Physics
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..marb31003t&link_type=abstract
American Physical Society, Annual APS March Meeting 2003, March 3-7, 2003, , abstract #B31.003
Physics
Scientific paper
There is considerable observational evidence that most of the mass detected gravitationally in large-scale structure is non-baryonic. We explore the astrophysical dark matter problem and analyze some of the solutions provided by theoretical particle physics. We critique the cold dark matter (CDM) theory and its two most popular dark matter candidates, the axion and the lightest supersymmetric partner (LSP). We constrain their masses using data from recent collider experiments. Finally, we discuss future experimental work that could find evidence of CDM particles and potentially resolve the dark matter problem.
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