Supplemental Material

Astrophysics, abstract
astro-ph/9912211

From: Mike Turner <mturner@oddjob.uchicago.edu>
Date: Thu, 9 Dec 1999 22:48:30 GMT (82kb)

Dark Matter, Dark Energy and Fundamental Physics

Author: Michael S. Turner
Comments: 15 pages LaTeX with 6 eps figures. To be published in The Proceedings of Physics in Collision (Ann Arbor, MI, 24 - 26 June 1999), edited by M. Campbell and T.M. Wells(World Scientific, NJ)

More than sixty years ago Zwicky made the case that the great clusters of galaxies are held together by the gravitational force of unseen (dark) matter. Today, the case is stronger and more precise: Dark, nonbaryonic matter accounts for 30% +/- 7% of the critical mass density, with baryons (most of which are dark) contributing only 4.5% +/- 0.5% of the critical density. The large-scale structure that exists in the Universe indicates that the bulk of the nonbaryonic dark matter must be cold (slowly moving particles). The SuperKamiokande detection of neutrino oscillations shows that particle dark matter exists, crossing an important threshold. Over the past few years a case has developed for a dark-energy problem. This dark component contributes about 80% +/- 20% of the critical density and is characterized by very negative pressure (p_X < -0.6 rho_X). Consistent with this picture of dark energy and dark matter are measurements of CMB anisotropy that indicate that total contribution of matter and energy is within 10% of the critical density. Fundamental physics beyond the standard model is implicated in both the dark matter and dark energy puzzles: new fundamental particles (e.g., axion or neutralino) and new forms of relativistic energy (e.g., vacuum energy or a light scalar field). A flood of observations will shed light on the dark side of the Universe over the next two decades; as it does it will advance our understanding of the Universe and the laws of physics that govern it.

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