Recent breakthroughs in radiance fields, particularly 3D Gaussian Splatting (3DGS), have unlocked real-time, high-quality rendering of complex environments, enabling a wide range of applications. However, the stringent requirements of mixed reality (MR) rendering, such as rapid refresh rates, high-resolution stereo viewing, and constrained computing budgets, remain out of reach for current 3DGS techniques. Nevertheless, the wide field-of-view design of MR displays, which mimics human vision, presents a unique opportunity to exploit human visual system’s own perceptual limitations to reduce computational overhead while not compromising user-perceived rendering quality.To this end, we propose a perception-guided, continuous level-of-detail (LOD) framework for 3DGS that maximizes perceived quality under given compute resources. We distill a visual quality metric, which encodes the spatial, temporal, and peripheral characteristics of human visual perception, into a lightweight, gaze-contingent model that predicts and adaptively modulates rendering LOD across the visual field based on each region’s contributions to perceptual quality. This budget-driven LOD modulation, guided by both scene content and gaze behavior, enables significant computation reduction with minimal loss in perceived quality. To support low-power, untethered MR setups, we design an edge-cloud collaborative rendering framework to partially offload computation to the cloud, further reducing overhead on the edge MR devices. Objective metrics and MR user study evidence that, compared to vanilla and foveated LOD baselines, our method achieves superior trade-offs between computational efficiency and user-perceived visual quality.

Neural Radiance Fields (NeRF) show impressive performances in photo-realistic free-view rendering of scenes. Recent improvements such as TensoRF and ZipNeRF employ explicit models for faster optimization and rendering. However, all these radiance fields require a dense sampling of images in the given scene for effective training. Their performances degrade significantly when only a sparse set of views is available. Existing depth priors used to supervise the radiance fields are either sparse or suffer from generalization issues. We seek to learn scene-specific dense depth priors to regularize the radiance fields. Further, we desire a framework of regularizations that can work across different radiance field models. We observe that certain features of the radiance fields, such as positional encoding, number of decomposed tensor components or size of the hash table, cause overfitting in the sparse-input scenario. We design augmented models by reducing the capacity of these features and train them along with the main radiance field. These augmented models learn simpler solutions, which estimate better depth in certain regions. By supervising the main radiance field with such depths, we significantly improve the performance of the radiance fields on popular forward-facing and 360ˆ datasets by employing the above regularization.