CMB

The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?

 Comment: Galaxy formation (SAM model) permits so many free params, so not so good a tool to constrain cosmology.
The higher z data needs less input from the SAM model, maybe ,so better constain.

Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination( W.Hu 2008)

Authors: Wayne Hu (KICP, U. Chicago)

宇宙微波背景辐射的偏振(极化)

本文部分内容编译自Wayne Hu的CMB主页:

http://background.uchicago.edu/~whu/

http://background.uchicago.edu/~whu/polar/webversion/polar.html

这实际上为 Hu的一篇名为“a CMB polarization primer”的review

未经过管理员同意,请不要随便转载本文。

一、介绍

聚合内容