Optimization of the Array Configuration for HUNT

The High-energy Underwater Neutrino Telescope (HUNT) is a proposed next-generation neutrino observatory with an instrumented volume of approximately 30 cubic kilometers. Its primary goal is to detect neutrino emissions from PeV cosmic-ray accelerators and identify dozens of high-energy neutrino sources within a ten-year observation period. We explore a multi-cluster design for HUNT, optimizing the array geometry by varying parameters such as cluster radius, height, and number of clusters to maximize the discovery potential for point-like neutrino sources at energies above tens of TeV.