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P r o ceed in gs of t h e XXX V I Z ako p ane Sch oo l o f Ph ysi cs, Z ak opa n e 200 1

L ocal Stat es of T ell u r iu m i n Is olate d H elic al C h ain s

J . St anek

a

, P. F o r na l

b

, S.S. H af ne r

c

an d A . Pf it zne r

d

aI nst i t ut e of P h ysi cs, Jagi ell oni an Uni versi ty of Cra cow Reym onta 4, 30-059 Cra cow, Po l and

bInsti tute of Physi cs, Techni cal Uni versi ty of Cra cow, 30-084 Cra cow, Pol and

cCenter of Ma teri al s Sciences, Uni versi ty of Ma r burg , 35032 Ma rburg , G erm any

dDepartm ent of Ino rga ni c Chem i stry , Uni versi ty of Si egen, G erm any T h e l ocal elect ro nic state of T e in the helical chains of C uX Y2 ( 1À x )T e2 x

(X = C l, Br ; Y = Se, S) w ere stu died usin g the M ossbauer sp ectroscop y of 12 5T e at 10 K and 70 K . T he isolated chains of T e in these comp ounds are less rigid than those in elemental T e. T he determined data of quadrup ol e splittin g and Debye temp erature ÈD are indicati ve of strong lo cal ordering of T e in one of the tw o non -equivalent crystallogra phi c positio ns. I t w as not p ossible to resolve crystallogra phi c positio ns by the M ossbauer spectroscopy .

PACS numb ers: 76.80. + y

1. I n t r o d u ct io n

Pro p erti es of elementa l tel l uri um , T e, such as for exa mpl e pha se tra nsform a- ti ons fro m the hexag onal semi conducti ng pha se to the m onocl i nic m etal l ic pha se at hi gh pressures, ha ve been i nterpreted i n term s of the l o cal T e b ondi ng [1]. The crysta l structure of elementa l Te [2] consists of i nÙnite hel i cal chai ns whi ch i nter- act wi th each other. Ho wever, tha t stro ng i ntera cti on between the chai ns m akes i t ra ther di £ cult to esti m ate l ocal bondi ng wi thi n the chai ns. In the present pa- p er we shoul d l i ke to di scuss some resul ts obta i ned fro m sampl es of comp ositi on of Cu+ XÀ Y2 ( 1À x )T e2 x, where X = Cl , Br ; Y = Se, S wi th the use of1 2 5T e M ossbauer spectro scopy. In these com p ounds the i nÙni te T eY hel i cal chai ns are, sim i lar to el ementa l T e, the m ain structura l elements. They are well separa ted i n these cases, b eing hel d to gether by Cu+ XÀ Cu+ bri dg es. Thi s m ay al l ow m ore di rect insi ght i nto the di sti nct l ocal el ectro ni c T e conÙgura ti on whi ch m ust l ead to the form ati on of the chai ns. Further, an i nteresti ng aspect of Cu+ XÀ Y2 (1À x )T e2 x com p ounds may

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b e the questi on of p ossibl e ato m ic orderi ng wi thi n the hel i cal chai ns o ver the T e, Y crysta l l ogra phi c p ositi ons, dep endi ng on the typ e of nearest nei ghb ours wi thi n the chai n or the typ e of connecti ng ani on X. For such study , M ossbauer spectro scopy

of 1 2 5T e m ay be an appro pri ate m etho d. X- ra y di ˜ra cti on studi es [3, 4] suggested

stro ng orderi ng of Te and Y over tw o non- equi val ent sites wi thi n the chai n.

2 . E x p er i m en t a l 2.1. Samples

The specim ens for thi s study were synthesi zed by m i xing CuCl , CuBr, T e, Se, S in appro pri ate pro porti ons and heati ng i n evacuated quartz capsul es at tem - p eratures o f ab out 300£C for few weeks [4].

Al l com p ounds b elong to the sam e structure typ e wi th the same structura l to p ol ogy. They crysta l l i ze i n the m onocl inic space group P 21= n. Pro j ecti ons of the crysta l structure are shown i n Fi gs. 1a and b. The chal cogen hel i cal chai ns are pa ra l l el to the b-axi s. They are hel d to gether by Cu { X{ Cu uni ts para l l el to the

c-axi s. There are two no n- equi val ent crysta l l ogra phi c positi ons for T e and Y :M 1

and M 2, wi thi n each chai n. These sites m ay b e di sti ng ui shed by thei r di stances to the ha l ide ani ons X or Cu. For the M 1 p ositi on the di stanceM 1{ X i s shorter tha n for M 2, whi l e for the M 2 positi on the M 2{ Cu di sta nce i s shorter tha n for

M 1. At Ùrst sight, S, Se, and Te may b e expected to enter b oth sites, M 1 as well asM . Ho wever, a previ ous study [3, 4] suggested tha t the T e ato ms pref erenti al l y o ccupy the M p ositi on.

For further di scussion three lo cal conÙgura ti ons of T e ato ms wi thi n one chai n wi l l be considered: conÙgura ti on˜ refers to Te wi th tw o other T e as nearest nei gh- b ours: { T e{ T e{ T e{ , conÙgura ti onÙrefers to Te wi th two Y as nearest nei ghb ours:

{ Y{ T e{ Y{ , and conÙgura ti on Û refers to T e wi th one T e and one Y as nearest

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nei ghb ours: { Te{ T e{Y{ . It i s to b e anti cipa ted tha t for our consi derati on of such conÙgura ti ons, i t wi l l b e i rrel evant whether the center p ositi on T e, or the nei gh- b ori ng Te, is l ocated at M 1 or M 2 site.

2.2. M ossbauer spect roscopy of1 2 5Te

M ossbauer spectro scopy of1 2 5T e i s ba sed on resona nt a bsorpti on of 35.48 keV

Û ra di ati on whi ch results fro m the decay of the Ùrst exci ted nucl ear sta te,

I = + 3 = 2, to the gro und sta te, I = +1 = 2. The rel ati vely hi gh energ y of the tra n- siti on requi res usual l y m easurem ent at l ow tem pera tures. The m ain di sadva ntag e

of 1 2 5T e spectro scopy i s the rel ati vel y bro ad na tura l l i ne wi dth À = 5 :0 2 m m/s

at hal f m axi mum of the resonant absorpti on. Theref ore, ra ther \ p oor resol uti on "

i s expected. G eneral l y,À i s a few ti m es l arg er tha n the ra ng e of observed i som er shi fts, £. It i s about 3 ti mes sm al l er tha n the la rgest nucl ear qua drup ole spli tti ng,

 , rep orted so far. A comprehensi ve revi ew on 1 2 5T e M ossbauer spectro scopy i s presented i n [5]. In the fol l owing a few poi nts rel evant to the experi m ents rep orted here are describ ed.

As source m etastabl e1 2 5 mT e was used. A Mg31 2 4T eO6 m atri x was acti vated at the Ha hn{ Mei tner- Insti tut Berl i n f or 10 da ys i n a neutro n Ûux of 2È 10 neutro n= s cm . D ue to the hi g h Debye tem p erature, È , of Mg TeO [6], i t was p ossibl e to observe resona nt absorpti on wi th source hel d at ro om tem p era- ture. The absorbi ng sam pl e wa s m oun ted i n a gas-Ûow cryo sta t. For the detecti on of the 35.48 keV ra di ati o n, a germ ani um detecto r of hi ghest puri ty was used. Al - terna ti vely, a pro p orti onal counter coul d al so b e empl oyed, regi steri ng the \ escap e p eak" . The powdered absorb ers were pressed to pel l ets whi ch po ssesseda di ame- ter of 1.0 cm and conta i ned 20 m g of na tura l tel l uri um p er cm2 i n each case. The e˜ecti ve absorb er thi ckness, t , cal culated f or o ne absorpti on li ne, wast 0:5 at 10 K and t 0:2 at 70 K, obta i ned wi th the use of È as determ i ned (see secti on b elow). Thus, the appro xi mati on of thi n absorb er coul d b e appl i ed for the eval uati on of the data .

3. R esu l t s

Sp ectra of al l sam pl es were recorded at 10 K and 70 K. They exhi bi ted the typi cal nucl ear qua drup ol e-spl i t do ubl et as shown i n Fi g. 2. The hyp erÙne pa ra meters such as i som er shift £ ref erred to Mg T eO at 295 K, qua drup ole spl itti ng Â, l i ne wi dth À, and resona nt absorpti on areaA are col l ected i n T abl e.

The £ val ues were found to b e the sam e for al l the sam pl es wi thi n the exper- i m enta l erro r. For the CuCl Se2 (1 )T e2 series exhi bi ted a signi Ùcant decrease wi th i ncreasingx as shown i n Fi g . 3. For CuCl ST e i s the same as for CuCl SeTe whi l e for CuBrST e i s substanti al l y smal l er. It i s i nteresti ng to no te tha t the Â

val ues di d no t change b etween 1 0 K and 70 K. However,À showed a t 10 K as well as at 70 K the sam e typi cal bro adeni ng wi th respect to i ts na tura l val ue.

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Fig. 2. M ossbauer spectra of 125 T e in CuC lSe2(1 À x )T e2 x. U pp er spectrum (x = 1) at 10 K (lef t) and at 70 K (right), low er spectrum (x = 0 : 2 5) at 10 K (lef t) and at 70 K (right). N ote the increased quadrup ol e splitting  w ith decreased f raction of T e. T he decreasing intensity w ith increasing temp erature is more pronounced f or the sample richer in T e.

Fig. 3. Dep endence of the quadrup ol e splitting  on x in C uC lSe2(1 À x )T e2 x. O pen circles ref er to the exp erimental data of T able. T he solid line is the dependence predicted assuming statistical distributi on of Se, T e over and . T he dashed line refers to complete ordering of T e into or .

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T AB L E

125 T e M ossbauer data of Cu+XÀ Y2(1 À x )T e2 x, X = Cl, Br; Y = S, Se.T

| temp erature, £ | isomer shif t referred to Mg3T eO6 source at 293 K , Â | nuclear quadrup ole splitting, À | f ull width at half maximum of the resonant absorption, A | resonant absorption area, ÈD | Debye temp erature.

T £ Â À A ÈD

[K ] [ mm /s] [mm/s] [mm/s] [K ]

C uC lST e 70 1.7(2) 11. 2(2) 6.4( 5) 19. 8 132 10 1.7(1) 11. 4(1) 7.3(2) 49. 2

C uBrST e 70 1.7(1) 10. 0(2) 7.9(4) 23. 6 138 10 1.7(1) 10. 5(1) 8.4(2) 53. 5

C uC lSe2(1 À x )T e2 x

x = 1 70 1.7(1) 9.6(2) 6.2(3) 17. 4 138

10 1.7(1) 9.6(1) 6.9(2) 39. 6

0.8 70 1.6(1) 9.6(2) 6.9(4) 19. 4 138

10 1.6(1) 9.6(1) 6.9(2) 43. 6

0.5 70 1.7(1) 11. 6(1) 7.5(3) 24. 0 148

10 1.7(1) 11. 5(1) 7.2(2) 47. 8

0.25 70 1.8(1) 11. 1(2) 6.4(4) 23. 9 147

10 1.7(1) 11. 1(1) 6.6(2) 48. 1

Fig. 4. Dep endenc e of the ratio of 125 T e recoil- f ree f raction 70 K 10 K on the Debye temp erature ÈD used for determination of ÈD values plotted in Fig. 5.

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The com pa ri son of the resonant absorpti on area, A, of the spectra mea- sured at two di ˜erent tem p eratures i n i denti cal geom etry al l owed determ i na ti o n of the Debye tem p erature ÈD for each sampl e. The cal cul ated rati o of

A ( T = 7 0 K)/ A ( T = 1 0 K) as functi on of ÈD for 1 2 5T e i s shown i n Fi g. 4.

Usi ng the experi m ental ra ti oA(7 0 K)/ A(1 0 K), ÈD was obta i ned for each sampl e.

The ÈD val ues are di splayed i n T abl e and Fi g. 5. In case of the CuCl Se2 (1À x )T e2 x

series an abrupt decrease i n ÈD b etween x = 0 : and x : was observed.

È

The i nvari able val ue of£ i n T abl e f or al l sam pl es is not surpri sing . The di ˜er- ence i n chem i cal bo ndi ng of T e i n Y conta i ni ng chai ns are, i n pri nci pl e, restri cted to sm all di ˜erences i n p shell p opul ati on, whi ch m ay onl y i ndi rectl y i nÛuence the el ectro n density at the T e nucl eus. Ho wever, i s expected to b e a qui te sensiti ve m easure of a ny ani sotro py of p shell .

4.1. Compar i son wi t h element al tel lur i um

The b ondi ng of Te i n two- coordi na ted T e i n T e b eari ng hel i cal chai ns i s predo mi na ntly determ i ned by px and py orbi ta l b ondi ng pa ra l l el to the shortest M{ M di sta nces i n the chai n. Howev er, the el ectri c Ùeld gradi ent whi ch determ i nes the nucl ear qua drup ol e spl itti ng results pri m ari ly fro m the lone pai r of el ectro ns i n ful l y occupi ed T e pz orbi ta l s pa ra l l el to the chai n axi s. It is i nteresti ng to note tha t  of elemental T e ( : m m /s at 4.8 K,  : m m/ s at 77 K)

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i s signi Ùcantl y sma ll er tha n  = 9 : 6 m m/ s found i n CuCl T e2. Thi s smal l er Â

suggests som e addi ti onal Ùll i ng of the b ondi ng 5 px, 5 py orbi tal s a nd, theref o re, som e addi ti ona l b ondi ng b etween Te chai ns. Thi s conclusi on i s i n agreement wi th our value ÈD = 138 K for CuCl T e2, whi ch i s rem ark abl y l ower tha n tha t for el ementa l T e (ÈD = 180Ï 15 K [7]). The decrease i n  as rep orted for elemental T e b etween 4.8 K and 77 K ha s been i nterpreted as a result of to rsiona l m oti ons of the spira l chai ns. Such tem p erature dep endence wa s no t observed for our sam pl es.

Our results ra ther hi nt tha t to rsio n of i sol ated spira l chai ns hel d to gether by Cu+ ClÀ bri dges i s fro zen.

4.2. O r der i n g of T e i n CuC lSe2 (1À x )Te2 x

Our 1 2 5Te spectra of CuCl T e2 exhi bi ted one do ubl et onl y, wi tho ut nota bl e

l i ne bro adeni ng . D i sti nct 1 2 5T e hyp erÙne spl itti ng s at the i ndi vi dua l M and M

sites coul d no t be resol ved. Theref ore, i t was not p ossibl e to identi fy M and M

sites by 1 2 5Te resona nce. The geom etri cal di sti ncti on of M andM a pp ears to b e so smal l tha t any detecti on of intri nsi c qua drup ol e spli tti ngs canno t b e expected.

The observed e˜e ct i ve spl i tti ng s  ra ther result fro m nearest M and/ or M

o ccupanci es by Te or an Y ato m other tha n T e, e.g . Se.

Fi rst, l et us consider the hyp otheti cal case of complete order i ng for a pa rti c- ul ar chem i cal com po siti on wi thi n the system CuCl Se2 (1À x )Te2 x. The pro ba bi l i ty

p x for the cluster ˜ : { T e{ { Te{ wi thi n the chai ns i s

p˜ x for < x < : ; and (1 )

p˜ x x : for : < x < ; (2 )

for the cluster Ù { Se{ { Se{ , i t i s

pÙ x for < x < : ; and (3 )

pÙ x = x x 2 for : < x < ; (4 )

and Ùnal l y for the cluster Û { Se{ { Te{ , i t i s

pÛ x for < x < : ; and (5 )

pÛ x = x x x for : < x < : (6 )

These pro ba bi l i ti es are di splayed i n Fi g. 6 (l eft). Acco rdi ngl y, the respecti ve pro b- abi l i ti esp for compl ete di sorder i ng, i .e. sta ti sti cal di stri buti on of Te o ver al l M

and M sites, are

p˜ x x2; (7 )

pÙ x x 2; (8 )

pÛ x x x ; (9 )

as shown i n Fi g. 6 (ri ght).

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Fig. 6. Probabil iti es p of the clusters ˜ , Ù, and Û on telluri um concentration, x, f or completely ordered phases (lef t) and completely disordered phases (right).

Acco rdi ng to thi s simpl e m odel , the observed values ( x ) i n a bi na ry sys- tem CuXY 2 (1À x )Te2 x represent wei ghted avera ges of ˜ ,  Ù, and ÂÛ, i.e. the i ndi vi dua l qua drup ol e spli tti ngs f or the clusters ˜ ,Ù, and Û, respecti vel y

 ( x p˜ x ˜ pÙ x ÂÙ pÛ x ÂÛ: (1 0)

The val ue of ˜ i s kno wn fro m the CuCl Te2 spectrum : ˜ : m m/s (T abl e).

Tha t of ÂÛ m ay b e assumed general l y asÂÛ : Â ˜ Â Ù . Fro m (1 0) Â Ù

m ay b e obta ined using , i n pri nci pl e, j ust one value of determ ined exp eri m ental l y fro m a sam pl e of arbi tra ry comp ositi onx:

 ٠m m=s  : p˜ pÛ = pÙ pÛ : (1 1)

In case of compl ete order, i t is readi l y seen, wi thi n the appro xi ma tio n o f thi s mo del, tha t Eq. (1 1) i s reduced by i nserti on of Eqs. (1 ), (3 ), and (5) to ÂÙ Â x for any comp ositi on wi th x < : .

W e may no w compa re the exp eri menta l qua drup ol e spli tti ngs of the sys- tem CuCl Se2 (1À x )T e2 x repo rted i n Tabl e wi th  deri ved f rom o ur sim pl e m odel for com pl etel y ordered pha ses as wel l as tho se for com pl etely di sordered ones by i nserti on of the appro pri a te pro babi li ty term s p deÙned i n Eqs. (1 ) to (9 ) i nto Eqs. (1 0) and (1 1). Fi rst, the com pl etely ordered pha ses wi l l be consi dered. In- serti ng the experi m ental  da ta f orx : andx : i nto (1 1) and using the

p val ues of Eqs. (1), (3 ), and (5) resul ts i n the mo del val uesÂ0 : 2 5 : m m/s

and  0 : 5 : m m/ s, respecti vely. Inserti ng the experi m enta l  for x :

i nto (1 1) and p of Eqs. (2 ), (4 ), and (6 ) accordi ngl y results i n the mo del val ue 9.6 m m/ s.

 x for the compl etely di sordered pha ses m ay b e cal culated wi th the use of Eqs. (7 ), (8 ), (9 ), and (10):

 x m m=s : x2 ÂÙ x 2 :  ٠x x ; or (1 2)

 ٠ : x = x : (1 3)

Equa ti on (1 3) i s val i d for the enti re ra ng e of com p ositi onsx < x < ).

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The sam e pro cedure was appl ied for the experi m ental ly determ i ned val ues

ÈD( x ). The predi cted, resul ti ng dep endence of ÈD on the concentra ti on x i s i l - l ustra ted i n Fi g. 5. The pri ncipa l sim i l arit y of Fi gs. 3 a nd 5 shoul d b e no ted i n vi ew of the no n- correl ated determ i nati on of  and resona nt absorpti on areas A

(T abl e). Com pari son of m easured and predi cted ÈD( x ) as well as the  ( x ) values, ba sed on our simpl e m odel of l ocal clusteri ng, favo urs stro ngl y lo cal orderi ng of T e o ver one of the M sites, whi ch may b eM 1 or M 2. As m enti oned at the b egi nni ng of thi s section, i t i s not p ossibl e to di sti ng ui sh between M 1 and M fro m T e spectro scopy al one.

4.3. T he rol e of chalcogen and hal i de ani ons

The substi tuti on of Se by S do es no t chang e the electro ni c state of T e sig- ni Ùcantl y as concl uded fro m the T e spectra of CuCl STe. Howev er, further re- pl acement of Cl by Br (T abl e) reduces the val ue of Â. Thi s is i ndi cati ve of some addi ti ona l electro n tra nsf er fro m Br to the p , p orbi tal s o f T e. The Y{ X di s- ta nce app ears to b e shorter at the M site tha n at theM site. Thus, the i nÛuence of Br substi tuti on for Cl on the electro ni c T e sta te, i ndeed, suggests tha t T e i s or- dered i nto the M p ositi on as i t was concluded fro m X- ra y di ˜ra cti on.

W e tha nk Doro thea Al b er, Ha hn{ Mei tner- Insti tut Berl i n for acti vati ng the T e sources. Thi s work was pa rtl y Ùnanced by the pro j ect W T Z POL 9 8-031 of D LR (BMBF), G erma ny.

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