2020-08-012024-05-13https://scholars.lib.ntu.edu.tw/handle/123456789/652803摘要：傳統冷暗物質(cold dark matter)在矮星系尺度與觀測不符，而波暗物質(wave dark matter)的量子特性有助解決此問題。本計畫將利用超高解析度之三維動態電腦模擬，以期了解在波暗物質架構下的星系演化過程，並與觀測作定量比較。此外，我們會將電腦模擬的原始程式和分析資料直接與學界分享，以促進科學可重復性和資料再利用。<br> Abstract: The conventional particle interpretation of cold dark matter (CDM) still lacks laboratory support and struggles to explain the basic properties of dwarf galaxies. This tension motivates wave dark matter (ψDM) composed of extremely light bosons, which suppresses structure below the kilo-parsec scale by the uncertainty principle but retains the large-scale structure predicted by CDM. In this project, we will conduct three-dimensional genuine ψDM simulations with an unprecedented high resolution capable of resolving dwarf galaxies. The aim is to identify unique and distinguishable properties of ψDM that can be directly tested by observations. We will also construct and release a ψDM halo catalog covering the mass range 10^8–10^12 solar mass to both foster scientific reproducibility and provide opportunities for other groups to re-analyze or explore the rich datasets generated by this project in new ways.暗物質數值模擬高效能運算dark matternumerical simulationhigh-performance computing