| | |
Summary: I. Basic Cosmology
Elements
I. Aretxaga
Jan 2008
Cosmological Principle
"The Universe is homogeneous and isotropic on large-scales"
As can be seen by the position of extragalactic radio-sources
(From R. Bender's notes)
Cosmological Principle
"The Universe is homogeneous and isotropic on large-scales"
As can be seen by Cosmic Microwave Background (CMB) radiation
(From R. Bender's notes)
Cosmological Principle
"The Universe is homogeneous and isotropic on large-scales"
As can be seen by the 2-point correlation function of galaxies, which are clustered
in scales of few x h-1 Mpc.
Other LSS scales: supercluster associations ~ 100 h-1 Mpc
filaments ~ 100 250 h-1 Mpc
voids ~ 60 h-1 Mpc
There is a characteristic scale 300 h-1 Mpc ! l ! cH0
|