Cosmology with Large scale structure using Machine Learning(CLML)
- Ω_m, σ_8 → 512_short
- 1116 data
- Lines and histograms are inversely proportional.
- Dark matter halos : Agglomeration of particles, Processed information
- Dark matter particles : Initial number of particles setting, Original information
- Add mass information
- Add velocity information
- Can cosmological parameters be determined as input data?