Doubt cast over dark energy?

Boud Roukema boud w
Wto, 16 Gru 2003, 15:44:03 CET

BTW, this stuff is highly important for OCRA analyses - whichever
way it works out.  We'll (hopefully) have lots of clusters and maybe
we'll use cosmology to understand cluster physics rather than the
other way around, but either way, getting all the bits of the puzzle
to be consistent is the challenge.

BTW(2) - Motyl proposes that we work on the grant proposal tomorrow
afternoon (Wed 17 Dec) @radio astronomy.


On Tue, 16 Dec 2003, Boud Roukema wrote:

> Niayesh Afshordi, Renyue Cen
> then the (1+z) factor becomes essentially (1+ not much) over the
> relevant redshift range.

> In other words, Blanchard et al's figures, with Afshordi & Cen's
> version of the T-M relation, give the concordance model.
> Again in simpler words, Blanchard et al think that clusters form
> in one way, Afshordi & Cen think they form in a somewhat different way,
> leading to moderately different T-M relations and hence totally different
> local curvature parameter inferences.

Więcej informacji o liście Cosmo-torun