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slides - Physics and Astronomy - University of Mississippi

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Sound waves <strong>and</strong> dark matter<br />

Anisotropy lead to<br />

clustering <strong>of</strong><br />

matter<br />

(galaxy clusters)<br />

Baryon acoustic<br />

oscillation peak<br />

Cosmological<br />

model fits help<br />

determine ratio <strong>of</strong><br />

baryonic to dark<br />

matter<br />

Eisenstein <strong>and</strong> Bennett, <strong>Physics</strong> Today, April 2008<br />

Ω ~ 1:5<br />

Dark matter:<br />

unknown structure, immune to light, but has mass.<br />

The <strong>University</strong> <strong>of</strong><br />

<strong>Mississippi</strong><br />

THE UNIVERSITY OF MISSISSIPPI<br />

Institute for Advanced<br />

Education in Geospatial<br />

Science<br />

J.R. Gladden

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