Using Galaxy Clusters for Cosmology and the XCS Ben Hoyle, Bob Nichol, David Bacon, Ed Lloyd-Davies, Kathy Romer & the XCS Cape Town April ‘08.
Improving mass and age estimates of unresolved stellar clusters Margaret Hanson & Bogdan Popescu Department of Physics.
Acceleration of Universe Background level Evolution of expansion: H(a), w(a) degeneracy: DE & MG Perturbation level Evolution of inhomogeneity:
Dark Matter! First clue came way back in the 1930’s. Fritz Zwicky studied the motions of galaxies in the Coma Cluster of galaxies – the nearest “relaxed”
Spacetime: just when you thought it was it throws you a.
J. Goodman – May 2003 Quarknet Symposium May 2003 Neutrinos, Dark Matter and the Cosmological Constant The Dark Side of the Universe Jordan Goodman University.
Finsler Geometry vs. phenomenological anomaly in ultra-high energy and large scale CHANG Zhe Institute of High Energy Physics Chinese Academy of Sciences.
Using Galaxy Clusters for Cosmology and the XCS
J. Goodman – May 2003 Ghosts in the Universe Jordan A. Goodman University of Maryland Fall 2003 The world we don’t see around us.
I. Experimental observations
