CMB Quadrupole induced polarisation from clusters and filaments
Astrophysics
2007-05-23 v1
Abstract
We present the estimates of the Cosmic Microwave Background (CMB) polarisation power spectrum from galaxy clusters and filaments using hydrodynamical simulations of large scale structure formation. We focus in the present study on the CMB Quadrupole induced polarisation, which is the dominate secondary polarisation effect, and give the E and B mode power spectra between to 20000.
Cite
@article{arxiv.astro-ph/0409297,
title = {CMB Quadrupole induced polarisation from clusters and filaments},
author = {Guo-Chin Liu and Antonio da Silva and Nabila Aghanim},
journal= {arXiv preprint arXiv:astro-ph/0409297},
year = {2007}
}
Comments
To appear in proceedings of the Moriond 2004 meeting