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Pergamon

Solid Srace Communications, Vol. 107. No. 5. pp. 217-22 I, lYY8 8 IYY8 Elsevirr Science Ltd Primed in Great Britain. All rights reserved 0038-lOY8/Y8 $lY.OO+.OO PII: s0038-1098(9@001%-3

PHASE TRANSITIONS OF zno.8d;eo.16se UNDER HIGH-PRESSURE

Chih-Ming Lin,” Der-San Chuu,“* Wu-Ching Choub Ji-an Xu,’ Eugene Huang,‘Jing-Zhu Hud and Jui-Hsiang Pei’ ‘Institute of Electra-Physics, National Chiao Tung University, Hsinchu, Taiwan, R.O.C.

bDepartment of Physics, Chung Yuan Christian University, Chung-Li, Taiwan, R.O.C.

“Institute of Earth Sciences, Academia Sinica, NanKang P.O. Box l-55, Taipei, Taiwan 11529, R.O.C. ‘Geophysical Laboratory Carnegie Institution of Washington, D.C., 20015 U.S.A.

‘National Hsinchu Teacher’s College, Hsinchu, Taiwan, R.O.C.

(Received 21 November 1997; accepted 14 April 1998 by S. Ushioda)

The energy-dispersive X-ray-diffraction (EDXD) and Raman spectroscopy were employed to study the pressure induced phase transitions of ZnO.s~FeO,lsSe crystal up to 21.0 and 32.0 GPa, respectively. A semi- conductor-metal transition was identified by EDXD and Raman spectro- scopic methods at 11.4 2 0.5 GPa. Other two phase transitions were found only in the Raman scattering study below 11.4 GPa. In addition, three unidentified Raman peaks were still observable above the metallization pressure. The existence of Fe impurity in the ZnSe up to a concentration of 0.16 reduced prominently the semiconductor-metal phase transition pressure. For Raman works, the three unidentified Raman peaks of ZnO.s~FeO.lsSe above 10.9 GPa are possibly the TO modes in the thin surface of the high pressure metallic phase. 0 1998 Elsevier Science Ltd. All rights reserved

Keywords: A. semiconductors, D. phase transitions, E. high pressure, E. synchrotron radiation.

Ternary compound semiconductors, especially those containing the transition metal ions, have attracted attentions due to their ability to tune both the band gap and the lattice constant for application in the opto-electric devices as well as for the study of basic physical properties. Among the ternary compounds, diluted magnetic semiconductors (DMS) [l] are the ones of the most interesting types of materials. DMS (also referred to as semimagnetic semiconductors), such as Cdl _,M,S, Cd,_,M,Se, Cd,_,M,Te, Zn, _.,M,S, Zn I _,M,Se and Zn I _xM,Te, etc. (where M is a transition metal like Cr, Mn, Fe and Co) are compound II-VI

semiconductor alloys with a fraction of the nonmagnetic cations replaced by the magnetic transition metal ions. Interesting phenomena such as spin glass transition [2], magnetic ordering in a two-dimensional system [3], spin flip Raman scattering [4], observation of polaron [5],

* Author to whom all the correspondence should be addressed.

metal insulator transition [6], giant Faraday rotation [7], magnetic tuning of quantum well band alignment [8], spin superlattice structures [9] and novel spin relaxation process [lo] have been discovered. Recently, attentions are also focused on the lattice vibration of the DMS [ 11, 121. Zn ,_,Fe,Se, crystallized in the zinc-blende structure which is similar to ZnSe in the range of Fe content 0 5 x 5 0.30 [ 131, is a member of the diluted magnetic semiconductor (DMS) family [ 141. Interesting magnetic as well as the magneto-optical properties were investi- gated on both Zn ,_,Fe,Se bulk crystals, thin films and quantum well [7, 13, 15, 161. Furthermore, the pressure induced phase transition of Znl_,Fe,Se crystal was also discussed [ 171 using the energy-dispersive X-ray- diffraction (EDXD) method. It was found that the existence of Fe in the crystal results in a reduction in the transition pressure; such a reduction was believed to be the result of the hybridization of 3d orbitals into the tetrahedral bonds [18]. Recently, the Raman scattering experiment has also been applied to study the pressure effect on Zn ,_,Fe,Se 1121, Zn l_,Co.,Se [ 191 and 217

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218 PHASE TRANSITIONS OF Znos4Feo ,&ie UNDER HIGH-PRESSURE Vol. 107, No. 5 Zni_,*Mn,Se [20, 211 crystals and two new phases were

found at 4.0 GPa and 8.0 GPa which were lower than the semiconductor-metal transition pressure in Zn i_,Mn,Se. In this work, the EDXD measurement combined with the Raman scattering study was used to investigate the pressure effect on the phase transition of ZnO.s~FeO.,$e crystals at high-pressure up to around 25.0 and 32.0 GPa, respectively. A phase transition at 4.7 GPa was found in Raman spectroscopic study, but not in EDXD measurement. The identification of the semiconductor- metal transition pressure for EDXD result is the change of the crystal structure, which is consistent with the disappearance of the Fe local and the longitudinal optical (LO) phonon modes of Raman scattering result.

ZnO.s~FeO.,sSe crystals were grown by the modified Bridgman method. The crystals were grounded to 1 pm size for EDXD measurement while in the Raman scatter- ing study, a tiny crystal of 50 pm size was used. We used a Mao-Bell type diamond anvil cell (DAC) with T304 stainless steel gaskets which were preindented to 15.0 GPa; the sample hole was 130 pm in diameter. The anvil parameters were l/3 carats with a 600 pm culet. Experimental details were described earlier by Xu [22]. For DAC EDXD experiment, pressure up to 21.0 GPa was used. The source is the superconductor wiggler synchrotron beam line Xl7C of the National Synchrotron Light Source (NSLS) of Brookhaven National Laboratory in U.S.A. The beam size was 50 X 50 km’. A Germanium energy dispersive detector was set in the position where the diffracted angle (0) was 5”. Deionized water and the ruby fluorescence scale method [23, 241 and methanol-ethanol 4 : 1 fluid and the internal gold standard [25] were used as a hydrostatic pressure medium and the pressure determination in Raman scattering and EDXD measurement, respectively. For EDXD, the peak positions were read out by a peak search program provided from the VAX computer in the beam line Xl7C. The equation of state (EOS) data were fitted to the Murnaghan equation by using a fitting program reported by [26]. The experimental detail on micro-Raman, up to 32.0 GPa and the reason for choosing deionized water as the pressure medium were described earlier [12, 271. For Raman scattering works, the Jandel Scientific Peakfit computer program for non- linear curve-fitting software produced by AISN Software was used in the deconvolution process and the deter- mination of the peak position, intensity and the full width at half maximum as in the previous work [28]. The component forms of deconvolution process were defined by Lorentzian function as:

LORENTZ(x) = %

2’ (1)

where, uo, a, and a2 are amplitude, center and width, respectively.

Zno.s~FeO,,sSe has a lattice parameter of 5.639 t 0.001 A from EDXD measurement at ambient pressure. It is only in the zinc-blende (B3) phase with (1 1 1), (2 2 0) and (3 1 1) peaks below 11.4 GPa. Above 11.4 GPa, the peaks of the B3 phase of Zno.s~FeO.,&Se disappear and an apparent peak in the Bl phase occurs. The Bl peaks, (2 0 0) and (2 2 0), exist up to 21.0 GPa. The d-spacings at 11.4 GPa are 3.112,2.556 and 1.802 A for zinc-blende (B3) phase and are 1.861 and 1.634 A for rock salt (Bl) phase. The variation of the interplanar distances dh kI and equation of state (EOS) relations of Zno.s4Feo ,$e as a function of pressure are shown in Fig. 1, where V. and V are volumes of Zno.s~FeO.rsSe at zero and certain pressure, respectively. The data for the two phases were fitted to the Murnaghan equation by a previously developed fitting process [26]. The Murnaghan equation is defined as:

P = &lK~)[(v,lvp- ‘1, (2)

where K0 is the isothermal bulk modulus at zero pressure and Kb is the pressure derivative of the isothermal bulk modulus evaluated at zero pressure. The values of K. and

Kb obtained from the fitting process are 58.85 * 2.37

and 4.12 +- 0.53, 80.15 -+ 1.05 and 3.64 5 0.55 for B3 and B 1, respectively. Kb values are consistent with the slopes of d-spaces for B3 and B 1 in Fig. 1. It is shown that Zn0.s4Fe0,,&Se in high-pressure region (Bl) is less compressible than that in low-pressure region (B3). Figure 1 also shows that there is no two-phase-co- existence ambiguity range and the phase transition occurred at 11.4 GPa. The lattice parameters of zinc- blende (ZB) and rock salt (RS) phases are 5.357 t 0.001 A and 5.104 % 0.001 A at 11.4 GPa, respectively.

Raman spectra for Zno.s~FeO.,,$e crystal at various pressure were reported by Lin et al. [ 121. The variation of the mode energies as a function of the pressure is shown in Fig. 2. The solid symbols correspond to the LO, Fe TO local, TO and TO split Raman modes of Zn0.s4Feo,isSe, respectively. The relationship of the mode frequencies vs pressure of ZnO.s~Feo,i$e is plotted as the dash curves in Fig. 2. These curves are obtained by a quadratic polynomial fitting using the equations listed in Table 1, where wi is the wavenumber in cm-’ and p is the pressure in GPa. At atmospheric pressure, two peaks labelled as LO and TO phonons were reported previously [29]. Between these two peaks, a Fe TO local (impurity) phonon mode could be labelled through the deconvolution process [29]. The phonon energy of Fe TO local and the LO and TO modes are increased with the pressure. As pressure rises up to 4.7 GPa, two new modes appear. The phonon mode labelled as TO split mode I exhibits red shift and the other mode labelled as TO split

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Vol. 107. No. 5

PHASE TRANSITIONS OF Zna.s4Fe0.,$e UNDER HIGH-PRESSURE

219

4.4 4.0 3.6 3.2 *6 Yi mj 2.8 2.4 0.80 0.85

P

0.80 N > 0.65 0.60 0 2 4 6 8 10 12 14 16 18 20 Pressure (GPa)

Fig. 1. The variation of

dh k, (A)

of ZnO.s~FeO.l&e

with

pressure (GPa) and the

V/V0 vs

pressure for the B3 and

B 1 phases of Zn0.s4Fe0,,$e.

mode II, as well as the LO phonon and Fe TO local mode,

exhibits blue shift as pressure is increased up to around

32.0 GPa. Although no structure transitions could be

identified in the EDXD works of ours and Qadri et

al. [

171 for a pressure below 10.0 GPa, Michel et al. [30]

reported that ZnSe follows the structural transition

sequence:

zinc-blende - cinnabar -

NaCl

- CmCn

with increasing pressure by using the ab initio pseudo-

potential calculations method. Ahuji et

al.

[31] also

indicated that CdTe follows the structural sequence:

zinc-blende - cinnabar -

NaCl -

orthorhombic

with

increasing pressure by using the full-potential linear

muffin-tin-orbital (EPLMTO) calculations in the study-

ing of the structural phase transition of CdTe under high-

pressure. Similar study of the ZB structure of CdTe [32]

showed that one more phase exists below the structure

Table 1. The quadratic polynomial fitting equation of the

Znn &en de

Raman modes

Quadratic polynomial

fitting equation

LO

Fe local

TO

TO split (I)

TO split (II)

254.4 + 3.37p - 0.1 33p2

228.3 + 6.14~ - 0.313~~

202.6 + 5.60~ - 0.11 lp2

216.5 + 0.15~ + 0.021~~

216.0 - 3.57~ + 0.099~~

_ _ _ quadratic polynomial fitting

0 LOmode = Felccalmode A TOmode v TO split mode I 0 TO split mode II 320

‘;E

sauu

s

$J

280 s E 260 l? 240 0 5 10 15 20 25 30 35 Pressure (GPa)

Fig. 2. Pressure dependence of Raman peaks in the

ZnO.s~FeO.lsSe

crystal. The dash lines are quadratic poly-

nomial fitting curves for Zno.srFeo,isSe crystal. The semi-

conductor-metal

phase

transition

pressure

of

Zn0,s4Fe~.,&e can be well identified.

transformation from ZB to RS structure. We therefore

attribute the appearance of the new phonon mode to the

broken symmetry of the structure transformation. The

splitting of TO phonon at 4.7 GPa could be also due to

the structure transition as zinc-blende phase transforms

into cinnabar phase. As the pressure increases further to

10.9 GPa, the semiconductor-metal transition pressure

of ZnO,s~FeO.lsSe,

both LO and Fe TO local modes

disappear. The arrows at 10.9 and 11.4 GPa labelling

as “A” and

‘ ‘B’ ’ symbols in Fig. 2 indicate the transition

pressures of B3 to Bl identified by Raman scattering

and EDXD measurement, respectively. The effects of

pressure on various Raman vibrational modes of

Zns,wFeo.l&Se at room temperature (298 K) are listed in

Table 2. The Griineisen parameter (ri) for a quasi-

harmonic mode i of frequency wi was defined by Cardona

et

al. [X3].

From the comparison of the values of y~o, yro

and y-&Lo

of ZnSe [12] and Zno.uFee.&e, we

may

conclude that ZnO.uFeo.i&Se has higher ionicity than

ZnSe. The Fe TO local mode in Zno.84Feo.&e behaves

the same way as the LO mode instead of the TO mode

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220 PHASE TRANSITIONS OF Zn0.84Fe0,,,$e UNDER HIGH-PRESSURE Vol. 107, No. 5 Table 2. Effect of pressure on various Raman vibrational modes of ZnO.s~FeO,,$e at room temperature (298 K). The values of mode frequencies Wi, pressure dependence dw)dp, mode Griineisen parameter yi are extrapolated at ambient conditions Mode wi dw;ldp YI d-r/Q (cm-‘) (cm-‘/GPa)

[(Ww;)(d~/dP)l

(l/GPa) LO 254.4 3.37 - 0.266~ 0.668 -0.076 1 + 1.7397 X lo- ‘p Fe local 228.3 6.14 - 0.626~ 1.395 -0.2125 + 8.1888 X lo-‘p TO 202.6 5.60 - 0.222~ 1.394 -0.0989 + 2.4740 X 10 -‘p

TO split (I) 216.5 0.15 + 0.042~ 0.043 -0.0121 + 1.6106 X lo-$

TO split (II) 216.0 -3.57 + 0.198~ -0.832 0.0127+4.1160X 10-3p

which splits into three components. These three com- ponents are still visible at the highest pressure achieved in our experiments. Furthermore, it was found the semi- conductor-metal transition pressure for Raman scattering measurement of the Zn0,s4Feo.,$e is 10.9 GPa which is 3.5 GPa lower than that of our previous ZnSe Raman works. The reduction in the transition pressure might be attributed partially to the hybridization of 3d orbitals of Fe ion into the tetrahedral bonds [ 181 and partially to the percentage of the volume change, AVlV,, of B3-to-B1 phase transition 1341. Our result was consistent with the study of pressure-induced phase transition of Zn0.s3Fe0.,+e by the EDXD measurement [ 171.

According to the data of resistance of ZnSe measured Itkin and co-workers [35], the onset of the metallization occured at 13.5 GPa. The calculated skin depth above phase transition pressure could be found to be about several tens A [ 121. Therefore, we suggest that the possible reason for the disappearance of LO phonon and Fe local phonon modes and the existence of TO and split TO phonon modes above metallization pressure may due to a thin skin depth could only sustain the propagation of transverse EM wave but forbid the longitudinal EM wave. In addition, the disappearance of the LO-TO splitting may be due to screening of the longitudinal phonon field by metallic electrons.

In summary, both Raman scattering and EDXD measurements show that the existence of the Fe element results in a reduction of phase transition pressure in the semiconductor-metal phase transformation. The disappearance of the LO and Fe local phonons above the transition pressure is attributed to the metallization of the Zn0.s4Fe0.,,$e crystal. The calculated Griineisen parameter implies that ZnO.~FeO.isSe has higher ionicity than ZnSe. Three visible TO phonon splitting com- ponents in Zn,,s~FeO.,sSe system are observed from a pressure below metallization transition up to 32.0 GPa for Raman scattering measurement. Structure transitions occur below the semiconductor-metal phase transition, which are obtained by Raman scattering, however, they are not observed in the EDXD measurement.

Acknowledgements-This work was supported by the National Science Council, Taiwan by the grant number NSC86-2112-M-009-006 at NCTU, NSC86 2 112-M-033-01 2, NSC-87-2 112-M-033-004 and NSC 87-2613-M-2 13-008 at CYCU. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. REFERENCES

Furdyna, J.K. and Kossut, J. (Editors), Semi-

conductors and Semimetals, Vol. 25, Diluted

Magnetic Semiconductors. Academic Press, New York, 1988; Balkanski, M. and Averous, M. (Editors), Semimagnetic Semiconductors and

Diluted Magnetic Semiconductors, Plenum Press,

New York, 1991; Kossut, J. and Dobrowolski, W., in Handbook of Magnetic Materials (Edited by K.H. Buschow), Vol. 7. North-Holland Publ. Co., Amsterdam. 1993.

Twardowski, A., Denissen, C.J.M., de Jonge, W.J.M., de WaeIe, A.T.A.M., Demianiuk, M. and Triboulet, R., Solid State Commun., 59, 1986, 199. Samarth, N., Klosowski, P., Luo, H., Furdyna, J.K., Rhyne, J.J., Larson, B.E. and Otsuka, N., Phys.

Rev., B44, 1991,470l.

Peterson, D.L., Bartholomew, D.U., Debska, U., Ramdas, A.K. and Rodriguez, S., Phys. Rev.,

B32, 1985, 323.

Awschalom, D.D., Freeman, M.R., Samarth, N., Luo, H. and Furdyna, J.K., Phys. Rev. Lett., 66,

1991, 1212.

von Molnar, S., Briggs, A., Flouquet, J. and Remenyi, G., Phys. Rev. Lett., 51, 1983, 706. Fu, L.P., Schmiedel, T., Petrou, A., Warnock, J. and Jonker, B.T., Appl. Phys. ht., 60, 1992, 583. Liu, X., Petrou, A., Warnock, J., Jonker, B.T., Prinz, G.A. and Krebs, J.J., Phys. Rev. Lett., 63,

1989,228O.

Chou, W.C., Petrou, A., Wamock, J. and Jonker, B.T., Phys. Rev. L&t., 67, 1991,382O.

Chou, WC., Petrou, A., Wamock, J. and Jonker, B.T., Phys. Rev., B46, 1992,4316.

Suh, E.K., Arora, A.K., Ramdas, A.K. and Rodriguez, S., Phys. Rev., B45, 1992, 3360; Oh, E., Alonso, R.G., Miotkowski, I. and Ramdas, A.K., Phys. Rev., B45, 1992, 10934.

Lin,C.M.,Chuu, D.S., Yang, T.J.,Chou, WC., Xu, J. and Huang, E., Phys. Rev., B55, 1997, 13641.

(5)

Vol. 107, No. 5

PHASE TRANSITIONS OF Zn0.s4Fe,,rsSe UNDER HIGH-PRESSURE

221

13.

14.

15.

16.

17.

18.

19.

20.

21.

22.

23.

24.

Samarth, N. and Furdyna, J.K.,

Mat. Res. Sot.

Symp. Proc.,

161, 1990, 427.

Furdyna, J.K.,

J. Appl.

Phys., 64, 1988, R29.

Twardowski, A., Gold, P., Pernambuco-Wise, P.,

Crow, J.E. and Demianiuk, M.,

Phys. Rev., B46,

1992,000.

Jonker, B.T., Krebs, J.J., Qadri, S.B. and Prinz,

G.A.,

Appl. Phys. Lett., 50, 1987, 848.

Qadri, S.B., Skelton, E.F., Webb, A.W., Moulton,

N., Hu, J.Z. and Furdyna, J.K.,

Phys. Rev., B45,

1992,567O.

Mahashwaranathan, P., Sladek, R.J. and Debska,

U.,

Phys. Rev.,

B31, 1985, 5212.

Bak, J., Venkateswaran, U., Mak, C.L., Soorya-

kumar, R. and Jonker, B.T.,

J. Phys. Chem. Solids,

56, 1995, 563.

Arora, A.K. and Sakuntala, T.,

Phys. Rev.,

B52,

1995, 11052.

Arora, A.K., Suh, E.K., Debska, U. and Ramdas,

A.K.,

Phys. Rev., B37, 1988,2927.

Xu,

J.,

High Temp.-High Press., 19, 1987, 661.

Mao, H.K., Xu, J. and Bell, P.M.,

J. Geophys. Res.,

91, 1986,4673.

Xu, J., Mao, H.K. and Bell, P.M.,

Acta Physicu

Sinica, 36, 1987, 500.

25.

26.

27.

28.

29.

30.

31.

32.

33.

34.

35.

Anderson

et al., J. Appl. Phys., 65, 1989, 1534.

Xu,

J., Hu, J.Z., Ming, L.C., Huang, E. and Xie, H.,

Geophys. Res. Lett.,

21, 1994, 161.

Xu, J., Yen, J., Wang, Y. and Huang, E.,

High- Pressure Res.,

15, 1996, 127.

Xu, J., Yeh, H.-W., Yen, J. and Huang, E.,

Jonl. Raman Spectr., 27, 1996, 823.

Mak, C.L., Sooryakumar, R., Jonker, B.T. and

Prinz, G.A.,

Phys. Rev., B45, 1992, 3344.

Cot&, M., Zakharov, O., Rubio, A. and Cohen,

M.L.,

Phys. Rev., B55, 1997, 13025.

Ahuji, R., James, P., Eriksson, O., Wills, J.M. and

Johansson, B.,

Phys. Status Solidi (b),

199, 1997,

75.

Nelmes, R.J., McMahon, M.I., Wright, N.G. and

Allan, D.R.,

Phys. Rev., B51, 1995, 15723.

Blackman, M. and Daniels, W.B., in

Light

Scattering in Solids IV

(Edited by M. Cardona

and G. Giintherodt), Chap. 8. Springer, Berlin,

1984.

Lin, Chih-Ming, Chuu, Der-San, Xu, Ji-an, Huang,

Eugene, Chou, Wu-Ching, Hu, Jing-Zhu and Pei,

Jui-Hsiang, accepted by

Phys. Rev.

B.

Itkin, G., Hearne, G.R., Sterer, E. and Pasternak,

M.P., Phys.

Rev.,

B51, 1995, 3195.

數據

Fig.  1. The  variation  of  dh k,  (A)  of  ZnO.s~FeO.l&e  with  pressure  (GPa)  and  the  V/V0  vs  pressure  for  the  B3  and  B 1 phases  of  Zn0.s4Fe0,,$e

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