Where the Dark Matter is ... and Isn't

Physics

Scientific paper

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Scientific paper

Observations of the cosmic microwave background combined with large redshift surveys suggest that Ωm ~ 0.3. Direct dynamical measurements combined with estimated of the universal luminosity density suggest Ωm = 0.1 - 0.2. The apparent discrepancy may result from variations in the dark matter fraction with mass and scale. Traditional techniques already indicate that these variations are present. Gravitational lensing maps combined with large redshift surveys promise to measure the dark matter distribution. The Hectopsec Survey of a field in the Deep Lens Survey is a first approach to this kind of measurement.

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