Slide 1 Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute 84.5% of the total matter in the universe – and…
Formation and structure of dark matter halos in N-body and SPH simulations Wei-Peng Lin The Partner Group of MPI for Astrophysics, Shanghai Astronomical Observatory, CAS,…
Science Case for Multi-object High Resolution Spectroscopy at Keck Science Case for Multi-object High Resolution Spectroscopy at Keck R. Michael Rich (UCLA) Judy Cohen (Caltech)…
Dark Matter Detection PHY 210 project Spring 2007 Bogdan, Doug, Jay and Ragnhild The idea WIMPs (Weakly Interacting Massive Particles) are hypothetical particles that offer…
Grand Unified Theory, Running Coupling Constants and the Universe Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute…