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Subspace Regularization

Updated 7 July 2026
  • Subspace regularization is a framework that restricts optimization to targeted low-dimensional subspaces via hard restrictions, projections, or penalty alignments.
  • It reduces computational costs and mitigates overfitting and instability by encoding prior structure, as seen in methods like Nyström ERM and Bayesian inverse problems.
  • Applications span from few-shot incremental learning and hyperspectral imaging to low-rank adaptations in large language models and subspace clustering.

Subspace regularization denotes a family of methods in which regularity is imposed by restricting optimization to a subspace, by penalizing deviation from a preferred subspace, or by projecting a high-dimensional problem onto a sequence of low-dimensional spaces. In the cited literature, the subspace may be a random span of training examples in regularized empirical risk minimization and Nyström kernel methods (Vecchia et al., 2022), a generalized Golub–Kahan solution space for Bayesian linear inverse problems (Li, 2023), the span of previously learned classifier weights in few-shot class incremental learning (Akyürek et al., 2021), a protected null space for low-rank adaptation in LLMs (Lu et al., 2024), or a spectral coefficient space for hyperspectral image super-resolution (Simões et al., 2014). Across these settings, subspaces are used to encode prior structure, reduce per-iteration or per-solve cost, and control instability, overfitting, or forgetting.

1. Core formulations and scope

A useful taxonomy is to distinguish between hard subspace restriction, projection-based regularization, and penalty-based alignment to a subspace. The same expression “subspace regularization” is therefore not attached to a single penalty or algorithmic template, but to a broader design principle.

Form Representative formulation Representative setting
Hard restriction to a subspace βλ,m=argminβSm{Ln(β)+λβ2}\beta_{\lambda,m} = \arg\min_{\beta\in S_m}\{L_n(\beta) + \lambda\|\beta\|^2\} Nyström ERM
Projection to an iterative subspace x=Vkyx=V_k\,y Bayesian and general-form inverse problems
Penalty toward a preferred subspace Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^2 Few-shot class incremental learning
Null-space protection R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^2 Controlled LoRA
Regularization on subspace coefficients X=EUX = E\,U; Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R Hyperspectral image super-resolution

In statistical learning, the subspace is frequently part of the hypothesis class itself. In inverse problems, it is often an iterative projection space generated by Krylov- or bidiagonalization-type procedures. In continual learning and PEFT, the subspace appears as a geometric prior on allowable updates. In imaging, the subspace is typically a low-dimensional coefficient domain in which spatial or tensor regularizers are applied. These variants are all present in the literature surveyed here (Vecchia et al., 2020, Li, 2023, Akyürek et al., 2021, Lu et al., 2024, Simões et al., 2014).

2. Random subspaces and regularized empirical risk minimization

A canonical learning-theoretic formulation appears in regularized ERM on random subspaces. In a real separable Hilbert space HH, the full problem is

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},

where L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)] and Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle). The subspace version restricts optimization to a random x=Vkyx=V_k\,y0-dimensional space x=Vkyx=V_k\,y1,

x=Vkyx=V_k\,y2

with the Nyström method arising when x=Vkyx=V_k\,y3 for a random subset of the data (Vecchia et al., 2020).

The analysis in "Regularized ERM on random subspaces" studies possibly data dependent subspaces spanned by a random subset of the data, recovering as a special case Nyström approaches for kernel methods, and extends statistical-computational tradeoff results from least squares and self-concordant losses to convex Lipschitz loss functions, including non-smooth losses such as the hinge loss (Vecchia et al., 2022). Under input boundedness, convex Lipschitz loss, and existence of a minimizer, the subspace excess-risk bound includes the additional projection term

x=Vkyx=V_k\,y4

which is controlled by requiring

x=Vkyx=V_k\,y5

with high probability. This yields

x=Vkyx=V_k\,y6

The sampling complexity for achieving the projection condition is stated as

x=Vkyx=V_k\,y7

under uniform sampling, or

x=Vkyx=V_k\,y8

under approximate-leverage-score sampling (Vecchia et al., 2020).

The computational point is explicit: full ERM with kernel methods costs x=Vkyx=V_k\,y9 to optimize or Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^20 to invert kernel matrices, whereas Nyström-subspace ERM reduces memory to Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^21, per-iteration cost to Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^22, and prediction to Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^23. The statistical point is equally explicit: the main results show the existence of different settings, depending on how hard the learning problem is, for which computational efficiency can be improved with no loss in performance (Vecchia et al., 2022). For hinge loss, the convex excess-risk bound transfers to excess classification error through Zhang’s inequality, and for polynomial eigenvalue decay Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^24 with Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^25, the detailed summary states that uniform sampling requires Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^26 while ALS sampling requires Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^27 to attain

Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^28

(Vecchia et al., 2020).

3. Projection-based regularization in inverse problems

In inverse problems, subspace regularization is often literally a projection method. A discrete operator equation Rsub=cC(t)(IPP)ηc2R_{\mathrm{sub}}=\sum_{c\in C^{(t)}}\|(\mathbf I - P\,P^\top)\,\eta_c\|^29 with non-closed range can be regularized by finite-rank projection-like operators R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^20 acting on a subspace R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^21 with R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^22, without requiring the ranges of R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^23 to be subspaces of the codomain. The discretized normal operators are

R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^24

and exact-data or noisy-data solutions are obtained from

R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^25

or from the finite-system Tikhonov variant

R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^26

The framework is stated to include truncated SVD, Ritz–Galerkin projection, and quadrature-collocation discretizations, with convergence controlled by R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^27 (Nair, 2016).

A Bayesian variant appears in subspace projection regularization for large-scale linear inverse problems with Gaussian noise and Gaussian prior. There the MAP estimator solves

R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^28

and the key step is to generate a sequence of solution subspaces by a generalized Golub–Kahan bidiagonalization in the weighted inner products R(ΔW)=λPΔWF2R(\Delta W)=\lambda\,\|P^\top\,\Delta W\|_F^29 and X=EUX = E\,U0. With X=EUX = E\,U1, the projected problem reduces to

X=EUX = E\,U2

and the iteration index X=EUX = E\,U3 plays the role of a regularization parameter. The method exhibits semi-convergence, and the detailed presentation lists three stopping rules: Discrepancy Principle, L-curve, and Generalized Cross Validation (Li, 2023).

A closely related general-form Tikhonov construction uses the preconditioned Golub–Kahan bidiagonalization for

X=EUX = E\,U4

with

X=EUX = E\,U5

The pGKB process generates a X=EUX = E\,U6-orthonormal basis X=EUX = E\,U7, and the projected small-scale problem is

X=EUX = E\,U8

The detailed exposition emphasizes two regularization mechanisms: the solution subspace learns the preferred directions embedded in X=EUX = E\,U9, and the iterates admit a filtered GSVD expansion. Because semi-convergence remains present, two hybrid schemes are introduced: weighted GCV and a secant update based on the discrepancy principle (Li, 2023).

The large-scale regime motivates further compression of the projection machinery itself. The sketched generalized Krylov subspace method sGKS compresses the tall projected matrices Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R0 and Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R1 by oblivious sketches Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R2 and Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R3, performs QR updates on the sketches, and skips explicit reorthogonalization of the basis. The sketched projected solve is

Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R4

and the paper states that sGKS preserves the approximation quality of the original method, produces iterates identical to those of standard GKS when sketching is omitted in the projected solve, and yields quasi-optimal residual norms controlled by the embedding quality (Palitta et al., 16 Jun 2026). The reported speedups are problem-dependent: for image deblurring, sGKS with Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R5 attains Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R6 in Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R7 iterations and Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R8 s, against GKS Z=C×3R\mathcal Z=\mathcal C\times_3\mathbf R9 in HH0 iterations and HH1 s; for dynamic CT, sGKS with HH2 gives HH3 in HH4 s, compared to full GKS HH5 in HH6 s (Palitta et al., 16 Jun 2026).

Subspace recycling gives a different augmentation-based perspective. A fixed finite-dimensional subspace HH7 is used to split the solution into a projected part and a complement,

HH8

and the reduced operator

HH9

is regularized on wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},0. The key theorem states that if wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},1 is a regularization for the projected equation and the compatibility condition

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},2

holds, then the augmented reconstructor

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},3

is also a regularization for the full problem (Ramlau et al., 2020). The augmented gradient method is described as a deflated steepest-descent step, and the experiments report acceleration by approximately a factor of two for Gaussian-blur deconvolution and up to a factor–4 speed-up in iteration count for adaptive-optics image deconvolution (Ramlau et al., 2020).

4. Regularized optimization on random or low-dimensional subspaces

In nonlinear optimization, subspace regularization often means minimizing a regularized local model inside a low-dimensional search space. Random-subspace Adaptive Regularization using Cubics (R-ARC) restricts the step to

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},4

and minimizes the reduced cubic model

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},5

where wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},6 and wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},7. Under standard assumptions and suitable embedding conditions, Theorem 4.2 states that with probability at least wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},8, R-ARC requires at most

wλ=argminwH{Ln(w)+λw2},w_\lambda = \arg\min_{w\in H}\{L_n(w) + \lambda\|w\|^2\},9

iterations to reach L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]0, and Theorem 6.1 gives

L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]1

for approximate second-order criticality, matching the full-space cubic bounds (Cartis et al., 16 Jan 2025). For low-rank functions, the adaptive variant R-ARC-D updates the subspace size via

L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]2

and the detailed report states that the method automatically “discovers” the correct subspace dimension. On low-rank targets, R-ARC-D often requires L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]3 fewer Hessian-vector products and runs L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]4–L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]5 faster while matching full-ARC’s final accuracy (Cartis et al., 16 Jan 2025).

A different regularization model is used in two-dimensional subspace minimization conjugate-gradient methods based on L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]6-regularization. There the local model is

L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]7

with

L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]8

The derived direction

L(w)=E(X,Y)[(Y,w,X)]L(w)=E_{(X,Y)}[\ell(Y,\langle w,X\rangle)]9

satisfies sufficient descent,

Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)0

and a gradient-proportional bound,

Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)1

which support global convergence under a modified nonmonotone Wolfe line search (Zhao et al., 2020). The paper further states global convergence to stationary points under mild assumptions and an Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)2-linear rate under convexity and a global error bound. On 145 CUTEr test problems, SMCG_PR1 with Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)3 solved Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)4 of Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)5 problems and outperformed four comparison methods on roughly Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)6–Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)7 of the tests in iteration count, function/gradient evaluations, and CPU time (Zhao et al., 2020).

5. Geometric regularization of representations, affinities, and updates

In subspace clustering, regularization frequently appears as a way of controlling the geometry of self-representation. Elastic Net Subspace Clustering solves, for each Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)8,

Ln(w)=(1/n)i(yi,w,xi)L_n(w)= (1/n)\sum_i \ell(y_i,\langle w,x_i\rangle)9

and its geometric analysis introduces the oracle point

x=Vkyx=V_k\,y00

and the oracle region

x=Vkyx=V_k\,y01

As x=Vkyx=V_k\,y02 the spherical caps shrink and promote subspace preservation; as x=Vkyx=V_k\,y03 they expand and improve within-subspace connectivity. The ORGEN active-set method exploits this structure and is stated to scale to x=Vkyx=V_k\,y04 up to x=Vkyx=V_k\,y05 points on synthetic data, with orders-of-magnitude speed-up over APG and ADMM (You et al., 2016).

A complementary line of work derives closed-form solutions for rank/norm regularized subspace clustering. Under the noiseless independent-subspace setting, the unique minimizer of

x=Vkyx=V_k\,y06

for any unitarily invariant norm is

x=Vkyx=V_k\,y07

the shape interaction matrix. In noisy settings, discrete and continuous shrinkage variants produce one-SVD algorithms such as DSSIM, CSSIM, and SSIM, and the detailed summary reports average accuracy around x=Vkyx=V_k\,y08–x=Vkyx=V_k\,y09 on Hopkins155 with two to three orders of magnitude speed-up relative to iterative low-rank solvers (Yu et al., 2012). Laplacian regularized low rank subspace clustering adds a graph penalty

x=Vkyx=V_k\,y10

to low-rank self-expressiveness, so that

x=Vkyx=V_k\,y11

The reported result is better subspace clustering results with lower clustering error than traditional low rank representation, low rank subspace clustering, and several other state-of-the-art subspace clustering models on Extended Yale B, USPS, and MNIST (Song et al., 2016).

In incremental learning, subspace regularization is used directly as a prior on classifier weights. For few-shot class incremental learning, the old class weights define

x=Vkyx=V_k\,y12

and new class weights are penalized by their squared distance to this span,

x=Vkyx=V_k\,y13

The paper argues that ordinary logistic regression with this penalty, combined with pretrained convolutional feature extractors, outperforms specialized few-shot incremental methods by up to x=Vkyx=V_k\,y14 on miniImageNet, and the detailed results report weighted average accuracies such as x=Vkyx=V_k\,y15 for fine-tuning plus subspace regularization and x=Vkyx=V_k\,y16 for semantic regularization in the last multi-session miniImageNet session, against x=Vkyx=V_k\,y17 for FT+memory (Akyürek et al., 2021).

In PEFT for LLMs, Controlled LoRA introduces a null-space constraint on the low-rank update x=Vkyx=V_k\,y18. If x=Vkyx=V_k\,y19 spans a trusted subspace, the regularizer on x=Vkyx=V_k\,y20 is

x=Vkyx=V_k\,y21

and similarly for x=Vkyx=V_k\,y22, leading to

x=Vkyx=V_k\,y23

The paper states that CLoRA aims to reduce the scale of output change while introduce minimal constraint on model capacity, and the reported commonsense results give in-domain average accuracy x=Vkyx=V_k\,y24 for CLoRA against x=Vkyx=V_k\,y25 for LoRA, with out-domain average accuracy x=Vkyx=V_k\,y26 for CLoRA against x=Vkyx=V_k\,y27 for LoRA and x=Vkyx=V_k\,y28 for the untuned base model (Lu et al., 2024).

A world-model analogue appears in Sub-JEPA, where Gaussian constraints are imposed in multiple random subspaces rather than in the original embedding space. With random orthonormal projectors x=Vkyx=V_k\,y29, latent tensors are projected as

x=Vkyx=V_k\,y30

and Gaussianity is penalized by an averaged Epps–Pulley statistic over random one-dimensional directions,

x=Vkyx=V_k\,y31

The paper explicitly frames the method as seeking a favorable operating point on the bias-variance frontier, and reports planning success gains over LeWM on all four environments: x=Vkyx=V_k\,y32 versus x=Vkyx=V_k\,y33 on Two-Room, x=Vkyx=V_k\,y34 versus x=Vkyx=V_k\,y35 on Reacher, x=Vkyx=V_k\,y36 versus x=Vkyx=V_k\,y37 on PushT, and x=Vkyx=V_k\,y38 versus x=Vkyx=V_k\,y39 on OGB-Cube (Zhao et al., 10 May 2026).

6. Coefficient-space regularization in hyperspectral imaging and recurring trade-offs

Hyperspectral image super-resolution provides a particularly clear example of subspace regularization in coefficient form. In the convex formulation of hyperspectral superresolution, the high-resolution HSI is written as

x=Vkyx=V_k\,y40

with x=Vkyx=V_k\,y41 a basis spanning the signal subspace and x=Vkyx=V_k\,y42 the low-dimensional coefficients. The estimation problem becomes

x=Vkyx=V_k\,y43

The vector-TV penalty enforces piecewise smoothness jointly across spectral bands, and ADMM/SALSA operates on x=Vkyx=V_k\,y44 arrays instead of x=Vkyx=V_k\,y45, reducing memory and per-iteration cost by a factor x=Vkyx=V_k\,y46. The detailed summary states that with x=Vkyx=V_k\,y47–x=Vkyx=V_k\,y48 versus x=Vkyx=V_k\,y49–x=Vkyx=V_k\,y50, the method yields a dramatic speedup and attains the lowest ERGAS, highest UIQI, and best spectral fidelity (SAM) among the compared methods (Simões et al., 2014).

A tensor generalization appears in JLRST, which factorizes the HR-HSI as

x=Vkyx=V_k\,y51

with x=Vkyx=V_k\,y52 a spectral basis and x=Vkyx=V_k\,y53 a coefficient tensor. The regularizer acts on clustered coefficient tensors through multi-mode gradients,

x=Vkyx=V_k\,y54

where the mode-3 logarithmic tensor nuclear norm is

x=Vkyx=V_k\,y55

The paper states that by enforcing priors on subspace coefficients rather than the entire HR-HSI data, the proposed method achieves improved computational efficiency and accuracy, and reports CPU times of x=Vkyx=V_k\,y56–x=Vkyx=V_k\,y57 s, compared to x=Vkyx=V_k\,y58–x=Vkyx=V_k\,y59 s for other high-accuracy tensor approaches, together with consistently highest PSNR and UIQI and lowest ERGAS and SAM across four datasets (Zhang et al., 5 Aug 2025).

Taken together, these works show that subspace regularization is not a single technique but a recurring structural strategy. The literature repeatedly frames it as a trade-off: computational savings versus learning accuracy in random-subspace ERM (Vecchia et al., 2022); subspace-preserving affinity versus connectivity in elastic-net clustering (You et al., 2016); model capacity versus degree of forgetting in CLoRA (Lu et al., 2024); and bias versus variance in Sub-JEPA (Zhao et al., 10 May 2026). This suggests that the central design question is not whether to regularize by a subspace, but which subspace to use, how to generate it, and whether the method should impose a hard restriction, a projection, or a soft penalty.

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