A Physics-Informed Hybrid Neural Operator for Transient Magnetization Prediction in Power Magnetics

arXiv cs.LG Papers

Summary

This preprint proposes PI-HNO, a physics-informed hybrid neural operator for transient magnetization prediction in power magnetics, achieving low B-H energy consistency errors with only 4,777 trainable parameters per material model.

arXiv:2608.02965v1 Announce Type: new Abstract: Magnetic components in high-frequency, high-power-density converters are increasingly driven by non-sinusoidal flux-density waveforms with fast transitions, minor-loop operation, dc bias, and temperature variation. Under these conditions, steady-state core-loss formulas and single-valued material curves cannot fully capture transient magnetization responses. This work proposes the Physics-Informed Hybrid Neural Operator (PI-HNO), a compact material-specific neural model with B-H energy-consistency regularization for core-loss-oriented transient magnetization prediction. Given the measured B(t)-H(t) history, the input B(t) series over the prediction interval and operating-condition information, PI-HNO predicts the H(t) series and the corresponding reconstructed B-H trajectory. The model integrates a local recurrent branch for boundary-state representation and rate-dependent response evolution with a Preisach-inspired global branch that extracts waveform-level hysteresis context. Evaluation on the MagNetX transient database using material-specific models for 14 ferrite materials demonstrates that PI-HNO achieves a compact trade-off between sequence accuracy and B(t)-H(t) energy consistency, with the mean and 95th percentile B(t)-H(t) energy consistency errors of 1.92% and 7.60%, respectively, using only 4777 trainable parameters per model. Ablation studies further demonstrate that the local, global, and energy-aware regularized components provide distinct contributions to transient magnetization prediction.
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# A Physics-Informed Hybrid Neural Operator for Transient Magnetization Prediction in Power Magnetics
Source: [https://arxiv.org/html/2608.02965](https://arxiv.org/html/2608.02965)
Yachao Zhu, Qiujie Huang, Sinan Li, Yang Li, Gang Lei, and Jianguo ZhuThis work is a preprint prepared for possible submission to IEEE Transactions on Power Electronics\.Yachao Zhu and Qiujie Huang are co\-first authors\. \(Corresponding author: Qiujie Huang\.\)Yachao Zhu and Gang Lei are with the School of Electrical and Data Engineering, the University of Technology Sydney, Ultimo, 2007 \(e\-mail:Yachao\.Zhu@uts\.edu\.au; Gang\.Lei@uts\.edu\.au\)Qiujie Huang, Sinan Li, and Jianguo Zhu are with the School of Electrical and Computer Engineering, the University of Sydney, Darlington, NSW, 2008, Australia \(e\-mail:qiujie\.huang@sydney\.edu\.au; sinan\.li@sydney\.edu\.au; jianguo\.zhu@sydney\.edu\.au\)Yang Li was with the National Railway Research and Design Institute of Signal and Communication, Beijing 100070, China \(e\-mail: 787511208@qq\.com\)

###### Abstract

Magnetic components in high\-frequency, high\-power\-density converters are increasingly driven by non\-sinusoidal flux\-density waveforms with fast transitions, minor\-loop operation, dc bias, and temperature variation\. Under these conditions, steady\-state core\-loss formulas and single\-valued material curves cannot fully capture transient magnetization responses\. This work proposes the Physics\-Informed Hybrid Neural Operator \(PI\-HNO\), a compact material\-specific neural model withBB–HHenergy\-consistency regularization for core\-loss\-oriented transient magnetization prediction\. Given the measuredB​\(t\)B\(t\)–H​\(t\)H\(t\)history, the inputB​\(t\)B\(t\)series over the prediction interval, and operating\-condition information, PI\-HNO predicts theH​\(t\)H\(t\)seires and the corresponding reconstructedBB–HHtrajectory\. The model integrates a local recurrent branch for boundary\-state representation and rate\-dependent response evolution with a Preisach\-inspired global branch that extracts waveform\-level hysteresis context\. Evaluation on the MagNetX transient database using material\-specific models for 14 ferrite materials demonstrates that PI\-HNO achieves a compact trade\-off between sequence accuracy andB​\(t\)B\(t\)–H​\(t\)H\(t\)energy consistency, with the mean and 95th percentileB​\(t\)B\(t\)–H​\(t\)H\(t\)energy consistency errors of 1\.92% and 7\.60%, respectively, using only 4777 trainable parameters per model\. Ablation studies further demonstrate that the local, global, and energy\-aware regularized components provide distinct contributions to transient magnetization prediction\.

###### Index Terms:

Power magnetics, magnetic hysteresis, transient magnetization, core loss,

BB–

HHtrajectory prediction, physics\-informed machine learning\.

## IIntroduction

High\-frequency and high\-power\-density power converters enabled by wide\-bandgap devices and advanced topologies impose increasing demands on magnetic components, including higher switching frequency, more complex excitation waveforms, and tighter thermal constraints\[[16](https://arxiv.org/html/2608.02965#bib.bib5),[10](https://arxiv.org/html/2608.02965#bib.bib17),[17](https://arxiv.org/html/2608.02965#bib.bib18)\]\. Inductors and transformers directly affect converter volume, core loss, temperature rise, current stress, and efficiency, making accurate magnetic material modeling essential for compact power magnetic design\[[22](https://arxiv.org/html/2608.02965#bib.bib20),[11](https://arxiv.org/html/2608.02965#bib.bib19),[19](https://arxiv.org/html/2608.02965#bib.bib2)\]\. However, modern converter excitations often involve fast transitions, dc bias, minor\-loop operation, and temperature variation, where scalar core\-loss models and single\-valued material curves cannot capture the transient magnetic response required for time\-domain analysis\. For a given flux\-density trajectoryB​\(t\)B\(t\), the correspondingH​\(t\)H\(t\)response depends on magnetic history, reversal behavior, temperature, and rate\-dependent effects, motivating compact models capable of predicting futureBB–HHtrajectories from available history and excitation information\.

These path\-, rate\-, and temperature\-dependent behaviors have traditionally been described using empirical core\-loss models and physics\-based hysteresis formulations\. Steinmetz\-based models and their extensions provide efficient loss estimation for periodic waveforms but cannot reconstruct transientBB–HHtrajectories under arbitrary excitation conditions\[[18](https://arxiv.org/html/2608.02965#bib.bib6),[15](https://arxiv.org/html/2608.02965#bib.bib7),[7](https://arxiv.org/html/2608.02965#bib.bib8),[21](https://arxiv.org/html/2608.02965#bib.bib9)\]\. Physics\-based models, including Preisach, Jiles–Atherton, and generalized dynamic circuit models, provide improved interpretability by representing hysteresis memory and dynamic loss mechanisms\[[1](https://arxiv.org/html/2608.02965#bib.bib10),[13](https://arxiv.org/html/2608.02965#bib.bib11),[8](https://arxiv.org/html/2608.02965#bib.bib12),[24](https://arxiv.org/html/2608.02965#bib.bib13),[6](https://arxiv.org/html/2608.02965#bib.bib14)\]\. However, these approaches often require material\-specific parameter identification and may lose accuracy when operating frequency, temperature, bias, or geometry varies\.

These challenges have motivated data\-driven modeling of power magnetic materials\. MagNet established a data foundation forBB–HHloop reconstruction and core\-loss modeling, while MagNet\-AI introduced neural datasheet concepts for loop prediction, loss estimation, and material recommendation\[[10](https://arxiv.org/html/2608.02965#bib.bib17),[11](https://arxiv.org/html/2608.02965#bib.bib19)\]\. HARDCORE further explored the time domainH​\(t\)H\(t\)reconstruction and loss estimation from reconstructed trajectories\[[9](https://arxiv.org/html/2608.02965#bib.bib21)\]\. More recently, MagNetX extended transient magnetic modeling through time\-domain excitation data and history\-conditioned prediction, while RHINO\-MAG investigated compact recursive temperature\-awareH​\(t\)H\(t\)inference under dynamic excitation\[[22](https://arxiv.org/html/2608.02965#bib.bib20),[20](https://arxiv.org/html/2608.02965#bib.bib25)\]\.

In parallel, hybrid physics\- and data\-driven learning has been developed to improve physical consistency and reduce the ambiguity of purely data\-driven magnetic models\. Analytical core\-loss\-informed networks primarily focus on scalar loss prediction\. In contrast, Preisach, Prandtl\-Ishlinskii, and phenomenological\-dynamics\-based approaches encode path dependence and the multivalued nature of theBB–HHcharacteristics\. Neural\-operator approaches have further explored nonlinear mappings between excitation trajectories and magnetic responses, providing potential advantages for waveform\-dependent modeling\[[14](https://arxiv.org/html/2608.02965#bib.bib22),[23](https://arxiv.org/html/2608.02965#bib.bib23),[3](https://arxiv.org/html/2608.02965#bib.bib26),[2](https://arxiv.org/html/2608.02965#bib.bib27),[5](https://arxiv.org/html/2608.02965#bib.bib16),[4](https://arxiv.org/html/2608.02965#bib.bib15)\]\. However, existing methods mainly focus on closed\-loop loss regression, quasi\-static hysteresis reconstruction, or constitutive mapping\. A compact transient model that learns boundary\-conditioned trajectory mappings while simultaneously providing accurateH​\(t\)H\(t\)prediction,BB–HHenergy consistency, and interpretable use of magnetization history and full\-waveformB​\(t\)B\(t\)information remains insufficiently explored\. This challenge is particularly important for finite prediction intervals, where reconstructedBB–HHtrajectories may be open and closed\-cycle loss evaluation alone is insufficient\.

Motivated by this gap, this work proposes the Physics\-Informed Hybrid Neural Operator \(PI\-HNO\), a compact neural material model for boundary\-conditioned transientBB–HHtrajectory prediction\. Unlike conventional sequence models that primarily learn pointwise temporal correlations, PI\-HNO formulates transient magnetization prediction as a boundary\-conditioned trajectory mapping between magnetic excitation, available history information, and future magnetic response\. Given the measured magnetic history before the prediction interval, the inputB​\(t\)B\(t\)trajectory over the interval, and operating\-condition features, PI\-HNO predicts the subsequentH​\(t\)H\(t\)response while improving theBB–HHenergy consistency of the reconstructed trajectory through physics\-guided regularization\.

The proposed physics\-guided framework incorporates magnetic knowledge at three levels\. First, the transient magnetic response is formulated based on a physics\-motivated decomposition of history\-dependent hysteresis behavior and rate\-dependent dynamic effects, which guides the design of complementary learning branches\. Second, magnetic memory and path dependence are represented using a Preisach\-inspired global feature\-extraction mechanism\. Third, an energy\-aware regularization term is introduced to improve the consistency of the reconstructedBB–HHtrajectory\. Using these physics\-guided representations and constraints, PI\-HNO provides a compact framework for predicting transient magnetic response\.

The main contributions are summarized as follows:

1. 1\.A boundary\-conditioned transient magnetization prediction framework is formulated for material\-specific modeling, where the futureH​\(t\)H\(t\)response is inferred from the measured magnetic history, the inputB​\(t\)B\(t\)trajectory over the prediction interval, temperature, and temporal\-position information\.
2. 2\.A compact hybrid neural architecture is developed by integrating local recurrent state propagation and global waveform\-level context extraction for transient magnetic\-response prediction\. The proposed design enables simultaneous modeling of the evolution of rate\-dependent response and path\-dependent hysteresis behavior under diverse excitation conditions\.
3. 3\.An energy\-aware training objective is developed to improve the accumulatedBB–HHenergy consistency of the predicted trajectory\. Extensive evaluations on the MagNetX dataset using 14 ferrite materials demonstrate that PI\-HNO achieves a favorable trade\-off among prediction accuracy, energy consistency, and model compactness\.

The remainder of this work is organized as follows\. Section II defines the prediction problem and presents the physical background\. Section III introduces the proposed PI\-HNO and its energy\-aware learning formulation\. Section IV describes the experimental setup and evaluation metrics\. Section V presents and discusses the comparative and ablation results\. Conclusions are drawn in Section VI\.

## IIPROBLEM FORMULATION AND PHYSICAL BACKGROUND

### II\-ABoundary\-Conditioned TransientH​\(t\)H\(t\)Prediction

![Refer to caption](https://arxiv.org/html/2608.02965v1/x1.png)Figure 1:Input–output arrangement of the boundary\-conditioned transientH​\(t\)H\(t\)prediction task\.The transient hysteresis prediction task is formulated as a boundary\-conditioned trajectory mapping problem\. As shown in Fig\.[1](https://arxiv.org/html/2608.02965#S2.F1), each transientBB–HHsequence containsLLsampled time steps\. A prediction boundaryssdivides the sequence into a measured\-history interval,0≤t<s0\\leq t<s, and a prediction interval,s≤t<Ls\\leq t<L\. Before the boundary, bothB​\(t\)B\(t\)andH​\(t\)H\(t\)are available and provide information about the magnetic state reached by the material\. Over the prediction interval, the inputB​\(t\)B\(t\)trajectory is known, whereas the correspondingH​\(t\)H\(t\)response is withheld from the model and used only as the training target or evaluation reference\.

The objective is to learn a nonlinear trajectory mapping from the measured magnetic history, the complete excitation trajectory, and operating conditions to the future magnetization response:

Hpred​\(t\)=𝒢θ​\(B​\(t\),Hhist​\(t\),T\),s≤t<L,H\_\{\\mathrm\{pred\}\}\(t\)=\\mathcal\{G\}\_\{\\theta\}\\bigl\(B\(t\),H\_\{\\mathrm\{hist\}\}\(t\),T\\bigr\),\\qquad s\\leq t<L,\(1\)where𝒢θ\\mathcal\{G\}\_\{\\theta\}denotes the learned nonlinear mapping from the input magnetic trajectories and operating conditions to the future magnetization response\. Here,Hhist​\(t\)H\_\{\\mathrm\{hist\}\}\(t\)represents the measured magnetic history before the prediction boundary, and the completeB​\(t\)B\(t\)trajectory includes both the measured\-history and prediction intervals\. Explicit frequency and waveform\-periodicity labels are not provided as separate inputs\.

The amount of measured history is controlled by the known\-history ratio as follows:

ρ=sL,\\rho=\\frac\{s\}\{L\},\(2\)where a smallerρ\\rhocorresponds to a less available magnetization history and a longer prediction interval, while a largerρ\\rhocorresponds to more available history and a shorter prediction interval\. The known\-history ratio is varied in the experiments to evaluate the proposed model under different levels of available magnetic\-history information\.

### II\-BHysteresis Memory and Energy Consistency

![Refer to caption](https://arxiv.org/html/2608.02965v1/x2.png)Figure 2:Physical interpretation of the magnetic response: \(a\) magnetic\-core excitation and winding\-levelBB–HHcharacterization; \(b\) microscopic domain evolution involving domain\-wall motion and domain rotation; and \(c\) macroscopic dynamic effects associated with global and local eddy\-current\.The transient magnetic response considered in this work arises from complex interactions among the excitation waveform, magnetization history, and rate\-dependent physical mechanisms\. As illustrated in Fig\.[2](https://arxiv.org/html/2608.02965#S2.F2), the measured electrical quantities are converted into macroscopicB​\(t\)B\(t\)–H​\(t\)H\(t\)trajectories, where the resulting magnetic response contains both history\-dependent hysteresis behavior and transient dynamic effects\.

The macroscopicBB–HHvariables used in this work are obtained from winding\-level measurements based on the standard lumped\-core approximation\. For the two\-winding magnetic characterization setup, the flux density is reconstructed from the secondary\-side voltage, while the magnetic field strength is derived from the primary\-side magnetizing current\[[22](https://arxiv.org/html/2608.02965#bib.bib20)\]:

B​\(t\)=B​\(t0\)\+1n2​Ae​∫t0tvs​\(τ\)​dτ,H​\(t\)≃n1​ip​\(t\)ℓe,B\(t\)=B\(t\_\{0\}\)\+\\frac\{1\}\{n\_\{2\}A\_\{e\}\}\\int\_\{t\_\{0\}\}^\{t\}v\_\{s\}\(\\tau\)\\,\\mathrm\{d\}\\tau,\\qquad H\(t\)\\simeq\\frac\{n\_\{1\}i\_\{p\}\(t\)\}\{\\ell\_\{e\}\},\(3\)wherevs​\(t\)v\_\{s\}\(t\)andip​\(t\)i\_\{p\}\(t\)denote the measured winding voltage and magnetizing current, respectively\.n1n\_\{1\},n2n\_\{2\},AeA\_\{e\}, andℓe\\ell\_\{e\}represent the winding turns, effective core area, and magnetic path length\. These relations establish the connection between electrical measurements and macroscopic magnetic trajectories, but they do not imply a unique instantaneous mapping betweenB​\(t\)B\(t\)andH​\(t\)H\(t\)\.

At the material level, the magnetic flux density is related to the magnetic field and magnetization by

B​\(t\)=μ0​\[H​\(t\)\+M​\(t\)\],B\(t\)=\\mu\_\{0\}\\bigl\[H\(t\)\+M\(t\)\\bigr\],\(4\)whereM​\(t\)M\(t\)represents the internal magnetization state\. Unlike linear magnetic materials, the evolution ofM​\(t\)M\(t\)in soft magnetic cores depends not only on the instantaneous flux density, but also on the previously experienced excitation trajectory\. This memory effect arises from microscopic processes, including domain\-wall displacement and magnetization rotation, that involve both reversible and irreversible mechanisms\[[8](https://arxiv.org/html/2608.02965#bib.bib12)\]\.

Consequently, identical instantaneous operating points in theBB–HHplane may lead to different subsequent magnetic responses when the underlying excitation histories differ\. As illustrated in Fig\.[2](https://arxiv.org/html/2608.02965#S2.F2)\(b\), reversal points, flux\-density extrema, dc bias, waveform asymmetry, and major and minor\-loop evolution can modify the internal magnetic state and in turn influence future magnetization trajectories\. This path dependence explains why transient magnetization prediction requires not only the instantaneous excitationB​\(t\)B\(t\), but also sufficient information describing the previous magnetization history\.

In addition to hysteresis memory, transient excitation introduces rate\-dependent magnetic effects beyond the quasi\-static hysteresis\. A time\-varying flux density induces eddy currents within the magnetic core, generating electrical fields that modify the measured magnetic field response\. Moreover, delayed magnetic relaxation associated with domain\-wall dynamics contributes to excess\-loss\-related dynamic behavior under high\-frequency or rapidly varying excitation\[[1](https://arxiv.org/html/2608.02965#bib.bib10)\]\. Therefore, the transient field response can be conceptually interpreted as:

H​\(t\)=Hhys​\(B​\(t\),ξ​\(t\),T\)\+Hdyn​\(t\),H\(t\)=H\_\{\\mathrm\{hys\}\}\\bigl\(B\(t\),\\xi\(t\),T\\bigr\)\+H\_\{\\mathrm\{dyn\}\}\(t\),\(5\)whereξ​\(t\)\\xi\(t\)denotes the internal magnetic state,HhysH\_\{\\mathrm\{hys\}\}represents the history\-dependent hysteretic contribution, andHdynH\_\{\\mathrm\{dyn\}\}represents rate\-dependent dynamic effects\. In practical measurements, the individual contributions cannot be uniquely separated, because hysteresis evolution and dynamic effects are strongly coupled in the observedBB–HHtrajectory\. Instead, this interpretation provides the physical motivation for incorporating both long\-range magnetic history and local excitation variation into transient prediction models\.

The predictedH​\(t\)H\(t\)response together with the inputB​\(t\)B\(t\)trajectory defines a reconstructedBB–HHpath over the prediction interval\. Therefore, evaluating transient magnetization prediction requires not only point\-wise agreement inH​\(t\)H\(t\), but also the consistency of the accumulatedBB–HHwork along the reconstructed trajectory\. For a closed periodic hysteresis loop, the contour integral∮H​dB\\oint H\\,\\mathrm\{d\}Brepresents the dissipated core\-loss energy density per cycle\. In contrast, the boundary\-conditioned prediction interval considered in this work generally forms an open trajectory𝒞\\mathcal\{C\}, as follows:

W𝒞=∫𝒞H​dB\.W\_\{\\mathcal\{C\}\}=\\int\_\{\\mathcal\{C\}\}H\\,\\mathrm\{d\}B\.\(6\)For an open trajectory,W𝒞W\_\{\\mathcal\{C\}\}includes both recoverable magnetic work variation and dissipative contributions, and therefore it is not interpreted as a direct core\-loss measurement\. Instead, the difference between the predicted and measured values ofW𝒞W\_\{\\mathcal\{C\}\}is used as an energy\-consistency measure of the reconstructed trajectory\. This trajectory\-level constraint complements the point\-wiseH​\(t\)H\(t\)prediction error and encourages physically consistent transient magnetization prediction\.

## IIIThe Proposed Physics\-Informed Hybrid Neural Operator

This section presents PI\-HNO for boundary\-conditioned transientBB–HHtrajectory prediction\. The model learns a boundary\-conditioned trajectory operator that maps the measured magnetization history, the complete inputB​\(t\)B\(t\)excitation trajectory, and temperature for the futureH​\(t\)H\(t\)response\. To achieve this trajectory\-level prediction, PI\-HNO combines a local recurrent branch for boundary\-state representation and rate\-dependent response evolution, a Preisach\-inspired global branch for waveform\-level hysteresis context extraction, and an energy\-aware regularization term to improve the accumulatedBB–HHenergy consistency of the reconstructed trajectory\.

### III\-AArchitecture Overview and Physics\-Guided Decomposition

![Refer to caption](https://arxiv.org/html/2608.02965v1/x3.png)Figure 3:Architecture of the proposed PI\-HNO\.Fig\.[3](https://arxiv.org/html/2608.02965#S3.F3)illustrates the overall architecture of PI\-HNO\. Motivated by the physical mechanisms discussed in Section II\-A, the proposed architecture incorporates a physics\-guided decomposition of transient magnetic response into two complementary learning branches\. Rather than explicitly identifying separate physical components, these branches are designed to learn representations related to history\-dependent hysteresis behavior and rate\-dependent magnetic dynamics\.

- •The global branch is designed to extract waveform\-level hysteresis context from the completeB​\(t\)B\(t\)trajectory\. Inspired by the memory\-weighting concept of the Preisach model, this branch learns path\-dependent magnetic information associated with features such as ascending and descending flux\-density trajectories, reversal points, and minor\-loop evolution\.
- •The local recurrent branch is designed to learn the boundary\-conditioned evolution of dynamic responses\. It utilizes the measuredB​\(t\)B\(t\)–H​\(t\)H\(t\)history before the prediction interval and the step\-to\-step variation of the inputB​\(t\)B\(t\)trajectory to propagate rate\-dependent magnetic behavior across the prediction boundary\.

Through this physics\-guided architecture design, PI\-HNO incorporates magnetic memory and dynamic\-response information into the learning process rather than relying on a purely empirical input–output mapping\. The representations learned from the local and global branches are jointly fused to predict the futureHpred​\(t\)H\_\{\\mathrm\{pred\}\}\(t\)sequence\. During training, an energy\-aware regularization term is further introduced to improve the accumulatedBB–HHenergy consistency of the predicted trajectory\.

### III\-BLocal Recurrent Branch for Dynamic Field Response

The local branch is designed to learn the boundary\-conditioned evolution of rate\-dependent magnetic response under time\-varying flux\-density excitation\. Following the physical interpretation discussed in Section II\-A, the transient magnetic response contains both history\-dependent hysteresis behavior and rate\-dependent dynamic effects\. The local branch does not explicitly identify analytical eddy\-current or excess\-loss components\. Instead, it learns an equivalent dynamic representation from measured magnetic trajectories\. The observedB​\(t\)B\(t\)–H​\(t\)H\(t\)history provides the magnetic state information at the prediction boundary, while the inputB​\(t\)B\(t\)waveforms over the prediction interval and their step\-to\-step variation determine the subsequent evolution of the excitation\. A GRU encoder–decoder structure is adopted because its gated recurrence provides a compact discrete\-time representation of relaxation\-type dynamics, in which the internal state is updated based on the current excitation while retaining relevant information from previous states\.

#### III\-B1History GRU

The history GRU reads the measuredB​\(t\)B\(t\)andH​\(t\)H\(t\)sequences before the prediction boundary and compresses them into a hidden\-state representationhhisth\_\{\\mathrm\{hist\}\}\. This representation provides initial magnetic\-state information for future prediction, including the current field strength, the flux\-density variation trend, remanent\-state\-related information, and reversal events in the measured history, thereby helping identify the active region of the hysteresis trajectory\.

The use of a gated recurrent update is motivated by the relaxation\-type behavior commonly observed in rate\-dependent magnetization dynamics\. An equivalent first\-order relaxation model for an internal dynamic state can be expressed as:

τt​d​h​\(t\)d​t=heq​\(xt\)−h​\(t\),\\tau\_\{t\}\\frac\{\\mathrm\{d\}h\(t\)\}\{\\mathrm\{d\}t\}=h\_\{\\mathrm\{eq\}\}\(x\_\{t\}\)\-h\(t\),\(7\)whereh​\(t\)h\(t\)represents an equivalent internal dynamic state,heq​\(xt\)h\_\{\\mathrm\{eq\}\}\(x\_\{t\}\)is the excitation\-dependent equilibrium state,xtx\_\{t\}denotes local excitation features, e\.g\.,BtB\_\{t\},Δ​Bt\\Delta B\_\{t\}, andTT\.τt\\tau\_\{t\}represents an effective relaxation time constant\. Using a forward\-Euler discretization, \([7](https://arxiv.org/html/2608.02965#S3.E7)\) becomes:

ht=\(1−ηt\)​ht−1\+ηt​heq​\(xt\),ηt=Δ​tτt\.h\_\{t\}=\(1\-\\eta\_\{t\}\)h\_\{t\-1\}\+\\eta\_\{t\}h\_\{\\mathrm\{eq\}\}\(x\_\{t\}\),\\qquad\\eta\_\{t\}=\\frac\{\\Delta t\}\{\\tau\_\{t\}\}\.\(8\)This update shares the same weighted form as the GRU state equation,

ht=\(1−zt\)⊙ht−1\+zt⊙h~t,h\_\{t\}=\(1\-z\_\{t\}\)\\odot h\_\{t\-1\}\+z\_\{t\}\\odot\\tilde\{h\}\_\{t\},\(9\)where the update gateztz\_\{t\}controls the contribution of previous states and current excitation information, andh~t\\tilde\{h\}\_\{t\}denotes the candidate hidden state determined by the current input\. This analogy provides a physics\-guided interpretation of the GRU update mechanism as a flexible discrete\-time representation for rate\-dependent magnetic response, rather than a direct analytical model of individual physical mechanisms such as eddy\-current diffusion or domain\-wall motion\.

#### III\-B2Initial Hidden State Conditioning

The initial state for future prediction cannot be determined solely from instantaneous magnetic variables because similar local magnetization states may exhibit different subsequent responses under different operating conditions\. In particular, temperature variations can influence permeability, coercivity, conductivity, and relaxation behavior\. In addition, the start\-position feature identifies the location of the prediction boundary input waveform, allowing the model to distinguish repeated local excitation patterns that occur at different stages of the magnetization trajectory\.

Therefore, the temperatureTTand start\-position feature are projected through two multilayer perceptrons and added to the hidden\-state representation obtained from the history GRU:

hinit=hhist\+htemp\+hpos,h\_\{\\mathrm\{init\}\}=h\_\{\\mathrm\{hist\}\}\+h\_\{\\mathrm\{temp\}\}\+h\_\{\\mathrm\{pos\}\},\(10\)wherehtemph\_\{\\mathrm\{temp\}\}andhposh\_\{\\mathrm\{pos\}\}denote the learned projections of temperature and start position, respectively\. The resulting statehinith\_\{\\mathrm\{init\}\}initializes the future GRU, enabling the predicted response to incorporate temperature\-dependent material behavior while using the start\-position feature as contextual information for the prediction boundary\.

#### III\-B3Future GRU

The future GRU uses the same gated recurrent structure as the history GRU to propagate the learned dynamic representation over the prediction horizon\. It is initialized byhinith\_\{\\mathrm\{init\}\}, which provides the boundary magnetic state inferred from the measuredB​\(t\)B\(t\)–H​\(t\)H\(t\)history\. Beyond this boundary, the future response is driven by the inputB​\(t\)B\(t\)trajectory\. Therefore, at each prediction step, the future GRU receives the input flux densityB​\(t\)B\(t\), its step\-to\-step incrementΔ​B​\(t\)\\Delta B\(t\), and a learned temporal\-position embedding\. The value ofB​\(t\)B\(t\)specifies the instantaneous flux\-density operating point, whileΔ​B​\(t\)\\Delta B\(t\)provides information about the local direction and rate of flux\-density variation\.

Including both inputs allows the future GRU to account for the fact that rate\-dependent magnetic behavior is influenced not only by the instantaneous flux\-density level, but also by how rapidly the excitation changes and the magnetic state accumulated from previous excitation history\. With these inputs, the future GRU sequentially updates the hidden state and produces the local representationhlocal​\(t\)h\_\{\\mathrm\{local\}\}\(t\)\. This representation encodes the rate\-dependent magnetic response conditioned on the measured boundary state, the future excitation trajectory, and its local variation, and is subsequently fused with the global hysteresis representation for futureH​\(t\)H\(t\)prediction\.

### III\-CGlobal Attention Branch for Quasi\-Static Hysteresis Context

The local recurrent branch propagates the rate\-dependent dynamic response step by step, but the quasi\-static hysteresis component requires a broader description of the excitation history\. As discussed in Section II\-B, hysteresis loss is path\-dependent\. It is affected by reversal points, flux\-density extrema, dc flux\-density offset, waveform asymmetry, and major\- or minor\-loop operation\. These long\-range waveform features can lead to differentH​\(t\)H\(t\)responses even when the local values ofB​\(t\)B\(t\)andΔ​B​\(t\)\\Delta B\(t\)are similar\.

A natural way to represent path\-dependent hysteresis memory is the Preisach model, which describes the quasi\-static hysteretic response as a weighted superposition of elementary hysteresis units:

Hhys​\(t\)=∬α≥βμ​\(α,β\)​γα​β​\[B\]​\(t\)​dα​dβ,H\_\{\\mathrm\{hys\}\}\(t\)=\\iint\_\{\\alpha\\geq\\beta\}\\mu\(\\alpha,\\beta\)\\,\\gamma\_\{\\alpha\\beta\}\[B\]\(t\)\\,\\mathrm\{d\}\\alpha\\,\\mathrm\{d\}\\beta,\(11\)whereγα​β​\[⋅\]\\gamma\_\{\\alpha\\beta\}\[\\cdot\]denotes an elementary hysteresis operator with switching thresholdsα\\alphaandβ\\beta, andμ​\(α,β\)\\mu\(\\alpha,\\beta\)represents the Preisach density function\. This formulation describes hysteresis memory through the weighted aggregation of hysteron states over the Preisach plane\.

![Refer to caption](https://arxiv.org/html/2608.02965v1/Fig/preisach.png)Figure 4:Preisach\-inspired global attention mechanism for extracting hysteresis\-related waveform context\.Motivated by the memory aggregation concept underlying Preisach\-type hysteresis descriptions, PI\-HNO introduces a Transformer\-based global branch, as illustrated in Fig\.[4](https://arxiv.org/html/2608.02965#S3.F4)\. The branch does not explicitly identify the Preisach density or implement physical hysterons\. Instead, it employs multi\-head self\-attention as a data\-driven memory aggregation mechanism, in which the learned attention weights capture the relevance of different portions of the excitation trajectory to predict the transient magnetic response\. For a projected flux\-density sequence, the attention weight from query positionqqto key positionkkis

Aq​k=exp⁡\(Qq​KkT/dk\)∑ℓ=1Nexp⁡\(Qq​KℓT/dk\),A\_\{qk\}=\\frac\{\\exp\\left\(Q\_\{q\}K\_\{k\}^\{\\mathrm\{T\}\}/\\sqrt\{d\_\{k\}\}\\right\)\}\{\\sum\_\{\\ell=1\}^\{N\}\\exp\\left\(Q\_\{q\}K\_\{\\ell\}^\{\\mathrm\{T\}\}/\\sqrt\{d\_\{k\}\}\\right\)\},\(12\)and the corresponding attention outputzqz\_\{q\}is

zq=∑k=1NAq​k​Vk\.z\_\{q\}=\\sum\_\{k=1\}^\{N\}A\_\{qk\}V\_\{k\}\.\(13\)Here,qqdenotes the query position at which the attention output is computed, andkkdenotes the key\-value position being attended to\.QqQ\_\{q\},KkK\_\{k\}, andVkV\_\{k\}are the query, key, and value vectors obtained through learned linear projections of the input embedding, respectively\.dkd\_\{k\}is the dimension of the key vector, which is used to scale the dot\-product similarity\.Aq​kA\_\{qk\}is the normalized attention weight that measures the contribution of the positionkkto positionqq\. Therefore, the attention output can be regarded as a data\-driven analog of Preisach\-type weighted superposition, where learned weights over sampled positions of the inputB​\(t\)B\(t\)waveform provide a discrete representation of the path\-dependent magnetization context\.

Following this interpretation, the global branch extracts the path\-dependent magnetization context from the complete inputB​\(t\)B\(t\)trajectory\. TheB​\(t\)B\(t\)sequence and the broadcast start\-position feature are projected and passed through the self\-attention block, where different portions of the excitation waveform are compared directly\. Mean pooling over the resulting time\-step representations produces the global vectorvglobalv\_\{\\mathrm\{global\}\}, which summarizes branch information, reversal locations, flux\-density extrema, dc offset, and minor\-loop structure\. This quasi\-static context complements the local dynamic branch by distinguishing prediction segments with similar instantaneousB​\(t\)B\(t\)andΔ​B​\(t\)\\Delta B\(t\)but different magnetization histories\.

### III\-DBranch Fusion and Output Layer

The local and global branches provide complementary representations for futureH​\(t\)H\(t\)prediction\. The local branch produces a time\-dependent representationhlocal​\(t\)h\_\{\\mathrm\{local\}\}\(t\)through sequential GRU updates, reflecting rate\-dependent dynamic field behavior\. In contrast, the global branch producesvglobal​\(t\)v\_\{\\mathrm\{global\}\}\(t\)from the complete inputB​\(t\)B\(t\)trajectory, providing sequence\-level context for quasi\-static, path\-dependent magnetization\. As shown in Fig\.[3](https://arxiv.org/html/2608.02965#S3.F3), these two representations are combined by additive fusion before the final output projection:

u​\(t\)=hlocal​\(t\)\+vglobal​\(t\),u\(t\)=h\_\{\\mathrm\{local\}\}\(t\)\+v\_\{\\mathrm\{global\}\}\(t\),\(14\)Hpred​\(t\)=MLPout​\(u​\(t\)\)\.H\_\{\\mathrm\{pred\}\}\(t\)=\\mathrm\{MLP\}\_\{\\mathrm\{out\}\}\\\!\\left\(u\(t\)\\right\)\.\(15\)
This additive fusion is motivated by the loss\-separation picture discussed in Section II\-B, in which the measured field response can be interpreted as the combined effect of quasi\-static hysteresis and dynamic eddy\-current\. In PI\-HNO, these components are not explicitly identified as analytical field terms\. Instead, the local and global branches learn equivalent physics\-guided representations that are summed in the latent space and mapped to the predicted futureHpred​\(t\)H\_\{\\mathrm\{pred\}\}\(t\)sequence\.

After the output projection,Hpred​\(t\)H\_\{\\mathrm\{pred\}\}\(t\)and the inputB​\(t\)B\(t\)trajectory form the predictedBB–HHtrajectory over the prediction interval\. During training, the energy\-aware regularization term shown in Fig\.[3](https://arxiv.org/html/2608.02965#S3.F3)penalizes inconsistency in the accumulatedBB–HHenergy of this trajectory\. This regularization is applied only during training\. For the inference, the model directly outputsHpred​\(t\)H\_\{\\mathrm\{pred\}\}\(t\)from the measured history, inputB​\(t\)B\(t\)trajectory, temperature, and temporal\-position features\.

### III\-EEnergy\-Aware Training Objective

The model is trained by combining pointwise waveform matching with a softBB–HHenergy\-consistency regularization term:

ℒ=ℒnorm\+λphys​ℒphys,\\mathcal\{L\}=\\mathcal\{L\}\_\{\\mathrm\{norm\}\}\+\\lambda\_\{\\mathrm\{phys\}\}\\mathcal\{L\}\_\{\\mathrm\{phys\}\},\(16\)whereℒnorm\\mathcal\{L\}\_\{\\mathrm\{norm\}\}is the smooth\-L1L\_\{1\}loss betweenHpred​\(t\)H\_\{\\mathrm\{pred\}\}\(t\)and the measured referenceHmeas​\(t\)H\_\{\\mathrm\{meas\}\}\(t\)in normalized units, andλphys\\lambda\_\{\\mathrm\{phys\}\}weights theBB–HHenergy\-consistency term\.

The energy\-consistency term is computed after converting the normalizedBBandHHvalues back to physical units\. Using the inputB​\(t\)B\(t\)trajectory over the prediction interval, the path integral ofH​d​BH\\,\\mathrm\{d\}Bis approximated by the trapezoidal rule for both the predicted and measuredBB–HHtrajectories\. The resulting open\-path quantities, denoted asWpredW\_\{\\mathrm\{pred\}\}andWmeasW\_\{\\mathrm\{meas\}\}, are used to regularize B–HHtrajectory consistency rather than to directly evaluate closed\-cycle core loss\. Since the prediction interval generally corresponds to an openBB–HHpath rather than a closed hysteresis loop, this energy consistency is imposed only as a soft regularization:

ℒphys=\|Wpred−Wmeas\|max⁡\(\|Wmeas\|,ϵ\)\+γ​max⁡\(0,−Wpred\),\\mathcal\{L\}\_\{\\mathrm\{phys\}\}=\\frac\{\\bigl\|W\_\{\\mathrm\{pred\}\}\-W\_\{\\mathrm\{meas\}\}\\bigr\|\}\{\\max\\bigl\(\|W\_\{\\mathrm\{meas\}\}\|,\\epsilon\\bigr\)\}\+\\gamma\\max\\bigl\(0,\-W\_\{\\mathrm\{pred\}\}\\bigr\),\(17\)where the first term penalizes inconsistency between the predicted and measured accumulatedBB–HHenergy, the second term introduces a one\-sided penalty for negative accumulated energy,ϵ\\epsilonavoids numerical instability when the reference energy approaches zero, andγ\\gammacontrols the strength of this penalty\. This composite regularization preserves supervision from the measuredH​\(t\)H\(t\)sequence while encouraging a physically consistent reconstructedBB–HHtrajectories\.

Therefore, the proposed energy term should be interpreted as a trajectory\-level physical regularization rather than a direct loss\-prediction objective\. It constrains the predicted magnetization path to preserve the energy\-related characteristics of the measured response\.

## IVExperimental Setup and Evaluation Metrics

### IV\-ADataset and Prediction\-Sequence Construction

The experiments use transient magnetic data from MagNetX\[[10](https://arxiv.org/html/2608.02965#bib.bib17),[22](https://arxiv.org/html/2608.02965#bib.bib20)\], following the history\-conditioned prediction formulation defined in Section II\. MagNetX measuresB​\(t\)B\(t\)andH​\(t\)H\(t\)using a two\-winding magnetic\-characterization setup, whereB​\(t\)B\(t\)is obtained from secondary\-side voltage integration andH​\(t\)H\(t\)is obtained from primary\-side current measurement\. The original transient measurements are collected under randomly varying duty\-cycle and frequency\-transition excitations\. The sampling window is adjusted based on the excitation frequency to capture multiple waveform cycles, with each measurement containing 100,000 samples and a 20\-MHz bandwidth limit\. Subsequently, it is down\-sampled to 10,000 samples by averaging every ten consecutive samples\[[22](https://arxiv.org/html/2608.02965#bib.bib20)\]\.

The evaluated material set contains 14 magnetic materials: 3C90, 3C92, 3C94, 3C95, 3E6, 3F4, 77, 78, N27, N30, N49, N87, FEC014, and T37\. Most materials include excitation frequencies of 50, 80, 100, 200, 300, 400, 600, and 800 kHz, except that 50 and 80 kHz are not available for N49\. The measured temperatures are 25, 50, and 70∘C\.

For the experiments in this work, the down\-sampled transient waveforms are further organized into fixed\-length sequences withL=1000L=1000time steps, consistent with the notation in \([2](https://arxiv.org/html/2608.02965#S2.E2)\)\. For each sequence, the prediction boundaryssis selected according to the test\-only known\-history ratiosρ∈\{0\.1,0\.5,0\.9\}\\rho\\in\\\{0\.1,0\.5,0\.9\\\}\. The same sequence construction is used for all evaluated models, so differences in performance arise from model structures rather than from different input horizons or waveform samples\.

### IV\-BTraining, Validation, and Testing Setup

The training, validation, and testing datasets are constructed separately for each material from the processed MagNetX transient measurements\. This material\-specific formulation is adopted because different magnetic materials exhibit distinct hysteresis characteristics, dynamic magnetic behaviors, and temperature\-dependent responses\. Therefore, this work focuses on developing compact transient magnetization models tailored to individual materials, rather than a single universal model across heterogeneous magnetic materials\. Within each material, the proposed model is evaluated under diverse excitation waveforms, frequency conditions, temperatures, and available magnetic\-history lengths\.

For each frequency\-temperature group, the measuredB​\(t\)B\(t\),H​\(t\)H\(t\), and temperature waveforms are first screened to remove invalid samples with inconsistent incremental magnetic responses\. The remaining waveforms are then sampled with a fixed random seed and divided into nonoverlapping 1000\-time\-step sequences\. The resulting material\-wise datasets contain alignedBB,HH, and temperature arrays for supervised training\.

For training, each 1000\-time\-step sequence is further divided into local prediction segments\. Within each segment, the most recentm=100m=100samples before the prediction boundary are used as the measuredB​\(t\)B\(t\)–H​\(t\)H\(t\)history for the history GRU, while the subsequent samples provide the prediction target for the future GRU\. The complete 1000\-time\-stepB​\(t\)B\(t\)sequence is retained as the input to the global branch\. For materials showing weaker validation performance in the low\-BppB\_\{\\mathrm\{pp\}\}region, additional low\-BppB\_\{\\mathrm\{pp\}\}training sequences are included to improve coverage of small\-signal transient behavior\. This data augmentation is determined solely from the corresponding training and validation results and does not involve the test data\.

A validation subset is held out from the training sequences and is used exclusively for model selection, early stopping, and hyperparameter tuning\. The test sequences remain independent throughout training and validation and are used only for final performance evaluation\. For the test\-only known\-history ratiosρ∈\{0\.1,0\.5,0\.9\}\\rho\\in\\\{0\.1,0\.5,0\.9\\\}, test sequences are constructed according to the corresponding prediction boundarys=ρ​Ls=\\rho L\. The same test set for eachρ\\rhois applied to all evaluated models within each material, ensuring a consistent comparison under different available\-history conditions\.

All comparison models are trained and evaluated using the same material\-specific data construction, training/validation/testing splits, inputB​\(t\)B\(t\)trajectories and evaluation metrics, ensuring that performance differences primarily reflect the model architecture rather than in experimental settings\.

### IV\-CImplementation Details of PI\-HNO

The history GRU has a hidden width of 8 and one layer, and the future GRU uses the same hidden width and depth\. The global branch is a single\-layer Transformer with width 8, two attention heads, and feed\-forward width 64\. The temperature and start\-position projection MLPs use sizes 1–8–8, the future\-position projection uses sizes 1–8, and the output projection MLP uses sizes 8–128–1 with a dropout rate of 0\.1\.

For training, each 1000\-time\-step training sequence is divided into five consecutive nonoverlapping 200\-time\-step local training segments\. In each segment, the first 100 time steps provide the measured history to the history GRU, and the last 100 time steps form the prediction target for the future GRU\. The complete 1000\-time\-stepB​\(t\)B\(t\)sequence serves as the global branch input for all five local segments\. The start\-position feature is the segment starting index normalized by the sequence length, and the future\-position features are the normalized indices of the 100 target time steps\.

Training minimizes the composite objective in Section[III\-E](https://arxiv.org/html/2608.02965#S3.SS5), withλphys=0\.1\\lambda\_\{\\mathrm\{phys\}\}=0\.1,γ=0\.01\\gamma=0\.01, andϵ=10−6\\epsilon=10^\{\-6\}\. A batch size of 64 is used for at most 1000 epochs with the AdamW optimizer and a one\-cycle learning\-rate schedule with a peak learning rate of10−210^\{\-2\}\. The weight decay is5×10−45\\times 10^\{\-4\}, the gradient norm is clipped at 0\.5, and an exponential moving average with decay 0\.999 is used for validation\. Training stops when the validation loss does not improve for 80 consecutive epochs\.

### IV\-DComparison Models and Ablation Settings

To evaluate the proposed PI\-HNO, six comparison models are implemented under the same data construction and evaluation procedure\. These models are selected to cover major categories of transient magnetic modeling approaches, including sequence\-to\-sequence recurrent models, convolutional neural models, physics\-inspired neural architectures, and attention\-based sequence models\. Existing neural operator approaches have primarily been developed to learn nonlinear mappings between input and output functions, with an emphasis on general operator approximation, discretization\-independent learning, or continuous field modeling\. In contrast, this work focuses on compact , boundary\-conditioned prediction of transient magnetization trajectories under material\-specific operating conditions, with computational efficiency and trajectory reconstruction accuracy as the primary objectives\. Therefore, task\-relevant magnetic response prediction models are selected as the primary references to provide meaningful, and computationally comparable baselines\.

The comparison models include the sequence\-to\-sequence MagLearn2 model\[[12](https://arxiv.org/html/2608.02965#bib.bib24)\], an LSTM model based on the MagNet Challenge 2 demonstration setting\[[22](https://arxiv.org/html/2608.02965#bib.bib20)\], the residual dilated\-convolution HARDCORE model for time\-domainH​\(t\)H\(t\)and loss estimation\[[9](https://arxiv.org/html/2608.02965#bib.bib21)\], the magnetization\-mechanism\-inspired neural network MMINN\[[5](https://arxiv.org/html/2608.02965#bib.bib16)\], a GRU\-only model, and a Transformer\-only model\. The GRU\-only model is configured with a parameter count close to that of PI\-HNO to evaluate the contribution of the proposed hybrid architecture beyond model size\. In contrast, the Transformer\-only model uses the same Transformer width, head count, and depth as the global branch of PI\-HNO with an independent output head to evaluate the contribution of the local recurrent branch\. The model configurations are summarized in Table[I](https://arxiv.org/html/2608.02965#S4.T1)\. All comparison models are trained and evaluated under the same material\-specific setting using identical training, validation, and testing procedures, inputB​\(t\)B\(t\)trajectories, and evaluation metrics\.

TABLE I:Configurations of PI\-HNO and the reference models\.The ablation study is designed to identify the contribution of each major architectural or conditioning component in PI\-HNO\. All ablation variants use the same dataset construction, training setup, and evaluation metrics as the full model, except for the stated modification\. As shown in Fig\.[5](https://arxiv.org/html/2608.02965#S4.F5), five variants are evaluated\. A1 removes the global branch to test the contribution of sequence\-level hysteresis context beyond the local measured history\. A2 removes the local recurrent branch to test the role of local dynamic\-state propagation and boundary\-state information\. A3 removes the incrementalΔ​B\\Delta Binput to assess the importance of local flux\-density variation for rate\-dependent field prediction\. A4 removes the future GRU to test whether the magnetic state must be propagated sequentially along the inputB​\(t\)B\(t\)trajectory\. A5 changes how temperature and start\-position information are used by feeding these scalar conditions directly to the future GRU rather than using them to initialize the hidden state, thereby conditioning the location rather than removing the conditions entirely\.

![Refer to caption](https://arxiv.org/html/2608.02965v1/x4.png)Figure 5:The visualization of ablation variants A1–A5 of PI\-HNO\.
### IV\-EEvaluation Metrics

Four metrics are used to evaluate complementary aspects of the predicted transient magnetization response\. The normalized sequence errorEseqE\_\{\\mathrm\{seq\}\}measures the overall waveform agreement between the predicted and measuredH​\(t\)H\(t\)sequences\. The peak\-field error,EHpkE\_\{H\_\{\\mathrm\{pk\}\}\}, evaluates whether the model correctly predicts the maximum field magnitude, which is relevant to the magnetic saturation margin and current\-stress estimation\. The relativeBB–HHenergy consistency errorEeneE\_\{\\mathrm\{ene\}\}measures the consistency of the accumulatedBB–HHwork along the predicted trajectory\. This quantity corresponds to core\-loss evaluation only when the reconstructed trajectory forms a closed cycle\. For the open trajectories considered in this work, it is used as a trajectory\-level energy consistency measure\. The energy\-sign mismatch rateηsgn\\eta\_\{\\mathrm\{sgn\}\}counts the fraction of test sequences for which the predicted and measured accumulatedBB–HHwork has opposite signs, indicating an inconsistent direction of accumulatedBB–HHwork over the prediction interval\. As defined in Section II,ssis the prediction boundary determined by the known\-history ratio in \([2](https://arxiv.org/html/2608.02965#S2.E2)\)\. All metrics are computed over the prediction intervalk=s,…,L−1k=s,\\ldots,L\-1\. For clarity, the sequence index is omitted in the following definitions\. For a given test sequence,Hmeas,kH\_\{\\mathrm\{meas\},k\},Hpred,kH\_\{\\mathrm\{pred\},k\}, andBkB\_\{k\}denote the measured field strength, predicted field strength, and input flux density at time stepkk, respectively\.

The normalized sequence error is

Eseq=1L−s​∑k=sL−1\(Hpred,k−Hmeas,k\)2max⁡\(1L−s​∑k=sL−1Hmeas,k2,ϵ\)×100%\.E\_\{\\mathrm\{seq\}\}=\\frac\{\\sqrt\{\\dfrac\{1\}\{L\-s\}\\sum\_\{k=s\}^\{L\-1\}\\left\(H\_\{\\mathrm\{pred\},k\}\-H\_\{\\mathrm\{meas\},k\}\\right\)^\{2\}\}\}\{\\max\\\!\\left\(\\sqrt\{\\dfrac\{1\}\{L\-s\}\\sum\_\{k=s\}^\{L\-1\}H\_\{\\mathrm\{meas\},k\}^\{2\}\},\\epsilon\\right\)\}\\times 100\\%\.\(18\)This metric measures the pointwise waveform error over the prediction horizon\. The peak\-field error is

EHpk=\|maxs≤k≤L−1⁡\|Hpred,k\|−maxs≤k≤L−1⁡\|Hmeas,k\|\|max⁡\(maxs≤k≤L−1⁡\|Hmeas,k\|,ϵ\)×100%\.E\_\{H\_\{\\mathrm\{pk\}\}\}=\\frac\{\\left\|\\max\\limits\_\{s\\leq k\\leq L\-1\}\\left\|H\_\{\\mathrm\{pred\},k\}\\right\|\-\\max\\limits\_\{s\\leq k\\leq L\-1\}\\left\|H\_\{\\mathrm\{meas\},k\}\\right\|\\right\|\}\{\\max\\\!\\left\(\\max\\limits\_\{s\\leq k\\leq L\-1\}\\left\|H\_\{\\mathrm\{meas\},k\}\\right\|,\\epsilon\\right\)\}\\times 100\\%\.\(19\)This metric evaluates the predicted maximum field magnitude\.

For implementation, the open\-path quantity in \([6](https://arxiv.org/html/2608.02965#S2.E6)\) is evaluated over the prediction interval using the trapezoidal rule\. For the predicted trajectory,

Wpred=∑k=sL−2Hpred,k\+1\+Hpred,k2​\(Bk\+1−Bk\)\.W\_\{\\mathrm\{pred\}\}=\\sum\_\{k=s\}^\{L\-2\}\\frac\{H\_\{\\mathrm\{pred\},k\+1\}\+H\_\{\\mathrm\{pred\},k\}\}\{2\}\\left\(B\_\{k\+1\}\-B\_\{k\}\\right\)\.\(20\)The measured counterpartWmeasW\_\{\\mathrm\{meas\}\}is obtained by replacingHpred,kH\_\{\\mathrm\{pred\},k\}withHmeas,kH\_\{\\mathrm\{meas\},k\}in \([20](https://arxiv.org/html/2608.02965#S4.E20)\)\. Since the prediction interval generally forms an openBB–HHtrajectory, these quantities are not interpreted as closed\-cycle core\-loss energy\. Their discrepancy is instead used as an energy\-related consistency measure that complements the point\-wise sequence error inH​\(t\)H\(t\)\. The relative energy error is

Eene=\|Wpred−Wmeas\|max⁡\(SE,ϵW\)×100%,E\_\{\\mathrm\{ene\}\}=\\frac\{\\left\|W\_\{\\mathrm\{pred\}\}\-W\_\{\\mathrm\{meas\}\}\\right\|\}\{\\max\\\!\\left\(S\_\{E\},\\epsilon\_\{W\}\\right\)\}\\times 100\\%,\(21\)whereSES\_\{E\}is the absolute accumulated\-energy scale of the test sequence\. This metric evaluates the consistency of the accumulatedBB–HHwork along the predicted trajectory\.

For an evaluation pool containingNseqN\_\{\\mathrm\{seq\}\}test sequences, the energy\-sign mismatch rate is

ηsgn=1Nseq​∑j=1Nseq𝟏​\[Wpred\(j\)​Wmeas\(j\)<0\]×100%,\\eta\_\{\\mathrm\{sgn\}\}=\\frac\{1\}\{N\_\{\\mathrm\{seq\}\}\}\\sum\_\{j=1\}^\{N\_\{\\mathrm\{seq\}\}\}\\mathbf\{1\}\\\!\\left\[W\_\{\\mathrm\{pred\}\}^\{\(j\)\}W\_\{\\mathrm\{meas\}\}^\{\(j\)\}<0\\right\]\\times 100\\%,\(22\)where𝟏​\[⋅\]\\mathbf\{1\}\[\\cdot\]is the indicator function\. This diagnostic identifies cases where the predicted accumulated work has the opposite sign to the measured reference\.

For each material, all valid test\-sequence evaluations are pooled across the evaluated known\-history ratios, frequency levels, and temperatures\. The distributions ofEseqE\_\{\\mathrm\{seq\}\}andEeneE\_\{\\mathrm\{ene\}\}are summarized by their mean and 95th\-percentile values,EHpkE\_\{H\_\{\\mathrm\{pk\}\}\}is reported by its mean value, andηsgn\\eta\_\{\\mathrm\{sgn\}\}is reported as the proportion of sign\-mismatched test sequences\. Overall results are obtained by taking the unweighted arithmetic mean of the corresponding material\-level statistics across the 14 materials\.

## VResults and Discussion

This section presents the experimental results for PI\-HNO and discusses its prediction accuracy, energy consistency, comparisons with baseline models, ablation results, and model compactness\. All results are obtained using the dataset construction, training setup, and evaluation metrics described in Section IV\.

### V\-AOverall Prediction Performance

Table[II](https://arxiv.org/html/2608.02965#S5.T2)summarizes the material\-wise prediction performance of PI\-HNO\. The overall statistics are computed as unweighted averages of the 14 material\-level results\. Across all evaluated materials, PI\-HNO achieves a mean sequence and energy errors of 13\.40% and 1\.92%, respectively, with corresponding 95th\-percentile values of 31\.39% and 7\.60%\. The mean peak\-field error is 6\.12%, and the energy\-sign mismatch rate is 1\.91%, indicating that most predicted trajectories preserve the direction of accumulatedBB–HHwork over the prediction interval\.

TABLE II:Material\-wise and overall error for sequence and energy of PI\-HNOThe material\-wise results show that the difficulty of sequence prediction varies noticeably across materials\. The lowest mean sequence errors are obtained for 3C95, FEC014, T37, and 3F4, all below 10%, whereas N30, 3C92, N87, and 3E6 show larger mean sequence errors above 17%\. The 95th\-percentile sequence error follows a similar trend, with N30 and N87 yielding the largest values\. In contrast, the energy error remains relatively low for most materials: the mean energy error is below 2\.5% for 12 of the 14 materials, and below 1\.3% for 3C92, 3C95, 3E6, and T37\. The main exception is N49, which has the highest mean and 95th\-percentile energy errors of 4\.08% and 16\.36%, respectively, and also the highest energy\-sign mismatch rate of 4\.13%\. This may be partly related to its different frequency coverage, since the 50 and 80 kHz conditions are not available for N49\.

Fig\.[6](https://arxiv.org/html/2608.02965#S5.F6)shows representative predictions for 3C90, 3C95, 3E6, and T37\. The upper plots compare the measured, predicted, and historicalH​\(t\)H\(t\)sequences, while the lower plots show selected predicted and measuredBB–HHsegments\. The predictions follow the main waveform trends and turning points, and the correspondingBB–HHsegments preserve the measured loop direction and branch location\. These examples visually support the sequence and energy\-error statistics in Table[II](https://arxiv.org/html/2608.02965#S5.T2)\.

![Refer to caption](https://arxiv.org/html/2608.02965v1/x5.png)Figure 6:Representative futureH​\(t\)H\(t\)prediction results for 3C90, 3C95, 3E6, and T37\.The difference between sequence\-error and energy\-error trends shows that waveform fitting and accumulated\-energy consistency are complementary criteria that ensure the measuredBB–HHpath is well followed to reproduce the accumulated energy, even when the point\-wise sequence error varies across materials\.

### V\-BComparison With Baseline Models

Table[III](https://arxiv.org/html/2608.02965#S5.T3)compares PI\-HNO with six baseline models under the same data construction, training procedure, evaluation metrics, and aggregation method\. Among the evaluated models, MagLearn2 achieves the lowest overall sequence errors, with mean and 95th\-percentile values of 12\.88% and 28\.47%, respectively\. The corresponding values of PI\-HNO are 13\.40% and 31\.39%, respectively, indicating that PI\-HNO does not achieve the best performance in terms of point\-wise waveform fitting alone\. However, transient magnetization modeling requires not only accurateH​\(t\)H\(t\)sequence prediction but also physically consistent reconstruction of the correspondingBB–HHtrajectory, which is further evaluated through theBB–HHenergy consistency and model compactness metrics\.

TABLE III:Overall sequence, energy, peak\-field, and energy\-sign errors compared with baseline models\.The advantage of PI\-HNO is more evident in energy\-related metrics\. It achieves the lowest mean and 95th\-percentile energy errors, at 1\.92% and 7\.60%, respectively, whereas MagLearn2 gives 4\.06% and 16\.46%\. The energy\-sign mismatch rate is also lower for PI\-HNO than for all baseline models\. These results indicate that the proposed physics\-guided architecture and energy\-aware training improve the consistency of the accumulatedBB–HHwork, even when MagLearn2 gives slightly lower pointwise sequence errors\.

Model compactness provides another important distinction\. PI\-HNO uses only 4777 trainable parameters, which is approximately1/1801/180of the parameter count of MagLearn2\. The GRU baseline has a comparable parameter count of 4758\. However, its mean and 95th\-percentile sequence errors increase to 18\.44% and 46\.17%, respectively, while its mean and 95th\-percentileBB–HHenergy consistency errors increase to 3\.68% and 16\.62%\. This comparison indicates that the performance of PI\-HNO is not achieved simply through increased model capacity, but through the integration of local dynamic\-state propagation, global hysteresis\-context extraction, andBB–HHenergy\-consistency regularization\. The remaining baseline models exhibit larger errors, particularly in the 95th\-percentile cases, suggesting that compact architectures without the combined dynamic, hysteresis\-memory, and trajectory\-consistency representations provide less favorable performance under the evaluated transient magnetization prediction conditions\.

The large sequence error of HARDCORE mainly reflects a task mismatch: it was designed for steady\-state core\-loss estimation from complete periodB​\(t\)B\(t\)waveforms, where the reconstructedH​\(t\)H\(t\)curve serves as an intermediate representation forBB–HHarea integration and residual loss correction\[[9](https://arxiv.org/html/2608.02965#bib.bib21)\]\. Its full\-cycle, circular\-padding CNN structure is therefore less suited to boundary\-conditioned prediction over finite, possibly openBB–HHtrajectories\.

Fig\.[7](https://arxiv.org/html/2608.02965#S5.F7)further compares the material\-level 95th\-percentile sequence and energy errors for PI\-HNO with those of the three strongest baseline models\. For the 95th\-percentile sequence error, the material\-level comparison shows noticeable variation across materials\. MagLearn2 gives lower 95th\-percentile sequence errors for several materials, such as 3C94, 3F4, N30, and FEC014, whereas PI\-HNO is lower for 3C90, 77, 78, and T37\. The two models therefore show comparable but material\-dependent sequence\-prediction behavior, rather than one model uniformly dominating the other\. In contrast, the LSTM and GRU baselines reach or exceed the 50% display cap for multiple materials, indicating weaker control of the largest sequence errors under the same evaluation setting\.

The material\-level energy comparison shows a clearer trend\. MagLearn2 exhibits large 95th\-percentile energy errors for several materials, including 3C90, 78, N27, and N49, with the 3C90 value exceeding the 50% display cap\. In contrast, the 95th\-percentile energy error of PI\-HNO remains below 20% for all 14 materials\. This material\-wise behavior supports the aggregate results in Table[III](https://arxiv.org/html/2608.02965#S5.T3): PI\-HNO does not always minimize pointwise sequence error, but it provides a more consistent balance between futureH​\(t\)H\(t\)prediction, accumulated\-energy accuracy, and parameter efficiency\.

![Refer to caption](https://arxiv.org/html/2608.02965v1/x6.png)Figure 7:Material\-level 95th\-percentile sequence \(top\) and energy \(bottom\) errors between PI\-HNO and three overall best reference models\. The axis limits are capped at 50%\.
### V\-CAblation Study and Physical Interpretation

Table[IV](https://arxiv.org/html/2608.02965#S5.T4)reports the ablation results for the variants defined in Fig\.[5](https://arxiv.org/html/2608.02965#S4.F5)\. All variants are evaluated using the same dataset construction, training setup, and metrics as the full model\. Each ablation increases the reported errors relative to PI\-HNO, indicating that the tested components contribute complementary information to the transientBB–HHprediction\.

TABLE IV:Overall error for the sequence and energy of the ablation study\.Removing the global branch \(A1\) reduces the parameter size from 4777 to 2241, but increases the mean sequence error from 13\.40% to 17\.77% and the 95th\-percentile sequence error from 31\.39% to 42\.19%\. The mean and 95th\-percentile energy errors also increased from 1\.92% and 7\.60% to 2\.86% and 9\.61%, respectively\. The degradation suggests that the completeB​\(t\)B\(t\)trajectory provides additional magnetic\-history information relevant to the magnetization process\. Physically, this is consistent with the path\-dependent nature of quasi\-static hysteresis: reversal locations, flux\-density extrema, dc offset, and minor\-loop context cannot be fully recovered from a short local history alone\.

Removing the local recurrent branch \(A2\) produces the largest peak\-field error and energy\-sign mismatch rate among the ablations, at 17\.80% and 5\.57%, respectively\. It also increases the 95th\-percentile sequence and energy errors to 49\.10% and 12\.50%\. This indicates that the local branch is essential for initializing the boundary magnetic state and preserving the rate\-dependent eddy currents behavior over the subsequent excitation interval\. Without this local dynamic state, the model loses accuracy in the field amplitude and is more likely to predict the wrong direction of accumulated magnetization\.

Removing the incrementalΔ​B\\Delta Binput \(A3\) gives the lowest mean sequence error among the ablated variants\. Still, it produces the largest mean and 95th\-percentileBB–HHenergy consistency errors, at 3\.73% and 12\.66%, respectively\. This behavior is physically meaningful\. The instantaneous value ofB​\(t\)B\(t\)identifies the operating point on the flux\-density axis, whereasΔ​B\\Delta Bprovides information on the direction of local variation and the excitation rate\. RemovingΔ​B\\Delta Btherefore reduces the model’s ability to capture transient magnetic effects associated with changing flux\-density excitation\. As a result, the predicted waveform can still achieve relatively small point\-wise errors, while the accumulatedBB–HHwork along the reconstructed trajectory becomes less consistent\.

Removing the future GRU \(A4\) raises the mean sequence error to 19\.01% and the 95th\-percentile energy error to 12\.18%\. The increased errors indicate thatH​\(t\)H\(t\)prediction requires sequential magnetic\-state propagation along the inputB​\(t\)B\(t\)trajectory, rather than a directB​\(t\)B\(t\)\-to\-H​\(t\)H\(t\)mapping\. This is consistent with dynamic hysteresis, which the instantaneous field depends on both the current flux density and the previously accumulated hysteretic state\.

Finally, bypassing temperature\- and start\-position\-conditioned hidden\-state initialization \(A5\) gives the largest sequence degradation, with mean and 95th\-percentile sequence errors of 24\.83% and 75\.68%, respectively\. Since temperature and start\-position information are still provided directly to the future GRU in this variant, the result does not imply that these inputs are unimportant\. Rather, it shows that their placement is important\. In this architecture, temperature\-dependent material behavior and prediction\-boundary context are more effectively introduced via the initial hidden state than as stepwise future inputs\.

Overall, the ablation results support the intended division of roles in PI\-HNO\. The global attention branch supplies a quasi\-static hysteresis context\. The local recurrent branch propagates rate\-dependent dynamic response\. TheΔ​B\\Delta Binput provides local excitation\-change information\. The future GRU maintains the evolving prediction state, and the conditioning projections initialize the model with temperature and boundary\-position context\. The full model gives the best overall balance of sequence accuracy, accumulated\-energy consistency, peak\-field prediction, and the directionality of energy dissipation\.

## VIConclusion

This work proposed PI\-HNO, a compact physics\-informed material\-specific neural model for core\-loss\-oriented transient magnetization prediction\. Given the completeB​\(t\)B\(t\)excitation trajectory, the recentH​\(t\)H\(t\)history before the prediction interval, temperature, and operating\-condition information, PI\-HNO predicts the subsequentH​\(t\)H\(t\)response and the corresponding reconstructedBB–HHtrajectory\. The proposed framework incorporates magnetic knowledge through a physics\-guided decomposition of transient magnetic response, a Preisach\-inspired global representation for capturing hysteresis\-related waveform context, and aBB–HHenergy\-consistency regularization term during training\. Specifically, the local recurrent branch learns a boundary\-conditioned representation of rate\-dependent magnetic response, while the global branch exploits the memory aggregation principle of Preisach hysteresis to extract long\-range excitation dependencies from the completeB​\(t\)B\(t\)trajectory\.

Evaluation using material\-specific models for 14 ferrite materials from the MagNetX transient dataset demonstrated that PI\-HNO achieved average sequence and accumulated\-energy consistency errors of 13\.40% and 1\.92%, respectively, with corresponding 95th\-percentile errors of 31\.39% and 7\.60%\. These results were obtained with only 4777 trainable parameters per material\-specific model, demonstrating the compactness of the proposed architecture for transient magnetization modeling\. The ablation study further demonstrated that the proposed architectural components and conditioning strategies provide complementary contributions to prediction accuracy and accumulated\-energy consistency, supporting the effectiveness of the physics\-guided design\.

Future work will focus on embedding PI\-HNO into transient electromagnetic and circuit\-field simulation workflowsand validating its impact on device\-level loss prediction, thermal assessment, and high\-frequency magnetic component optimization across a broader range of excitation and operating conditions\.

## References

- \[1\]\(1988\)General properties of power losses in soft ferromagnetic materials\.IEEE Transactions on magnetics24\(1\),pp\. 621–630\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2),[§II\-B](https://arxiv.org/html/2608.02965#S2.SS2.p5.6)\.
- \[2\]A\. Chandra, B\. Daniels, M\. Curti, K\. Tiels, and E\. A\. Lomonova\(2024\)Magnetic hysteresis modeling with neural operators\.IEEE Transactions on Magnetics61\(1\),pp\. 1–11\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8)\.
- \[3\]A\. Chandra, T\. Kapoor, B\. Daniels, M\. Curti, K\. Tiels, D\. M\. Tartakovsky, and E\. A\. Lomonova\(2025\)Generalizable models of magnetic hysteresis via physics\-aware recurrent neural networks\.Computer Physics Communications314,pp\. 109650\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8)\.
- \[4\]Q\. Huang, Y\. Li, Y\. Dou, Y\. Li, J\. Zhu, and S\. Li\(2025\)History\-dependent prandtl\-ishlinskii neural network for quasi\-static core loss prediction under arbitrary excitation waveforms\.IEEE Transactions on Power Electronics\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8)\.
- \[5\]Q\. Huang, Y\. Li, J\. Zhu, and S\. Li\(2024\)Magnetization mechanism\-inspired neural networks for core loss estimation\.IEEE Transactions on Power Electronics39\(12\),pp\. 16382–16390\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8),[§IV\-D](https://arxiv.org/html/2608.02965#S4.SS4.p2.2)\.
- \[6\]S\. Hui, J\. G\. Zhu, and V\. Ramsden\(1996\)A generalized dynamic circuit model of magnetic cores for low\-and high\-frequency applications\. ii\. circuit model formulation and implementation\.IEEE Transactions on Power Electronics11\(2\),pp\. 251–259\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[7\]L\. Jieli, T\. Abdallah, and C\. R\. Sullivan\(2001\)Improved calculation of core loss with nonsinusoidal waveforms\.InConference record of the 2001 IEEE industry applications conference\. 36th IAS annual meeting \(Cat\. No\. 01CH37248\),Vol\.4,pp\. 2203–2210\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[8\]D\. C\. Jiles and D\. L\. Atherton\(1986\)Theory of ferromagnetic hysteresis\.Journal of magnetism and magnetic materials61\(1\-2\),pp\. 48–60\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2),[§II\-B](https://arxiv.org/html/2608.02965#S2.SS2.p3.2)\.
- \[9\]W\. Kirchgässner, N\. Förster, T\. Piepenbrock, O\. Schweins, and O\. Wallscheid\(2024\)HARDCORE: h\-field and power loss estimation for arbitrary waveforms with residual, dilated convolutional neural networks in ferrite cores\.IEEE Transactions on Power Electronics40\(2\),pp\. 3326–3335\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p3.4),[§IV\-D](https://arxiv.org/html/2608.02965#S4.SS4.p2.2),[§V\-B](https://arxiv.org/html/2608.02965#S5.SS2.p4.6)\.
- \[10\]H\. Li, D\. Serrano, T\. Guillod, S\. Wang, E\. Dogariu, A\. Nadler, M\. Luo, V\. Bansal, N\. K\. Jha, Y\. Chen,et al\.\(2023\)How magnet: machine learning framework for modeling power magnetic material characteristics\.IEEE Transactions on Power Electronics38\(12\),pp\. 15829–15853\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4),[§I](https://arxiv.org/html/2608.02965#S1.p3.4),[§IV\-A](https://arxiv.org/html/2608.02965#S4.SS1.p1.4)\.
- \[11\]H\. Li, D\. Serrano, S\. Wang, and M\. Chen\(2023\)MagNet\-ai: neural network as datasheet for magnetics modeling and material recommendation\.IEEE Transactions on Power Electronics38\(12\),pp\. 15854–15869\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4),[§I](https://arxiv.org/html/2608.02965#S1.p3.4)\.
- \[12\]MagLearn2\.Note:Open\-source software repositoryAccessed: Jul\. 12, 2026External Links:[Link](https://github.com/JunWang-Bristol/MagLearn2)Cited by:[§IV\-D](https://arxiv.org/html/2608.02965#S4.SS4.p2.2)\.
- \[13\]F\. Preisach\(1935\)Über die magnetische nachwirkung\.Zeitschrift für physik94\(5\),pp\. 277–302\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[14\]N\. Rajput, H\. B\. Sandhibigraha, N\. Agrawal, and V\. M\. Iyer\(2025\)An empirical model informed neural network core loss predictor for soft magnetic materials\.IEEE Transactions on Power Electronics\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8)\.
- \[15\]J\. Reinert, A\. Brockmeyer, and R\. W\. De Doncker\(2001\)Calculation of losses in ferro\-and ferrimagnetic materials based on the modified steinmetz equation\.IEEE Transactions on Industry applications37\(4\),pp\. 1055–1061\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[16\]W\. Roshen\(1991\)Ferrite core loss for power magnetic components design\.IEEE Transactions on Magnetics27\(6\),pp\. 4407–4415\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4)\.
- \[17\]D\. Serrano, H\. Li, S\. Wang, T\. Guillod, M\. Luo, V\. Bansal, N\. K\. Jha, Y\. Chen, C\. R\. Sullivan, and M\. Chen\(2023\)Why magnet: quantifying the complexity of modeling power magnetic material characteristics\.IEEE Transactions on Power Electronics38\(11\),pp\. 14292–14316\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4)\.
- \[18\]C\. P\. Steinmetz\(1892\)On the law of hysteresis\.Transactions of the American Institute of Electrical Engineers9\(1\),pp\. 1–64\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[19\]Y\. Teng, Y\. Wei, Y\. Li, X\. Guo, and Y\. Li\(2026\)An overview of current source converters: state\-of\-the\-art and future trends\.IEEE Transactions on Power Electronics\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4)\.
- \[20\]H\. Vater, O\. Schweins, L\. Hölsch, W\. Kirchgässner, T\. Piepenbrock, and O\. Wallscheid\(2026\)RHINO\-mag: recursive h\-field inference based on observed magnetic flux under dynamic excitation\.arXiv preprint arXiv:2603\.29745\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p3.4)\.
- \[21\]K\. Venkatachalam, C\. R\. Sullivan, T\. Abdallah, and H\. Tacca\(2002\)Accurate prediction of ferrite core loss with nonsinusoidal waveforms using only steinmetz parameters\.In2002 IEEE Workshop on Computers in Power Electronics, 2002\. Proceedings\.,pp\. 36–41\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.
- \[22\]S\. Wang, H\. Kwon, H\. Li, T\. Guillod, H\. Wouters, C\. R\. Sullivan, and M\. Chen\(2026\)MagNetX: data\-driven time\-domain foundation models for power magnetics in transient\.IEEE Transactions on Power Electronics\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p1.4),[§I](https://arxiv.org/html/2608.02965#S1.p3.4),[§II\-B](https://arxiv.org/html/2608.02965#S2.SS2.p2.2),[§IV\-A](https://arxiv.org/html/2608.02965#S4.SS1.p1.4),[§IV\-D](https://arxiv.org/html/2608.02965#S4.SS4.p2.2)\.
- \[23\]Y\. Xiao, C\. Li, and Z\. Zheng\(2026\)A magnetic core loss model based on physics\-informed neural network with cross\-attention\.IEEE Transactions on Power Electronics41\(1\),pp\. 92–96\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p4.8)\.
- \[24\]J\. G\. Zhu, S\. Hui, and V\. Ramsden\(1996\)A generalized dynamic circuit model of magnetic cores for low\-and high\-frequency applications\. i\. theoretical calculation of the equivalent core loss resistance\.IEEE Transactions on Power Electronics11\(2\),pp\. 246–250\.Cited by:[§I](https://arxiv.org/html/2608.02965#S1.p2.2)\.

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