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Proximity effects in CeCu6/Nb bilayers

Otop, A.; Süllow, S.; Hesselberth, M.B.S.; Aarts, J.

Citation

Otop, A., Süllow, S., Hesselberth, M. B. S., & Aarts, J. (2003). Proximity

effects in CeCu6/Nb bilayers. Acta Physica Polonica B, 34(2),

1169-1172. Retrieved from https://hdl.handle.net/1887/45422

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Not Applicable (or Unknown)

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Leiden University Non-exclusive license

Downloaded from:

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PROXIMITY EFFECTS IN CeCu 6 /Nb BILAYERS  A. Otop a;b , S. Süllow a , M.B.S. Hesselberth b and J. Aarts b a

InstitutfürMetallphysikundNukleareFestkörperphysik Te hnis heUniversitätBrauns hweig

Mendelssohnstr. 3,38106Brauns hweig,Germany b

KamerlinghOnnesLaboratory,Leiden University Niels Bohrweg2,2300RALeiden,TheNetherlands

(Re eivedJuly10,2002)

We studied theproximityee t in order to probethe response of the heavy-fermion metal CeCu

6

to indu ed super ondu tivity. High-quality CeCu

6

lmswere grownbysputter deposition. Resistivity measurements showthat the orrelatedele tronstateis formed. Bilayerswereprepared ofCeCu

6

(75nm)/Nb(d Nb

),withtheNbthi knessd Nb

between10nmand 50nm. Measuredwerethesuper ondu tingtransitiontemperatureT

and theparallel riti alelds H

jj 2

. Wend that theinterfa etransparen y is high, indi ating that Fermi-velo ity mismat h ee ts are not signi ant, butthe oheren e lengthoftheindu edsuper ondu tivityissmall, whi h isprobablyduetotheverylowFermi-velo ityintheheavyfermionmetal.

PACSnumbers: 71.27.+a,74.50.+r

1. Introdu tion

Insimplenormalmetals su hasAuor Pd, questionsabout their ability to sustainsuper ondu ting orrelations orunbalan edspins areofmu h in-terest. Similar questions an be raised about a metalli ground state with strong intrinsi orrelationssu h asinheavy fermion(HF)systems. Spe if-i ally, ifa metal isin onta t witha super ondu tor, it an be asked what the me hanism is for pair breaking of Cooper pairs diusing out of the su-per ondu tor. For normal metals (N) the me hanism is dephasing due to a nite temperature; for ferromagnets (F) it is the ee t of the ex hange eld; fora HFgroundstatetheanswerisnotknown,and ould involve e.g. spin u tuations. Anintrinsi problemfor su hstudies isthatthematerial has to be available in thinlm form. Herewe present the rst results of a



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study of the proximity ee t in asystem onsistingof thin lms of theHF material CeCu

6

ombined with thin lms of a super ondu tor (S), in this ase Nb. Among the dierent HF systems, CeCu

6

is of parti ular interest sin e itdoesnot order magneti allydown to mKtemperatures[1,2℄.

2. Sample preparation

SetsofCeCu 6

lmsandbilayersofCeCu 6

/Nbweremadeby DC-magnet-ron sputtering. We used an ultra high va uum system with a ba kground pressure of the order of 510

10

mbar, and an Ar sputtering pressure of 2:510

3

mbar. Crystalline CeCu 6

was grown as reported before [3℄, at a temperature of 350

Æ

C using Si-substrates with amorphous Si 3

N 4

buer layers to prevent Cudiusion at thosetemperatures.

The Nb was deposited on top of the CeCu 6

after ooling the substrate holder with old nitrogen gas to lose to room temperature. Composi-tion, thi kness and rystallinity of the lms were determined by Ruther-ford ba ks attering (RBS) measurements together with X-ray dira tion measurements at low and highangles. The RBS measurements show good agreement with the expe ted stoi hiometry for CeCu

6

and no diusion is found eitherofCeor Cuinto thesubstrate or ofNb intotheCeCu

6

. Fig.1 showspartoftheRBSspe trumforCeCu

6

(75nm)/Nb(15nm)onaSi/Si 3

N 4 substrate and at of thedata withouttakinganydiusion into a ount.

340

360

380

400

420

440

460

Channel

0

10

20

30

40

50

60

N

o

rm

al

iz

ed

Y

ie

ld

1.4

1.5

1.6

1.7

1.8

Energy (MeV)

Cu

Nb

Ce

Fig.1. RBSmeasurementusing 4

He-ionsof2MeV onasample Si/Si 3 N 4 /CeCu 6

(75 nm)/Nb(15 nm). The dierent elements are indi ated. The thin smoothlineisatto themeasured urve.

Fig.2(a)showstheele tri alresistivityasafun tionoftemperatureT for two single lms ofCeCu

6

(4)

and inprevious investigations on sputteredCeCu 6

lms [3℄. We de idedto use 75 nm thi k CeCu

6

layer, whi h with T max

= 4 K suggest only little deviation from thebulkproperties.

0

10

20

30

40

50

0

1

2

3

4

5

6

7

8

9

10

0

5

10

15

20

25

30

35

40

76

78

80

82

84

86

88

90

92

T

c

(K

)

d

Nb

(nm)

CeCu

6

/Nb

Nb

(b)

(a)

r

(

m

W

cm

)

T(K)

CeCu

6

d=188 nm

CeCu

6

d=75 nm

Fig.2. (a)Resistivityasafun tion oftemperatureforCeCu 6

lmsof75 nmand 188 nm. (b) Criti al temperature asa fun tion of Nb thi kness d

Nb

for bilayers CeCu

6

/Nb andsingleNb lms. Thesolid linerepresentsthetypi albehaviorfor Nbsinglelmsfromdierentdepositionsystems,trianglesshowvaluesforNblms made inthesamesystemastheCeCu

6

/Nb bilayers,thedotted lineis aguide to theeye.

3. CeCu 6

/Nb bilayers; results and dis ussion

The super ondu ting transition temperature T

was determined from resistivity measurements on a set of CeCu

6 (75 nm)/Nb(d Nb ) withvariable Nb thi kness d Nb

in the range 10 nm to 50 nm. As seen in Fig. 2(b), T

shows a strong suppression, with a riti al thi kness d r

for onset of super ondu tivityrea hedaround12nm. Thiswouldbeequivalentto24nm inatrilayer onguration,andofasimilarmagnitudeasfoundinFe/Nb/Fe trilayers [5℄. It has to be kept in mind however that single thin Nb lms also show a de rease of T

at small thi kness (see Fig. 2(b)), whi h makes the orre t determination of d

r

more di ult. The result shows, however, that the interfa e does allow parti le ex hange, oppositeto what might be expe tedfromthehugeFermivelo itymismat hinthesystemoforder10

3 .

Also theparallel riti al eldH jj 2

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2

3

4

5

6

7

8

9

0

1

2

3

4

2

3

4

5

0

1

2

3

4

(a)

(b)

m

0

H

c

2

(T

)

T (K)

d

Nb

=50 nm

d

Nb

=31 nm

d

Nb

=25 nm

d

Nb

=17 nm

d

Nb

=15 nm

d

Nb

=13.5 nm

T

DCO

m

0

H

c

2

(T

)

T (K)

Cu/Nb(15 nm)

CeCu

6

/Nb(15 nm)

Fig.3. Upperparallel riti al eld as afun tion of temperature for: (a) bilayers CeCu

6

(75 nm)/Nb, d Nb

as indi ated; (b) bilayersof CeCu 6

(75 nm)/Nb(15 nm) andCu(75nm)/Nb(15nm) withT

DCO

indi ated.

Absen eoftheDCOmeansthatnoappre iableamountof super ondu -tivity leaks into the HF metal; together with the nite transparen y this means either appre iable pair breaking by the HF metal, or a very small diusivity due to the low Fermi velo ity v

F

. Whether a small v F

alone is able to explainthe experimentsispresently under investigation.

WorkatLeidenUniversityispartoftheresear hprogramofthe `Sti ht-ing F.O.M.'. We a knowledgete hni al supportbyT.J. Gortenmulder and R.W.A. Hendrikx. A.O. a knowledges support of the European S ien e Foundation(programmeFERLIN)andofF.O.M.forshorttermfellowships.

REFERENCES

[1℄ H.v. Löhneysen,J.Phys. Condens. Matter8,9689(1996).

[2℄ H. Tsujii, E. Tanaka, Y. Ode, T. Katoh, T. Mamiya, S. Araki, R. Settai, Y.Onuki,Phys. Rev.Lett.84, 5407(2000).

[3℄ D.Groten,G.J.C.vanBaarle,J.Aarts,G.J.Nieuwenhuys,J.A.Mydosh,Phys. Rev. B64,144425(2001).

[4℄ A.Amato,D.Ja ard,E.Walker,J.Flouquet, SolidStateCommun.55,1131 (1985).

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