CPLUOS Astrophysics team meeting
Monday 25 Oct 2021, 16:30
→
17:55
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
COSMOLOGY
1
Dr.Sangnam Park's Report - FDM_Offset
Speaker
:
Sangnam Park
2
Hyeonmo's report - CDM Halo Evolution for Gadget2 Simulation
Minutes
Speaker
:
Hyeonmo Koo
(
University of Seoul
)
CDM Halo Evolution for Gadget2 Simulation
Position-box - velocity graph
Set M = 50
Peak = X-axis 33 position-box
M = 50
➝ 18 ~ 25
M = 30 ➝ (18 ~ 25)(5/3)
M = 40 ➝ Initial velocity increases more than when M = 50.
3
Young's report. FoF and MST algorithm
Minutes
Speaker
:
Young Ju
FoF and MST algorithm
Number density : Add 5000 noise data, minimum member = 50
Radius : 3
σ = 30, ρ = N/((4π/3)(σ^3))
Cluster id - ρ graph
MGS's ρ is bigger than MST's ρ.
The mean of ρ is about 0.0018.
Number density : Add 5000 noise data
True density (from random) VS Recovered density (from MGS)
True density - Recovered density graph
The mean increases proportionally.
Number density 2 : Add 5000 noise data, minimum member = 3
The number of galaxies in cluster VS The number of clusters.
Number of galaxies - Number of Clusters graph
The number of Number of clusters in MGS is about twice as high as the number of Number of clusters in MST.
4
CHOA(Cosmology of High-Order Statistics)
Speaker
:
Sumi Kim
(
University of Seoul
)
5
Dr.Sabiu's Report
Speaker
:
Dr
Cristiano Sabiu
(
University of Seoul
)
6
Discussion