Spectroohimica
Ireland Press,1976. Printedin Northern Acta, Vol. 32A, pp. 1155to 1157. Persamon
The i.r. spectra of several rare-earth formates J. TH. M. DE HOSSON~, J. P. M. MAAS and M. P. GROENEWEGE Vakgroep Algemene Chemie, State University Utrecht, The Netherlrmds (Received 8 July 1976) Abstract-The i.r. spectr8 of some rem-earth formates 8re recorded in the mnge 400940 cm-‘. The following compounds were studied: CB(HCO~)~, Pr(HCO&, Nd(HCO,),, Sm(HCO,),, Eu(HCO,), and Gd(HCO,),. Some compounds were 81~0studied upon de&oration and at lowered temper&true. Nearly 811bands could be assigned asd the expected fctctor group splitting was observed. A shift to higher frequencies wes observed with increasing atomic number.
INTRODUCTION
RESULTS
FERRARO and BECKER [l] have studied La(HCO,),, Le(DCO,),
and Nd(HCO,),;
they
ment in terms of metaloxygen far
i.r. frequencies.
bands
according
We
to the factor
the c8se of gadolinium the
structure
formate,
has been
oerium-,
recorded clusion
formctte. spectra
are The
from
8nd indicates
that
all
an8lysis
in
by
18ttice
GY
and
with
gado-
resemblance
of all
supports
Mayers
con-
europium
formate
also
of gadolinium
belongs in this series.
has
spacegroup.
Table
of the factorgroup
1 contains
an8lysis.
Table
2
Ntot
Nac
N
tr
N
NpTm3te rot
activity
1nt
Table 2. W8venumbers and assignments for gadoliniumformate
EXPERIMENTAL All compounds were prepared by dissolving the oxydes (FLUKA, puriss.) in diluted nitric &cid, precipitating the carbonates by 8dding sodiumcarbonato (BDH, Analar). The precipitates were washed out with deionized water until 8 pH of ‘7-8 w&s obtained. These washed out precipitates were dissolved in formic 8cid (BDH, Analsr). When the precipitated carbonates were still wet, the formed formates st8yed dissolved and could be obtained by slow eveporation. Dried, the carbonates gave 8 solid state reaction without dissolution of the formate. Only gadolinium formate is soluble in water. We used both methods without distinction. Checking upon one compound revesled that there is no difference in the spectre, indicating, that the structure of the compounds, -made by the two methodsis identical. The spectra, were recorded 8s potassiumbromide discs and polyethylene discs on 8 Hitachi EPI G3 i.r. 8nd 8 Beckman-RIIC FS 720 Fourier f8r i.r. spectrophotometer. The low temperature spectra were recorded using &home-madeliquidnitrogen cryostat,which could attain st least -160’ C.
Description
”
C-8
Y
o-c-ii
2915
)
Gd(DC0 1: 2220
1583
c-o asp 6
cdiiico
0rvc-i) (
Ode-c-n
vC-O~w
7575
'15116
7413
1059
1368
( 1328
i 1360
%CO*) Or b(C0,)
13LO
917
6o-c-o 307 298 265 233 198 178 168
155
136
t present address: Laboratorium voor Fysische Metealkunde, Nijenborgh 18, Groningen, The Netherlands. 10
formate
It h8s 8 rhombohedml
Tctble 1. Fsotor group splitting for gadolinium formate with spacegroup Cgp
studies,
neodymium-
Css,(R3m)
the results
PAESST [Z].
his X-ray
isostnmtural striking
greatly
for some nearly
for which compound
praseodymium-,
semariumformate linium
group
revealed
MAYER [3] has concluded that
assign
structure
been studied by PAEST [2].
gave an assign-
stretching
could
The crystal
1156
Intensity
Overtone and combination
bands.
Ga(Hco2)3
2840
Gd(DC02)3
assignment
3545
2220 + 1328
2987
2220 + 780
2913
2 x 1583
2853
1546 + 1340
2633
2 x 1328
2375
1328 + 1059
2160 1328 + 780
2090 1426 (v)
1436 (str)
1358
Table 3. Wavenumbers for the rare-earth formates
rco 2
DCO2 3545 2987
'208'
*2856a
2918
2918
!915
2845
2845
!840
2220
v
2913 2840
2830 2750
2763
2675
2685
2853
2633 2375 2160 2090
*..1605~ * 1580"
158Sa 1550*,
1428' * 1405L
1056~
1600
1583
br ,str
1578
1575
1546
sh or shp
1432
1432
1436
1426
stlp.str
1408
1410
1410
1413
1059
silp,str
1382
1383
1380
1358
Y.Y.
1368
1340
shp,str sh or shp
1596
1586’
1595
1575
1544
1582
1577
1578
1425
1415
1429
1430
1404
1052
1409
1598
1594
1602
* 1358’
i334*
332
1362
I 365
1365
1366
*
1328
322
1357
1359
i357
1358
360
1328
915
?ngl
1100
1093
,090
917
T.V.
775
786
786
786
789
‘180
shp .m
778
780
778
780
283
286
292
282&
303
300
240~
265
* *
77ga
* *
307
shp
306
298
br,str
261
266
265
br ,str
306
*
280a
sh or shp
*
26aa
250
253
253
*
238
228
233
228
240
236
236
233
br,str
198
197
194
203
198
sh or shp
186
* 16ya
174
178
183=
185
178
180
178
br,str
150a
155
161
163~
169
166
168
155
m.shp
J(’ 1218
124
132
133a
139
t37-
141
136
m,shp
* *
a)
data from Ferraro
g
= fundamental
and Becker
[l]
1156
1167
The ix. spectra of several rare-earth formates Table 4. Calculations of the moments of inertia for the formatsgroup in Gd(HCO,), and Gd(DCO,),. Data for carbon and oxygen are taken from PABST [2]. The hydrogen atom is supposed to have a carbonhydrogen distance of 1.09 A and to make equal angles with the two carbon-oxygen bonds -
EC0
DCOp
L9.5cl4
8.281
0.95L
0.724
/
Rario
41.218
6.000
41.217
2
203fi9a
0.9753
100/17a
0.9888
2.3390
L1.820
1.ooo
0.0
7.8855
2.5307
0.0
6.0126
1.5063
0.0
5.9s
3.1357
0.0
6.387;
1 1
Nd
1
I 1 I
0.9645
the observed
ments
for
and the assign-
formate.
In
listed the data for all the studied indicating
the resemblance
as the shift
in frequency
Table
3 are
formates,
clearly
of the spectra
as well
with
increasing
atomic.
number.
The assignment formate hyde
[6],
assuming
numbers
formate
[l]
the E-mode
than the Al-mode;
“molecular”
argument,
that
The
higher
bands
on the vibra-
than the symmetfeature
in this region
Ferraro
and Becker
(I&,).
the shifted
in the 1400-
are assigned
as a splitting
Their
by
of the in plane
deuteration
study
showed
band to be single, thus the splitting
the rocking
being
showed
undetectable.
what
between
These
bands
the are
therefore
two
of the
very weak band some-
bands
from
temperature
that
of
Our deuteration
the same shift for the lower
two bands and a remaining
think
in wave-
region.
two
rocking
study
and formalde-
asymmetrical
There is a striking
1460 cm-l
wave-
for sodium
this is based
tions are higher in wavenumbers rical ones.
formate
on the assignment
[4], lanthanum
1
I
I
I I
I I
I
Gd(CHO,),.
independent;
this band
we
is a combination
I
I
I
I I
II I I I I
I I
I
I
I I
I
IA I
I
1550 1450
1400
In gadolinium
for the internal
is based
I I
I I
I
I?.
I’ I
I
1350
750
Fig. 1. Wavenumbers for the rare earth formates Ce, Pr, Nd, Sm, and Gd. The shift to higher wavenumbers and the increase of crystal field splitting in the series cerium to gadolinium. For comparison some of the wavenumbers of sodiumformate are given (Na: solid, Na* : aqueous solution).
DISCUSSION
numbers
I I
I600
frequencies
gadolinium
I
I I
I
I
Pr
100
I
I
Ce
Eu
iLlI
150
I
NO
Cd
0.9226
200
1
No*
Sml
16l3/155
contains
250
300
symmetry, metry
formate
the formate
species and can mix.
The assign
translational
modes
are more
diacult
to
; the spectra show 3 broad bands with in
some spectra
an additional
sharp band.
tion gives only a very small calculated cannot
be seen in the spectra,
accuracy
in the wave number
We think therefore the
ion has C,
thus R, and R, are in the same sym-
region
modes,
to distinguish additional
because
of the in-
of the broad
bands.
that the three broad bands in
200-300 cm-l
translational
Deutera-
shift, which
are
the
but we have
them between
sharp bands
T,,
three
species
no information T, and T,.
The
must then be assigned
to
the A, species. Assuming changes
an
identical
structure
in the cell dimensions
see the shift to higher frequencies the crystal
field
with increasing
splitting atomic
small to
and the increase of
of nearly
number,
with
it is remarkable
all vibrations
as shown in Fig. 1.
band, which owing to Fermi resonance has grown in intensity. Deuteration assignment
studies
are
very
of the librational
the results are listed of calculations of
inertia
formate.
for
Studies
site symmetry ‘Rw
’
formate.
the
‘RR.
formategroup
on sodium
for the formate
helpful
modes.
in
the
In Table
4
of the moments in
formate
gadolinium [6] with
ion indicate
C’s
QRz >
more clearly than in the case gadolinium
[l] [2] [3]
[4] [5]
[6]
J. R. FERRARO and M. BECKER: J. Iwor. Nucl. Chem., 24, 637 (1962). A. PABST: J. Chem. Phys., 11, 145 (1943). I. MAYER, M. STEINBERQ, F. FEIQENBLATT and A. GLASNER: J. Chem. Phya., 66, 1737 (1962). R. NEWMAN: J. C&m. Phys., 20, 1663 (1962). P. COSSEEand J. H. SCEACHTSCRNEIDER: J. Chem. Phys., 44, 97 (1966). to be published.