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Mixed valency in the high-temperature phases of transition metal molybdates,AMoO4 (A=Fe, Co, Ni)

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9 Printed in India.

Mixed valency in the high-temperature phases of transition metal molybdates, A M o 0 4 (A = Fe, Co, Ni)i"

R A M O H A N RAM and J G O P A L A K R I S H N A N *

Solid State and Structural Chemistry Unit, Indian Institute of Science, Bangalore 560012, India

MS received 26 November 1985

Abstract. Transition metal molybdates of the formula AMoO4 where A = Fe, Co or Ni exhibit a first-order phase transition between 670 K-970 K. An investigation of the low- temperature (Lr) and high-temperature {fir) phases by x-ray photoelectron spectroscopy, x-ray absorption spectroscopy, magnetic susceptibility and other physical methods shows that the phase transition is associated with a valence change of the type A 2+ + Mo o+ ~.~A 3§

+Mo 5+ in the cases of iron and cobalt molybdates.

Keywm'ds. Transition metal molybdates; mixed valency; high-temperature phases.

1. Introduction

Divalent metal molybdates AMoO4, where A = Fe, Co or Ni, crystallize under ambient conditions in a defect rocksalt structure (Lr phase) with the transition metal atoms in octahedral coordination (Smith and Ibers 1965). These molybdates undergo first-order phase transitions at high temperatures (670-970 K) with a large change ( ~ 6 ~o) in volume (Sleight and Chamberland 1968). The high temperature (rrr) phase can be quenched in the case o f the iron compound. The structure o f the nTphase has not been determined but powder diffraction data reveal that the n r phase is isostructural with M n M o O 4 (Abrahams and Reddy 1965; Sleight et al 1968) wherein Mn is in octahedral and Mo in tetrahedral coordination. The main structural change associated with the phase transition appears to be a change in Mo coordination from six to four.

Since the transition occurs only in F e M o O 4 , C o M o O , and N i M o O 4 and not in the other divalent metal molybdates (Sleight and Chamberland 1968), it has been suspected that the transition may involve valence change o f the type, A 2§ + M o 6§ ~,-~A 3§

+ Mo 5 +. We have prepared AMoO4 molybdates of Fe, Co and Ni and characterized both the H'r and LT phases by x-ray photoelectron spectroscopy, x-ray absorption spectroscopy, M6ssbauer spectroscopy, magnetic susceptibility and electrical resis- tivity measurements besides x-ray crystallography. The results reveal that the transition is likely to be associated with a valence change o f the cations at least in the cases o f iron and cobalt molybdates and that the HT phases are mixed valent as described, by ~ A2+ A3+ 1 - x ~ x M O l - x M o x 0 4 . 6+ 5+

t Contribution No. 311 from the Solid State and Structural Chemistry Unit.

* To whom all correspondence should be addressed.

291

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292 R A Mohan Ram and J Gopalakrishnan 2. Experimental

FeMoO4 was prepared by heating the required quantities of Fe, Fe203 and MoO3 in a sealed tube at 1270 K for 48 hours. Depending on the cooling rate, either the Hr or the LT phase was obtained (Sleight et ai 1968). The pure LT phase was obtained by slow cooling, first to room temperature and then to liquid nitrogen temperature. The Ha- phase was obtained by quenching the sealed tube from 870 K to room temperature.

La- phases of CoMoO4 and NiMoO, were prepared by heating stoichiometric quantities of nickel oxide or cobalt oxalate respectively with MoO3 at 1270 K for 48 hours in air, followed by slow cooling to room temperature (Sieber et al 1983). tit phases of CoMoO4 and NiMoO4 could not be obtained by quenching from high temperatures. Ha" CoMoO4 could, however, be prepared (Chojnacki et al 1974) by precipitating CoMoO4. xH20 through the addition of cobalt(II) nitrate to a solution of ammonium paramolybdate at a pH of 5.5 and heating the precipitate at 670 K for 18 hours in air. Ha- NiMoO4 could not be prepared by this precipitation method.

Formation of compounds and their phase purity were ascertained by x-ray powder diffraction (Philips Pw 1050/70 diffractometer). The unit cell parameters agree with the reported values of the fir and L'r phases of the AMoO4 compounds (Sleight et at 1968).

The HT-La- transition of AMoO4 was studied by differential scanning calorimetry (Perkin-Elmer, Model 2) using indium as standard. X-ray photoelectron spectra (xws) were reported using an ESCA-III mark 2 spectrometer with AI K~t radiation. X-ray absorption spectra were recorded using a bent crystal spectrograph; analysis of the spectra was carried out by using a Carl-Zeiss Mt)-100 microdensitometer. Magnetic susceptibility measurements were made in the 15-1000K range using a Faraday balance. Electrical resistivity of pressed pellets of FeMoO4 was measured using the four-probe technique. Room temperature (300 K) M6ssbauer spectra were recorded using 25 mc/57Co (Rh) source; the spectra were least-squares fitted assuming Lorentian line shape.

3. Results and discussion

All the three molybdates undergo a first-order phase transition showing an exothermic peak in osc or DTA. The transition temperatures are in the order, Fe (650 K) < Co (780 K) < Ni(990 K). It is interesting that the transition temperature correlates with the stability of the trivalent oxidation states of the A metal atoms; Ni(III) is the least stable and the transition temperature of NiMoO4 is the highest. This is also consistent with the inability to quench the HT phase of NiMoO4. The transitions were irreversible in OSC/DTA in all the three cases. The heats of transition estimated from the area under the peak are 5.8, 3.6 and 2-5 kJ tool-1 for the iron, cobalt and nickel compounds respectively.

X-ray photoelectron spectra (xPs) of the LT phases of all the three molybdates show the presence of Mo 6+ and ,42+ cations as illustrated in figure 1 with a Mo(3ds/,) binding energy of 232.6 eV characteristic of Mo 6+ (Sarma and Rao 1980, Rao et al 1978). xr,s of the Ha- phases of FeMoO4 and CoMoO4 show evidence for the presence of mixed valent Mo and Fe/Co as illustrated in figure 1. Thus, in the Mo(3d) region there is a shoulder on the lower binding energy side of the Mo(3d~/2) peak at 231-8 eV due to Mo 5 § A rough estimate of the Mo 6 + to Mo ~ + ratio obtained by the deconvolution of

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(a)

1 I J t I I I I

705 710

BE(eV)

21 i i ].

i ~ . _ . HT

LT

2p 312

, 1 1 J 1 , 1 ,

715 720

(b)

6~

300K /

,

LT

~ l J 1 I I I I I I I [

230 235 240

BE (r

tc) ~ i Id) , i

_ _ ~ 3d5/2 3 d 3 / 2 ~ HT

LT

[ i I J I I ! I I I k i t I I, t = 1 i i J t I t ~ J

780 785 230 235 240

BE(eV) BE(eV)

Figure 1. xPs of AMoO4 molybdates. (a) Fe(2p) spectra of t.T and HT FeMoO,=; (b) Mo(3d) spectra of LT and HT FeMoO,=. The corresponding Co and Mo spectra of CoMoO4 are shown in (c) and (d).

the peaks in the case o f nx FeMoO4 is 60 : 40. The spectra in the Fe(2p) and Co(2p) regions also show changes indicating the coexistence of 2 + and 3 + ions.

LT FeMoO4 and LT C o M o O 4 show characteristic satellites at 3.5-4.0 eV and 6-2 eV respectively in the F e / C o (2p) spectra similar to FeO and C o O (Rao et al 1978). In HT FeMoO4 the satellite is at 5.5 eV confirming the presence of Fe 3+ (Vasudevan et al 1979); a similar change is observed in the Co(2p) spectrum o f nT C o M o O 4 .

Further evidence for the mixed valence character of the HT phases o f FeMoO4 and C o M o O 4 is provided by x-ray absorption spectroscopy. Chemical shifts of the K- absorption edges o f transition metals are known to reflect changes in the oxidation

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294 R A Mohan Ram and J Gopalakrishnan

states o f transition metals (Sarode et al 1979), T h e shifts in the case o f the molybdates are listed in table 1. The chemical shifts in the K-edges o f b o t h the M o and A metal ions in LT phases are consistent with M o 6 + and A 2 + states (Sarode et a11979; M a n t h i r a m ez al 1980). T h e M o K-edge shows a smaller chemical shift in the aT phases;

correspondingly, the Fe and C o edges show larger chemical shifts as c o m p a r e d to the LT phases consistent with the presence o f 3 + ions as well.

The M 6 s s b a u e r spectrum o f LT F e M o O 4 at r o o m temperature (figure 2a) exhibits a two-finger pattern similar to that reported with an isomer shift o f 0.92 m m sec- ~ a n d q u a d r u p o l e splitting o f 1.77 m m s e c - 1 (Sleight et al 1968). T h e spectrum is consistent with the presence o f high-spin Fe 2 + in LT F e M o O , . T h e M 6 s s b a u e r spectrum o f HT F e M o O 4 shows a four-finger pattern indicating the presence o f two sets o f iron a t o m s (figure 2b). T h e spectrum o f HT F e M o O 4 has been attributed to two different kinds o f iron sites b o t h containing high-spin Fe 2 + (Sleight et a11968). Considering lines 1 and 3

Table i. Chemical shifts of the K-absorption edge of the AMoO4 molybdates.

Chemical shift in cV (•

Compound A ion Mo ion

LT FeMoO4 6-4 13-9

HT FeMoO4 10-4 13.1

LT CoMoO4 7-8 13.3

HT CoMoO4 9-4 12.9

LT NiMoO4 6-9 13"9

100 ! - 0 99 09B 0.97 0 9E 0 ~ 094

100 099 0.98 0.97 0.96 0.95

,-- ,..

~

'.'~ ..-...~-

I I I I 1 I

-1 0 1 2 3 &

V~locl ty (ram sec- t)

Figure 2. M6ssbauer spectra of (a) LT FeMoO4 and (b) 8T FeMoO, at room temperature.

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as belonging to one type of iron and lines 2 and 4 as belonging to another set of iron atoms, we derive isomer shifts of 1-45 and 0"57 mm sec- t with quadrupole splittings of 1.97 and 1.91 mm sec- t respectively. These results can be taken to support the existence of Fe 2 + and Fe 3 § ions in the HT phase in agreement with xPs and absorption edge measurements. The large quadrupole splittings may be due to a highly distorted environment around the iron atoms.

Magnetic susceptibility of the molybdates was measured in the 15-1000 K range to characterize the phase transition. F e M o O 4 was sealed in an evacuated silica tube to prevent oxidation. Susceptibilities of the other two molybdates were determined in vacuum (10-*torr). The Z~,LT(K) plots (figure 3) give /~eff (and 0 values in parentheses) of 4.98 (28), 4.76 (10) and 3.40 (24) for the LT phases o f Fe, Co and Ni molybdates, respectively, consistent with their formulation as A 2+ Mo 6§ 0 4 with divalent Fe and Co in the high-spin states. FeMoO4 and C o M o O , show a sharp decrease in the susceptibility beyond the transition and the/Left values of the HT phases ( ~ 1-4 BM) are smaller than those expected for either A a+ (HS) Mo 5+ O4 or A2+_x (HS) a 3 + ( . s ) M o t _ x M o ~ O~. One possibility is that the Fe 3+ and Co 3+ are in the low- 6+ 5+

spin state, tlowever, it is more likely that this is due to the itinerant nature of d-electrons

800

" ~ 600

0

E

3

E 400

200

,A 6 X 9 ==--- 6 X

A A & X X

A X =

X X X A

XA AXA

o o

oo

& X o

& X X o o

A x X ~ o ~

6 X oO

& g

0 0 0 0 0 6 & AX X X " o

%xiX xx ooO o ~ 1 7 6

&X ^ oO o

~ X 0 0 0 o

o ooOO o

I I I

200 400 600

T(K)

X X.~

X o X

o X

o

o o

600

450

300

150

Figure 3. X,; LT(K) plots of FeMoO4 (circles), CoMoO4 (crosses) and NiMoO, (triangles).

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296 R A Mohan Ram and J Gopalakrishnan

in the Hr phases. Accordingly, we do find that HT FeMoO4 shows a considerably lower electrical resistivity ( ~ 50ohrn-cm) than LI FeMoO4 ( ~ 3 x 103 ohm-cm); the lower resistivity o f HT FeMoO4 would arise from the itinerancy o f the d-electrons caused by the mixed valency.

4. Conclusions

Transition metal molybdates o f the formula AMoO4 where A = Fe, Co or Ni exhibit a first order phase transition between 670 K and 970 K. An investigation of the low temperature and high temperature phases by various physical methods including x-ray photoelectron spectroscopy and magnetic susceptibility measurement has revealed that the phase transition is associated with a valence change of the type, A 2 + + Mo 6 § ~ A 3 +

+ Mo 5 § at least in the cases o f Fe and Co molybdates.

Acknowledgements

The authors wish to express their grateful thanks to Professor C N R Rao, for suggesting the problem and for valuable discussions. Thanks are due to the uc, c and the DST, New Delhi, for support of this research.

References

Abrahams S C and Reddy J M 1965 J. Chem. Phys. 43 2533

Chojnacki J, Kozlowski R and Haber J 1974 J. Solid State Chem. I1 106

Manthiram A, Sarode P R, Madhusudan W H, Gopalakrishnan J and Rao C N R 1980 J. Phys. Chem. 84 2200 Rao C N R, Sarma D D, Vasudevan S and Hegde M S 1978 Proc. R. Soc. London A367 239

Sarma D D and Rao C N R 1980 J. Electron Spectrosc. Relat. Phenom 20 25

Sarode P R, Madhusudan W H, Ramasesha S and Rao C N R 1979 J. Phys. CI2 2439 Sieber K, Kershaw R, Dwight K and Wold A 1983 lnorg. Chem. 22 2667

Sleight A W and Chamberland B L 1968 lnorg. Chem 7 1672

Sleight A W, Chamberland B L and Weiher J F 1968 Inorg. Chem. 7 1093 Smith G W and Ibers J A 1965 Acta Crystallogr. 19 269

Vasudevan S, Vasan H N and Rao C N R 1979 Chem. Phys. Lett. 65 444

References

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