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Uncertainty Estimation by Density Aware Evidential Deep Learning

ICML 2024 · Label-efficient and robust learning › OOD and anomaly detection · approach: Uncertainty and misclassification detection · 2 citations (OpenAlex)

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Proposes DAEDL, which multiplies EDL logits by a GDA-based normalized feature-space density and uses an exponential activation with no "1" prior term, improving OOD detection, classification, and calibration.

Problem

Evidential deep learning (EDL) fails to reflect distance from training data when quantifying uncertainty, hurting OOD detection, and its parameterization limits classification accuracy.

Approach

Integrate a normalized Gaussian discriminant analysis feature-space density of the test example with EDL logits at prediction time, and replace the conventional parameterization (alpha = 1 + ReLU(logits)) with alpha = exp(logits), which removes the uniform prior term and aligns expected class probabilities with softmax; spectral normalization is added to keep feature distances meaningful.

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Use DAEDL instead of I-EDLOOD detection · MNIST → KMNIST and MNIST → FMNISTAUPR: improvements of 1.56, 1.59, 0.94, and 1.01Helped
Use DAEDL instead of I-EDLOOD detection · CIFAR-10 → SVHN and CIFAR-10 → CIFAR-100AUPR: improvements of 2.24, 2.58, 2.81, and 3.35Helped
Use DAEDL instead of the strongest baselineCIFAR-10 classification and confidence calibration · CIFAR-10test accuracy, AUPR, and Brier score: 1.91; 0.36; 8.57Helped
Use DAEDL instead of MSPdistribution shift detection · MNIST-CAUPR: +6.37Helped
Use DAEDL instead of MSPdistribution shift detection · CIFAR-10-C severity levels 1–5AUPR: +1.50, +1.35, +1.67, +2.30, and +2.73Helped
Add EXP (alternative exponential parameterization) to EDL (ablation)EDL · CIFAR-10test accuracy: 83.55 $\pm$ 0.6 -> 88.59 $\pm$ 0.4Helped
Add EXP to EDL (ablation)EDL · CIFAR-10AUPR (misclassified image detection): 97.86 $\pm$ 0.2 -> 98.42 $\pm$ 0.1Helped
Add feature-space density integration (DE) to EXP (ablation)DAEDL without spectral normalization · CIFAR-10AUPR (misclassified image detection): 98.42 $\pm$ 0.1 -> 99.01 $\pm$ 0.0Helped
Add DE to EXP (ablation)DAEDL without spectral normalization · CIFAR-10 → SVHNAUPR (aleatoric): 80.39 $\pm$ 2.0 -> 85.02 $\pm$ 0.7Helped
Add spectral normalization (SN) to EXP (ablation)DAEDL without density integration · CIFAR-10test accuracy: 88.59 $\pm$ 0.4 -> 91.11 $\pm$ 0.2Helped
Add SN to EXP (ablation)DAEDL without density integration · CIFAR-10 → SVHNAUPR (aleatoric): 80.39 $\pm$ 2.0 -> 84.53 $\pm$ 0.9Helped
Add DE to EXP + SN (ablation)DAEDL · CIFAR-10test accuracy: 91.11 $\pm$ 0.2 -> 91.11 $\pm$ 0.2No clear effect

Surprising findings

Limitations

Experimental setup

Datasets: MNIST CIFAR-10 FMNIST KMNIST SVHN CIFAR-100 MNIST-C CIFAR-10-C

Benchmarks: MNIST CIFAR-10 FMNIST KMNIST SVHN CIFAR-100 MNIST-C CIFAR-10-C

Metrics: AUPR AUROC test accuracy Brier score

Baselines: Dropout KL-PN RKL-PN PostNet EDL I-EDL MSP

Builds on: evidential deep learning posterior network I-EDL spectral normalization

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