🤖 AI Summary
This work addresses the computational redundancy incurred in detecting cosmic web structures—such as filaments, walls, and clusters—in high-dimensional, noisy point clouds, particularly within dense hub regions. The authors propose a two-stage approach that first rapidly identifies and models these dense hubs, then integrates a likelihood-based model with a pheromone-guided strategy to enable agents to traverse congested areas efficiently. By introducing a hub-aware mechanism that uniquely combines biologically inspired search with probabilistic modeling, the method substantially reduces the computational overhead of the Locally Aligned Ant Technique (LAAT) in hub-dominated zones. Experiments demonstrate that the proposed framework significantly enhances both the efficiency and robustness of cosmic structure detection across synthetic datasets and large-scale cosmological N-body simulations.
📝 Abstract
Finding manifold structures in noisy and high-dimensional point clouds is a challenging but important problem. In astronomical observation survey and simulation data the detection of filaments, streams (1D), walls (2D) and clusters (3D) gives rise to deeper understanding of the evolution of our universe. The Locally Aligned Ant Technique (LAAT) uses biologically inspired agents to efficiently recover faint and multidimensional structures. However, very dense hubs (e.g. nodes or globular clusters) dominate the ants' activity, creating unnecessary computational overheads. In this paper we propose a two-stage solution. First a fast preprocessing step locates the hubs and replaces them with a tailored likelihood model. Subsequently, a mixed likelihood-pheromone strategy guides the ants to efficiently bridge the dense regions. We demonstrate improvements in detection efficiency and robustness of LAAT with synthetic and a large-scale astronomical N-body simulation of the cosmic web.