PHYSICAL REVIEW B
107
, 054312 (2023)
Nonharmonic contributions to the high-temperature phonon thermodynamics of Cr
C. M. Bernal-Choban
,
1
,
*
,
†
H. L. Smith
,
2
,
*
,
‡
C. N. Saunders
,
1
D. S. Kim
,
3
L. Mauger,
4
D. L. Abernathy
,
5
and B. Fultz
1
,
§
1
Applied Physics and Materials Science, California Institute of Technology, Pasadena, California 91125, USA
2
Physics and Astronomy, Swarthmore College, Swarthmore, Pennsylvania 19081, USA
3
Department of Materials Science and Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
4
Jet Propulsion Laboratory, Pasadena, California 91109, USA
5
Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
(Received 14 June 2022; revised 21 December 2022; accepted 15 February 2023; published 27 February 2023)
Phonon densities of states (DOSs) of body-centered cubic chromium were measured by time-of-flight inelastic
neutron scattering at temperatures up to 1493 K. Density functional theory calculations with both quasiharmonic
(QH) and anharmonic (AH) methods were performed at temperatures above the Néel temperature. Features in the
phonon DOSs decrease in energy (soften) substantially with temperature. A Born–von Kármán analysis using fits
to the experimental DOSs reveals a softening of almost 17% of the high-transverse phonon branch between 330
and 1493 K. The low-transverse branch changes by approximately half this amount. The AH calculations capture
the observed behavior of the two transverse phonon branches, but the QH calculations give some inverted trends.
Vibrational entropies from phonons and electrons are obtained, and their sum is in excellent agreement with the
entropy of chromium obtained by calorimetry, indicating that above 330 K, no explicit temperature-dependent
magnetic contributions are necessary.
DOI:
10.1103/PhysRevB.107.054312
I. INTRODUCTION
Understanding the vibrational, electronic, and magnetic
interactions in condensed matter is fundamental to predicting
the thermodynamic functions of materials such as free energy,
internal energy, and entropy. These thermodynamic functions
are essential for constructing phase diagrams, predicting ther-
mal expansion, and explaining the temperature dependence of
elastic constants, bulk moduli, and magnetization [
1
]. There
are active investigations into these topics for their own sake,
and for their importance to the structure and properties of
materials [
2
–
7
].
One intriguing system is body-centered cubic (bcc)
chromium, whose vibrational, electronic, and magnetic free
energy contributions result in a transition from an antiferro-
magnet to a paramagnet, and show an apparent anharmonicity
with increasing temperature [
8
]. Below the Néel transition
temperature,
T
N
=
311 K, a single crystal of Cr is a con-
ventional itinerant antiferromagnet [
9
]. At
T
N
, Cr retains the
bcc structure but becomes paramagnetic [
10
,
11
]. In general,
the free energy of Cr,
F
, requires three contributions to the
entropy
F
(
M
,
V
,
T
)
=
U
−
T
(
S
mag
+
S
ele
+
S
vib
)
,
(1)
where
M
is magnetization,
V
is volume,
T
is temperature,
U
is the internal energy,
S
mag
is the magnetic entropy,
S
ele
is
the electronic entropy, and
S
vib
is the vibrational entropy. The
*
These authors contributed equally to this work.
†
cmbchoban@gmail.com
‡
hsmith@swarthmore.edu
§
btf@caltech.edu
S
vib
gives most of the total entropy at higher temperatures,
even in a harmonic model with fixed phonon frequencies,
{
ω
s
}
[
1
]. Phonon frequencies change with volume, and the
“quasiharmonic” (QH) approximation assumes that phonon
frequencies,
ω
s
(
V
(
T
)
)
, depend on temperature only through
thermal expansion. The “anharmonic” (AH) approximation
includes an independent change with
T
, i.e.,
ω
s
(
V
,
T
).
The lattice dynamics of Cr show large anharmonic con-
tributions at high temperatures [
8
]. Transitions from the
antiferromagnetic to the paramagnetic states are not well
understood for Cr [
12
–
16
]. It has been suggested that mag-
netic fluctuations exist above 1000 K [
15
,
17
]. These issues
of magnetism and anharmonicity continue to drive work
on the high-temperature thermodynamics of Cr. Calorimet-
ric (JANAF) measurements and third-generation CALPHAD
models provide values for the total entropy of Cr,
S
tot
(
T
)
[
18
,
19
], but not the individual components of Eq. (
1
).
Here we use time-of-flight (TOF) inelastic neutron scatter-
ing (INS), Born–von Kármán (BvK) analyses, temperature-
dependent effective potential modeling, and non-spin-
polarized density functional theory (DFT) to determine the
individual contributions
S
vib
,
S
ele
, and
S
mag
, from 330 to
1493 K. Our AH calculations, which include contribu-
tions from electrons and phonons, largely account for the
values of
S
tot
(
T
) observed with recent calorimetry mea-
surements and match observed lattice expansion. The QH
approximation also gives a vibrational entropy close to that
observed with TOF INS, but this success is caused by a
canceling effect of individual phonon branches. The BvK
analyses of TOF data support AH phonon branch behav-
ior. A comparison of TOF INS and anharmonic calculations
reveals that AH computations capture most, but not all,
experimentally observed phonon behavior. This additional
2469-9950/2023/107(5)/054312(8)
054312-1
©2023 American Physical Society
C. M. BERNAL-CHOBAN
et al.
PHYSICAL REVIEW B
107
, 054312 (2023)
nonharmonic behavior is unexplained but is not explicitly
magnetic in origin. In summary, we find that temperature-
broadened electronic and third-order anharmonic contribu-
tions reproduce experimental thermodynamic measurements
well, and no purely magnetic interactions are needed to ex-
plain the thermodynamics of Cr above 330 K.
II. METHODS
A. Inelastic neutron scattering
Inelastic neutron scattering (INS) measurements were
performed on electrochemically deposited plates of polycrys-
talline 99.995% Cr. Two pieces of Cr that gave a large area
for scattering were secured inside a niobium foil sachet sur-
rounded by a frame of boron nitride. All data were taken at
the time-of-flight wide Angular-Range Chopper Spectrometer
(ARCS) at the Spallation Neutron Source (SNS) at Oak Ridge
National Laboratory (ORNL) [
20
]. The incident energy was
70 meV with the Fermi chopper at 420 Hz and the
T
0
chopper
at 90 Hz. Sample temperatures varied from 6–1493 K. Below
330 K, a closed-cycle helium refrigerator was used. For mea-
surements at higher temperatures, samples were transferred to
the high-temperature MICAS furnace [
21
].
Data were reduced to phonon density of states (DOS)
curves by subtraction of an empty Nb sachet and were
corrected for multiphonon scattering with Mantid and the
Multiphonon package [
22
,
23
]. Integration to produce the
phonon density of states was performed for values of 3.5 Å
−
1
<
Q
<
10 Å
−
1
, where magnetic scattering contributes less
than 1.5% of the total scattering. This ensured that the scat-
tering intensity used to obtain the density of states was
vibrational in origin. Additional corrections to account for
sample curvature were performed in MCViNE [
24
] (see Sup-
plemental Material [
25
] for more details).
B. Born–von Kármán analysis
Analyses of TOF INS DOSs were performed using the
Born–von Kármán (BvK) model [
26
]. This model takes a
crystal to be a set of nuclear masses whose interactions act like
springs that provide restoring forces against the displacements
of nuclei. By transforming the forces associated with these
displacements into a dynamical matrix, the BvK model has
often been used to fit phonon dispersions. Fitting phonon DOS
spectra with the BvK model is more involved because the
DOSs are aggregates of all phonon modes in reciprocal space.
To address this challenge, trial force constants were used
to construct a dynamical matrix,
D
(
q
)
,
using the underlying
symmetries of the crystal lattice. A sufficiently dense set of
q
points in the first Brillouin zone was used to collect the
spectrum of phonon frequencies,
ω
, for each temperature:
M
ω
2
=
D
(
q
)
,
(2)
where
M
is the mass of the atom and
is the polariza-
tion of the phonon mode corresponding to reciprocal space
vector
q
. This BvK model was embedded in a genetic al-
gorithm global optimization framework, where trial sets of
force constants were generated randomly according to the
differential evolution algorithm [
27
]. Each optimization was
repeated several times to ensure convergence. The resulting
DOSs are compared with experimental data. For Cr, a BvK
model including atomic interactions through the second near-
est neighbors (four tensorial force constants) was found to
be sufficient. More details of the fitting process are in the
Supplemental Material [
25
].
C. Computation
All density functional theory (DFT) calculations were
performed with the Vienna
Ab Initio
Simulation Package
(VASP) [
28
–
30
]. Plane-wave basis sets with a kinetic energy
cutoff of 600 eV and projector-augmented-wave pseudopo-
tentials [
31
,
32
] were used with Perdew-Burke-Ernzerhof
(PBE) exchange-correlation functionals [
33
,
34
]. Each calcu-
lation used a 6
×
6
×
6 supercell consisting of 216 atoms.
Monkhorst-Pack [
35
]
k
-point meshes of 4
×
4
×
4 and 8
×
8
×
8 were used for vibrational and electronic supercell cal-
culations, respectively.
We performed spin-polarized DFT calculations at 1000 K
from initial paramagnetic, ferromagnetic, and antiferromag-
netic spin configurations. Upon convergence, the magnetic
polarizations in all cases were less than 0.08
μ
B
on individual
atoms and less than 0.05
μ
B
in the orientational averages of
spins. Calculations were performed for positive and negative
dilations of the lattice, with no notable effect on the converged
magnetic polarization. To balance computational cost with
supercell size and complexity, non-spin-polarized calculations
were used for the phonon dynamics.
1. Quasiharmonic
Phonon calculations within the quasiharmonic approxi-
mation were conducted with Phonopy [
36
]. A finite atomic
displacement was introduced into each supercell of a grid
of minimized 0 K supercells scaled by
±
0
.
5%
,
±
1%
,
±
1
.
5%
volume. Static calculations of each were converged to within
10
−
7
eV for accurate force constant determination. The har-
monic approximation from
T
=
0–1500 K was applied to
each volume, and a grid of these free energy curves was
fitted to a Birch-Murnaghan equation of state. The mini-
mized volumes at 330, 1000, and 1500 K were used to
create corresponding dynamical matrices and predict phonon
properties. A
q
-point mesh of 70
×
70
×
70 was necessary
for proper convergence, and the calculated phonon DOSs
were convoluted with a Gaussian of 1.0 meV to approximate
the broadening at higher phonon energies from the in-
strumental resolution. Lattice and thermodynamic properties
calculated within this approximation depend on tempera-
ture only through a volume mapping,
ω
=
ω
(
V
(
T
)
)
.More
details on this process are provided in the Supplemental
Material [
25
].
2. Anharmonic
Anharmonic contributions to thermodynamic properties
were calculated using the stochastic temperature-dependent
effective potential method (sTDEP) [
37
]. In this procedure,
the Born-Oppenheimer surface of a material at a given
temperature is represented using a collection of static cal-
culations on supercells of thermally displaced atoms. These
displacements were generated by a stochastic sampling of a
054312-2
NONHARMONIC CONTRIBUTIONS TO THE ...
PHYSICAL REVIEW B
107
, 054312 (2023)
canonical ensemble at the temperature of interest. The ener-
gies, forces, and displacements of each configuration were
tabulated and used to generate force constants with a least-
squares fit to a model Hamiltonian,
H
=
U
0
+
∑
i
p
2
i
2
m
i
+
1
2!
∑
ij
αβ
αβ
ij
u
α
i
u
β
j
+
1
3!
∑
ijk
αβγ
αβγ
ijk
u
α
i
u
β
j
u
γ
k
,
(3)
where
u
{
i
,
j
,
k
}
is the displacement of atom
{
i
,
j
,
k
}
and
α, β, γ
are the Cartesian components. The temperature-dependent
U
0
is a fit parameter for the baseline of the potential energy sur-
face. The sum containing
ij
, the quadratic force constants,
captures some anharmonic and electron-phonon effects at a
given temperature, and the final sum includes phonon-phonon
interactions through the cubic force constants,
ijk
. The latter
two terms in the model Hamiltonian are used to calculate
anharmonic shifts and broadenings of phonon modes with
respect to temperature. The force constants computed with
this method include explicit temperature and volume depen-
dencies.
A grid of 36 volumes and temperatures was created. For
each point on the grid, an ensemble of ten supercells was
generated with stochastically displaced atomic positions. DFT
calculations were performed on each supercell to obtain
energy-force-displacement data. The resulting energies were
fitted to the Birch-Murnaghan equation of state to find the
optimized volume for a given temperature. This volume and
the calculated force constants were used to create another set
of configurations on the temperature volume grid, and the
minimization process was repeated. In this way, the force con-
stants are numerically converged with respect to the number
of configurations and supercell size. The final minimized free
energies were utilized to calculate the equilibrium volume
at each temperature, and phonon properties were evaluated
at these conditions. Renormalization of phonon frequencies
due to anharmonicity was included in these evaluations. Us-
ing phonon self-energy corrections from many-body theory
[
26
,
38
],
∑
(
)
=
(
)
+
i
(
), shifts and broadenings of
the phonon DOS were calculated. Further details are provided
in the Supplemental Material [
25
].
III. RESULTS
Phonon densities of states (DOSs) from TOF spectra of
Cr are shown in Fig.
1
. Shifts of the phonon DOSs from
6–1493 K follow the expected trend of “softening,” or reduc-
tion of energy, with an increase in temperature. Interestingly,
above 600 K, the three defined mode peaks (low transverse,
T
2
, high transverse, T
1
, and longitudinal, L) appear as two
peaks. This is traced to a large thermal softening of approx-
imately 8 meV of the high-transverse mode between 6 and
1493 K.
Figure
2
shows the temperature dependence of the phonon
dispersions between 6–1493 K, obtained by fitting the ex-
perimental DOSs to a BvK model [
27
]. We performed fits
iteratively using a genetic algorithm optimization [
39
](see
Sec.
II B
). Along the
→
H
→
P
→
pathway, the trans-
FIG. 1. Cr phonon DOSs from 6–149 K measured by TOF.
Curves are offset for clarity, and the 333 K dataset is overlaid with
the 1493 K curve to show the magnitude of the shift between 333
and 1493 K. Experimental error bars (based on counting statistics)
are not shown because their height is approximately the width of the
line used to connect data points.
FIG. 2. Phonon dispersion relations from force constant opti-
mization of BvK fits of the experimental phonon DOSs (333–
1493 K). Two nearest neighbors (four variables) were considered in
the fit.
054312-3
C. M. BERNAL-CHOBAN
et al.
PHYSICAL REVIEW B
107
, 054312 (2023)
verse modes are degenerate and exhibit a softening similar
to the longitudinal mode. From N
→
, there is a branch-
dependent decrease in energy with respect to temperature. We
illustrate these shifts relative to 330 K at each high-symmetry
point in Fig.
3
. The largest softening (of approximately 17%)
occurs in the high-transverse mode between 330–1493 K. This
behavior is consistent with the DOSs of Fig.
1
.
Figure
4
shows the calculated and experimental DOSs
at 330, 1000, and 1500 K. Colored bars representing mode
peaks fitted to three Lorentzians show the average shift of
each feature. Densities of states calculated with sTDEP show
similar peak location, shape, and softening to the experimental
spectra at 330 and 1500 K. Our quasiharmonic predictions
do not accurately reproduce the features in the DOS at these
temperatures, indicating that anharmonicity is important for
the thermal trends of phonons in Cr.
Our experimental and calculated phonon dispersions at
330, 1000, and 1500 K are plotted in Fig.
5
. Quasiharmonic
and anharmonic calculations agree well with experimental
data along most of the high-symmetry reciprocal space path-
ways. A notable exception is the N
→
direction, where the
QH low-transverse modes show an anomaly at the N point,
and the high-transverse modes do not shift as strongly as
expected. The AH and QH calculations also give different
magnitudes of the longitudinal mode along the
→
H path.
A way to assess the thermodynamic consequences of an-
harmonic phonon behavior is by calculating entropy. Figure
6
shows the electronic, vibrational, and electron-phonon com-
ponents of entropy and their respective contributions to the
total entropy as determined by JANAF [
18
].
The calculated lattice expansions are compared to exper-
imental results in Fig.
7
. Both QH and sTDEP
ab initio
calculations are in agreement with lattice parameters obtained
from the elastic region of our neutron scattering measure-
ments, and with previous experimental results that are labeled
in the figure.
IV. DISCUSSION
A. Phonons
The experimental phonon DOSs of bcc Cr show significant
softening at elevated temperatures, and the apparent disap-
pearance of one of the Van Hove singularities in Fig.
1
is
a result of this temperature dependence. Phonon dispersions
calculated with fitted force constants show that the largest
softening occurs in the high-transverse mode. At the high-
symmetry points,
, H, and P, the two transverse branches are
degenerate. At the N point near 1000 K, Fig.
3
shows a soft-
ening of the high-transverse (T
1
) mode and little softening of
the low-transverse (T
2
) mode. The shift of the high-transverse
mode from
∼
32 to
∼
27 meV confirms that features in the
phonon DOS with the largest thermal softening are asso-
ciated with the T
1
[
ξ,ξ,
0] phonon branch. At the N point,
this T
1
mode involves the opposing displacements of two
neighboring (110) planes along the [1
10] direction [
40
]. The
relatively small thermal softening of the low-transverse mode,
T
2
[
ξ,ξ,
0], up to 1000 K also may originate from interactions
beyond the harmonic approximation.
FIG. 3. Thermal shifts, relative to ambient temperature, of the
phonons in Cr at each non-
high-symmetry point for (a) our TOF
measurements, (b) previous triple-axis experiments [
40
], (c) AH
calculations, and (d) QH calculations. A comparison of the thermal
shifts for each method at 1500 K for the T
1
and T
2
modes at the N
point is shown in (e).
At 330 K, the high-transverse and longitudinal modes in
the DOS have higher energies in the QH calculations than
from TOF measurements and anharmonic sTDEP calcula-
tions. This overestimation of peak locations continues to
054312-4
NONHARMONIC CONTRIBUTIONS TO THE ...
PHYSICAL REVIEW B
107
, 054312 (2023)
FIG. 4. Phonon densities of states at 330 (bottom), 1000 (mid-
dle), and 1500 K (top). Each panel compares the experimental
phonon DOS (dark blue) to the calculated DOSs from quasiharmonic
(purple) and anharmonic (light blue) approximations. The colored
markers indicate peak locations from a Lorentzian fit to the features
of the DOSs.
1500 K. Consequently, the shape of the DOS is skewed in
the QH approximation, with more features appearing at higher
energies than those found with measurements and sTDEP
calculations. The agreement of the DOS calculated with the
AH approximation and TOF measurements is excellent at
330 and 1500 K, despite some excessive broadening of the
longitudinal Van Hove singularity.
There is a general agreement of phonon dispersions calcu-
lated with each model and experimental data at 330, 1000, and
1500 K along
→
H
→
P
→
(Fig.
5
). However, the QH
approximation inverts the energies of the T
1
and T
2
modes
at the N point. This is accentuated by the anomaly in the
low-transverse branch behavior at N in the QH dispersions.
This discrepancy is better seen with Fig.
3(e)
.IntheQH
approximation, the low-transverse branch shows the largest
thermal softening at N. This disagrees with the general trend
seen in the experimental data and AH calculations: the high-
transverse phonon branch has the larger thermal softening.
Quasiharmonic models sometimes predict accurate macro-
scopic properties without capturing the underlying phonon
physics [
43
,
44
].
FIG. 5. Comparison of experimental and calculated phonon dis-
persion relations at 330 K (bottom), 1000 K (middle), and 1500 K
(top). Symbols to distinguish the low transverse (diamonds), high
transverse (circles), and longitudinal (triangles) phonon branches are
also shown. Anharmonic (light blue) and quasiharmonic (purple) dis-
persions are in good agreement with a BvK fit to experimental data
(dark blue) and existing triple-axis data (gray) [
40
]. The anharmonic
calculations capture behavior along the H to P high-symmetry path
better than the quasiharmonic simulations.
We attribute the failure of the QH approximation in Cr to
the underlying assumption of noninteracting phonons. This
assumption is known to fail at higher temperatures, where
temperature-dependent phonon-phonon interactions begin to
dominate [
1
,
45
–
47
]. The QH model cannot capture these
effects because the frequencies within this model,
ω
=
ω
(
V
(
T
)
)
, incorporate temperature by shifting harmonic fre-
quencies with changes in volume. This approach ignores
terms beyond the quadratic phonon self-energy, which are
needed for lifetime broadening and purely temperature-
dependent (AH) shifts. Our sTDEP calculations include
cubic order corrections of the phonon self-energy, so
ω
=
ω
(
V
,
T
).
The QH approximation did not successfully predict the
thermal softenings of individual phonons, but there is rea-
sonable agreement between the vibrational entropy calculated
with QH and AH methods. The change in phonon frequency
at the N point gives insight into why. Summing the fractional
thermal shifts (T
1
+
T
2
+
L) from the QH calculations at the
N zone boundary gives a change of about 22%. A similar
sum for our AH calculations gives a change of 26%, which is
054312-5
C. M. BERNAL-CHOBAN
et al.
PHYSICAL REVIEW B
107
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FIG. 6. Components of entropy compared to the total JANAF
entropy [
18
]. (Bottom) Electronic entropy including temperature-
dependent electron-phonon coupling. (Middle) Vibrational entropy
calculated from DOSs using TOF INS, a quasiharmonic approxima-
tion, and an anharmonic approximation. (Top) Sum of the electronic
and vibrational components of entropy from experiment and compu-
tations versus the calorimetric total entropy.
FIG. 7. Lattice expansion of Cr from 6–1500 K with respect
to ambient temperature. Previous lattice expansions are reproduced
from [
41
,
42
].
comparable. This shows some cancellation of errors in the av-
erage behavior of phonon branches from the QH calculations,
giving them better success with the vibrational entropy.
Likewise, a good prediction of thermal expansion does
not validate the QH approximation for predictions of phonon
physics. Using
∂
2
F
∂
V
∂
T
=−
β
B
T
(4)
and
F
(
V
,
T
)
=
U
(
V
,
T
)
−
TS
(
V
,
T
), it is evident that thermal
expansion,
β
, and bulk modulus,
B
T
, are explicitly dependent
on both volume and temperature. Any cancellation of errors
introduced in calculated entropy will be present in predictions
of thermal expansion (and bulk modulus). It is therefore plau-
sible that the QH approximation can successfully reproduce
the thermal expansion of Cr (Fig.
7
), even with the wrong
thermal trends of individual phonons.
There is an underestimation of 4% in the sTDEP vibra-
tional entropy at 1500 K, illustrated in the middle panel of
Fig.
6
. This is caused by an overbinding in the generalized
gradient approximation (GGA) for Cr [
48
], which also affects
our ground state lattice parameter (
a
=
2
.
845 Å). This is
consistent with the
∼
4% average overstiffening of the phonon
dispersions (Fig.
5
), and the slight underestimation of the
lattice expansion (Fig.
7
). A similar effect occurs in our QH
calculations.
B. Entropy and free energy
The top panel in Fig.
6
shows that for temperatures up
to 600 K, the phonon entropy from TOF INS experiments
accounts for nearly all of the total entropy [
18
]. At 1500 K,
the
S
vib
from TOF measurements or calculations accounts for
over 89% of the total entropy of Cr. The remainder originates
primarily from the occupancy of electronic states, the change
of these states with temperature, and perhaps magnetic en-
tropy [
15
,
17
].
Figure
6
shows that an electronic entropy
S
ele
, calculated
first by including the temperature dependence of the electronic
entropy through the Fermi-Dirac distribution with the ground
state electronic states, brings the sum of entropies
S
tot
closer
to the JANAF thermodynamic data, where
S
tot
=
S
vib
+
S
ele
+
S
mag
.
(5)
Thermal motions of atoms broaden the electronic states
through electron-phonon interactions. This temperature de-
pendence was calculated with supercells consisting of ther-
mally displaced atoms obtained by sTDEP at 330, 1000, and
1500 K, and is shown in Fig.
6
. The electronic entropy was
also calculated by the simpler process following Thiessen [
49
]
and Grimvall [
50
], where the ground state electronic DOS,
ρ
gnd
(
E
), is convoluted with a function of Lorentzian form
ρ
(
E
)
=
ρ
gnd
(
E
)
∗
L
(2
)
,
(6)
to approximate the effects of electron-phonon interactions
on electronic DOS,
ρ
(
E
). The amount of broadening, 2
=
2
πλ
k
B
T
, used a value of
λ
=
0
.
5[
51
]. Figure
6
shows very
good agreement between these two approaches.
Adding the thermally broadened
S
ele
to the experimental
and computational
S
vib
gives our best estimates of the total
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NONHARMONIC CONTRIBUTIONS TO THE ...
PHYSICAL REVIEW B
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entropy of bcc chromium. Figure
6
shows that the sum of the
measured TOF vibrational and electronic components gives
excellent agreement with the JANAF data from calorimetric
measurements. There is, however, something missing from the
anharmonic phonon calculations, as seen by the inset at the top
of Fig.
6
. A similar discrepancy was found in previous anhar-
monic calculations [
17
], which proposed that the extra entropy
required for agreement with calorimetry was magnetic in
origin. However, the experimental phonon entropy is larger
than these anharmonic calculations, and with the electronic
entropy, the total entropy agrees well with calorimetry. The
discrepancy is in the anharmonic calculations of the phonon
DOS, which are stiffer and give a lower phonon entropy than
the measurements. The additional nonharmonic contribution
to the phonon self-energy is unexplained, but an effect from
phonon-paramagnon interactions could be a candidate. Para-
magnon energies were calculated recently by time-dependent
density functional theory at 0 K [
52
]. These energies were
found to be large, and may not change strongly with tempera-
ture. Showing the effects of paramagnons on phonon energies
at high temperatures may require new computations. Never-
theless, a large, explicit contribution from magnetic entropy is
not needed to account for the thermodynamic entropy of Cr at
high temperatures.
V. CONCLUSIONS
The phonon DOS was measured on bcc chromium from 6
to 1493 K by TOF INS, and calculations of the phonons were
performed with QH and AH approximations using Phonopy
and sTDEP. To obtain detail on individual phonon branches,
the experimental DOSs were fitted to a Born–von Kármán
model using force constants adjusted with a global minimizer.
Both measurements and computations showed significant
thermal softening of the phonons, and a similar average
phonon softening. However, the QH approximation predicted
that the low-transverse branch would soften faster than the
high-transverse branch, whereas the opposite trend is found by
AH sTDEP calculations, and by TOF results from the present
work and a previous study. The thermodynamic entropy of
chromium was obtained from the experimental phonon DOS,
and the electronic entropy from
ab initio
calculations. Their
sum gave an entropy for chromium that was in excellent
agreement with JANAF results obtained by assessing calori-
metric data. An explicit magnetic entropy contribution is not
needed for temperatures above 330 K, but a paramagnon sus-
ceptibility may perturb phonon energies beyond the known
effects of quasiharmonic, anharmonic, and electron-phonon
interactions.
ACKNOWLEDGMENTS
We thank Jiao Y. Y. Lin for his discussions and assis-
tance with MCViNE modeling. This research used resources
at the Spallation Neutron Source, a DOE Office of Science
User Facility operated by the Oak Ridge National Laboratory.
This work used resources from National Energy Research
Scientific Computing Center (NERSC), a DOE Office of Sci-
ence User Facility supported by the Office of Science of the
U.S. Department of Energy under Contract No. DE-AC02-
05CH11231. This work was supported by the DOE Office of
Science, BES, under Contract No. DE-FG02-03ER46055.
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