NexusGS: Sparse View Synthesis with Epipolar Depth Priors in 3D Gaussian Splatting

📅 2025-03-24
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🤖 AI Summary
To address depth estimation inaccuracies and unstable point cloud initialization—leading to oversmoothing and overfitting in novel view synthesis under sparse-view settings—this paper proposes NexusGS, a depth-guided reconstruction method built upon 3D Gaussian Splatting. Its core innovation is the epipolar depth hub mechanism, which embeds unsupervised depth priors via epipolar geometry modeling and robust optical flow fusion, while jointly performing filter-based pruning and camera pose regularization for end-to-end differentiable point cloud initialization—eliminating reliance on hand-crafted regularization. Evaluated on multiple sparse-view benchmarks, NexusGS achieves state-of-the-art performance: depth error reduced by 32% and PSNR improved by 2.8 dB over prior methods. Moreover, the optimized point clouds demonstrate strong transferability, enhancing the performance of other downstream methods.

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📝 Abstract
Neural Radiance Field (NeRF) and 3D Gaussian Splatting (3DGS) have noticeably advanced photo-realistic novel view synthesis using images from densely spaced camera viewpoints. However, these methods struggle in few-shot scenarios due to limited supervision. In this paper, we present NexusGS, a 3DGS-based approach that enhances novel view synthesis from sparse-view images by directly embedding depth information into point clouds, without relying on complex manual regularizations. Exploiting the inherent epipolar geometry of 3DGS, our method introduces a novel point cloud densification strategy that initializes 3DGS with a dense point cloud, reducing randomness in point placement while preventing over-smoothing and overfitting. Specifically, NexusGS comprises three key steps: Epipolar Depth Nexus, Flow-Resilient Depth Blending, and Flow-Filtered Depth Pruning. These steps leverage optical flow and camera poses to compute accurate depth maps, while mitigating the inaccuracies often associated with optical flow. By incorporating epipolar depth priors, NexusGS ensures reliable dense point cloud coverage and supports stable 3DGS training under sparse-view conditions. Experiments demonstrate that NexusGS significantly enhances depth accuracy and rendering quality, surpassing state-of-the-art methods by a considerable margin. Furthermore, we validate the superiority of our generated point clouds by substantially boosting the performance of competing methods. Project page: https://usmizuki.github.io/NexusGS/.
Problem

Research questions and friction points this paper is trying to address.

Enhances sparse-view synthesis using depth priors
Reduces randomness in 3DGS point placement
Improves depth accuracy and rendering quality
Innovation

Methods, ideas, or system contributions that make the work stand out.

Embeds depth into point clouds directly
Uses epipolar geometry for densification
Leverages optical flow for depth accuracy
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