在大尺度结构和暗物质的波动模式相演变分析程序

This project mainly focuses on the evolution of LSS and fluctuation of CDM especially at relatively low redshifts, where the non-gaussianity and mode-phase correlation occur as a result of gravitational non-linearity. Results from cosmological perturbation theory is adopted in the project to investigate the Fourier modes and phases, and updated programs contained in the project has realized some predictions by theories with the method of computation simulations. Either N-body simulation or SDSS can serve as data sources for the project.

Mandelbrot
m1
m2
m3
m4
m5
m6
m7