Abstract

Modern neural networks (NNs) often do not generalize well in the presence of a ‘covariate shift’; that is, in situations where the training and test data distributions differ, but the conditional distribution of classification labels given the data remains unchanged. In such cases, NN generalization can be reduced to a problem of learning more robust, domain-invariant features. Domain adaptation (DA) methods include a broad range of techniques aimed at achieving this; however, these methods have struggled with the need for extensive hyperparameter tuning, which then incurs significant computational costs. In this work, we introduce SInkhorn Dynamic Domain Adaptation (SIDDA), an out-of-the-box DA training algorithm built upon the Sinkhorn divergence, that can achieve effective domain alignment with minimal hyperparameter tuning and computational overhead. We demonstrate the efficacy of our method on multiple simulated and real datasets of varying complexity, including simple shapes, handwritten digits, real astronomical observations, and remote sensing data. These datasets exhibit covariate shifts due to noise, blurring, differences between telescopes, and variations in imaging wavelengths. SIDDA is compatible with a variety of NN architectures, and it works particularly well in improving classification accuracy and model calibration when paired with symmetry-aware equivariant NNs (ENNs). We find that SIDDA consistently enhances the generalization capabilities of NNs, achieving up to a 40% improvement in classification accuracy on unlabeled target data, while also providing a more modest performance gain of 1% on labeled source data. We also study the efficacy of DA on ENNs with respect to the varying group orders of the dihedral group DN, and find that the model performance improves as the degree of equivariance increases. Finally, if SIDDA achieves proper domain alignment, it also enhances model calibration on both source and target data, with the most significant gains in the unlabeled target domain—achieving over an order of magnitude improvement in the expected calibration error and Brier score. SIDDA’s versatility across various NN models and datasets, combined with its automated approach to domain alignment, has the potential to significantly advance multi-dataset studies by enabling the development of highly generalizable models.

Details

Title
SIDDA: SInkhorn Dynamic Domain Adaptation for image classification with equivariant neural networks
Author
Pandya, Sneh 1   VIAFID ORCID Logo  ; Patel, Purvik 2 ; Nord, Brian D 3   VIAFID ORCID Logo  ; Walmsley, Mike 4 ; Ćiprijanović, Aleksandra 5   VIAFID ORCID Logo 

 Department of Physics, Northeastern University , Boston, MA, 02115, United States of America; NSF AI Institute for Artificial Intelligence & Fundamental Interactions (IAIFI) , Cambridge, MA, 02139, United States of America; Fermi National Accelerator Laboratory , Batavia, IL, 60510, United States of America 
 Khoury College of Computer Science, Northeastern University , Boston, MA, 02115, United States of America 
 Fermi National Accelerator Laboratory , Batavia, IL, 60510, United States of America; Department of Astronomy and Astrophysics, University of Chicago , Chicago, IL, 60637, United States of America; Kavli Institute for Cosmological Physics, University of Chicago , Chicago, IL, 60637, United States of America 
 Dunlap Institute for Astronomy & Astrophysics, University of Toronto , Toronto, ON M5S 3H4, Canada; Jodrell Bank Centre for Astrophysics, Department of Physics & Astronomy, University of Manchester , Manchester M13 9PL, United Kingdom 
 Fermi National Accelerator Laboratory , Batavia, IL, 60510, United States of America; Department of Astronomy and Astrophysics, University of Chicago , Chicago, IL, 60637, United States of America; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut St., Chicago, IL 60611, United States of America 
First page
035032
Publication year
2025
Publication date
Sep 2025
Publisher
IOP Publishing
e-ISSN
26322153
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3239775380
Copyright
© 2025 The Author(s) and Fermi Forward Discovery Group, LLC. Published by IOP Publishing Ltd. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.