang, Jeng, and Hein ich in hei s udy o esonance e ec s in Ti02. Acco ding o hese au ho s he alence-band spec a can be analyzed in e ms o h ee Gaussians, labeled "bond- ing, ""nonbonding, "and "o e lapping, " he wid hs and ene gies o which a e summa ized in Table I o he whole se ies o spec a. A ypical i is shown in Fig. 4(a) o he VB spec um measu ed a h =50 eV. Ob iously he high- and he low-binding-ene gy componen s in ol e p edominan ly he bonding and nonbonding o bi als, e- spec i ely, whe eas he componen labeled "o e lapping" helps o ge abe e i o he alence band. Amo e quan i a i e insigh in o he esonance e ec s TABLE I. Bes - i pa ame e s binding ene gy (Eb) and ull wid h a hal maximum (FWHM) o he line shape o he alence band a di e en pho on ene gies. Th ee and wo Gaussians we e used o Z 02 and Z O, espec i ely. The mean, s anda d de ia ion (SD), and median alue a e gi en o each pa ame e . 0- LU Z10- 0- I'I'I'I'1'I'II 14 12 10 86420-2 BINDING ENERGY (eV) FIG. 4. Analysis o he alence-band pho oemission spec- um a h =50 eV using h ee and wo Gaussians o Z O& (a) and Z O (b), espec i ely. can be gained by in eg a ing he a eas associa ed wi h he di e en componen s o he alence band and hus gen- e a ing spec a equi alen o he usual cons an -ini ial- s a e (CIS) cu es. The pho on ene gy dependence o he o al in ensi y o he alence band has hus been depic ed in Fig. 5 oge he wi h ha o he in ensi y o he bond- ing, nonbonding, and o e lapping componen s and o he emission band in he gap. The p o iles a e a he com- plex and qui e unlike he ideal Fano-like cu es. In he case o he o al alence-band in ensi y (cu e a) he p o61e is cha ac e ized by a ise a 36 eV wi h amax- imum a h =39 eV, and by asecond b oad maximum a ene gies be ween 45 and 50 eV. The in ensi y o he bonding componen (cu e b) eaches he main maximum I'I'I'I'I'I'I'I'I e 35— 30- 25- N20— I— 15 -~ 10- Eb {eV) Mean SD FWHM {eV) Median Mean SD Median 0- Bonding 8.74 Nonbonding 5.67 O e lap 7.14 Bonding 8.63 Nonbonding 6.51 0.06 0.07 0.07 0.09 0.20 Z 02 8.75 5.68 7.15 Z O 8.65 6.60 2.32 2.09 1.89 2.53 2.57 0.05 0.03 0.01 0.07 0.04 2.31 2.10 1.89 2.57 2.57 IIiIiI~I I I IiIsI 30 35 40 45 50 55 60 65 70 PHOTON ENERGY (eV) FIG. 5. Pho on ene gy dependence o he in eg a ed in ensi y o he o al alence-band emission (0) {cu e a) and o he band-gap emission {0)(cu e e) as well as o he bonding (A) (cu e b), nonbonding (0)(cu e c), and o e lapping (Q) (cu e d) componen s. 52 ELECTRONIC STRUCTURE OF STOICHIOMETRIC AND A +-. . . 11 715 a app oxima ely 39 eV ollowed by ab oad pla eau which ex ends up o 50 eV. On he o he hand, he eso- nance p o ile o he nonbonding componen (cu e c) con- sis s o asmall bump a 39 eV and ag adual ise up o -50 eV o all o a highe ene gies, so ha in his case he maximum enhancemen o he in ensi y is p oduced a pho on ene gies a ound 45— 50 eV. The o e lapping componen (cu e d) shows no clea e idence o esonan beha io , bu shows a he cons an in ensi y up o 50 eV pho on ene gy. The p o ile co esponding o he s a es in he band gap (cu e e) sugges s aweak esonance a 39 eV, bu because o he low in ensi y and possible e o s in he backg ound sub ac ion p ocedu e an unambiguous cha ac e iza ion is di icul . The lack o asys ema ic pic- u e in he obse a ion o he wo esonances (i.e.,a 39 and 50 eV) may be linked o he ac ha none o he peaks used in he i ing p ocedu e ac ually co espond o pu e bonding o pu e nonbonding o bi als. In o de o ollow he changes obse ed in he alence-band shape in ameaning ul way, i is use ul o compu e he 39/36 eV di e ence spec um by sub ac ing he EDC measu ed a 36 eV (o esonance) om ha measu ed a 39 eV (on esonance). The esul is labeled b in Fig. 6. The cu e labeled aco esponds o an XPS alence-band spec um (i.e.,h = 1253.6eV) om Re . 26. Fo compa ison we ha e included se e al cu es la- beled om c o which ep esen he Z and 0PDOS's ob ained by di e en me hods. Cu es cand a e he calcula ed Z and 02p pa ial densi y o s a es, espec- i ely (see Fig. 2) scaled by he ela i e pho oemission c oss sec ions a h = 1253.6eV. Since he Z 5s and Z 5p con ibu ions a e negligible, we will use cu e c o ep esen he Z 4d densi y o s a es. Cu es dand ea e in ended o ep esen he 02p densi y o s a es. Cu e d I'I'I'I'I'I'I'I'I Z 02 a) XPS Z 4d b) c) 02p d) I'I'I'I'I'I'I'I'I 14 12 10 86420-2 BINDING ENERGY (eV) FIG. 6. Cu e a: XPS spec um o he alence band om s oichiome ic Z 02. Cu e b: Z 4d con ibu ion o he alence band as de i ed om he esonance a h =39 eV. Cu e c: Calcula ed Z pa ial densi y o s a es ( om Re . 8). Cu es d : 02p con ibu ion — o he alence band as de e - mined om (cu e d) pho oemission a h =70 eV, (cu e e) he XPS spec um (a) a e sub ac ion o ib), and (cu e Pelec- onic s uc u e calcula ions (Re . 8). is he alence band o Z 02 measu ed a h =70 eV (see Fig. 3), which is expec ed o e iec he 02p PDOS since he a io o he 02p and Z 4d pho oemission c oss sec- ions is &30 a ha pho on ene gy. "Cu e eis he e- sul o he sub ac ion o he Z con ibu ion as ep esen ed by spec um b om he expe imen al XPS alence band (i.e.,cu e a) (see de ails below). Resonan pho oemission o he Z 4d s a es in Z 02 is expec ed o occu when he pho on ene gy is uned o e he Z 4p ~48 ansi ion ene gy a — 31 eV. The 4p~4d ansi ion c ea es an exci ed s a e [Z 4p 4d']' which emains highly localized on he ca ion si e. The exci ed s a e can hen elax in adi ec ecombina ion p ocess which in ol es he Z 4d s a es pa icipa ing in he alence band; i.e.,[Z 4p 4d 'VB"]~Z 4p 4d VB" '+e, which is he same inal s a e as in con en ional pho oemission. In his manne he e is a possible in e e ence be ween bo h p ocesses, gi ing ise o he esonan enhancemen o hose pa s o he spec- um wi h an impo an ca ionic cha ac e . In he p esen s udy Fig. 6clea ly demons a es ha his is he case o he esonance obse ed a h =39 eV. The good ag eemen exis ing be ween he 39/36 eV di e ence spec- um, cu e b, and he calcula ed Z 4d PDOS, cu e c, clea ly con i ms ha he phenomenon can be used o iden i y he Z -de i ed s a es in he alence band. Fu - he mo e, he di e ence spec um bp o ides expe imen- al e idence ha he pa ial co alen cha ac e o he Z - 0bond is la ge in he bonding egion han in he non- bonding pa o he alence band. The e o e, he bonding con ibu ion should esona e mo e s ongly han he non- bonding one in good ag eemen wi h he expe imen al ob- se a ion (see Fig. 5). The esonance a h =39 eV is hen consis en wi h he esonan pho oemission o he Z 4d s a es and wi h he assump ion o apu e in a-a omic elaxa ion o he exci ed s a e. I is impo an o men ion he e ha he esonan pho- oemission o he ds a es a 39 eV occu s a an 8.4eV highe ene gy han he Z 4p binding ene gy (E~=30.6 eV) as measu ed by pho oemission (see Fig. 1). Simila delays be ween he h eshold (Z 4p binding ene gy) and he esonance ene gies ha e also been obse ed in me al- lic Z (— 10 eV), 'as well as in he zi conium ni ides Z N (— 10 eV), and Z 3N4( — 11.5eV), and seem o be acommon obse a ion in he ligh e ansi ion me als and hei compounds. In gene al, he binding ene gy o he [4p 4d "+' ]*exci ed s a e measu ed om esonan pho oemission p o iles ag ees well wi h he esul s o o h- e measu emen s such as op ical abso p ion o elec on- ene gy-loss spec oscopy (EELS). Fo Z 02, he Z 4p co e losses ha e been shown o exhibi amaximum in en- si y a ound 42 eV,"in easonable ag eemen wi h he ene gy measu ed by esonan pho oemission. Figu e 6also allows he compa ison be ween he spec- um assigned o he Z 4d s a es and he alence-band spec um ob ained by XPS. In e es ingly, i is obse ed ha he XPS spec um is mo e in ense a ound he op o he alence band (i.e., he nonbonding egion). Clea ly his is due o he 02p-de i ed s a es, because he ca ionic con ibu ions om Z 5s and Z 5p s a es a e negligible. The O2p s a es canno be neglec ed: al hough hei c oss 11 716 C. MORANT e al. 52 sec ion a XPS ene gies is ou imes lowe han ha o he Z 4d o bi als, he much la ge 02p pa ial DOS compensa es. We ha e a emp ed o ex ac he 02p con ibu ion om he expe imen al XPS alence band by sub ac ing he Z 4d con ibu ion de e mined by eso- nan pho oemission. The esul is labeled as ein Fig. 6 and shows good ag eemen wi h he calcula ed pa ial 0 2p densi y o s a es depic ed in he same igu e as . This ag eemen is no su p ising because he di e ence was ob ained by sub ac ing ap ope ly scaled di e ence spec um, o which he scaling ac o was de e mined by ap e ious i ing o he expe imen al XPS alence band in e ms o he calcula ed pa ial densi ies o s a es and he espec i e c oss sec ions as abula ed by Yeh and Lin- dau, so ha he ela i e 02p/Z 4d con ibu ions o he alence band we e de e mined acco ding o heo e i- cal calcula ions. A p esen we do no ha e asa is ac o y explana ion o he b oad esonance occu ing a an ene gy nea 50 eV. Recen ly, Heise and co-wo ke s ''pe o med a RPES and pho oelec on di ac ion (XPD) s udy o he TiOz(110) su ace o de e mine he Ti 3d and 02p alence-band pa ial densi ies o s a es. The RPES e- sul s show di e en displacemen s o he esonance maxi- Ina o di e en ea u es o he VB, which he au ho s sugges a e associa ed wi h di e en symme y- esol ed ini ial and inal s a es, al hough he de ails o he assign- men emain unclea . Assuming apu ely in a-a omic di ec ecombina ion mechanism, he esonance could be associa ed wi h ansi ions o he Z 4p — +Z 5sp ype, whe e a4p elec on is exci ed in o he emp y 5sp band al- lowing a esonance wi h he ca ionic Z 5s s a es in ol ed in he alence band o Z 02. Ob iously, he Z 5p s a es should no play any ole since ansi ions 4@~5p a e di- pole o bidden. In ac , his mechanism was p e iously used o explain ex a esonances in RPES expe imen s on Ti02 (Re . 37) and MoSz. The p o ile o he esonance indica es ha in ha case he [Z 4p 5s']* exci ed s a e lies 9eV abo e he [Z 4p d']* s a e, in good ag eemen wi h p e ious XAS expe imen ' which loca e he Z 5' band -9eV abo e he emp y dband. Howe e , he cal- cula ed Z 5s PDOS does no appea o be in ense enough o gi e ise o he obse ed enhancemen . Un o una ely, he EELS spec a o Z 02 do no show any dis inguish- able ea u e which could be associa ed wi h he esonance a 45 eV; hus ei he he co esponding exci ed s a e is no a ailable wi h EELS o he exci a ion c oss sec ion is e y low. C. A + bomba dmen e ec s Figu e 7shows alence-band spec a in he 0— 14 eV binding-ene gy ange, aken a h =39 eV (i.e.,on eso- nance), o he ini ial Z Oz su ace (lowes cu e) and a e a ious deg ees o A + bomba dmen . In addi ion, he band-gap egion (4 eV ~EiI ~0) a e sub ac ion o he main O2p alence band is displayed on an expanded scale on he igh -hand side o Fig. 7. The igu e clea ly shows ha he elec onic s uc u e o Z O2 is sensi i e o bomba dmen wi h A + ions o 2keV and ha he spec- oscopic changes in oduced by low-ene gy spu e ing 2keV A + Z 02 15 Spu e ing ime (min. )I EF ','.EF I ~, I~ I0 I I I .i I 130 i~'~— 50 Ie ~~ ~~ i l —13 ~~ ~~ j 0 I~IcI~giIaI~II~II, I 10 505432 10-1-2 BINDING ENERGY (eV) FIG. 7. Pho oemission spec a (h =39 eV) o he alence band o Z 02 (le ) and band-gap emission on an expanded scale ( igh ) as a unc ion o he spu e ing ime wi h 2keV A + ions. begin o appea immedia ely upon bomba dmen . The spec a ob ained om a esh Z 02 su ace as well as a e he i s h ee minu es o spu e ing exhibi a b oad s uc u e o cons an shape in he band gap, he in- ensi y o which inc eases wi h spu e ing ime, and whose shape emains unchanged. I s emission maximum is ound a E~=2.5eV and i s o igin was explained in Sec. IIIAin e ms o oxygen acancies. A highe A + doses he s uc u e is obse ed o de elop wo addi ional ea u es a ound 1.7and 3.7eV which also g ow upon u - he A + bomba dmen . In o de o ollow he di e en ea u es sepa a ely he emission in he band gap was i s analyzed by accoun ing o he b oad emission a 2.5eV. Di e ence spec a we e gene a ed by emo ing he maximum possible con ibu- ion o he o iginal s uc u e (i.e.,0min) om he spec a a di e en spu e ing imes, so ha he o he wo ea u es could be clea ly dis inguished. These di e ence spec a a e displayed in he inse o Fig. 8labeled wi h he scaling ac o Fwhich was used o each spec um. Abo e 3min spu e ing ime (i.e.,— 1X10' ions cm ) wo peaks a 3.8and 1.2eV can be clea ly dis inguished, and hei g ow h can be ollowed as he spu e ing p o- cess p oceeds. The in eg a ed in ensi ies o he espec i e ea u es ha e been depic ed in Fig. 8as a unc ion o he spu e ing ime, oge he wi h he o al in ensi y o he emission band in he gap. The in ensi y o he whole emission band induced by A + ions o 0.5keV has also been included o compa ison. The igu e shows ha he in ensi ies o he di e en ea u es and o he whole emis- sion band inc ease p og essi ely un il as a iona y s a e is eached o spu e ing imes abo e 60 min (i.e.,2.2X10' ions cm ). Wha is he o igin o he h ee di e en gap emissions which can be p oduced by A + bomba dmen ? The i s ype is he b oad emission a 2.5eV binding ene gy, 52 ELECTRONIC STRUCTURE OF STOICHIOMETRIC AND A +-. ..11 717 M8 7- Cg ~6- I— M5- Z'. LLI I— Z' (0 I—3- 0 UJ LL 2 Cl Spu enng Time (min. )."'. E, F 130 '.: !' ~~3.S IS .-' 2.3 0)~- 14 e4 2 0-2 ~BINDING ENERGY (e ) ke I— ( ) LLj ~0 0 o eo ~o eo 10 ~3 I 0~ oe 0~ o~ oe .. 'Z 02 b o~ 0'I 0~ I'I'I'I'I'I'I'I'I 14 12 10 86420-2 BINDING ENERGY (eV) 0- 50 100 150 FIG. 9. Valence-band pho oemission spec a om bo h s oichiome ic Z 02 and educed Z O measu ed a h =39 eV. SPUTTERING TIME (ITiin) FIG. 8. In ensi y o he band-gap emission as a unc ion o he spu e ing ime wi h 2keV (~)and 0.5keV (0) A + ions. Fo 2keV A + ions he in ensi ies o h ee di e en con ibu- ions a 1.2eV (V), 2.5eV (o), and 3.8eV (4) ha e been in- cluded. Inse : band-gap emission a e sub ac ion o he spec- um a 0min scaled wi h a ac o F. which o ms a e any deg ee o educ ion o he su ace and is p esen e en on a esh Z 02 su ace. I has been assigned o elec ons apped on oxygen acancies ha popula e he 4d o bi als o adjacen Z a oms. The nea- su ed ene gy o his band is in good ag eemen wi h he calcula ions by Sobole e al. using asel -consis en sca e ed-wa e me hod. Fu he mo e, Munnix and Sch nei s' ha e also shown ha an emission band a ound 1.3eV obse ed in Ti02 could be accoun ed o by sub- su ace oxygen acancies. In ac , i seems o be agen- e al inding in TMO's ha oxygen acancies induce elec- onic s a es in he band gap. ' A highe A + dose he inc ease in he concen a ion o oxygen acancies p oduces mo e complex de ec s uc- u es and e en signi ican changes o s oichiome y. This is p obably he o igin o he wo sha p ea u es ob- se ed only a e hea y educ ion o he su ace (i.e., high-de ec -densi y su aces). The high-binding-ene gy ea u e a 3.8eV we assign o bulk Z -0 acancy com- plexes associa ed wi h he o ma ion o lowe oxida ion s a es (i.e.,Z +, Z +). Fu he mo e, he band can be ela ed o an op ical abso p ion a 3.31 eV obse ed in cubic zi conia and a ibu ed o six old-coo dina ed Z + by Azzoni and Palea i using elec on pa amagne ic eso- nance. In con as , he weakes band obse ed a 1.2 eV equi es s ill hea ie educ ion o be unambiguously dis inguished. I is en a i ely asc ibed o he o ma ion o small clus e s o Z + and e en Z in he limi ing species o he spu e ing p ocess when A + bomba dmen p oduces much highe de ec densi ies, and mo e elec- ons popula e he Z 4d o bi als. In ac , he o ma ion o mixed oxida ion s a es (i.e.,Z +, Z +, Z +, and Z ) has been demons a ed by XPS. The ca ionic cha ac e o all hese band-gap s a es is con i med by he esonan pho oemission spec a shown below. Al hough he mos signi ican e ec o he A + bom- ba dmen is he g ow h o he emission ea u es in he gap, he 02p alence band is also obse ed o unde go changes. Figu e 9compa es he alence-band pho oemis- sion spec a o he s oichiome ic and se e ely educed su aces. In gene al, we obse ed adec ease in he alence-band wid h and an inc ease in i s in ensi y due o he p esence o addi ional educed ca ions, which in- c ease he dcon ibu ion. The alence band maximum mo es 0.45 eV away om he Fe mi le el (i.e, band bend- ing) as aconsequence o he educ ion o he su ace. In ac , i is well es ablished ha elec ons apped in oxy- gen acancies occupy localized emp y o bi als o he ca - ions, pushing up he Fe mi le el and bending he whole elec onic s uc u e o highe binding ene gies. Figu e 10 shows pho oemission spec a o Z O a e i s exposu e o inc easing amoun s o 02 a empe a u es be ween 298 and 473 K(as labeled). The igu e shows a he clea ly ha an oxygen exposu e o 100 La 298 K causes asigni ican dec ease in he in ensi y o he gap s a es. On he con a y, p ac ically no change is ob- se ed in he shape o he 02p band. Only a e expo- su es abo e 300 La 423 Kdoes he alence-band spec- um eco e he shape o ha o Z 02. Thus, al hough gene a ion o s a es in he band gap and modi ica ion o he alence-band shape occu simul aneously du ing A + bomba dmen , he second e ec emains e en a e emo- al o he oxygen acancies by 02 adso p ion a low em- pe a u es. This ac sugges s ha he shape could be e- la ed o he amo phiza ion and loss o he h ee- dimensional o de o Z 02 by A + bo nba d nen . Fu - he mo e, acco ding o hese esul s he modi ied s uc- u e cha ac e ized by ahighe co alency (see below) is p ese ed un il he s uc u e is annealed abo e 423 K. In o de o obse e any possible inAuence om he ion ene gy we pe o med asimila de ailed s udy o he e ec s induced by 0.5keV A + ions. The e ec s a e qual- i a i ely e y simila o hose discussed abo e o 2keV A + ions, bu no so in ense. A e asimila spu e ing ime we obse ed ha he s eady s a e eached a 0.5keV consis s o an al e ed laye wi h conside ably ewe de- ec s han ha ob ained by spu e ing wi h 2keV A + ions (Fig. 8). In he ollowing esonan pho oemission ex- pe imen s on he educed su ace using 0.5keV ions a e desc ibed. 11 718 C. MORANT e al. ~I~III~I~I~I~ EF +100 L02 473K ~4 +100 L02 423K +100 L02 298K A ' 2keV I'I'IIII'I 14 12 10 86420 BINDING ENERGY (eV) ~I FIG. 10. Pho oemission spec a (h =39 eV) o he alence band o Z O (2 keV A + ions) a e oxygen exposu e a in- c easing empe a u es. D. Resonan pho oemission o Z O„ Figu e 11 shows an o e iew pho oemission spec um aken a e bomba dmen wi h 0.5keV A + ions o 135 min (i.e.,s eady s a e). Compa ed wi h he spec um o Z 02 in Fig. 1 he e ec s o A bomba dmen a e clea - ly obse able in all he bands including he Z 4p, he 0 2s, he 02p, and he emission band in he gap. The Z 4p peak is b oadened, sugges ing ha Z species ha ing alence s a es lowe han 4+ a e now p esen . The Z 4p/0 2s in ensi y a io inc eases upon ion bomba dmen , con i ming he p e e en ial loss o oxygen. An es ima ion Z Ox EF h (eV)~E 'la jW~ 60 50 o he su ace composi ion in e ms o he Z 4p and 02s in ensi ies gi es an a e age s oichiome y Z O» which is in good ag eemen wi h he a e age composi ion (-Z O) o he al e ed laye caused by 3keV A + ions, as de e - mined by XPS. In Fig. 12 we show he alence-band pho oemission spec a o Z O„ in he 0— 15 eV binding- ene gy egion, measu ed a pho on ene gies in he ange 30~h ~60 eV. On he igh -hand side o he igu e, he band-gap emission has been depic ed on an expanded scale. Again, he in ensi y and shape o he gap s a es measu ed a h = 30 eV a e s ongly a ec ed by he con- ibu ion o he Z 4p co e le els exci ed wi h second- o de ligh and will no be conside ed in he quan i a i e analysis. E ec s associa ed wi h he esonan p ocess a e clea ly obse able and ha e been quan i a i ely analyzed in a simila manne o ha o s oichiome ic Z 02 in Sec. IIIB. Figu e 13 shows he dependence o he pho on en- e gy wi h espec o he in ensi y o he alence band and he emission in he band gap. Again we show he beha io o he espec i e in ensi ies o wo Gaussians la- beled as "bonding" and "nonbonding. "In his case, howe e , he alence-band spec a could be analyzed in e ms o only wo o such cu es, he wid hs and ene gy posi ions o which a e summa ized in Table I. A ypical i is shown in Fig. 4(b). The Gaussian labeled as non- bonding is assigned o he lowes -binding-ene gy co n- ponen , whe eas he bonding one has been assigned o he highes -binding-ene gy componen . The esonance p o iles o Fig. 13 show abeha io simi- la o hose measu ed o s oichiome ic Z 02. In pa ic- ula , all he p o iles a e cha ac e ized by wo maxima a ound 40 eV and 45— 50 eV. Whe eas he in ensi y o he bonding componen eaches i s main maximum a 40 eV, we no e ha he esonance p o ile o he nonbonding componen shows abump a ha ene gy ollowed by an ~10 C 8 CQ 6 g) 4- UJ z I— 0- Z O„, hU=50eV EF 15 I 10 50 45 42 41 —40 38 37 36 ~o ~'!M~+ /0 C w ~Q ) IIIII~I 54321 0-1-2 IIII I II 50 40 30 20 10 BINDING ENERGY (eV) FICx. 11. Pho oemission spec um measu ed a h =50 eV om Z O& a e bomba dmen wi h 0.5keV A + ions (135 min). BINDING ENERGY (eV) FICx. 12. Pho oemission spec a o he alence band (le ) and he band-gap emission ( igh ) om Z O„(see Fig. 11)as a unc- ion o he pho on ene gy. 52 ELECTRONIC STRUCTURE OF STOICHIOMETRIC AND A +-. . . 11 719 45— l/l 40 35— lg 30— I— 25— Z', UJ I- 20— Z'. 15— 10— 0I~I~ I ~II~I~I 30 35 40 45 50 55 60 PHOTON ENERGY (eV) FIG. 13. Pho on ene gy dependence o he in eg a ed in ensi- y o he o al alence band (~)(cu e a) and he band-gap emission (~)(cu e e) as well as o he bonding (A) (cu e b) and nonbonding (0)(cu e c) componen s. absolu e maximum a -50eV. The esonance a 40 eV is associa ed wi h he enhancemen o he Z 4d s a es in- ol ed in he alence band, while he o igin o he eso- nance a 45— 50 eV is unknown. The esonan beha io o he s a es in he band gap is mo e clea ly obse ed in his case due o he inc eased in ensi y in his spec al e- gion. The maximum a 40 eV clea ly con i ms he ca ion- ic cha ac e o hese s a es. All he p o iles show ha he esonance a 40 eV has b oadened signi ican ly compa ed wi h he sha p peak obse ed o s oichiome ic Z Oz. As in Sec. III8we calcula ed di e ence cu es in o - de o poin ou hose egions o he spec a which a e enhanced when he ene gy o esonance is eached. The esul ing cu e ob ained a e sub ac ing he pho oemis- sion spec a measu ed a 36 eV (o esonance) om ha measu ed a 40 eV (on esonance) is shown in Fig. 14. This igu e also includes he XPS alence-band spec um Z O„ XPS '~ I'I'I'I'I'I'I' 'I 14 12 10 86420-2 BINDING ENERGY (eV) FIC . 14. Z 4d con ibu ion o he alence band as de e - mined om he esonances a h =40 eV. Fo compa ison we ha e included he XPS spec um o he alence band o Z O„ om Re . 26. o Z Oz bomba ded wi h 3keV A + ions published in Re . 26. Acco ding o he in e p e a ion gi en abo e he 40/36 eV di e ence spec um should e lec he Z 4d pa ial densi y o s a es in Z O; un o una ely, he e a e no band s uc u e calcula ions o compa ison. Compa - ing wi h he equi alen spec um o Z Oz (see Fig. 6) in- dica es asigni ican inc ease in he Z 4d con ibu ion, mainly in he low-binding-ene gy egion o he alence band (i.e., he nonbonding egion), as a esul o he spu e ing. The inc ease in he ca ionic con ibu ion clea ly sugges s asigni ican inc ease in co alency due o he p e e en ial loss o oxygen a oms and he co espond- ing educ ion o he ca ion. This e ec is also con i med by compa ing he 40/36 eV di e ence cu e, labeled Z 4d in Fig. 14, wi h he XPS alence band o Z O ob- ained a e bomba dmen wi h 3keV A + ions. Con- a y o he compa ison made in Fig. 6 o Z 02, we ob- se e in he case o Z O easonable ag eemen be ween he XPS alence-band spec um and he Z 4d con ibu- ion ep esen ed by he di e ence cu e 40/36 eV. This indica es ha he 02p con ibu ion o he alence band o Z O is quan i a i ely less impo an han o Z 02. The small di e ences should be accoun ed o by he 02p con ibu ion. Acompa ison be ween he analysis o he XPS alence band o Z 02 (Fig. 6) and Z O (Fig. 14) leads o he conclusion ha whe eas he 02p componen is signi ican ly educed in in ensi y he Z 4d con ibu ion inc eases o e he wid h o he alence band bu mo e s ongly in he nonbonding egion. Al hough he ca ion- ic componen is p obably o e es ima ed, he da a indica e ha he c ea ion o oxygen acancies and he hea y educ ion o he oxide by A + bomba dmen causes a signi ican dec ease in he numbe o ionic Z -0 bonds and aconside able inc ease in co alency o he modi ied su ace. IV. SUMMARY AND CONCLUSIONS The elec onic s uc u e o he mally g own Z 02 hin ilms be o e and a e A + bomba dmen was s udied wi h esonan pho oemission spec oscopy using synch o- on adia ion. Good ag eemen has been ound be ween he alence-band spec a o he mally g own Z 02 hin ilms and he calcula ed densi y o s a es o bulk Z 02. Fo bo h s oichiome ic and A +-bomba ded Z 02 hin ilms, esonan pho oemission om he alence band was obse ed when he pho on ene gy was uned h ough he Z 4p — +4d ansi ion ene gy. A a he complex depen- dence o he o al alence-band in ensi y on he pho on ene gy was ound. The esonance p o ile exhibi s amax- imum a h = 39 eV ollowed by asecond b oad s uc u e a 45— 50 eV. The in ensi y enhancemen obse ed a 39 eV is consis en wi h he esonan pho oemission o Z 4d s a es in ol ed in he alence band. In ac , he phenomenon has been used o iden i y hose egions o he alence band wi h an impo an Z 4d cha ac e and also o es ima e he deg ee o Z 4d/0 2p hyb idiza ion. The second esonance a pho on ene gies be ween 45 and 50 eV is associa ed wi h he nonbonding egion o he alence band; howe e , i s o igin emains unexplained. In addi ion, we ha e s udied he changes ha occu in