... WMAP and other constraints. (0.094 < 0 h2 < 0.129) 1 Cornell LC Workshop July 2003 19 David Strom UO ~ · Detection of of and ... WMAP 0.15 0. 1 0.05 0 80 100 120 140 m(slepton) 160 180 200 WMAP makes a very precise prediction for mslepton Cornell LC ...
... Hence, the expected temperature anisotropy at the surface of last scattering is 1/40000 = 2.5 x 10 -5 which is consistent with the WMAP observations. ...
... then all the luminous matter seen in galaxies contributes only 0.5% of the mass required to eventually halt the expansion (note that the recent WMAP results have substantially lowered the amount of dark matter required to reach a flat/critical Universe ...
... 0.7 - 2 · 10-7 1 - 5 · 10-7 BABAR or Belle B ( , , ) PDG2004 B (µ e ) < 1.2 · 10-11 PDG2004 B (µ eee) < 1.0 · 10-12 < 0.129 WMAP C D M h2 [0, 40 · 10-9 ] g-2 with ahadr from e+ e- + - , aµ µ not neglecting data [-0.0022, 0.0017] 3 , PDG2004 B (b s ) [2.2 ...