Homepage of the Cryogenic Dark Matter Search experiment at the University of California, Berkeley. The experiment uses a large germanium crystal cooled to 20 mK to search for weakly interacting, massive particles (WIMPs) - proposed constituents of dark matter.

Summary of the properties of dark matter, its influence on cosmic evolution, and the different ways it can be detected. Suitable for a general audience; by Chris Miller.

Homepage of the CRESST experiment (Cryogenic Rare Event Search with Superconducting Thermometers), a European collaboration to search for particle constituents of dark matter in the Gran Sasso laboratories.

Homepage of the DArk MAtter experiment, which uses low-activity scintillator to search for particle constituents of dark matter in the Gran Sasso laboratories. Includes information about the experiment itself, members of the collaboration, results, and publications.

Description of dark matter, its properties and consequences. Includes texts, plots, graphs and schematics. By Martin White (University of California, Berkeley).

Discusses the theory that Brownian motion can be applied on a galactic scale and that the results suggest that dark satellite galaxies should exist. Includes an animated simulation.

Elementary introduction to dark matter, suitable for a general audience. The pages are part of the public outreach effort of the Chandra X-Ray Observatory, and hosted by Harvard University.

A review of the methods and findings of searches for particle constituents of nonbaryonic dark matter. Requires some previous knowledge of particle physics and cosmology. By Bernard Sadoulet (Lawrence Berkeley National Laboratory and University of California, Berkeley). [PDF]

Transcript of an on-air discussion between physicists Michio Kaku and Stuart Samuel on the subject of dark matter. Suitable for a general audience. Aired on WBAI's "Explorations in Science" on December 3, 1997.

Article about the discovery of, and early research on, dark matter by Zwicky, Smith, Babcock and Oort in the 1930's and 1940's. By Sidney van den Bergh (Dominion Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada).