CPLUOS Astrophysics team meeting

Asia/Seoul
물리학과

물리학과

Zoom Meeting https://uos-ac-kr.zoom.us/j/8264902652 Meeting ID: 826 490 2652
Description

https://uos-ac-kr.zoom.us/j/8264902652

    • 16:30 17:30
      COSMOLOGY
      • 16:30
        Hyeonmo's report - FDM vs CDM Halo Collision 10m
        Speaker: Hyeonmo Koo (University of Seoul)
      • 16:40
        Young's report. FoF and MST algorithm 10m
        Speaker: Young Ju
      • 16:50
        CHOA(Cosmology of High-Order Statistics) 10m
        Speaker: Sumi Kim (University of Seoul)
      • 17:00
        CLML 10m

        Cosmology with Large scale structure using Machine Learning

        Speaker: Se Yeon Hwang

        CLML(Cosmology with Large scale structure using Machine Learning)

        • Outlook
          • Started on the machine learning!(arXIv : 1908.10590) which is using 3d convolution network
            • input(3d density field of dark matter halo) → CNN CNN CNN Fully connected Fully connected Fully connected → output(Ω_m, σ_8 → Cosmological parameter)
        • Data
          • xyz position of dark matter halo
            • Box size = 256(Mpc/h)
            • Number of particles = 256^3
          • 3d histogram of 32 voxels(density field)
            • 1 voxel have 8(Mpc/h) information
        • Change for the data
          • 128
            • Boxsize = 256(Mpc/h)
            • Number of particles = 128^3
          • 256
            • Boxsize = 256(Mpc/h)
            • Number of particles = 256^3
          • 512
            • Boxsize = 256(Mpc/h)
            • Number of particles = 512^3
        • Data
          • Number of halo
            • The number of halo(128) : 9225
            • The number of halo(256) : 74646
            • The number of halo(512) : 504649
          • Halo mass
            • Ω_m = 0.33, σ_8 = 0.62
            • ρ = N(↑)*M(↓)/V
          • 1 voxel have 2(Mpc/h) information using 32 voxel(then one side should be 64(Mpc/h)
            • Short version
              • Only using 0(Mpc/h) < x, y, z < 64 (Mpc/h)
              • Including only 0~64 information
            • Cut version
              • At each side : [0, 64] [64, 128] [128, 192] [192 256] >> 32 voxel histogram
              • Including all information of the box scale
              • Total 64(4^3) for one cosmology
        • Data set
          • 128_short, 256_short, 512_short, 128_cut, 256_cut, 512_cut
        • Model
          • Model 1
          • Model 2
          • Model 3
          • Model 4
        • Conclusion
          • Don't sure about what is going on.
          • There are possibility of my mistakes + possibility of different results each time when run it even
          • Used same model and same data(I have to check)
        • Next step
          • Wil try running with different cosmology + same seed
          • Also, have to understand about mathematics on how each layer works
      • 17:10
        Hannah's Report - Weak Lensing with Machine Learning 10m
        Speaker: Hannah Jhee (University of Seoul)
      • 17:20
        Dr.Sabiu's Report - N-PCF 10m
        Speaker: Dr Cristiano Sabiu (University of Seoul)
    • 17:30 17:40
      Discussion 10m