Accueil > Séminaires d’Astrophysique > Can LCDM cosmology explain clusters of galaxies ?

 

Can LCDM cosmology explain clusters of galaxies ?

Richard Lieu (Physics Department, University of Alabama, USA)

Par Stephane Charpinet - 21/05/2007

 

Séminaires d’Astrophysique

de l’Observatoire Midi-Pyrénées


Séminaire exceptionnel de

Richard LIEU

 (Physics Department, University of Alabama, USA)

Lundi 28 Mai 2007 à 11h

LATT - Salle Coriolis


Can LCDM cosmology explain clusters of galaxies ?

I will focus upon two observational properties of clusters, the `UV excess’ and the surprisingly low level of Sunyaev-Zel’dovich effect (SZE) in the WMAP data of a large sample of clusters. In this seminar I will argue that the two apparent diverse `anomalies’ of clusters might in fact have a common cause. Firstly, I present the evidence as to why, after more than a decade of research, the `UV excess’ in the core region of clusters is increasingly looking like a non-thermal phenomenon. Secondly, this power-law spectrum of emitted photons could account for a substantial fraction of the X-ray luminosity of some clusters, i.e. the actual amount of virialized thermal gas available for producing a SZE on the microwave background may be less than previously expected. I will then discuss the repercussions these aspects of cluster physics have on the standard LCDM cosmological model. If time permits, I will talk a bit about the origin of the non-thermal particles, and ways of testing the content and state of the near Universe by gravitational lensing (even on the 3rd CMB acoustic peak) and time delay observations.

 

 

[Page Précédente] [Dans la même rubrique] [Sommaire]

 

 

Site du CNRS Logo OMP
Logo UPS
Logo INSU-CNRS

Annuaire

Rechercher

Sur ce site



Bibliotheque

Laboratoire Astrophysique de Toulouse - Tarbes (UMR5572)

CNRS (Midi-Pyrénées)

Univ. Paul Sabatier

Liens utiles

Accueil Imprimer Contact mail Plan du site Crédits