Can we test cosmic homogeneity and isotropy?
Dr. Jenny Wagner, 2024-03-19
Galaxy & Cosmology Seminar
https://astro.tsinghua.edu.cn/info/1120/2798.htm
Introduction
simple Friedmann equation at 0-rd level.
boundary condition

- [ ] average against GR?
- define homogeneity and isotropy

clever option 2!
nowadays idea: op3.
Test of cosmic homogeneity and isotropy

possible tensions between observation and theory?
Matter test

- arc distrubution of GRB, galaxy.
Matter 2: do we have a peculiar velocity?
right fig: degenaracy between the peculiar velocity and hubble flow.

Matter 3: CMB dipole v.s. cosmic matter dipole 

- radio galaxies from NVSS, 2.7 sigma
- ~million quasars from WISE, 4.4 sigma
- (wait for 5 sigma)
- possible solution:
- see the redshift evolution?

Space-time test
- uniqueness of Friedmann model parameters
- Hubble tension

- curvature test

general comments
fitting problem in cosmology 
Summary

data-driven era now!
Shu-Hu