Astroparticle Physics and the Dark Matter Question

Physics

Scientific paper

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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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