Astrofisica

CMB Secondary Anisotropies due to Galaxy Clusters

Name: CMB Secondary Anisotropies due to Galaxy Clusters
Start: 2008-06-19T15:00:00+02:00
End: 2008-06-19T17:00:00+02:00
Location: Dip. di Fisica - Edificio E. Fermi

by Nabila Aghanim (IAS (Institut d’Astrophysique Spatiale) – Centre universitaire d’Orsay - Paris-Orasy - France)

Thursday 19 Jun 2008, 15:00 → 17:00 Europe/Rome

Aula 3 (Dip. di Fisica - Edificio E. Fermi)

Aula 3

Dip. di Fisica - Edificio E. Fermi

Description

Cosmic Microwave Background Secondary Anisotropies are becoming more and more important for future CMB experiments as they contribute to the both polarisation and temperature anisotropies at small angular scales. I will present some of the issues associated with the dominant secondary anistropies.