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Dynamics at
in the half-integer isotropic high spin
molecules
Zaher Salman1, Amit Keren1, Philippe Mendels2,
Valerie Marvaud 3, Ariane Scuiller 3,
Michel Verdaguer3, James S. Lord4, and Chris Baines5
1Technion-Israel Institute of Technology, Physics
Department, Haifa 32000, Israel
2Laboratoire de Physique des
Solides, Bâtiment 510, UMR 8502 CNRS Université Paris Sud,
91405 Orsay, France
3 Laboratoire de Chimie des Métaux de
Transition, URA CNRS 419 Université Pierre et Marie Curie, 75252
Paris, France
4ISIS Facility, Rutherford Appleton Laboratory,
Chilton Didcot, Oxfordshire OX11 0QX, U.K.
5 Paul Scherrer
Institute, CH 5232 Villegen PSI, Switzerland
Abstract:
We investigate the dynamical spin-spin auto-correlation function of
the isotropic high spin molecules CrCu6 (S=9/2), CrNi6
(S=15/2) and CrMn6 (S=27/2 ), using magnetization,
SR
and NMR measurements. We find that the field autocorrelation time
of the molecule's spin at zero and low fields is nearly
temperature independent as
mK. The high temperatures
is very different between the molecules. Surprisingly, it is
identical (
10 nsec) at low temperature. This suggests that
is governed by hyperfine interactions.
High spin molecules (HSM) consist of clusters of metal ions, they are
ordered in a crystal lattice, and coupled by Heisenberg ferromagnetic
or antiferromagnetic interactions with coupling constant J, only
between spins
in the molecule. At low temperatures
kBT<J these spins lie parallel or anti-parallel to each other,
and the molecule is in its ground spin state, where
is high, with quantum number S, and
2S+1 degeneracy. At even lower temperatures,
the
degeneracy can be removed by additional anisotropic interactions such
as the uniaxial term DSz2, or rhombic term
E[Sx2-Sy2] etc. Experiments on the two most famous high
spin molecules Mn12 [1] and
Fe8 [2,3] show that at low T the
main interaction is, indeed, the uniaxial anisotropy, where up and
down spin states
are degenerate, and tunneling is
induced between these states by an additional term in the Hamiltonian
that does not commute with Sz. This quantum tunneling of the
magnetization (QTM) phenomenon has received considerable attention in
recent years, focusing mainly on the additional terms in the
Hamiltonian which are responsible for the tunneling [3,4,5]. Nevertheless, the
theoretical picture is far from being clear and existing models are
controversial, and often contradict each other [6]. In
some cases, even qualitative understanding of the observed
experimental data is absent [7].
In this paper we investigate three simple HSM systems, which are
isotropic (D,E=0). In these systems no tunneling is observed due to
the absence of the uniaxial term DSz2. However, spin dynamics
is observed even at very low temperatures (T=50 mK). Therefore, the
additional terms in the spin Hamiltonian could be probed directly in
these systems. Such a study can highlight the role of phonons
[6,8], dipolar interactions, and nuclear
fluctuations [5] in a simple setup. In addition, it
could serve as a large S limit for isotropic models usually applied
only for the S=1/2 case [6], or it could serve as a
test case for anisotropic HSM models [9].
We present an experimental investigation using three types of
measurements: magnetization, spin lattice relaxation (T1-1) of
muon spin (
SR), and of proton spin (NMR). Our molecules are
[Cr{(CN)Cu(tren)}6 ](ClO4)21 [10],
[Cr{(CN)Ni(tetren)}6 ](ClO4 )9
[11,12] and [Cr{(CN)Mn(tetren)}6](ClO4)9 [10,13] which we label as CrCu6,
CrNi6 and CrMn6 respectively. In these molecules a Cr(III)
ion is surrounded by six cyanide ions, each bonded to a Cu(II), Ni(II)
or Mn(II) ion. The coordination sphere of Cr and Cu/Ni/Mn can be
described as a slightly distorted octahedral. The objective in this
work is to find the spin-spin correlation time
in the three
systems, and to compare them. Our main findings are: (I)
is
nearly T independent at low temperatures, and (II) at very low
temperature
does not depend on S or J in this isotropic
case.
Figure 1:
The magnetization of CrCu6, CrNi6 and CrMn6 as a
function of the external applied field at T=2 K, respectively. The solid
lines are the S=9/2, S=15/2 and S=27/2 Brillouin functions (see text).
 |
In Fig. 1 we show the magnetization M per molecule in units
of
as a function of applied field H for the three
molecules. The data are taken at T=2 K. In all cases M increases
as the applied field is increased. The magnetization reaches a
saturation value of
,
and
in CrCu6, CrNi6 and
CrMn6 respectively. These saturation values are consistent with
6 Cu (S=1/2), Ni (S=1) or Mn (S=5/2) ions ferromagnetically
(or anti-ferromagnetically in the case of CrMn6) coupled only to
a Cr ion of spin 3/2. The solid lines are Brillouin functions of the
respective S. In Refs [10,11,12,13]
the susceptibility was fitted to the one expected from the Heisenberg
Hamiltonian and the values
K,
K and
K where
found. Therefore, the highest spin value of each molecule is well
seperated from other spin states (a few tens of degrees K). High field
ESR measurements (on CrNi6) [14] and susceptibility
measurements (on CrCu6, CrNi6 and CrMn6) found no
evidence for anisotropy, namely,
. This is consistent with
the octahedral character of the molecules.
In our
SR experiments we measure the polarization P(t,H) of a
positive muon spin implanted in the sample, as a function of time t
and magnetic field H, where P(0,H)=1. The field is applied in the
direction of the initial muon polarization. The positive muon decays
to a positron which is emitted in the direction of the muon spin, and
the polarization as a function of time is reconstructed by the
detection of the emitted positrons.
The measurements in all molecules are done at temperatures ranging
from 25 mK up to 300 K, and in fields ranging between zero and
20 kG. These experiments were performed at both ISIS and PSI,
exploiting the long time window in the first facility for slow
relaxation (high T), and the high time resolution in the second
facility for fast relaxation (low T).
Figure 2:
The spin polarization as a function of time. (a) At zero field and
different temperatures. (b) At field H=20 kG and different temperatures.
The solid lines are fits of the data to square root exponential functions.
 |
In Fig. 2(a) and (b) we present the muon spin
polarization as a function of time and for different temperatures in
CrNi6 in zero field, and in H=20 kG, respectively. In zero
field, the relaxation rate increases, as the temperature is decreased,
and saturates at
K. The increase at high temperatures is
caused by thermally activated tarnsitions between excited spin
states. However, at low temperatures, only the ground spin state is
populated, and only transitions within the degenerate ground state are
possible. In contrast, at H=20 kG, and temperatures lower than
K, the relaxation rate decreases as the temperature is decreased,
and does not saturate.
In Ref. [15] we demonstrated that the magnetic field experienced
by the muon in all molecules is dynamically fluctuating even at T=50 mK.
We therefore analyze our data using spin lattice relaxation theory. In this
theory, the polarization of a local probe (muon or nucleus), in the fast
fluctuation limit, is given by
![\begin{displaymath}
P(H,t)=\left( P_{0}-P_{\infty }\right) \exp \left[ -t/T_{1}\right]
+P_{\infty }
\end{displaymath}](img26.png) |
(1) |
where P0 is the initial polarization,
is the equilibrium
polarization [16],
| T1(H) |
= |
A+BH2, |
|
| A |
= |
 |
(2) |
| B |
= |
 |
|
and
is the probe gyromagnetic ratio. The correlation time
and mean square of the transverse field distribution at the probe site in
frequency units
are defined by
 |
(3) |
The fast fluctuation limit is obeyed when
.
In
SR
, and the muon could occupy many different sites
in the sample, because the molecules are fairly large (
Å
diameter) and are embedded in an organic surrounding. As a result one must
average over
. Using the distribution [16]
![\begin{displaymath}
\rho (\Delta )=\sqrt{\frac{1}{2\pi }}\frac{\Delta ^{\ast }}...
...\left[ \frac{\Delta ^{\ast }}{\Delta }\right] ^{2}\right)
,
\end{displaymath}](img37.png) |
(4) |
and allowing for a constant background (Bg) due to muons stopping
outside the sample one obtains
 |
(5) |
where
is the muon spin relaxation rate. This form is
in agreement with the experimental results (see below). In addition,
Eq. 2 still holds, while in Eq. 2 and
,
is replaced by
.
The solid lines in Fig. 2 are fits of the data to
Eq. 5 where P0 is a global parameter. The parameter
Bg is free within 10% of its mean value since the high fields
affect the positron trajectory in a manner that is reflected in
Bg. The fit is satisfactory in all cases apart from the highest
H and lowest T in CrNi6. The relaxation rate
in the different compounds, obtained from the fits is presented in
Fig. 3 as a function of temperature for different values of
H. As pointed out above, at low fields
increases
with decreasing temperatures, and saturates at low temperatures. In
addition the value of
increases as the spin of the
compound is higher, as expected from Eqs. 2-
and 3, and the saturation temperature increases as the
coupling constant J increases. This is in strong contrast to
Mn12 [17] and Fe8
[18] where in zero field
increases
continuously upon cooling until the correlation time
becomes
so long that the molecule appears static in the muon dynamical window,
and no T1 saturation is observed at low temperatures.
Figure 3:
1/T1 as a function of temperatures for different external
fields, measured by
SR and by NMR (after scaling) in (a) CrCu6 (b) CrNi6 and (b) CrMn6.
 |
In Fig. 4 we plot the average relaxation time
at
as a function of H2 for all compounds,
for fields up to 2 kG (note the axis break). We find that
obeys Eqs. 2-
. This implies that
the muon spin relaxation is indeed due to dynamical field
fluctuations, and that at low T the field autocorrelation can be
described by a single correlation time as long as the applied field is
not too strong. At high fields (> 2 kG) we find deviations (not
shown) from the linear relation between T1 and H2. The
deviation might be due to the impact of the field on the spin
dynamics, i.e. the correlation function given by
Eq. 3. From the linear fits in Fig. 4, and taking
from
Eq. 2 and
, where
MHz/kG, we find that for CrCu6
MHz
(
G), for CrNi6
MHz
(
G), and for CrMn6
MHz
(
G); the subscript 0 stands for
. Using
from the same equation we find
nsec for CrCu6,
nsec for
CrNi6 and
nsec for CrMn6. These values
of
and
are self consistent with the
fast fluctuation limit. Most striking is the fact that all
values are nearly equal.
Although our data support a picture where the muon spin relaxes due to
dynamically fluctuating magnetic fields, they leave open the
interpretation of these fluctuations. Are they due to the fluctuations
of the molecular spins or a result of muon diffusion, muonium
formation, etc.? In order to address this question we performed proton
NMR T1 measurements. We find that in all applied fields smaller
than 20 kG the proton T1 is shorter than the experimental
window around the peak in
. Only in a field of
kG were we able to perform the experiment at all temperatures. We
measure T1 using a saturation
pulse sequence. The
proton polarization recovery follows Eq. 1 with P0=0 from
which we obtained T1H.
Figure 4:
The saturation relaxation time as a function of H2 for CrCu6
, CrNi6 and CrMn6. The solid lines are linear fits of the data.
 |
Since the proton gyromagnetic ratio
MHz/kG is very
different from that of the muon, we scale the NMR results and plot them
together with the
SR results in Fig. 3, for CrNi6 (b)
and CrMn6 (c). The scaling factor C used in Fig. 3 is 0.6
for CrNi6 and 8.8 for CrMn6. It was chosen so that the scaled
NMR relaxation rates will agree with the
SR rates at high T. After
this scaling, we find a good agreement between the
SR and NMR data at
all temperatures. In fields lower than 20 kG, where the NMR T1 was
measurable only at high T, we obtained the same agreement between the two
techniques.
The scaling factor provides information on the ratio of the field
experienced by a muon and by a proton. At high temperatures where
T1 shows no field dependence one can assume that
in
Eqs. 2-
, and therefore
. Using the
definition of
given in Eq. 3 we can write
where
is the RMS of the transverse field at the
proton site, and
is the RMS of the field at the muon site in its general sense given
by Eq. 4. The proximity of C to 1 especially in the
CrNi6 is very encouraging and suggests that the muon sites are
close to a proton in this system. Thus, we prove that in both
techniques we are measuring the probe's spin lattice relaxation time
due to the molecular spin fluctuations.
Finally, we would like to obtain the correlation time at all temperatures.
This could be calculated from
combined with magnetization
measurements, at zero (or very low) fields. In zero order approximation we
assume that
is
proportional to
which is different
from S(S+1) since at temperatures
, states other than the
ground state S can be populated. Therefore in zero field
 |
(6) |
Taking
 |
(7) |
where N is the number of molecules,
is Bohr magneton, kB
is the Boltzman factor, and g=2, we find
 |
(8) |
In the insets of Fig. 5 we present
, obtained from
DC-susceptibility measurements and Eq. 7, as a function of
temperature for CrCu6, CrNi6 and CrMn6. In
Fig. 5 we present
as calculated using Eq. 8 for the different compounds. The T dependence of the
correlation time
, unlike the muon spin lattice relaxation
rate, reflects the dynamics of the molecular spin without the T
dependence of the field at the muon site. At
K there is
more than an order of magnitude difference in
between the
different molecules. As the temperature is lowered the correlation
time in all compounds increases as the temperature is decreased, but
reaches a common saturation value of
nsec (within
experimental error) at
K. At this temperature only the
ground state S is populated. In other words, when the HSM are formed
they all have the same correlation time at low T.
Figure 5:
The correlation time
as given by Eq. 8 as
a function of temperature for CrCu6, CrNi6 and CrMn6. The inset
shows
as obtained from Eq. 7
 |
At very low temperatures one can interpret the correlation time
in terms of a broadening of the spin levels, due to interactions
between a molecular spins and other molecular spins, or the
enviroment. This interaction is considered as a purturbation, the
strength of which should be of the order of
. Therefore,
our results have two major indications. First, the broadening in the
limit is not due to phonons since these die out
exponentially with temperature at 0.05-1 K. Second, the broadening
cannot be explained by interactions which are quadratic in S or have
higher S dependence. This rules out the dipolar interaction between
neighboring molecules since in the three compounds the nearest
neighbor distance is
Å. Similarly, crystal field terms
which are allowed by the octahedral symmetry (S4 or higher
[19]) are unlikely.
The only mechanisem suggested to date for level broadening of HSM, which is
weakly (linear) S dependent is the hyperfine interaction between nuclear
and electronic spins. This mechanism can account for the finite spin
lattice relaxation rate at very low temperatures [20]. The
hyperfine interactions in unisotropic high spin molecules were studied
recently [22,23], and their effect on QTM is
becoming clearer [24,25]. We believe that this
interaction also governs the fluctuations of the isotropic molecules at very
low temperatures (T<3 K). However, at high temperature (T>10 K) the
fluctuations are governed by spin-phonon interactions [21].
We would like to thank the ISIS and PSI muon facilities for their kind
hospitality and B. Barbara for helpful discussion. These experiments were
supported by the European Union through its TMR Program for Large Scale
Facilities, the French Israeli cooperation program AFIRST, and the Israeli
Ministry of Science.
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Zaher Salman
2002-10-28