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[Masamichi Nishino](https://orcid.org/0000-0002-2060-2303), Seiji Miyashita

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[Atomistic Model Study on Magnetic Properties of Permanent Magnets—Treatment of Thermal Fluctuation and Thermal Effects, and Future Perspective—](https://mdr.nims.go.jp/datasets/4e621c9d-c03b-4a03-a167-2a7f64aca4a9)

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Atomistic Model Study on Magnetic Properties of Permanent Magnets—Treatment of Thermal Fluctuation and Thermal Effects, and Future Perspective—Atomistic Model Study on Magnetic Properties of Permanent Magnets—Treatmentof Thermal Fluctuation and Thermal Effects, and Future Perspective—+1Masamichi Nishino1,+2 and Seiji Miyashita21National Institute for Materials Science, Tsukuba 305-0047, Japan2Graduate School of Science, The University of Tokyo, Tokyo 113-0033, JapanWe review atomistic spin model studies, a new approach for theoretical investigations, on magnetic properties of permanent magnets. Inthe atomistic modeling, the microscopic details of magnetic parameters and lattice structures are realistically considered, and the temperatureeffect, including thermal fluctuation, is properly treated based on statistical physics methods: Monte Carlo methods and stochastic Landau-Lifshitz-Gilbert equation methods. We introduce how to treat thermal effects for static and dynamical properties using these methods. Focusingespecially on neodymium permanent magnets, we discuss features of magnetization, domain wall, coercivity of a grain, nucleation and pinningfields, and dysprosium substitution effect, which were first elucidated with those methods. [doi:10.2320/matertrans.MT-M2024132](Received August 28, 2024; Accepted October 28, 2024; Published December 25, 2024)Keywords: atomistic spin model, thermal fluctuation, thermal effects, permanent magnets, stochastic Landau-Lifshitz-Gilbert (LLG) equation,Monte Carlo method1. IntroductionThe control of the coercive force (coercive field) ofpermanent magnets is an important issue for achieving highenergy conversion efficiency. Neodymium magnets (Nd-Fe-Bmagnets) [1–9] are known as powerful permanent magnetsand used in motors, generators, electrical appliances, etc.Their application is expected to expand in the future due tothe growing demand for electric vehicle motors. Neodymiummagnets have a problem with coercivity at high temperaturesand are often reinforced by adding heavy rare earths suchas dysprosium (Dy). Japan depends on foreign countries forthe rare earth resources, but due to price instability, etc.,development of high-performance permanent magnets withreduced use of rare elements is required.Against this background, the Elements Strategy InitiativeCenter for Magnetic Materials (ESICMM) project (2012–2021), a national project based at National Institute forMaterials Science (NIMS), has been carried out for 10 yearssince 2012, and coercivity research has made significantprogress in both experimental and theoretical aspects [10]. Inthis review, we mainly focus on the microscopic modelingbased on the electron theory and theoretical studies on thecoercivity at finite temperatures which were developed by theauthors and collaborators in ESICMM [11–28].Theoretical studies of the magnetic properties and coerciveforce of permanent magnets have been developed in the fieldof micromagnetics [29]. For details of micromagneticssimulations, please refer to the review by Tomohiro Tanakain the same special issue. In micromagnetics simulations,a continuum model in which the magnetization is spatiallycontinuous with nm-order block magnetization (fixedmagnitude of magnetization) as the smallest unit isconsidered, and magnetic materials are described with asmall number of macroscopic magnetic parameters, mainlyexchange stiffness constant (A) and magnetic anisotropyenergy (K ). This method has the advantage that the system(the size is on the order of µm) of the aggregate of grainsconstituting a magnetic material can be treated, and manysimulations of magnetic properties such as magnetizationreversal have been carried out. However, due to the coarsegraining of the model, the microscopic mechanism of themagnetic properties induced by atomic-scale magneticinteractions cannot be treated. In addition, there is a problemin handling thermal fluctuations and temperature effects, asdescribed below.Coercivity at finite temperatures is a phenomenon thatinvolves the collapse of a metastable magnetic state due tothermal activation. The magnetization reversal is a stochasticprocess, since it requires crossing the energy barrier and iscaused by thermal fluctuations. In order to study such effectsquantitatively, it is necessary to treat entropy effects attemperature T correctly according to statistical mechanics.In thermal equilibrium, using the energy E(i) of state i, theprobability of realization of state i, Peq(i), in the canonicalensemble is expressed asPeq ¼1Ze�¢EðiÞ: ð1ÞHere, ¢ is defined by ¢ ¼ 1kBTusing the Boltzmann constantkB. Z is a quantity called the partition function and defined byZ ¼Xallie�¢EðiÞ: ð2ÞThe sum is taken for all states. Thus, the value of the thermalequilibrium state ©Aª of any physical quantity A is given bythe average in the canonical ensemble as followshAi ¼ 1ZXalliAðiÞe�¢EðiÞ: ð3ÞWhen using the coarse-grained Hamiltonian for thecontinuum model of micromagnetics, the degrees of freedom(entropy) of the states are unclear and it is difficult to applythe above probabilities. In order to properly handle temper-+1This Paper was Originally Published in Japanese in J. Japan Inst. Met.Mater. 87 (2023) 158–172.+2Corresponding author, E-mail: nishino.masamichi@nims.go.jpMaterials Transactions, Vol. 66, No. 1 (2025) pp. 1 to 16©2024 The Japan Institute of Metals and Materials OVERVIEWhttps://doi.org/10.2320/matertrans.MT-M2024132ature effects, it is necessary to use statistical mechanicsmethods with the canonical ensemble. By constructing a spinmodel based on atomistic theory that takes into account thespin of all atoms in the system, the state and number of states(entropy) can be defined, and statistical mechanics methodscan be used to correctly incorporate temperature effects in theanalysis. In this paper, we will focus on neodymium magnetsin particular, explain the atomistic spin model, and introducestatistical mechanics methods for calculating magneticproperties at finite temperatures (including absolute zero).Various magnetic properties revealed by using the method-ologies will be discussed.2. Atomistic Spin ModelThe unit cell of Nd2Fe14B, the hard magnet phase ofneodymium magnets, is shown in Fig. 1 [30]. There are twotypes of Nd sites, six types of Fe sites and one type of B site.We adopt the following atomistic Hamiltonian as a micro-scopic model for neodymium magnets [13–15, 24]. Thissystem is a three-dimensional ferromagnet, and we treat thespins classically.H ¼ �Xi<j2Jijsi � sj �XFeiDiðszi Þ2þXNdiXl;m�l;iAml;ihrliiÔml;i � hXiSzi : ð4ÞJij is the exchange interaction between the ith and jth atomsand Di is the anisotropy energy of the ith Fe atom. The thirdterm is the crystal electric field (CEF) energy of Nd, where©l,i, Aml;i, ©rlªi and Ôml;i are the Stevens factor, coefficient of thespherical harmonics of the crystalline electric field, averageof rl over the radial wave function, and Stevens operator,respectively. The fourth term is the Zeeman term, where h isthe external magnetic field. We consider l = 2, 4, 6 and m = 0(diagonal terms). Ôml;i is expressed as Ô02 ¼ 3J2z � J2, etc.For Fe and B atoms, si denotes the magnetic moment of thei-th site, whereas for Nd, si is the moment of the valenceelectrons (5d and 6s) and strongly coupled to the moment ofthe 4-f electrons, J i ¼ gTJi®B through the Hund couplingas shown in Fig. 2(a). Here, gT is Landé g-factor and Ji is thetotal angular momentum consisting of the orbital angularmomentum L and the spin angular momentum S. J ¼ L�S ¼ 9=2 and gT = 8/11. Therefore, the total moment of Ndatoms is Si ¼ si þJ i. For Fe and B atoms, we define Si = si.Note that si of a Nd atom and Si (= si) of an Fe atom areantiferromagnetically coupled, while Si of a Nd atom and Siof an Fe atom are ferromagnetically coupled.We used the magnetic moments and exchange interactionsestimated by Korringa-Kohn-Rostoker (KKR) [31] ab initiocalculations. The values are given in Ref. [24]. Nd2Fe14B hasitinerant electrons, but no methodology has been establishedto incorporate the effect of itinerant magnetism. Here, weassumed that Jij is widely distributed with respect to thedistance due to the itinerancy. We then considered Jij in therange of r = 3.52¡, where the contribution to the magneticinteractions is large [13]. For the anisotropy of Fe, we adoptthe literature values estimated by a first-principles calculation[32]. For Nd atoms, the first-principles estimates of thecrystal field coefficients Aml;i are not yet established, so weadopted the experimental estimates [33], and for ©rlªi we usedthe values of a Hartree-Fock calculation [34]. For the systemsize treated in this review (less than a few tens of nm scale),the magnetic dipole interaction is not so important and wasnot considered here, but its treatment will be discussed inchapter 8.3. Computational Methods for Thermodynamic Quan-tities and DynamicsIf an atomistic spin model such as eq. (4) is constructed,the states and number of states of the system can be clearlydefined, and finite temperature properties can be calculatedusing statistical mechanics methods. Here we mainly describeMonte Carlo methods used to calculate thermal equilibriumstates, and the stochastic Landau-Lifshitz-Gilbert (sLLG)equation [11, 35] used to calculate time-dependent dynamics.3.1 Monte Carlo method3.1.1 Canonical ensemble Monte Carlo methodMonte Carlo methods are often used to calculate thephysical quantity ©Aª in thermal equilibrium. In Monte Carlomethods, the eq. (3) is realized by sampling with aprobability dependent on the state i (importance sampling)and taking the sampling average. Let the spin state(S1*Sk*SN) be the state i at time t, then the probabilityof state i at t + ¦t is given by the following master equationPði; tþ�tÞ ¼ Pði; tÞ �Xj 6¼iWði ! jÞ�tPði; tÞþXj 6¼iWðj ! iÞ�tPðj; tÞ: ð5ÞHere, W(i ¼ j) is the transition probability per unit time froma bc(a)(b)(c)12.198.80Fig. 1 (a) Unit cell of Nd2Fe14B. Nd, Fe, and B atoms are denoted by red,blue, and yellow spheres, respectively. The lattice constants for the a, b,and c axes are da = db = 8.80¡, and dc = 12.19¡, respectively. (b) Sideview (from a or b axis). (c) Top view (from c axis). Reprinted figure withpermission from [M. Nishino et al., Phys. Rev. B 103, 014418 (2021)].Copyright (2021) by the American Physical Society. (online color)M. Nishino and S. Miyashita2state i to state j. In Monte Carlo methods, the state is updatedevery one step (one Monte Carlo step) with ¦t = 1. If thefollowing ergodicity and detail balance are satisfied for thetransition probability W(i¼ j) for any states i, j, then startingfrom any initial state, convergence to a unique stationary stateis guaranteed, generating an equilibrium distribution (ca-nonical distribution).(I) Ergodicity (connectivity condition): for any states i, j, thetransition probability W(i ¼ j) is non-zero, or can beexpressed as the product of a finite number of non-zerotransition probabilities.(II) Detailed balance (this is a sufficient conditions and thereare some methods which do not satisfy the detailed balance[36]):PðiÞeqWði ! jÞ ¼ PðjÞeqWðj ! iÞ: ð6ÞLet P(i)eq = e¹¢E(i)/Z (equilibrium distribution). In theMetropolis algorithm, which is often used to practice theseconditions, the state update of i ¼ j is performed with theprobability W(i ¼ j) = 1 for HðiÞ � HðjÞ and Wði ! jÞ ¼expð�¢ðHðjÞ �HðiÞÞÞ for HðiÞ < HðjÞ. The transitionprobabilities can be chosen arbitrarily if (I) and (II) aresatisfied. Since the Monte Carlo step is different from realtime, Monte Carlo methods are used for the calculation ofphysical quantities in equilibrium and of the free energy asshown in Sec. 3.1.2, while the method described in Sec. 3.2is used for the analysis of real time dynamics.3.1.2 Generalized ensemble methods and free energycalculationsThe partition function can also be expressed using thedensity of states ³(E) with respect to energy asZ ¼XE�ðEÞe�¢E: ð7ÞOnce the density of states is known, the partition function isobtained and the free energy F can be calculated by thefollowing equation.F ¼ � 1¢lnZ: ð8ÞUsing the multi-canonical Monte Carlo method [37, 38] it ispossible to calculate the free energy.In the canonical ensemble Monte Carlo method justdescribed, the sampling is based on the Boltzmann factore¹¢E. In this sampling, the states near a high energy barrierhave low probabilities of realization P(E) (£ e¹¢E) and arenot sampled well. Therefore, the energy histogramH(E) £ ³(E)P(E) £ ³(E)e¹¢E is close to zero for energiesnear high barriers. The multicanonical method samples by anon-Boltzmann factor e¹f (E) so that high energy states arealso sampled. The probability of realization P(E) is adjustedso that the energy histogram H(E) is flat (H(E) = C(const-ant)), and finally a random walk on the energy space isrealized to obtain PðEÞ ’ C�ðEÞ. When ³(E)/C is obtained,the free energy can be calculated from the eqs. (7) and (8)(where C is the contribution of constant). This method ismore laborious than canonical ensemble Monte Carlomethods, but the Wang-Landau method [38], which is akind of the multi-canonical method, is often used. The multi-canonical method and the replica exchange method thattakes into account transitions between different temperatures[39], etc., are called generalized ensemble methods. Thesemethods were developed for the calculation of first-ordertransitions and for the calculation of global minima insystems with multi-valley structures of potential energy, andare used in various fields such as spin glass relaxation andprotein structure calculations.In coercive force (field) analysis, it is convenient toconsider the probability of realization in the magnetizationspace. Using the density of states as a function of energy andmagnetization Mz, the partition function is expressed asZ ¼XMzXE�ðE;MzÞe�¢E �XMzZðMzÞ: ð9ÞWith the formulaFðMzÞ ¼ � 1¢lnZðMzÞ; ð10Þthe free energy in the magnetization space (free energylandscape) can be calculated, and the energy barrier as afunction of magnetization can be obtained. Here, thehistogram H(Mz) for magnetization is H(Mz) £ Z(Mz) in thecanonical ensemble, but H(Mz) £ Z(Mz)P(Mz) in the multi-canonical method, and the probability of realization ofmagnetization P(Mz) is adjusted so that H(Mz) = C as in theenergy case [40, 41]. Finally, P(Mz) = C/Z(Mz) is obtained,and F(Mz) is obtained from the formula (10).3.2 Stochastic LLG equation methodThe Monte Carlo method is an effective method forExNdFe4f5dHundSOIExDyFe4f5dHundSOI(a) (b)s sFig. 2 (a) Magnetic coupling between Nd and Fe atoms. The total moment in an Nd atom and that in an Fe atom are ferromagneticallycoupled. Ex and SOI represent the exchange interaction and spin-orbit interaction, respectively. (b) Magnetic coupling between Dy andFe atoms. The total magnetic moment of a Dy atom and that of an Fe atom are antiferromagnetically coupled. Reprinted figure withpermission from [M. Nishino et al., Phys. Rev. B 106, 054422 (2022)]. Copyright (2022) by the American Physical Society. (onlinecolor)Atomistic Model Study on Magnetic Properties of Permanent Magnets 3calculating zero-temperature or finite-temperature equilib-rium states, but it does not provide concrete information onreal-time dynamics, such as what the state will be after acertain number of seconds. For real-time dynamics, it isnecessary to solve the equations of motion for spins. TheLLG equation (eq. (11)) is a standard equation, whichconsists of the equation of motion of the torque representingthe precession motion of the magnetization and its relaxationterms.ddtSi ¼ � £1þ ¡2iSi � heffi � ¡i£ð1þ ¡2i ÞSiSi � ½Si � heffi �:ð11ÞHere, £ is the electron gyromagnetic ratio and ¡i is thedamping constant.heffi ¼ � @H@Sið12Þis the effective magnetic field applied to the i-site, includingthe external magnetic field, exchange interactions and dipoleinteractions around the i-site, and magnetic field due to themagnetic anisotropy energy of the i-site.At absolute zero temperature, there are no processescrossing the energy barrier because there are no thermalfluctuations, and the dynamics of magnetization can becalculated using this equation. In contrast, in the finitetemperature case, thermal fluctuations can cause a relaxationprocess from a metastable state to a stable state crossing theenergy barrier. The effect of thermal fluctuations is given byintroducing a noise field ²i(t) [11, 35]. heffi is modified asfollows.heffi ¼ � @H@Siþ �iðtÞ: ð13ÞHere, �iðtÞ ¼ ð²xi ; ²yi ; ²zi Þ is the white Gaussian noise andsatisfies the following relationsh²®i ðtÞi ¼ 0; h²®i ðtÞ²¯jðsÞi ¼ 2Di¤ij¤®¯¤ðt� sÞ: ð14ÞThis noise is related to temperature as shown below. The timeevolution equation of the probability distribution functionequivalent to this sLLG equation (Stratonovich representa-tion of the Fokker-Planck equation) [11] is given by@@tPðS1; � � � ; SN; tÞ ¼Xi£1þ ¡2i@@Si���¡iSiSi � ðSi �Heffi Þ� £DiSi � Si �@@Si� ��PðS1; � � � ;SN; tÞ�þXi£1þ ¡2iðSi �Heffi Þ � @@SiPðS1; � � � ;SN; tÞ: ð15ÞNow, if the following fluctuation-dissipation relation issatisfiedDi ¼¡ikBT£Si; ð16Þit can be proved that the distribution function in the steadystate (t ¼ ¨) at temperature T corresponds to the canonicaldistribution [11, 35]PeqðS1; � � � ;SNÞ / expð�¢HðS1; � � � ;SNÞÞ: ð17ÞThat is, given a damping constant, the temperature T can becontrolled by changing the magnitude (amplitude) of thenoise. The sLLG equation is a stochastic differentialequation, and since the noise is multiplied by the physicalquantity (magnetization), it is a so-called multiplicativeprocess, and care must be taken in the method of integration.4. Thermodynamic Properties4.1 MagnetizationFigure 3 shows the temperature dependence of magnet-izations of Nd2Fe14B magnets in equilibrium, calculated bythe sLLG and Monte Carlo methods (Metropolis algorithm).M is the magnitude of magnetization, Mz is the z componentof magnetization (c-axis component), and Mxy is the xycomponent of magnetization (ab-plane component). Thecalculated values of the sLLG equation and those of theMonte Carlo method are in good agreement, and theequilibrium state (canonical distribution) is realized in thecalculations with both methods.The spin-reorientation transition is confirmed by simu-lations to occur around 150K, where Mz has a maximum[4, 6–8]. Figure 4(a) illustrates the temperature dependenceof the crystal electric field (CEF) energy of Nd atoms inNd2Fe14B. ª is the angle from the c-axis. At absolute zerotemperature, the potential minimum exists at ª ’ 0:2³ andª ’ 0:8³, but above the spin-reorientation transition temper-ature, the minimum shifts to ª = 0 and ª = ³, and it isunderstood that the spin-reorientation transition occurs.The Curie temperature TC is about 870K (the estimatedvalue of TC for the infinite system by Binder plot [42]), whichoverestimates the experimental value of about 600K [4, 5].This is due to the overestimation of the magnetic interactionsin the first-principles calculation. However, considering thecurrent accuracy of first-principles calculations, it is asufficiently reliable value. Therefore, we will henceforthexpress temperature in units of TC. In our experience, forobtaining physical quantities in equilibrium, the Monte Carlomethod requires shorter simulation time.Magnetization [ B / formula unit]05101520253035400 200 400 600 800 1000 1200M(sLLG)Mz(sLLG)Mxy(sLLG)M(MC)Mz(MC)Mxy(MC)T [K]Fig. 3 Temperature dependences of M, Mz, and Mxy of the atomistic modelfor the Nd2Fe14B magnet with comparison between Monte Carlo andstochastic-LLG methods. 6 © 6 © 6 unit cells with periodic boundaryconditions. (online color)M. Nishino and S. Miyashita44.2 Domain wallThe properties of domain walls are important in the studyof the magnetization reversal process. In this section, weshow the variation of the domain wall shape and width withtemperature calculated by the Monte Carlo method (Metrop-olis method). Since neodymium magnets have anisotropyalong the c-axis, two types of domain walls are possible, asshown in Fig. 5(a). One is a Bloch-type domain wall thatmoves along the a-axis (or b-axis), and the other is a Néel-type domain wall that moves along the c-axis. Regarding thedomain walls of Bloch and Néel, the magnetization {Mz(x)}at position x in the a-axis and c-axis, respectively, wascalculated by the Monte Carlo method, and superimositionsof the obtained snapshots (symbols) are shown in Fig. 5(b)and Fig. 5(c) [14]. The abscissa is in units of the latticeconstant. Next, from these plots, we obtained the domainwall width. The domain wall width is defined in thecontinuum model as follows [29]. Let m(T ) be the magnitudeof magnetization at temperature T, the z component ofmagnetization at position x from the center of the domainwall (mx(x) = 0) ismzðxÞ ¼ �mðT Þ tanh x¤0� �: ð18Þ¤0 is called the wall parameter and is defined by ¤0 �ffiffiffiffiffiAK1p,where A and K1 are the stiffness constant and the firstmagnetic anisotropy constant, respectively, of the continuummodel. The domain wall width is given by¤W ¼ ³¤0 ¼ ³ffiffiffiffiffiffiffiAK1r: ð19ÞBy fitting mz(x) (eq. (18)) with ¤0 and m(T ) as fittingparameters to the snapshot data of Mz obtained by the MonteCarlo method, ¤0 is obtained and the domain wall width ¤Wcan be evaluated. The temperature dependence of the domainwall width is given in Fig. 5(d). At high temperatures, thedomain wall broadens. At around room temperature, it isabout 6–7 nm. The domain wall widths estimated byexperiments for A and K1 [29, 43, 44] are 3.6–5.4 nm, andthose observed by electron microscopy [45–47] are 1–10 nm.The calculated values are close to the experimental ones.The fact of the narrower width of the Néel wall than that ofthe Bloch wall is considered to be due to the lattice structurein which the Nd surface is perpendicular to the c-axis. Theexchange interactions between adjacent Nd and Fe atoms aresmaller than those between adjacent Fe atoms. The exchangeenergies «2Jijsisj« are 1.60³7.10meV (r ¯ 3.52¡) for theformer, while the latter are 16.22³44.6meV. The temperaturedependences of the Bloch and Néel domain walls can alsobe evaluated by determining the macroscopic parameters, thestiffness constant and magnetic anisotropy constant, fromatomistic models. The Monte Carlo method for the canonicalensemble is used to find the domain wall energy EDW(T ) attemperature T, and by using a constrained Monte Carlomethod with a fixed magnetization direction [48], ª-depen-dence of the finite temperature magnetic anisotropy energy(a) (b)0 K0.34TC0.46TC0 K0.34TC0.46TC0501001502002500 0.2 0.4 0.6 0.8 1Energy [K]0501001502002500 0.2 0.4 0.6 0.8 1Energy [K]0.69TC0.69TCNd DyFig. 4 Crystal electric field energy (a) for a Nd atom and (b) for a Dy atom as a function of ª at zero and finite temperatures. Reprintedfigure with permission from [M. Nishino et al., Phys. Rev. B 106, 054422 (2022)]. Copyright (2022) by the American Physical Society.(online color)x/da-3-2-10123-10 -5 0 5 10Mzx/dc-3-2-10123-10 -5 0 5 10Mz(a) (d)(b) (c)02468100.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8W [nm]T/TcabccabBlochNéelFig. 5 (a) Bloch-type wall and Néel-type wall. (b) Mz along a-axis (Bloch-type) at 0.46TC. The unit of the vertical axis is ®B/atom.The functions mz(x) is given by a solid line. Here symbols denote Mz(x) at different MC steps. (c) Mz along c-axis (Néel-type) at 0.46TC.(d) Temperature variation of ¤W for Bloch-type (triangles) and Néel-type (circles) walls. Reprinted figure with permission from[M. Nishino et al., Phys. Rev. B 95, 094429 (2017)]. Copyright (2017) by the American Physical Society. (online color)Atomistic Model Study on Magnetic Properties of Permanent Magnets 5EAðT Þ ¼ K1ðT Þ sin2 ª þK2ðT Þ sin4 ª þK4ðT Þ sin6 ª ð20Þcan be calculated. K1(T ), K2(T ), and K4(T ) for Nd2Fe14B areobtained by fitting the coefficients of EA(T ) [13, 17]. Thestiffness constant A(T ) is obtained by the relation:EDWðT Þ ¼ 2ffiffiffiffiffiffiffiffiffiffiAðT Þp Z ³0dªffiffiffiffiffiffiffiffiffiffiffiffiffiEAðT Þp: ð21ÞFrom the magnetic anisotropy energy and stiffness constant,the temperature dependence of the domain wall width dW ¼³ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiAðT ÞEAðT Þ³=2�EAðT Þ0pis obtained. The A(T ) obtained in this wayis actually smaller in the c-axis than in the a-axis, and thetemperature dependences of both domain wall widths dW arevery close to those in Fig. 5(d) [17].5. Coercivity of NanograinThe coercive force (field) is the threshold field at which themetastable magnetization collapses. At absolute zero temper-ature, it is the field at which the energy barrier vanishes, butat finite temperatures, the process of jumping over the freeenergy barrier becomes possible due to thermal fluctuations.When the inverse magnetic field is strong or the temperatureis high, the barrier disappears and the magnetization relaxesdeterministically and smoothly, as shown in Fig. 6(a). Onthe other hand, when the magnetic field is weak and thetemperature is low, there is a barrier as shown in Fig. 6(b),and the relaxation is caused by thermal fluctuations andoccurs stochastically as a kind of Poisson process, resulting(a) (b)MZ MZF F(c)Fig. 6 (a) Deterministic process. (b) Stochastic process by barrier-crossing dynamics. (c) Snapshots of the magnetization reversal for thenano grain from the all-down spin state under a reversed field (h = 4.0 T). Red and blue parts denote down-spin and up-spin states,respectively. Reprinted figure (c) with permission from [M. Nishino et al., Phys. Rev. B 102, 020413(R) (2020)]. Copyright (2020) bythe American Physical Society. (online color)M. Nishino and S. Miyashita6in a longer relaxation time. In this section, we describemethods to investigate the coercivity of nanograins.The magnetization reversal dynamics by the sLLG methodwas studied for a nanograin of 12 © 12 © 9 unit cells atT = 0.46TC (near room temperature) [19]. Figure 6(c) showssnapshots of the magnetization reversal from the down spinstate at ¡ = 0.1 under the reversed magnetic field h = 4.0 T.This relaxation is in the stochastic regime. Nucleation occursfrom a corner, and the reversal region was first expandedwith a Bloch-type domain wall parallel to the ab-plane, andthen grew in the direction of the c-axis with a Néel-typedomain wall. This trend is independent of ¡. This process isdue to the fact that the exchange interactions along the a- andb-axes are stronger than those along the c-axis. When a singlenucleation is the rate-determining event, the large distributionof relaxation times makes it difficult to evaluate the meanrelaxation time. To overcome this difficulty, we introduced astatistical relation between the reversal probability p and therelaxation time ¸ as a statistical method for evaluating therelaxation time.If an event (relaxation) occurs with probability p in unittime, the probability that the event occurs for the first time inperiod [t, t + ¦t] is pe¹pt¦t. Thus the average relaxation time©¸ª is given by the following formula.h¸i ¼ pZ 10te�ptdt ¼ 1p: ð22ÞThe probability that an event occurs in period [0, t] isP(t) = 1 ¹ e¹pt. Thus, after running N simulations, thenumber of samples of non magnetization reversal (survived)is Nsv(t) = N ¹ Ndone(t) = Ne¹pt. From this relation, p (and ¸)can be obtained from the slope of the graph of ln(Nsv(t)/N ).Figure 7(a) shows the magnetic field dependence of therelaxation times for various ¡ values. The relaxation timeincreases rapidly as the magnetic field decreases below 4.2 T.From a real-time simulation of 0.5 ns, a sub-µs relaxation canbe calculated by using the statistical relation. Since coercivityis a relaxation phenomenon of 1 s in the experiment, thefollowing fitting function was used to estimate the 1 srelaxation (a long relaxation time). For long relaxation times,a single exponential decay of Arrhenius type is expected.Therefore, the relaxation time was extrapolated by includinga correction term in the form of a double exponential fittingof eq. (23).¸ðhÞ ¼ Ae�ah þ Be�bh ¼ Ae�ahð1þ Ce�dhÞ; ð23Þwhere C = B/A and d = b ¹ a. In Fig. 7(b), the fitted linesby this equation are depicted. The intersection of each lineand ¸ = 1 s gives the coercive force. The coercive force wasestimated to be about 3 T (Hc = 3–3.2 T). From Fig. 7(b),we can see that the threshold field obtained from the realisticsimulation time (ns) is about 20–25% larger than thethreshold field corresponding to the relaxation of 1 s. In thefollowing sections, we estimate the coercive force from therelaxation of the order of ns, which is about 20% higher thanthe coercive force corresponding to 1 s.In the above, we directly measured the relaxation time ofmagnetization reversal and obtained the relaxation time fromNsv(t), but we can also estimate the coercivity from thesurvival probability P(H ) = Nsv(H )/N for a magnetic fieldsweep (the field h is denoted by H(t) as a function of time).The probability of Arrhenius relaxation is given by p ¼1¸0e�¢EBðH Þ. For ¸0 we adopt the value ¸0 = 10¹11 s [49],which is often used in magnetization reversal. Theprobability of no relaxation (survival) when the magneticfield is swept from H = ¹¨ (down spin state) to H as alinear function of time H(t) = vt is given by the followingformula [28].PðHÞ ¼ exp � 1v¸0Z H�11e¢EBðhÞ dh� �: ð24ÞHere, the phenomenological relation often used in the studyof magnetization reversal in permanent magnets [50, 51]EBðHÞ ¼ E0 1� HH0� �nð25Þis applied. E0 is the energy barrier under zero magnetic fieldand H0 is the magnetic field for zero barrier. The value ofthe exponent n is established as n = 1³2 for many magneticmaterials. In the case of coherent magnetization reversal asin the Stoner-Wohlfarth model, the exponent is n = 2 [52]. Ithas been experimentally shown that n ’ 1 in neodymium10-1210-1010-810-610-40.0110 1 2 3 4 5 6 7 8 = 0.1 = 0.15 = 0.2MC [s]h [T]0 1 2 3 4 5 6 7 8(b)10-1210-1110-1010-910-810-73 4 5 6 7 8 = 0.1 = 0.15 = 0.20MC [s]h [T](a)Fig. 7 (a) Magnetic field dependence of the relaxation time (magnetization reversal time) with the damping factor (¡) dependence.(b) Extrapolation of the relaxation time. MC denotes the relaxation time of the Arrhenius law (¸ = ¸0e¦F) estimated in a Monte Carlostudy [21]. Reprinted figure with permission from [M. Nishino et al., Phys. Rev. B 102, 020413(R) (2020)]. Copyright (2020) by theAmerican Physical Society. (online color)Atomistic Model Study on Magnetic Properties of Permanent Magnets 7magnets [50, 53]. Here, n = 1 is adopted. The aboveprobabilities can also be computed for n = 2. In fact, n = 1gives a closer value than n = 2 to the coercivity estimated forthe above system [28]. Using eq. (25), we obtainlnð�lnPðHÞÞ ¼ ¢E0H0H þ ln e�¢E0H0v¸0¢E0� �ð26Þand E0 and H0 can be evaluated from the slope and y-intercept when the left-hand side is plotted as a function ofmagnetic field.On the other hand, the relaxation time ¸ is ¸ =¸0 exp(¢¦F ), and from this relation ¢¦F = 25.3 when ¸ =1 s and ¸0 = 10¹11 s. Setting ¦F = EB(H ),¢�F ¼ ¢E0 1� HcH0� �¼ 25:3: ð27ÞFrom this relation, the coercive force is given using H0 and¢E0 asHc ¼ H0 1� 25:3¢E0� �: ð28ÞThe coercive force can be calculated using E0 and H0evaluated with the formula (26). In fact, applying thismethod to the above nanograin, we obtained a coercivity ofabout 3 T [28].The coercive force of the nanograin can also be obtainedby calculating the free energy for magnetization using theMonte Carlo method described in Sec. 3.1.2. The Wang-Landau method is used to obtain F(Mz,H = 0) under zeromagnetic field H = 0. The free energy under a magneticfield H is obtained asFðMz;HÞ ¼ FðMz;H ¼ 0Þ �HMz: ð29ÞThe left panel of Fig. 8(a) shows the relation between themagnetizationMz (M in the figure) and free energy for severalmagnetic fields including H = 0, and the right panel presentsthe energy barrier at 3.5 T. Figure 8(b) shows energy barriersto the magnetic field for several sizes of grains. Since theenergy barrier corresponding to ¢F = 25.3 can be crossed bythermally activated effects, the coercive field is the magneticfield at the point where the free energy curve intersects25.3kBT. In the system of 12 © 12 © 9 unit cells, theintersection of the blue curve and 25.3kBT is Hc = 3.3 T[21]. This value is close to the coercive force obtained by thereal-time dynamics method described above, indicating thevalidity of the coercivity evaluation of both methods. Asshown in Fig. 8(b), the coercivity almost saturates when thegrain size exceeds 20 nm.6. Nucleation and Pinning Fields6.1 Hard–soft–hard magnet modelIn order to realize stronger coercivity at high temperatures,it is necessary to investigate the effect of grain and grainboundary structures and properties on the coercivity. For thispurpose, a hard-soft-hard magnet model (Fig. 9) in whichhard magnets are in contact with an intermediate soft magnethas been studied [54–57]. This model captures the essence ofnucleation and pinning in inhomogeneous systems and hasbeen used to analyze various phenomena in experimental andtheoretical studies of magnetic materials including GMRsensors [50, 58, 59]. In particular, for a continuum model of ahard–soft–hard magnet at zero temperature, one-dimensionalnonlinear equations are solved with stiffness and magneticanisotropy constants as parameters. The obtained diagramrepresenting the nucleation and depinning field thresholds(the former is called nucleation field and the latter pinningfield) as a function of the ratio of the parameters is wellknown and has been used in the interpretation of experiments[55, 56].Here we will see how the diagram is modified by the effectof thermal fluctuations. For this purpose, we consider amodel of hard–soft–hard magnet in a simple cubic lattice ofthe Heisenberg model with an anisotropy term. First, in orderto define the parameters, the continuum model HamiltonianH ¼ZdrA2ðrmðrÞÞ2 �KmzðrÞ2 �MH �mðrÞ� �ð30Þis considered. Here, m is the unit vector of the magnetizationdirection at position r, and A is the exchange stiffnessconstant, K is the anisotropy constant, H is the magneticfield, and M is the magnitude of magnetization. The magnetic(a)MzMz, HMtMz(b)Fig. 8 (a) Free energies as a function of Mz of the Nd2Fe14B grain at0.46TC. Lx = Ly = 14.1 nm, Lz = 14.6 nm. Red line is for H = 0 and otherlines are for applying H. (b) Free-energy barriers as a function of themagnetic field for four system sizes: Lx = 10.6 nm, 14.1 nm, 21.1 nm,24.6 nm (Lx = Ly, Lz = 1.038Lx). Reprinted figure with permission from[Toga et al., npj Comput. Mater. 6, 67 (2020)]. Copyright 2020 NPG.(online color)L1 L2 L3xyzHard Soft HardRegion I Region II Region IIIFig. 9 Schematic picture of a system consisting of two bulk hard magnetsand a boundary soft magnet. Regions I and III are characterized by J1, D1and S1, while region II is characterized by J2, D2 and S2. Free boundaryconditions are adopted for the lattice model. (online color)M. Nishino and S. Miyashita8properties of the hard (soft) magnets are specified by thestiffness constant A1 (A2), the anisotropy constant K1 (K2),and the magnitude of magnetization M1 (M2). Normalizedexternal magnetic fieldh ¼ HHSW; HSW � 2K1M1ð31Þand parametersF ¼ A2M2A1M1ð32ÞE ¼ A2K2A1K1; ð33Þare defined [12, 55]. HSW is the Stoner-Wohlfarth field of thehard magnets.Consider the case where the magnetization of the system isoriented in the positive direction (z direction) and a reversedmagnetic field is applied. The state of magnetization in eachof the regions I to III is defined as follows.• (+++) is a state in which the magnetizations inregions I, II, and III are in the positive direction.• (+¹+) is a state in which nucleation and thenmagnetization reversal have occurred in region II,while the magnetizations in the other regions remainpositive.• (+¹¹) is a state where the magnetization is keptwithout reversal only in region I.• (¹¹¹) is a state where the magnetizations in thewhole region are reversed.The threshold field at which (+++)¼ (+¹+) occurs atT = 0, i.e., the threshold field at which nucleation occurs inregion II (soft phase) is given byhNCIIð0Þ ¼EF: ð34ÞHowever, this is calculated in the limit of infinite width of W,and the threshold value is slightly larger than this value whenW is of finite width [55]. The threshold field at which(+¹+) ¼ (¹¹¹) or (+¹¹) ¼ (¹¹¹) occurs at T = 0,i.e., the threshold field at which the domain wall propagatesfrom region II to regions I and III (hard magnet phase) isgiven byhDWPð0Þ ¼1� Eð1þffiffiffiffiFpÞ2 : ð35ÞThis magnetic field is called the pinning field. Forh < hDWP(0), the domain wall does not propagate into thehard magnetic phase. For hNCII(0) < h < hDWP(0), the mag-netization reversed by nucleation is confined to region II andthe state is (+¹+). For the magnetization reversal of thewhole system, the threshold field (nucleation field) is thelarger value of hNCII(0) and hDWP(0),hNCð0Þ ¼ maxEF;1� Eð1þffiffiffiffiFpÞ2� �: ð36ÞThe dotted line (straight line) in Fig. 10(a) illustrates thisrelation for F = 0.5.In the following, we treated the anisotropic Heisenbergmodel on the lattice (37) to investigate temperature effects[12]. We observed how this diagram changes with temper-ature effects. The system is the following spin model on asimple cubic lattice with Lx © Ly © Lz = 60 © 6 © 6 sites.L1 = L2 = L3 = 20.H ¼ �Xhi;jiJi;jsi � sj �XNi¼1DiS2i;z �HXNi¼1Si;z: ð37ÞFor Ji, j > 0, only the nearest neighbor interaction wasconsidered, and g®B = 1 was the unit.In this case, J was used instead of A, D instead of K, andthe parameters F and E were defined asF ¼ J2S2J1S1; ð38ÞE ¼ J2D2J1D1: ð39ÞThe magnitudes of magnetization were set equal in regions I,II, and III («Si« = S1 = S2 = 1) and the magnetic anisotropyenergy of the hard phase was set to D1 = 0.2J1. The Curietemperature of the hard phase is TC ’ 1:5J1. Here, for themagnetic field, we used the normalized field h = H/HSW as ineq. (31). Here, HSW = 2D1/S1.Using the sLLG method, we simulated the time evolutionof the states by applying a reversed magnetic field to the(+++) state and investigated the magnetic field thresholds.(a) (b) (c)E/F(1-E )/(1+ F1/2)2Fig. 10 Threshold fields between (+++) and (+¹+) (blue upward triangles) and between (+¹+) and (¹¹¹) (red downwardtriangles) for F = 0.5 at (a) T = 0, (b) T = 0.3J1, and (c) T = 0.5J1. The dotted lines denote hNCII(0) in (34) and hDWP(0) in (35).Reprinted figure with modification from [S. Mohakud et al., Phys. Rev. B 94, 054430 (2016)]. Copyright (2016) by the AmericanPhysical Society. (online color)Atomistic Model Study on Magnetic Properties of Permanent Magnets 9Figure 10(a) shows the magnetic field thresholds for(+++)¼ (+¹+) (blue line) and (+¹+)¼ (¹¹¹) (redline) at T = 0. It can be seen that the analytical value forthe continuum model (dotted line) is a good approximation.Figure 11(a) gives the threshold field of (+¹¹) ¼ (¹¹¹)at T = 0. In this case, the magnetic field thresholds for smallE coincide with the analytical values of the continuum model,but for large E, the magnetic field thresholds shift upwardfrom the analytical values. This is due to the so-called narrowdomain wall effect, which makes the continuum approx-imation poor [12]. As seen in Figs. 10(b) and 10(c), the fieldthresholds of (+++) ¼ (+¹+) and (+¹+) ¼ (¹¹¹)decrease significantly from the field thresholds of T = 0 asthe temperature increases, and the (+¹+) region expands.As shown in Figs. 11(b) and 11(c), the threshold field of(+¹¹)¼ (¹¹¹) also decreases due to the temperatureeffect, but the E dependence becomes moderate. Especially inthe narrow domain wall situation, the magnetization state ofregions II and III has little influence on region I, and thesurface nucleation in region I becomes important [12].6.2 Nucleation and pinning fields in Nd2Fe14BThe nucleation and pinning fields were evaluated for thecases of Bloch and Néel walls, respectively, by simulatinga hard-soft-hard magnet model composed of the atomisticmodel (4) of Nd2Fe14B [20]. In the case of Bloch wall, the adirection corresponds to the x direction in Fig. 9, and the cdirection to the x direction in the case of Néel wall. Thesoft magnet phase (grain boundary) is complex with anamorphous-like structure that depends on experimentalconditions. Since the first-principles study [60, 61] has justbegun and it is difficult to use the microscopic parametersestablished at this time, we assumed the same structure asthe hard magnet phase. The parameters E and F are definedas in the previous section. However, in Nd2Fe14B, there arevarious kinds of exchange interactions and magneticanisotropy energies, which were scaled in the sameproportion. Figure 12(a) shows for the Bloch and Néeldomain walls the E-dependences of the threshold fieldbetween (+++) and (+¹+) and between (+¹+) and(¹¹¹) at T = 0K. We assumed F = 0.5. L1 = L2 = L3 =12 unit cells and the height and depth are 5 unit cells. Theoutline of the diagram is similar to that of the anisotropicHeisenberg model described in the previous section. Thethreshold field is lower in the case of the Néel wall, reflectingthe weaker exchange interaction in the c-axis. Figure 12(b)exhibits the threshold field between (+¹¹) and (¹¹¹) atT = 0K. This pinning field is not so different between thetwo domain walls as in the case of the nucleation field. WhereE is large, the threshold value increases reflecting the natureof the narrow down wall.Figure 13(a) depicts the magnetic field thresholds between(+++) and (+¹+) and between (+¹+) and (¹¹¹) atT = 0.34TC, and Fig. 13(b) shows the threshold fieldbetween (+¹¹) and (¹¹¹). Compared with the changeof the threshold field between T = 0 and T = 0.5J1(a) (b) (c)Fig. 11 Threshold fields between (+¹¹) and (¹¹¹) (red downward triangles) for F = 0.5 at (a) T = 0, (b) T = 0.3J1, and (c) T =0.5J1. Blue dashed lines denote threshold fields between (+¹+) and (¹¹¹) in Fig. 10. Reprinted figure with permission from[S. Mohakud et al., Phys. Rev. B 94, 054430 (2016)]. Copyright (2016) by the American Physical Society. (online color)(a) (b)Fig. 12 (a) Threshold fields at 0K between (+++) and (+¹+) (circles) and between (+¹+) and (¹¹¹) (triangles) with thecomparison between Bloch and Néel domain walls. (b) Threshold fields at 0K between (+¹¹) and (¹¹¹) with the comparisonbetween Bloch and Néel domain walls. Reprinted figure with permission from [I.E. Uysal et al., Phys. Rev. B 101, 094421 (2020)].Copyright (2020) by the American Physical Society. (online color)M. Nishino and S. Miyashita10(’ 0:33TC) for F = 0.5 in the anisotropic Heisenberg modelof the previous section, the threshold field of Nd2Fe14Bshows a larger decrease rate due to temperature effects. Thisis may be due to the sensitiveness to temperature effectsbecause of the weaker exchange interaction between Nd andFe compared to that between Fe and due to the property ofthe magnetic anisotropy energy of Nd, which is the origin ofthe spin rearrangement transition.7. Dysprosium Substitution EffectAs mentioned in the introduction, Nd magnets haveproblems in high-temperature properties and are oftensubstituted with Dy to suppress the decrease in coerciveforce at high temperatures. Experiments using the methodof grain boundary diffusion process have shown that thecoercivity can be enhanced without loosing remanence [62–66]. Dy-rich shells have been observed to form between thegrain boundary and core grains [66]. The effect of thiscoercivity enhancement by Dy substitution has been studiedby micromagnetics calculations using macroscopic parame-ters of the Dy-substituted phase [67, 68]. The enhancementeffect at absolute zero temperature has also been investigatedin a simplified crystal lattice model [69]. However, themicroscopic origin of the coercivity-enhancing effect of Dysubstitution, including the temperature effect, can be under-stood only by the method of atomistic modeling.Here we explain the mechanism and effect of the coercivityenhancement by Dy substitution based on an atomistic model[27]. The Hamiltonian (4) has the energy term of the crystalelectric field of eq. (40).H ¼XNd,DyiXl;m�l;iAml;ihrliiÔml;i ð40Þis composed of Nd and Dy atoms. For Dy, the coefficients ofthe crystal electric field, etc. are those of Dy. For Dy atoms,J ¼ Lþ S ¼ 15=2 and gT = 4/3. As shown in Fig. 2(b), siof Dy atoms and Si (= si) of Fe atoms are antiferromagneti-cally coupled. The magnitude of this exchange interaction isalmost the same as that between Nd and Fe atoms [27]. Inthis case, unlike Fig. 2(a), Si (¼ si þJ i) of a Dy atom and Si(= si) of an Fe atom are antiferromagnetically coupled.As shown in Fig. 14, the Nd layers are numbered fromn = 1 at the (001) surface of the hard magnet phase ofNd2Fe14B to n = 2 and n = 3* toward the interior. Weconsidered two systems: the system in Fig. 14(a) where thesurface is in contact with the vacuum (system A) and thesystem in Fig. 14(b) where the surface is in contact with thesoft magnet phase (system B). The hard magnet phaseconsists of 12 © 12 © 9 unit cells, the soft magnet phase12 © 12 © 3 unit cells, with periodic boundary conditions inthe a and b axes, and a free boundary condition for system Aand periodic boundary condition for system B in the c axis.Here, all Nd atoms from layer 1 to layer n were replaced by(a) (b)Fig. 13 (a) Threshold fields at 0.34TC between (+++) and (+¹+) (circles) and between (+¹+) and (¹¹¹) (triangles) with thecomparison between Bloch and Néel domain walls. (b) Threshold fields at 0.34TC between (+¹¹) and (¹¹¹) with the comparisonbetween Bloch and Néel domain walls. Reprinted figure with permission from [I.E. Uysal et al., Phys. Rev. B 101, 094421 (2020)].Copyright (2020) by the American Physical Society. (online color)(a) (b)n=1n=2n=3Vacuum Soft phasen=1n=2n=3Fig. 14 (a) System A. The Nd surface layers were in contact with vacuum. In this example, Nd atoms (red) in the first Nd layerwere substituted by Dy atoms (orange). The Nd layers are numbered as n = 1, 2,* . (b) System B. The Nd surface layers were incontact with a soft magnet phase. [M. Nishino et al., Phys. Rev. B 106, 054422 (2022)]. Copyright (2022) by the American PhysicalSociety. (online color)Atomistic Model Study on Magnetic Properties of Permanent Magnets 11Dy atoms, and the threshold field of magnetization reversalwas investigated. As in the previous section, the soft magnetphase was assumed to have the same structure as the hardmagnet phase, and small magnetic parameters (exchangeinteractions by a factor of 0.5 and magnetic anisotropyenergies by a factor of 0.2) were adopted as in themicromagnetics calculations. The threshold field of magnet-ization reversal was estimated by real-time simulation of thesLLG method.Figure 15 presents the n dependence of the threshold fieldand its temperature dependence for system A (dotted line)and system B (solid line). n = 0 means no Dy substitution(original system). The ratios (%) in the figures are thoseagainst the value of n = 0. Since magnetization reversaloccurs more easily in the grain boundary phase, domainwalls are more easily generated at the phase boundary, andsurface nucleation of the hard magnet phase tends to occur.Therefore, the coercive force is greatly reduced compared tothat of the vacuum surface. However, the ratio against n = 0when n increases in system B is larger than that in system A,and the coercive force increases by a large ratio with Dysubstitution in system B. In other words, the enhancementof coercivity is more intensely in system B. This is acharacteristic feature of Dy substitution, and it suggests thatDy substitution has a strong pinning effect hindering thedomain wall motion to the hard magnet phase. The rate ofincrease of coercivity (¦hC/¦n) with respect to the numberof Dy substitution layers (n) is constant at finite temperatureand almost equal for both systems.Regarding system A, we investigated n-dependence of thecoercivity for the system with the magnetic anisotropy of Ndatoms enhanced by a factor of 2 instead of Dy substitution[22], and compared it with that of Dy substitution. Wecompared the ratios of increase of n = 5 against n = 0 for0.34TC, 0.46TC, and 0.69TC. In the case of Dy-substitution,the increase is 144%, 140%, and 132%, respectively, whilein the case of doubly enhanced magnetic anisotropy of Ndatoms, the increase is 123%, 121%, and 111% [22]. Thisindicates that the coercivity enhancement effect is maintainedat high temperatures in the case of Dy substitution.Next, we observed at the change in nucleation dynamicswhen the substituted Dy layer was increased. Figure 16shows the nucleation of n = 1 and n = 5 in system B. Themagnetic field was used near the threshold value.Figure 16(a) shows the case with n = 1 where only onelayer was Dy-substituted. A large part of the soft magnetphase was reversed before the magnetization of the hardmagnet phase was reversed, indicating that depinning occursfrom the surface of the hard magnet phase. On the other hand,Fig. 16(b) has five Dy-substituted layers and nucleationoccurred from the inside of the hard magnet part. Surfacenucleation is suppressed by Dy substitution, and is replacedby bulk nucleation. This change in nucleation mechanismwas also observed in system A, but n boundary for thechange from surface nucleation to internal nucleation wasn ’ 2 in system A and n ’ 3 in system B.There are two possible microscopic origins of thecoercivity enhancement effect of Dy substitution and itsmaintenance at high temperatures. The first is the differencein magnetic interactions. The interaction between Nd andFe atoms is ferromagnetic, while that between Dy and Fe isantiferromagnetic. This antiferromagnetic coupling stabilizesthe Dy moment under the reversed magnetic field andprevents nucleation for reversal. The second is the featureof the temperature dependence of the CEF energy of Dy.Figure 4(b) depicts the temperature dependence of the CEFenergy of Dy atoms in the Nd magnet. Compared withFig. 4(a), the CEF energy of Dy atoms has a minimum at123456780 1 2 3 4 5 6h (T)n106% 121% 132%108%129% 141%116%138%158%123456780 1 2 3 4 5 6h (T)n103%122%140%123456780 1 2 3 4 5 6h (T)n121%151%178%107%123%144%1015202530350 1 2 3 4 5 6h (T)n105%100% 101%150%173%185%(a) (b)(c) (d)0 K 0.34 TC0.46 TC0.69 TCFig. 15 n dependence of the threshold filed in systems A (dotted lines) and B (solid lines) at (a) 0K, (b) 0.34TC, (c) 0.46TC, and (d)0.69TC. Reprinted figure with permission from [M. Nishino et al., Phys. Rev. B 106, 054422 (2022)]. Copyright (2022) by the AmericanPhysical Society. (online color)M. Nishino and S. Miyashita12ª = 0 regardless of temperature, and the potential barrier isrelatively high at all temperatures. Furthermore, when wefocus on the change of the potential barrier between 0.46TC(near room temperature) and 0.69TC, we find that thepotential barrier of Dy is 27% higher than that of Nd at0.46TC, but is 79% higher at 0.69TC. In other words, Dy hasa relatively higher potential barrier at high temperatures. Thismay be the reason why Dy substitution is effective at hightemperatures.8. Magnetic Dipole InteractionSince the atomistic model method takes into account thespins of all atoms, the computable scale is realistically limitedto the order of tens of nm. The magnetic dipole interactionis much smaller than the exchange interaction and is notvery important at that scale. Therefore, the magnetic dipoleinteraction14³®0Xi6¼k1r3ikSi � Sk �3ðrik � SiÞðrik � SkÞr2ik� �ð41Þhas not been taken into account, but it becomes important atthe scale of an assembly of grains (µm) because of theappearance of uniform magnetization in ferromagnets. Thedemagnetization field effect given by this interaction has theeffect of breaking the uniform order, and experiments andmicromagnetic calculations have shown a decrease incoercivity (increase in demagnetization field effect) withrespect to grain size [70–73]. The coercivity of nanograinsshown in this paper (saturation at about 20 nm) is consideredto give an approximation of the upper limit of the coercivityincluding the effect of thermal fluctuations of grain assembly.The exchange interaction is of short range and thecomputational cost of the simulation is proportional to thespin number N, while the magnetic dipole interaction is oflong range and thus it increases with the square of the spinnumber (N2). In Monte Carlo methods, the stochastic cutoff(SCO) and other methods have been proposed to overcomethis difficulty [74, 75]. The SCO method accelerates thecalculation by reducing the selectivity of long-range weakinteractions in a state-update process of the Monte Carlomethod while maintaining the detailed balance condition andensuring that the simulation reaches equilibrium correctly asa steady state. For a 3-dimensional system of magnetic dipoleinteractions, a single Monte Carlo step can be computed inO(N lnN ) time. However, the conventional SCO method hasdifficulties that make the procedure cumbersome for systemswith complex unit cells such as Nd magnets, but a modifiedSCO method (MSCO) using Walker’s algorithm has beendeveloped and the effect of magnetic dipole interaction hasbeen investigated in a thin film system of an atomistic modelof Nd [15]. In addition, magnetic profiles have been studiedusing MSCO for a simple anisotropic Heisenberg model withparameters of anisotropy constant, dipole interaction, andsystem thickness [26].9. Summary and Future PerspectiveThis paper introduces the methodologies for studying theeffects of temperature and thermal fluctuations on themagnetic properties of permanent magnets and describesthe magnetic properties obtained by applying the method-ologies, especially focusing on the properties of neodymiummagnets. The method of the atomistic model introduced hereis an extension of the study of thermal fluctuation effectsinitiated by Brown [76], and correctly treats entropy effectsand temperature effects including local thermal fluctuations inmany-body systems of spins with cooperative interactions. Inthis paper, we first presented a modeling of the interactionfrom the atomic level in Nd2Fe14B. Then, the characteristicsof magnetization process, domain wall, coercivity ofnanograin, nucleation and pinning fields, and dysprosiumsubstitution effect were explained using Monte Carlo andsLLG methods. There, the understanding of thermal(a)(b)n=1n=5Fig. 16 Snapshots of the spin configuration in nucleation for (a) n = 1 and (b) n = 5 at the threshold fields h = 3.70T and h = 5.05T,respectively, at 0:46TC ’ Troom in system B. The yellow-boxed regions correspond to the soft magnetic phase. Red and blue parts denoteup-spin and down-spin ones, respectively. Reprinted figure with permission from [M. Nishino et al., Phys. Rev. B 106, 054422 (2022)].Copyright (2022) by the American Physical Society. (online color)Atomistic Model Study on Magnetic Properties of Permanent Magnets 13fluctuations and temperature effects and their microscopicmechanisms in the magnetic properties of permanentmagnets, which had not been well understood, was advanced,as seen in the significant decrease in coercive force due tothermal fluctuations.Although we did not mention them due to space limitation,the angular dependence of nucleation and pinning fields andthe effect of the orientation distribution of magneticanisotropy of grains are also important for coercivity studies,and studies of their finite temperature properties have beenstarted using the above methodologies [77]. A nontrivialbehavior in the temperature dependence of the ferromagneticresonance of neodymium magnets has also been clarified bythe method of atomistic modeling [18].The magnetization reversal of individual grains has beenobserved experimentally, and the effect of thermal fluctua-tions on the process has become a realistic problem [78].Therefore, the rigorous treatment of thermal fluctuations andtemperature effects by this atomistic model is expected tobecome more and more important in the future. In fact,during the ESICMM project, European and Chinese groupshave also started to study the atomistic model of Nd2Fe14B[79–83], and the study of permanent magnets using thisapproach is expected to be developed hereafter. However,when using the atomistic model, the current computingpower is limited to calculations on the scale of a few tensof nm. This is the range in which a single grain or a fewgrains can be included. Coercivity appears as a property ofan assembly of grains. The assembly of grains requirescalculations on the order of µm, which is done inmicromagnetics calculations.If we start from an atomistic model and obtain macro-scopic A(T ) and K(T ) using the constraint Monte Carlomethod introduced in 4.2, the LLG calculation for micro-magnetics cannot handle thermal activation processes.Adding a noise field for thermal fluctuations leads to adouble temperature effect, which is inappropriate. Therefore,it is necessary to develop a methodology that starts from anatomistic model and connects it to the µm order scale. Forthis purpose, it is necessary to construct a coarse-grainedmodel consisting of local spin variables that incorporates theeffects of thermal fluctuations. For example, the followingmethod can be considered. For a spin set in a certain region,we introduce a coarse-grained magnetization M. Themagnitude of this coarse-grained magnetization is variabledue to temperature effects, and the magnetization distributionP(M ) can be calculated by the Wang-Landau method usingan atomistic model. For this coarse-grained magnetization,we construct a coarse-grained Hamiltonian.H ¼ �Xi;jJi;jMi �Mj þXiEselfðMiÞ; ð42Þwhere Eself (Mi) is the magnetic anisotropy energy and othercontributions. The renormalized parameters (Ji, j, etc.) areadjusted to reproduce the values of physical quantitiesobtained in the original atomistic Hamiltonian. It isconceivable to apply this coarse-grained Hamiltonian tolarge systems, including magnetic dipole interactions. Thedetails are under investigation.AcknowledgementsThe study presented here was supported by the ElementsStrategy Initiative Center for Magnetic Materials (ESICMM)(project number JPMXP0112101004) funded by the Ministryof Education, Culture, Sports, Science and Technology(MEXT) of Japan. 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