S Shanmukharao Samatham1, Akhilesh Kumar Patel2, Ashish Kumar Mishra3, Alexey V Lukoyanov4,5, Lyubov N Gramateeva4, Archana Lakhani3, Ganesan Vedachalaiyer6,3, Suresh Krishnawarrier Gopinatha Warrier2. 1. Department of Physics, Chaitanya Bharathi Institute of Technology, Gandipet, Hyderabad 500075, India. 2. Magnetic Materials Laboratory, Department of Physics, Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India. 3. UGC-DAE Consortium for Scientific Research, University Campus, Khandwa Road, Indore 452001, Madhya Pradesh, India. 4. M. N. Miheev Institute of Metal Physics of Ural Branch of Russian Academy of Sciences, 620108 Ekaterinburg, Russia. 5. Ural Federal University, 620002 Ekaterinburg, Russia. 6. Medi-Caps University, A.B. Road, Pigdamber, Rau, Indore 453331, Madhya Pradesh, India.
Abstract
We report a comprehensive investigation of MnNi0.7Fe0.3Ge Heusler alloy to explore its magnetic, caloric, and electrical transport properties. The alloy undergoes a ferromagnetic transition across T C ∼ 212 K and a weak-antiferromagnetic transition across T t ∼ 180 K followed by a spin-glass transition below T f ∼ 51.85 K. A second-order phase transition across T C with mixed short and long-range magnetic interactions is confirmed through the critical exponent study and universal scaling of magnetic entropy and magnetoresistance. A weak first-order phase transition is evident across T t from magnetization and specific heat data. The frequency dependent cusp in χAC(T) along with the absence of a clear magnetic transition in specific heat C(T) and resistivity ρ(T) establish the spin glass behavior below T f. Mixed ferromagnetic and antiferromagnetic interactions with dominant ferromagnetic coupling, as revealed by density functional calculations, are experimentally evident from the large positive Weiss temperature, magnetic saturation, and negative magnetic-entropy and magnetoresistance.
We report a comprehensive investigation of MnNi0.7Fe0.3Ge Heusler alloy to explore its magnetic, caloric, and electrical transport properties. The alloy undergoes a ferromagnetic transition across T C ∼ 212 K and a weak-antiferromagnetic transition across T t ∼ 180 K followed by a spin-glass transition below T f ∼ 51.85 K. A second-order phase transition across T C with mixed short and long-range magnetic interactions is confirmed through the critical exponent study and universal scaling of magnetic entropy and magnetoresistance. A weak first-order phase transition is evident across T t from magnetization and specific heat data. The frequency dependent cusp in χAC(T) along with the absence of a clear magnetic transition in specific heat C(T) and resistivity ρ(T) establish the spin glass behavior below T f. Mixed ferromagnetic and antiferromagnetic interactions with dominant ferromagnetic coupling, as revealed by density functional calculations, are experimentally evident from the large positive Weiss temperature, magnetic saturation, and negative magnetic-entropy and magnetoresistance.
The physics of phase transitions is important
to understand the
properties of compounds. Exploration of the critical phenomena across
the transition temperature unveils the nature of the phase transition.
A second-order phase transition (SOPT) from paramagnetic (PM) to ferromagnetic
(FM) state is characterized by a continuous variation of the spontaneous
magnetization, an order parameter. Nevertheless, the magnetic properties
of the compounds are governed by the exchange interactions among the
spins. FM compounds with a large change in magnetic entropy and adiabatic
temperature Tad (change in temperature
of the system under adiabatic condition without exchange of heat)
across the transition temperature near room temperature are potential
candidates for technological applications such as magnetic refrigeration.
In recent times, Heusler compounds have become materials of topical
interest for their multifunctional and peculiar properties such as
topological insulators,[1,2] Weyl semimetals,[3] spin-gapless semiconductors,[4] shape memory effect,[5,6] half-metals,[7−9] exchange bias,
large magnetoresistance, and magnetocaloric effect.[10,11]Heusler alloys with 1:1:1 stoichiometry have been receiving
a great
deal of attention due to their tunable magnetic properties with substitution,
magnetic field, and hydrostatic pressure. Substitution/disorder driven
suppression of a first-order magneto-structural transition in 1:1:1
stoichiometric Heusler alloy MnNiGe was reported.[12,13] It undergoes a structural transition at Tt = 470 K from high-temperature Ni2In-type hexagonal austenite
to a TiNiSi-type orthorhombic martensite structure.[14,15] In addition, it is reported to order antiferromagnetically at = 346 K in the martensitic
state, followed
by a ferromagnetic phase below = 205 K. The magnetic
properties of MnNiGe
have been reported to be substitution and site specific. A gradual
replacement of Fe at Mn site, Mn1–FeNiGe, has suppressed Tt down to 84 K at x = 0.26. The alloys
with x > 0.26 crystallize in a Ni2In-type
hexagonal structure with a glassy phase at low temperatures.[12] On the other hand, in MnNi1–FeGe where Ni is gradually
replaced by Fe, the systems remain in the ferromagnetic austenite
phase for x > 0.3.[12] MnNi0.7Fe0.3Ge is reported to undergo a structural
transition
at Tt = 189 K (below which a small thermal
hysteresis was noticed) and austenite ferromagnetic transition at = 211 K.[12] Recently,
MnNi0.8Fe0.2Ge has been investigated for its
successive magnetic transitions with a field-induced conversion of
the low-temperature magnetic state to the FM state.[16] Nevertheless, the universality class of the high-T SOPT and transport behavior of MnNi0.7Fe0.3Ge are unclear.In the present study, we report on
the universality class and critical
magnetic behavior of MnNi0.7Fe0.3Ge using the
combined results of magnetization and specific heat, combined with
ab initio calculations. The study has been focused on understanding
the phenomena across and Tt. Our
results reveal that the alloy crystallizes in a Ni2In-type
hexagonal structure at room temperature and undergoes a second-order
phase transition at TC ∼ 212.5
K. A narrow thermal hysteresis below 180 K disappears in a field of
∼5 kOe above which the system behaves ferromagnetically down
to 2 K. Mixed (short- and long-range) interactions are suggested by
the critical exponents. The Sommerfeld coefficient of electronic specific
heat (γel = 15.9 ± 0.5 J·mol–1.K–2) and electrical resistivity confirm the metallic
character. The self-consistency of the critical exponents, extracted
using magnetization, is established through the analysis of the magnetocaloric
and the magnetoresistance methods. A second-order phase transition
across TC ∼ 212 K is confirmed
through universal scaling of the magnetic-entropy and magnetoresistance
data. A cluster-glass type behavior with weakly coupled magnetic clusters
is reported below 50 K. The dual transitions can be carefully manifested/tuned
to achieve a table-like magneto-caloric effect for magnetic refrigeration.
The effect of the magnetic field on the electrical resistivity across
the magnetic transition temperature can be utilized in magneto-resistive
applications.
Methods
A polycrystalline MnNi0.7Fe0.3Ge has been
prepared by the arc-melting method. The constituent elements Mn, Ni,
Fe, and Ge (of purity better than 99.999%) were taken in a stoichiometric
ratio and were loaded into a copper hearth. The elements were melted
under a continuous supply of argon gas. The ingot was melted several
times by flipping each time. X-ray diffraction pattern at room temperature
is collected on a powder specimen using PANalytic X’Pert Pro
X-ray diffractometer with Cu–Kα radiation.
Energy-dispersive X-ray (EDAX) spectroscopy measurements (not shown
here) were carried out using JSM-7600F. The atomic percentages of
Mn, Ni, Fe, and Ge are in good agreement with the originally taken
stoichiometric ratio within the experimental error. Magnetization
was measured with the help of a commercial superconducting quantum
interference device-vibrating sample magnetometer (SQUID-VSM) under
zero-field cooling (ZFC), field-cooled cooling (FCC), and field-cooled
warming (FCW) conditions. Under ZFC conditions, magnetization was
recorded during warming (under the ambiance of required set field)
after the sample was cooled to 2 K from 400 K in zero-field. Under
FCC conditions, magnetization was recorded while the sample was cooled
in a finite magnetic field. Consequently, under FCW conditions, magnetization
was recorded under warming, without switching off magnetic field.
Isothermal magnetization versus field curves were measured, under
ZFC condition, by ramping the magnetic field. Electrical resistivity
was measured using a standard dc-four probe method using a 9 T-Physical
Property Measurement System (PPMS). The specific heat was measured
using relaxation calorimetry with the help of commercial 14 T PPMS.The electronic structure was calculated in the Quantum ESPRESSO
software[17] using the scalar-relativistic
potentials in a local density approximation of Perdew–Zunger-type,
included in the standard QE library. Wave functions were decomposed
into plane waves, and interactions between ions and valence electrons
were taken into account of method of attached plane waves (PAW). To
model the concentration of Fe closest to the experiments, we constructed
a supercell with 4 f.u. of MnNiGe with 1 Ni ion substituted by Fe
that finally resulted in the MnNi0.75Fe0.25Ge
composition. For the sufficient convergence in our first-principles
calculations, the energy cutoff, i.e., energetic limit, 60 Ry, was
taken. A k-mesh of 8 × 8 × 8 k-points was used for the tetrahedron method integration in a reciprocal
space.
Results
Figure a shows
the room-temperature X-ray diffraction pattern of MnNi0.7Fe0.3Ge, along with Rietveld refinement using the FullProf
suite.[18] The alloy crystallizes in a Ni2In-type hexagonal structure with the P63/mmc space group. The lattice parameters
are a = b = 4.102 Å and c = 5.368 Å. The obtained structure is drawn using
visualization for electronic and structure analysis (VESTA),[19] as shown in Figure b. Mn occupies the 2a (0, 0, 0) position
and Ni/Fe share the 2d (1/3, 2/3, 3/4) positions, while Ge occupies
the 2c (1/3, 2/3, 1/4) position. The shortest Mn–Mn distance
along the c-axis is 2.6839(1) Å.
Figure 1
(a) Refined X-ray diffraction
pattern of MnNi0.7Fe0.3Ge using the P63/mmc space group. The global
χ2 = 2.31 with Bragg factor
= 14.6 and RF-factor = 15.2. (b) Crystal structure with lattice parameters a = b = 4.102 Å and c = 5.368 Å. Ni atom shares 30% of its occupancy with Fe. Mn–Mn
nearest distance along the c-axis is 2.684 Å.
(c) Temperature dependence of magnetization under 100 Oe in ZFC, FCC,
and FCW processes. ZFC and FCW curves are separated from each other
below Tt = 180 K. Inset: A narrow thermal
hysteresis is noticed between FCC and FCW in the temperature range
75–215 K. (d) Curie–Weiss fit of the inverse susceptibility.
The Weiss temperature and the effective magnetic moment are found
to be (233.64 ± 0.11) K and μeff = (4.981 ±
0.003) μB/f.u., respectively.
(a) Refined X-ray diffraction
pattern of MnNi0.7Fe0.3Ge using the P63/mmc space group. The global
χ2 = 2.31 with Bragg factor
= 14.6 and RF-factor = 15.2. (b) Crystal structure with lattice parameters a = b = 4.102 Å and c = 5.368 Å. Ni atom shares 30% of its occupancy with Fe. Mn–Mn
nearest distance along the c-axis is 2.684 Å.
(c) Temperature dependence of magnetization under 100 Oe in ZFC, FCC,
and FCW processes. ZFC and FCW curves are separated from each other
below Tt = 180 K. Inset: A narrow thermal
hysteresis is noticed between FCC and FCW in the temperature range
75–215 K. (d) Curie–Weiss fit of the inverse susceptibility.
The Weiss temperature and the effective magnetic moment are found
to be (233.64 ± 0.11) K and μeff = (4.981 ±
0.003) μB/f.u., respectively.The temperature dependence of the magnetization M(T) curve under the influence of 100 Oe is shown
in Figure c. M(T) rises sharply below 250 K before it
takes a down turn around 180 K along with a separation between the
ZFC and FCW magnetization curves. In addition, a narrow thermal hysteresis
between FCC and FCW is observed in the temperature range 75 to 215
K, as shown in the inset of Figure c. Further, M(T)
exhibits a down turn below Tf, noted as
a freezing temperature. In 100 Oe, the inverse susceptibility χ–1(T) is fit, as shown in Figure d, to the Curie–Weiss
law using eq where C is the Curie–Weiss
constant from which the effective magnetic moment is calculated as (kB is the
Boltzmann constant and NA is the Avogadro
number). Thus, the obtained effective magnetic moment is μeff = 4.981 ± 0.003 μB/f.u. A positive
and large Weiss temperature θW = (233.64 ± 0.11)
K indicates the prevailing ferromagnetic exchange correlations above
the transition temperature. M(T)
in 1 kOe is shown in Figure a. The bifurcation between ZFC and FCW is found to decrease
with increasing H. However, the kink at Tt and the thermal hysteresis, observed below 180 K in
100 Oe, shift toward low-temperature with increasing H up to 3 kOe. In H ≥ 5 kOe, the kink at Tt is smeared out with simultaneous vanishing
of thermal hysteresis. Such a phenomenon resembles the field-induced
weak-AFM to FM transition. Shown in Figure b are M(T) curves, measured in constant magnetic fields ranging from 100 Oe
to 50 kOe.
Figure 2
(a) M(T) measured in 1 kOe in
ZFC, FCC, and FCW protocols. Reduced bifurcation of ZFC and FCW curves
is noticed when compared to 100 Oe. (b) M(T) measured under a few representative magnetic fields.
(c) Isothermal magnetization versus field at 2 K. M increases sharply with H with a saturation magnetization
of Ms ∼ 2.6 μB/f.u. at a saturation field of Hs ∼
6.6 kOe. (d) Isothermal magnetization versus field curves at a few
representative temperatures. In the paramagnetic region (at 300 K), M develops linearly with H.
(a) M(T) measured in 1 kOe in
ZFC, FCC, and FCW protocols. Reduced bifurcation of ZFC and FCW curves
is noticed when compared to 100 Oe. (b) M(T) measured under a few representative magnetic fields.
(c) Isothermal magnetization versus field at 2 K. M increases sharply with H with a saturation magnetization
of Ms ∼ 2.6 μB/f.u. at a saturation field of Hs ∼
6.6 kOe. (d) Isothermal magnetization versus field curves at a few
representative temperatures. In the paramagnetic region (at 300 K), M develops linearly with H.Figure c
shows
an isothermal magnetization versus field M(H) up to 70 kOe, recorded at 2 K. M(H) is measured in five quadrants (0 → 70 kOe →
0 kOe → −70 kOe → 0 kOe → 70 kOe). Remnant
magnetization MR is zero, indicative of
soft ferromagnetic behavior which is supported by zero coercive field Hc. The saturation magnetization Ms is about 2.6 μB/f.u. Figure d shows the isothermal M(H) curves, measured at a few selected
temperatures. As the temperature is increased, the linearity from
the high-field region is extended to low-fields. In the paramagnetic
state (at 300 K), M linearly increases with H.
Discussion
Critical Behavior across TC
In order to understand the magnetism
of MnNi0.7Fe0.3Ge i.e. whether localized or
itinerant, Rhodes–Wohlfarth
(RW) ratio qc/qs[20,21] is calculated, where qc is the number of magnetic carriers per atom and qs is the saturation magnetic moment. qs = 2.6 μB/f.u. for the present case. qc = 4.08 μB/f.u. is estimated
from the effective magnetic moment as μeff = . The RW ratio is obtained
as qc/qs >
1, indicating an itinerant
magnetic behavior of the alloy. Further, with an aim of realizing
the universality class and the type of magnetic interactions in MnNi0.7Fe0.3Ge, a critical study has been carried out
with the help of isothermal magnetization curves. A set of M(H) curves were measured in the temperature
range 201–209 by 1 K difference, 210–220 by 0.5 K difference,
and 221–230 K by 1 K difference, as shown in Figure a. In regard to the SOPT from
the PM to the FM state, the spontaneous magnetization Ms below the critical transition temperature TC, the inverse susceptibility χ–1 above TC, and the isothermal magnetization
at TC follow power-laws given by eqs , 3, and 4, respectively[22,23]where t = 1 – T/TC is the reduced temperature
and the critical exponents associated with Ms, χ0, and TC are
β, γ, and δ, respectively, while Ms0, χ00 ,and D are the
critical amplitudes. Arrott plots[24] with
mean-field theory exponents (β = 0.5 and γ = 1.0), i.e., M2 versus H/M, are shown in Figure b. In these isotherms, the downward concave curvature of the Arrott
plot in high fields hints at SOPT, following Banerjee’s criterion.[25] To estimate the correct critical exponents,
we have used the modified Arrott plot method (MAP) using Arrott and
Noakes magnetic equation of state, eq (26)where c1 and c2 are constants. Different universal magnetic
behaviors such as 3D-Heisenberg (β = 0.365, γ = 1.386),
3D-Ising model (β = 0.325, γ = 1.24),[27] and tricritical mean field theory (β = 0.25, γ
= 1.0)[28] were tested by plottng M1/β versus (H/M)1/γ curves (not shown here).
Figure 3
(a) Isothermal
magnetization versus curves of MnNi0.7Fe0.3Ge
at a few selected temperatures in the temperature
range 201–230 K. In particular, M(H) curves are measured with 0.5 K difference in the vicinity
of critical transition. (b) Arrott plot M2 versus H/M with mean-field theory
exponents (β = 0.5 and γ = 1). The positive slope of the
high-field curves indicate the second order phase transition. (c)
Modified Arrott plot M1/β versus
(H/M)1/γ with parallel
set of lines with critical exponents β = 0.395 and γ =
1.381. Critical transition isotherm passing through origin is shown
in red and the linear fit is shown in dashed lines. (d) M(H) at 212.5 K (≡ TC), a power-law fit (shown in solid line) using eq yields an exponent δ = 4.176
± 0.011.
(a) Isothermal
magnetization versus curves of MnNi0.7Fe0.3Ge
at a few selected temperatures in the temperature
range 201–230 K. In particular, M(H) curves are measured with 0.5 K difference in the vicinity
of critical transition. (b) Arrott plot M2 versus H/M with mean-field theory
exponents (β = 0.5 and γ = 1). The positive slope of the
high-field curves indicate the second order phase transition. (c)
Modified Arrott plot M1/β versus
(H/M)1/γ with parallel
set of lines with critical exponents β = 0.395 and γ =
1.381. Critical transition isotherm passing through origin is shown
in red and the linear fit is shown in dashed lines. (d) M(H) at 212.5 K (≡ TC), a power-law fit (shown in solid line) using eq yields an exponent δ = 4.176
± 0.011.Various trials were made to obtain
the correct critical exponents
by taking initial values of β = 0.365 and γ = 1.386. M(H) curves were subjected to the demagnetization
correction Heff = Happlied – NDM. Every time, the newly obtained exponents are validated for the
sufficient condition using eq and checked that the modified isotherm of transition temperature
passes through the origin (M1/β =
0, (H/M)1/γ = 0).
After a rigorous exercise, a set of parallel isotherms were obtained,
satisfying eq with
β = 0.395 and γ = 1.381, for which M1/β versus (H/M)1/γ curves are shown in Figure c. Ms and are extracted from the intercepts
of the M1/β and (H/M)1/γ axis, respectively. Thus,
obtained Ms(T) and , shown in Figure a,b, are fit using
the respective eqs and 3. The obtained critical exponents and transition
temperatures through
the MAP method are TC = (212.51 ±
0.14) K and β = 0.315 ± 0.076; TC = (212.57 ± 0.10) K, γ = 1.327 ± 0.045. Further,
more accurate exponents are obtained through the Kouvel–Fisher
(KF) method. The plots of Ms[1/(dMs/dT)] and χ–1[1/(dχ–1/dT)] as a function of temperature are shown in Figure c,d. The inverse slopes of the linearly fit
curves give the exponents β = 0.409 ± 0.002 and γ
= 1.293 ± 0.019 with critical temperatures TC = (212.45 ± 0.23) K and TC = (212.63 ± 0.17) K, respectively. Using Widom’s
relation,[29,30] δ = 1 + γ/β, the estimated
δ values through MAP and KF methods are δ = 5.212 ±
1.162 and 4.161 ± 0.062, respectively, which are in good agreement
with δ (= 4.176 ± 0.011) directly obtained through the
critical isotherm fit using eq , as shown in Figure d. The critical exponents do not straight away indicate a
single universality class but closely resemble 3D-Heisenberg and 3D-Ising
models. The exchange interaction J(r), where r is the distance of interaction, depends
on the spatial dimensionality d and the length of
interaction σ through a relation J(r) ∼ r–(σ+. σ can be calculated from γ using eq (31)where Δσ = (σ – d/2) and G(d/2) = 3 –
(d2/16). For the present compound, with d = 3, σ ∼ 1.75 is obtained and exchange interaction
varies as J(r) ∼ r–4.75 which falls in between the ranges
for Mean-field model (r–4.5, σ
≤ 3/2) and 3D Heisenberg model (r–5, σ ≥ 2). This indicates the mixed exchange interactions
of long-range and short-range MnNi0.7Fe0.3Ge.
Nevertheless, the closeness of the critical exponents to other models
3D-Ising or 3D-XY point out anisotropic exchange interactions. On
the other hand, Pinninti et al. reported a single magnetic transition
and 3D-Heisenberg universality with short-range magnetic interactions
in MnCo0.7Fe0.3Ge[32] and enhancement of transition temperature with Fe substitution in
Mn0.7Fe0.3Co0.7Fe0.3Ge.[33]
Figure 4
(a) Temperature dependence of spontaneous magnetization Ms. A critical exponent fit of the data using eq produces β = 0.315
± 0.076 and TC = (212.51 ± 0.14)
K. (b) Inverse susceptibility 1/χ0(T). γ = 1.327 ± 0.10 and TC = (212.57 ± 0.045) K are obtained by fitting the data using eq . (c) Kouvel–Fisher
plot of Ms(T) yielding
the exponent β = 0.409 ± 0.002 and critical temperature TC = (212.45 ± 0.23) K. (d) Kouvel-Fisher
fit of 1/χ0(T) with γ = 1.293
± 0.019 and TC = (212.63 ± 0.17)
K.
(a) Temperature dependence of spontaneous magnetization Ms. A critical exponent fit of the data using eq produces β = 0.315
± 0.076 and TC = (212.51 ± 0.14)
K. (b) Inverse susceptibility 1/χ0(T). γ = 1.327 ± 0.10 and TC = (212.57 ± 0.045) K are obtained by fitting the data using eq . (c) Kouvel–Fisher
plot of Ms(T) yielding
the exponent β = 0.409 ± 0.002 and critical temperature TC = (212.45 ± 0.23) K. (d) Kouvel-Fisher
fit of 1/χ0(T) with γ = 1.293
± 0.019 and TC = (212.63 ± 0.17)
K.
Spin-Glass Behavior below
52 K
Real (χ′)
and imaginary parts (χ″) of AC-susceptibility
χAC are shown in parts a and b, respectively, of Figure . The measurements
were carried out in an AC-drive field of HAC = 5 Oe and HDC = 0 Oe under the effect
of a few selected frequencies ν = 1, 47, 97, 197, 297, 397,
and 497 Hz. The temperature variation of dχ′/dT (not shown here) exhibits a dip around
213 K, followed by a peak around 180 K, which are in good agreement
with TC and Tt. The dip around 213 K is found to be frequency independent, indicating
the long-range magnetic order. However, a dispersion in χ′(T) is visible below Tt. In ν
= 1 Hz, dχ′/dT exhibits
a peak around the freezing temperature Tf ∼ 51.85 K which shifts toward high temperatures with increasing
frequency, indicating short-range correlations among the spins. In
order to understand these short-range correlations, Mydosh parameter
which represents the relative shift of a freezing temperature is estimated
as ϕ = ΔTf/TfΔ[ log10ν] where ΔTf = and Δ[ log10ν]
= log10ν2 – log10ν1, with ν1 = 1 Hz and ν2 =
497 Hz. For the present compound ϕ ∼ 0.12, which is larger
than ϕ reported for cluster spin-glasses and matches with ϕ
reported for superparamagnetic systems (ϕ ∈ [0.10, 0.13]).[34] Further, relaxation time is obtained with the
help of relation between Tf and ν
for the dynamical slowing down of spin fluctuations[34,35] above the glass transition temperature of a spin glass, i.e., τ
= , where
τ = 1/ν, τ0 is the single spin-flip relaxation
time, and zν′ is an exponent. Figure c shows a linear
fit of log10τ = log10τ0 – zν′log10(Tf/Tg – 1).
The currently obtained value of zν′
(= 3.67 ± 0.05) is close to that reported for spin-glass
systems.[34] However, τ0 ∼ 2.67× 10–5 s is 2 orders of magnitude
higher than that reported for cluster spin-glass systems (10–7–10–10 s).[36]Figure d shows a linear
fit of Tf = T0 – (Ea/kB)[1/ ln(ν/ν0)] which is a Vogel–Fulcher
law, a modified Arrhenius relation,[34,37] where Ea is the energy barrier arising from the anisotropy
and volume of the particle (in case of nanosystems), T0 is the characteristic temperature, and kB is the Boltzmann constant (8.617 × 10–5 eV·K–1). The Vogel–Fulcher fit results
are T0 = (46.45 ± 0.36) K and Ea/kB = (92.71 ±
1.82) K. Non-zero T0(38]δTTh = 0.1 suggests the cluster-glass nature (δTTh ∈ [0.05, 0.5]). Although τ0 is relatively large, it can be deduced from the results of AC susceptibility
that MnNi0.7Fe0.3Ge behaves as a cluster spin-glass
with weak coupling among the clusters, below 50 K.
Figure 5
(a, b) and measured in labeled frequencies
under HAC = 5 Oe and HDC = 0 Oe. The curves show a peak at 213 K along with
a hump around
180 K. Below about 52 K, dispersion in with a shift in Tf toward high-T. (c) Fit of critical dynamical
slowing in relation to Tf(ν) which
gives a relaxation time τ0 ∼ 2.7× 10–5 s. (d) Fit of Vogel–Fulcher law which yields
a characteristic temperature T0 = (46.45
± 0.36) K and Ea/kB = (92.71 ± 1.82) K.
(a, b) and measured in labeled frequencies
under HAC = 5 Oe and HDC = 0 Oe. The curves show a peak at 213 K along with
a hump around
180 K. Below about 52 K, dispersion in with a shift in Tf toward high-T. (c) Fit of critical dynamical
slowing in relation to Tf(ν) which
gives a relaxation time τ0 ∼ 2.7× 10–5 s. (d) Fit of Vogel–Fulcher law which yields
a characteristic temperature T0 = (46.45
± 0.36) K and Ea/kB = (92.71 ± 1.82) K.
Density Functional Calculations
To theoretically calculate
the electronic structure and magnetic properties of the experimental
MnNi0.7Fe0.3Ge composition, a supercell comprising
4 f.u. was taken with 1 Ni ion substituted by Fe; this resulted in
the very close composition MnNi0.75Fe0.25Ge.
For this setup, the calculations were carried out for ferromagnetic
and different antiferromagnetic configurations of the Mn and Fe magnetic
moments. The ferromagnetic solution was found to be the most stable
with the total energy of −3235.1737 Ry per supercell. Other
initial AFM configurations converged to the ferrimagnetic solution
with 0.13 μB/f.u. and have a total energy 2.5 mRy
(34 meV) higher.This calculated FM ordering of the Mn and Fe
magnetic moments has a total magnetic moment of 2.8 μB/f.u., including 2.7 and 2.9 μB per each of the
two Mn ions, 0.8 μB/Fe, 0.1 μB/Ni,
and −0.2 μB/Ge. The calculated FM total magnetic
moment 2.8 μB/f.u. is very close to the saturation
magnetic moment 2.6 μB/f.u. obtained from the experimental
measurements reported above. In ref (39), we reported the calculated exchange interaction
parameters for MnNiGe with the strong AFM nearest neighbor Mn ions JNN = 705 K coupling between the Mn ions, much
larger than the FM coupling JNN = −302
K and AFM JNNN = 67 K. In MnNi0.7Fe0.3Ge, due to the presence of Fe in the Ni positions,
the FM coupling JNN = −881 K between
the Mn ions becomes large and dominates in the Mn subsystem over the
AFM coupling JNN = 299 K and JNNN = 45 K. The moderate magnetic moment of the Fe ion
causes much smaller values of the exchange coupling with the highest
value between Fe and the nearest Mn ion as FM JNN = −95 K. Thus, the FM and smaller AFM couplings among
the Mn ions are determining the magnetic properties of MnNi0.7Fe0.3Ge.In Figure , the
first-principles electronic structure for MnNi1–FeGe (x = 0.25) is shown corresponding to the ferromagnetic arrangement
of the Mn and Fe magnetic moments. The partial densities are plotted
for the total and Fe-3d states on the highest panel, then the Mn and
Ni-3d states, and finally, the Ge-4p and Ge-4s states. In the calculated
total and partial densities of states (DOS), the strongly spin-polarized
Mn-3d contribute from −5 to +5 eV with strong peaks near −2.8,
−1.1, and +1.0 eV. Notice the two different types of the Mn
ions (plotted as Mn and Mn1) due to the presence of Fe. The Ni and
Ge ions also subdivided into two types; this difference in DOS and
magnetic moments is negligible. The Ni states are almost nonmagnetic
with deviating densities of states mostly below the Fermi energy (EF) in both spin projections with the peaks from
−5.0 to −0.5 eV below EF. The selected MnNi0.75Fe0.25Ge supercell is
very close to the experimental composition. In order to check exact
electronic concentration for Fe with x = 0.30, we
added the rigid band approximation line in Figure , and it came very close to the Fermi energy
and accounts for the 0.05 difference in x.
Figure 6
Calculated
total and partial densities of states for MnNi1–FeGe (x = 0.25) given for two spin projections (↑ and ↓). The solid orange line close to the
Fermi energy (EF = 0 eV) corresponds to
the rigid band shift for x = 0.30.
Calculated
total and partial densities of states for MnNi1–FeGe (x = 0.25) given for two spin projections (↑ and ↓). The solid orange line close to the
Fermi energy (EF = 0 eV) corresponds to
the rigid band shift for x = 0.30.
Specific Heat and Resistivity
Specific heat C(T), measured in the presence of a few
selected magnetic fields, is shown in Figure a. It exhibits two successive peaks at TC and Tt which are
in agreement with the magnetization data (see Table ). The peak at TC is broad and indicates a second-order phase transition from PM to
FM, while a relatively sharp peak at Tt gives a hint of first-order phase transition. In addition, TC gradually shifts toward high-T in applied magnetic fields, whereas Tt is found to be independent of H up to 5 kOe. Nevertheless,
in higher fields (typically H > 5 kOe) C(Tt) gets smeared out with
a gradual
shift of Tt toward high-T, implying a field-induced transition from a weak-AFM to FM state.
This observation is in good agreement with a tiny/narrowed thermal
hysteresis between FCC and FCW curves across Tt. Except for a strong FOPT, a tiny thermal hysteresis (weak-FOPT)
cannot be traced out by heating and cooling curves of specific heat
using commercial PPMS.[40] Zero-field C versus T is shown in the inset of Figure a. The data below
10 K is fit to the equation C = γelT + βT3 to estimate
the Sommerfeld parameter for the electronic contribution of specific
heat (γel) and the Debye temperature (θD). Thus, obtained γel and (where p is the number
of atoms in a formula unit) are (3.86 ± 0.1) mJ mol–1·K–2 and (499 ± 5) K, respectively. γel indicates the metallic nature of the alloy and the density
of states at the Fermi level are found to be about 1.64 states/eV/f.u.
The absence of a clear transition at Tf in C(T) along with a frequency
dependent cusp in χAC(T) indicates
the glassy behavior.
Figure 7
(a) Specific
heat as a function of temperature from 160 to 240
K, measured in a few selected magnetic fields. TC and Tt are shown by arrows. Inset:
Zero-field data; a fit of C(T) =
γelT + βT3 below 10 K with γel = (3.86 ±
0.1) mJ mol–1·K–2 and θD = (499 ± 5) K and the specific heat data from 2 to 70
K. (b) Change in magnetic entropy under the effect of labeled magnetic
fields. It is negative and exhibits two dips, respectively, at TC and Tt. (c) Magnetic
field dependence of is fit to a power-law using eq , yielding an exponent n = 0.559 ± 0.012. (d) RCP versus magnetic field. A
power-law fit using eq yields an exponent δ = 4.852 ± 0.465.
Table 1
List of
Transition Temperatures Inferred
from the Temperature Dependence of Magnetization, Specific Heat, and
Resistivity Data
temp
magnetization
specific
heat
resistivity
TC (K)
212
210
210
Tt (K)
180
178.5
180
Tf (K)
51.85
no feature
no feature
(a) Specific
heat as a function of temperature from 160 to 240
K, measured in a few selected magnetic fields. TC and Tt are shown by arrows. Inset:
Zero-field data; a fit of C(T) =
γelT + βT3 below 10 K with γel = (3.86 ±
0.1) mJ mol–1·K–2 and θD = (499 ± 5) K and the specific heat data from 2 to 70
K. (b) Change in magnetic entropy under the effect of labeled magnetic
fields. It is negative and exhibits two dips, respectively, at TC and Tt. (c) Magnetic
field dependence of is fit to a power-law using eq , yielding an exponent n = 0.559 ± 0.012. (d) RCP versus magnetic field. A
power-law fit using eq yields an exponent δ = 4.852 ± 0.465.Figure d
shows
the temperature variation of magnetic entropy ΔSmag (referred to MCE hereafter) which is estimated using eq . Conventionally, MCE is
negative for a ferromagnet. For MnNi0.7Fe0.3Ge, MCE shows two dips, respectively, TC and Tt. Negative MCE around Tt suggests the dominant ferromagnetic interactions
in the alloy. An absolute MCE value at TC, in an applied of 70 kOe, is found to be 0.5 J·kg–1·K–1.Here, RCP is the relative
cooling power defined
as RCP = . Though MCE and RCP values of MnNi0.7Fe0.3Ge are not comparable to that of some of
the prominent MCE materials,[41,42] magnetically distinct
dual transitions (one at high-T) with a temperature
difference of about 32 K can be tuned (by hydrostatic pressure or
substitution) to achieve a table-like ΔSmag(T). Parts c and d of Figure show the field dependence
of and RCP, which are
fit to the power-law
dependences given in eqs and 8b, respectively. The critical
exponents, obtained from MCE plots using the relations given by eqs and 8d,[43,44] are β = 0.331 ± 0.086, γ
= 1.186 ± 0.322, and δ = 4.852 ± 0.465.Figure a shows
the temperature dependence of resistivity ρ(T), measured in a few representative magnetic fields. The metallic
character of the samples is evident from the positive slope of ρ(T). As shown in the inset of Figure a, dρ/dT exhibits two peaks respectively at TC and Tt which are in agreement with that
of obtained from magnetization and specific heat (see Table ). Magnetoresistance, MR = [ρ(H) – ρ(0)]/ρ(0), is shown in Figure b. Under an applied
field of 90 kOe, absolute MR is found to be about 6.0%. It is negative
arising from the suppression of magnetic fluctuations by the application
of field. The dip temperature Td increases
with application of magnetic fields, as expected for a ferromagnet.
In addition, there is a minor kink at Tt = 180 K. Parts c and d of Figure show the magnetic field variation of and , respectively. A similar
method, described
to extract the exponents from MCE using eqs and 8b, is followed.
Thus, extracted critical exponents, β = 0.392 ± 0.130,
γ = 1.779 ± 0.672, and δ = 5.545 ± 1.239, are
in good agreement with those obtained MAP, KF, and magnetic entropy
methods. For the sake of completeness, we have obtained an exponent
α from resistivity. Considering the magnetic contributions,
it has been theoretically proposed[45−52] and experimentally verified[53−56] that the temperature derivative of resistivity (dρ/dT) and specific heat (C) exhibit similar temperature dependent behaviors in the
critical region. Figure a shows zero-field (1/ρ(TC)(dρ/dT) versus the t curve. A critical exponent α is extracted using a power-law
given by eq (27)where A and B are constants, α is a critical exponent, and t is the reduced temperature. For the present alloy, the
critical
fit yields α = 0.55 ± 0.05. Positive α indicates
the Ising type universality class, though it is larger about four
times. α along with β and γ satisfies the universal
scaling equation α + 2β + γ = 2.[27] Experimentally obtained exponents α, β, and
γ using modified Arrott plots, Kouvel Fisher, magnetocaloric,
and magnetoresistance methods, listed in Table , are in good agreement within the error
bars, establishing the self-consistency of the critical exponents.
Figure 8
(a) Resistivity
as a function of temperature, measured in labeled
magnetic fields. It decreases with reduction in the temperature, revealing
the metallic nature of MnNi0.7Fe0.3Ge. Inset
shows the derivative dρ/dT which depicts two peaks corresponding to TC and Tt. (b) Percentage of magnetoresistance.
It is negative, indicating the suppression of magnetic fluctuations
in external magnetic fields. In 90 kOe, MR is about 6.0%. (c) Maximum
of absolute MR (taken from (b)) versus change in the magnetic field,
ΔH. A power-law fit to the data yields an exponent n = 0.72 ± 0.01. (d) Power-law fit of RCPMR versus ΔH, yielding an exponent δ =
5.545 ± 1.239. The significance of the power-law fits is discussed
in the text.
Figure 9
(a) Reduced temperature dependence of in zero field. The data above critical
temperature is fit (red solid line) to the eq , which yields a critical exponent α
= 0.55 ± 0.05. (b) Magnetic field dependence of MR%. The curves
are fit (red solid line) to the power-law MR ∝ −Hm. A quadratic field dependence in the paramagnetic
state suggests the suppression of spin fluctuations by applying external
fields. As T approaches TC, the magnitude of MR increases. Below TC, a reduction in MR% with linear dependence on H is noticed. (c, d) Rescaled magnetic entropy and magnetoresistance
against a reduced temperature θ. The data scales well by falling
onto a single universal curve, irrespective of the strength of H, indicating a SOPT. However, the deviation from the universal
scaling around Tt hints at a first-order
phase transition.
Table 2
Critical
Exponents of MnNi0.7Fe0.3Ge
method
TC (K)
β
γ
δ
α
ref
modified Arrott Plot
212.51 ± 0.14
0.315 ± 0.076
1.327 ± 0.045
5.212 ± 1.162
this work
Kouvel-Fisher
212.45 ± 0.23
0.406 ± 0.002
1.293 ± 0.019
4.161 ± 0.062a
this work
critical isotherm
212.5
4.176 ± 0.011a
this work
magnetoresistance
∼213
0.392 ± 0.130
1.779 ± 0.672
5.545 ± 1.239
0.55 ± 0.05b
this work
magnetocaloric
∼213
0.331 ± 0.086
1.186 ± 0.322
4.852 ± 0.465
this
work
mean-field theory
0.5
1.0
3.0
0.0
(27)
3D Heisenberg model
0.365
1.386
4.80
–0.0115
(27)
3D-Ising model
0.325
1.241
4.82
0.110
(27)
3D-XY model
0.346
1.316
4.81
(27)
tricritical model
0.25
1.0
5.0
(27)
δ is obtained using Widom’s
relation δ = 1 + γ/β.
α is extracted from the resistivity
and specific heat using eq .
(a) Resistivity
as a function of temperature, measured in labeled
magnetic fields. It decreases with reduction in the temperature, revealing
the metallic nature of MnNi0.7Fe0.3Ge. Inset
shows the derivative dρ/dT which depicts two peaks corresponding to TC and Tt. (b) Percentage of magnetoresistance.
It is negative, indicating the suppression of magnetic fluctuations
in external magnetic fields. In 90 kOe, MR is about 6.0%. (c) Maximum
of absolute MR (taken from (b)) versus change in the magnetic field,
ΔH. A power-law fit to the data yields an exponent n = 0.72 ± 0.01. (d) Power-law fit of RCPMR versus ΔH, yielding an exponent δ =
5.545 ± 1.239. The significance of the power-law fits is discussed
in the text.(a) Reduced temperature dependence of in zero field. The data above critical
temperature is fit (red solid line) to the eq , which yields a critical exponent α
= 0.55 ± 0.05. (b) Magnetic field dependence of MR%. The curves
are fit (red solid line) to the power-law MR ∝ −Hm. A quadratic field dependence in the paramagnetic
state suggests the suppression of spin fluctuations by applying external
fields. As T approaches TC, the magnitude of MR increases. Below TC, a reduction in MR% with linear dependence on H is noticed. (c, d) Rescaled magnetic entropy and magnetoresistance
against a reduced temperature θ. The data scales well by falling
onto a single universal curve, irrespective of the strength of H, indicating a SOPT. However, the deviation from the universal
scaling around Tt hints at a first-order
phase transition.δ is obtained using Widom’s
relation δ = 1 + γ/β.α is extracted from the resistivity
and specific heat using eq .Magnetic field
variation of MR, measured at a few representative
temperatures, is shown in Figure b. It is negative, as expected for a ferromagnetic
metal, and isotropic against positive and negative applied fields.
The absolute magnitude of MR increases as T → TC. MR is fit to a power-law dependence MR ∼
−H.[57] A near quadratic dependence (−H1.8) in the paramagnetic region (at 300 K) which
indicates the suppression of spin fluctuations in the presence of
magnetic fields.[58] Near the Curie temperature
MR varies as – H0.74. While further
reducing the temperature below 20 K, MR is observed to follow near-linear
dependence with m = 0.92. The isotropic (independent
of magnetic field’s direction) negative MR was attributed to
the effect of spin alignment toward the interference contribution.[59] Later, Agrinskaya et al.[60] have attributed the observed unusual negative linear MR
in narrow-band gap two-dimensional (2D) quantum well structures of
GaAs-AlGaAs to the magnetic exchange interactions between localized
and delocalized (thermally activated charge carriers) spins. For the
present case, negative linear MR can be attributed to arise from the
scattering of conduction electrons (s and p) from the itinerant d-electrons
of constituent magnetic atoms.In Figure c,d,
the rescaled magnetic entropy and magnetoresistance are plotted against
a reduced temperature θwhere Tp is the
temperature at which absolute ΔSmag and MR are maximum and Tcold and Thot are the hot and cold temperatures taken
from the full width at half-maximum of ΔSmag and |MR|. Overall, the data scale well by falling onto
a single universal curve, irrespective of the strength of the applied
magnetic field, inferring a second-order nature of the phase transition.[44,61] However, the curves are observed to deviate from the universal scaling
below the structural transition Tt. Such
a deviation from the scaling behavior is attributed to the first order
phase transition below Tt.
Summary
MnNi0.7Fe0.3Ge alloy has been studied using
the combined results of magnetization, specific heat, and resistivity
along with electronic structure calculations. The alloy shows a ferromagnetic
transition (TC ∼ 212 K) and an
antiferromagnetic-like transition at (Tt ∼ 180 K) followed by a spin-glass transition (Tg ∼ 51.85 K). Across TC, (i) a well-scaled normalized magnetoresistance and magnetic-entropy,
(ii) frequency independent hump in χAC(T), (iii) the critical exponents and J(r) ∼ r–4.75 suggest mixed
(short and long-range) magnetic interactions with unclassified universality
class of a second-order phase transition. Across Tt, the deviation from the scaling, a narrow thermal hysteresis
between FCC and FCW, and relatively sharp transition in C(T) and 1/ρ(dρ/dT) indicate a weak first-order phase transition. Across Tg, the absence of a clear magnetic transition
in C(T) and the analysis of a frequency-dependent
cusp in χAC(T) reveal cluster spin-glass
behavior. Density functional calculations reveal mixed ferro- and
antiferromagnetic interactions with the dominating ferromagnetic coupling,
which is experimentally evident from the large positive Weiss temperature,
magnetic saturation, and overall negative magnetic-entropy and magnetoresistance.
The magnetically distinct dual transitions of MnNi0.7Fe0.3Ge can be tuned to achieve large table-like MCE.
Authors: R Kainuma; Y Imano; W Ito; Y Sutou; H Morito; S Okamoto; O Kitakami; K Oikawa; A Fujita; T Kanomata; K Ishida Journal: Nature Date: 2006-02-23 Impact factor: 49.962
Authors: Hao Yang; Jiabin Yu; Stuart S P Parkin; Claudia Felser; Chao-Xing Liu; Binghai Yan Journal: Phys Rev Lett Date: 2017-09-28 Impact factor: 9.161
Authors: Z K Liu; L X Yang; S-C Wu; C Shekhar; J Jiang; H F Yang; Y Zhang; S-K Mo; Z Hussain; B Yan; C Felser; Y L Chen Journal: Nat Commun Date: 2016-09-27 Impact factor: 14.919