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Radial Müntz-Szász Networks: Neural Architectures with Learnable Power Bases for Multidimensional Singularities

Gnankan Landry Regis N'guessan, Bum Jun Kim

TL;DR

Radial Müntz-Szász Networks (RMN)Address radial singularities by using learnable radial power bases $r^{\mu}$ with negative exponents and a limit-stable log-primitive to realize $\log r$. A separability obstruction shows coordinate-wise power bases cannot efficiently approximate non-quadratic radial functions, motivating RMN's architecture that directly parameterizes radial structure. RMN variants include RMN-Angular for angular dependence via spherical harmonics and RMN-MC for learnable singularity centers, with closed-form derivatives enabling physics-informed training. Across 10 benchmarks in 2D and 3D, RMN achieves up to $50\times$ lower RMSE with far fewer parameters than MLPs and SIREN, while preserving interpretability through learned exponent spectra that reflect physical singularities. The approach offers a compact, structure-aware alternative for singular problems, with clear limitations for strongly non-radial targets and opportunities for future physics-informed and time-dependent extensions.

Abstract

Radial singular fields, such as $1/r$, $\log r$, and crack-tip profiles, are difficult to model for coordinate-separable neural architectures. We show that any $C^2$ function that is both radial and additively separable must be quadratic, establishing a fundamental obstruction for coordinate-wise power-law models. Motivated by this result, we introduce Radial Müntz-Szász Networks (RMN), which represent fields as linear combinations of learnable radial powers $r^μ$, including negative exponents, together with a limit-stable log-primitive for exact $\log r$ behavior. RMN admits closed-form spatial gradients and Laplacians, enabling physics-informed learning on punctured domains. Across ten 2D and 3D benchmarks, RMN achieves 1.5$\times$--51$\times$ lower RMSE than MLPs and 10$\times$--100$\times$ lower RMSE than SIREN while using 27 parameters, compared with 33,537 for MLPs and 8,577 for SIREN. We extend RMN to angular dependence (RMN-Angular) and to multiple sources with learnable centers (RMN-MC); when optimization converges, source-center recovery errors fall below $10^{-4}$. We also report controlled failures on smooth, strongly non-radial targets to delineate RMN's operating regime.

Radial Müntz-Szász Networks: Neural Architectures with Learnable Power Bases for Multidimensional Singularities

TL;DR

Radial Müntz-Szász Networks (RMN)Address radial singularities by using learnable radial power bases with negative exponents and a limit-stable log-primitive to realize . A separability obstruction shows coordinate-wise power bases cannot efficiently approximate non-quadratic radial functions, motivating RMN's architecture that directly parameterizes radial structure. RMN variants include RMN-Angular for angular dependence via spherical harmonics and RMN-MC for learnable singularity centers, with closed-form derivatives enabling physics-informed training. Across 10 benchmarks in 2D and 3D, RMN achieves up to lower RMSE with far fewer parameters than MLPs and SIREN, while preserving interpretability through learned exponent spectra that reflect physical singularities. The approach offers a compact, structure-aware alternative for singular problems, with clear limitations for strongly non-radial targets and opportunities for future physics-informed and time-dependent extensions.

Abstract

Radial singular fields, such as , , and crack-tip profiles, are difficult to model for coordinate-separable neural architectures. We show that any function that is both radial and additively separable must be quadratic, establishing a fundamental obstruction for coordinate-wise power-law models. Motivated by this result, we introduce Radial Müntz-Szász Networks (RMN), which represent fields as linear combinations of learnable radial powers , including negative exponents, together with a limit-stable log-primitive for exact behavior. RMN admits closed-form spatial gradients and Laplacians, enabling physics-informed learning on punctured domains. Across ten 2D and 3D benchmarks, RMN achieves 1.5--51 lower RMSE than MLPs and 10--100 lower RMSE than SIREN while using 27 parameters, compared with 33,537 for MLPs and 8,577 for SIREN. We extend RMN to angular dependence (RMN-Angular) and to multiple sources with learnable centers (RMN-MC); when optimization converges, source-center recovery errors fall below . We also report controlled failures on smooth, strongly non-radial targets to delineate RMN's operating regime.
Paper Structure (127 sections, 13 theorems, 67 equations, 13 figures, 11 tables)

This paper contains 127 sections, 13 theorems, 67 equations, 13 figures, 11 tables.

Key Result

Corollary 3.2

The radial power $r^\mu$ is harmonic $\Delta r^\mu = 0$ in $\mathbb{R}^d \setminus \{0\}$ if and only if $\mu = 0$ or $\mu = 2 - d$.

Figures (13)

  • Figure 1: The separability obstruction visualized. (a) The target $\log r$ has circular level sets. (b) The coordinate-separable MSN produces diamond-shaped artifacts due to its axis-aligned structure. (c) RMN precisely matches the radial structure, achieving a 72$\times$ lower error.
  • Figure 2: Three RMN architectural variants. RMN-Direct: purely radial singularities. RMN-Angular: adds spherical harmonics for angular-dependent fields. RMN-MC: learns multiple singularity locations.
  • Figure 3: RMN achieves orders-of-magnitude improvement on singular functions. Top: RMSE comparison across four benchmarks. Middle left: Improvement factors. Middle right: Pareto frontier. Bottom left: Convergence. Bottom right: Architecture summary.
  • Figure 4: RMSE heatmap across all experiments and methods. Green = low error (good), red = high error (poor). RMN variants dominate on radial singularities; MLP excels on smooth functions.
  • Figure 5: Pareto frontier: accuracy--model size trade-off. RMN occupies the optimal efficient region with low error and low parameter count.
  • ...and 8 more figures

Theorems & Definitions (42)

  • Definition 3.1: Radial function
  • Corollary 3.2
  • Proposition 3.3: $L^p$ integrability of radial powers
  • proof
  • Remark 3.4: Punctured Domains and Evaluation Protocol
  • Theorem 3.5: Müntz-Szász muntz1914szasz1916
  • Example 3.6: Satisfying and violating the Müntz condition
  • Definition 3.7: Radial Müntz space
  • Theorem 3.8: Radial Müntz-Szász Density
  • proof
  • ...and 32 more