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Non-parametric Representation Learning with Kernels

AAAI 2024 · Label-efficient and robust learning › Self-supervised and contrastive · approach: Invariance-based self-supervised learning · 3 citations (OpenAlex)

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Introduces kernel versions of contrastive self-supervised learning (simple and spectral contrastive losses) and a kernel autoencoder, with new representer theorems and generalisation bounds, evaluated on small datasets against kernel PCA and neural networks.

Problem

Representation learning has been dominated by neural networks; non-parametric kernel methods for self-supervised and reconstruction-based representation learning are largely unexplored, especially in small-data regimes.

Approach

Kernelize a single hidden layer for contrastive (simple and spectral) losses and an autoencoder, prove representer theorems (including under orthonormality constraints) showing learned embeddings can be written via kernel matrices, and derive generalisation bounds for these kernel models.

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Use a learned kernel representation instead of the original featuresKernel representation learning with k-NN · Circles, Cubes, Iris, and IonosphereaccuracyHelped
Use the proposed kernel representation methods instead of Kernel PCAKernel representation learning · Circles, Cubes, Iris, and Ionosphereclassification performanceNo clear effect
Use kernel representation learning instead of a one-hidden-layer neural network representationKernel representation learning · CIFAR-10 and MNIST (first two classes; n=500)classification performanceNo clear effect
Use Kernel AE instead of neural network AEKernel AE · MNIST, CIFAR-10, and SVHN denoisingmean squared errorHelped
Increase the number of unlabelled datapointsKernel representation learning · Circles (linear and ReLU kernels)accuracyHelped

Surprising findings

Limitations

Experimental setup

Datasets: concentric circles cubes Iris Ionosphere CIFAR-10 MNIST SVHN

Benchmarks: concentric circles cubes Iris Ionosphere MNIST CIFAR-10 SVHN

Metrics: k-NN classification accuracy mean squared error on denoising test set

Baselines: Kernel PCA k-nearest neighbours on original features neural network contrastive model neural network autoencoder

Builds on: kernel PCA spectral contrastive loss neural tangent kernel representer theorem

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