Slides from the talk - CP3-Origins
Slides from the talk - CP3-Origins
Slides from the talk - CP3-Origins
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From <strong>the</strong> CMB to <strong>the</strong> Large-Scale Structure<br />
The CMB provides a snapshot of <strong>the</strong> Universe at<br />
very high redshift and its power spectrum<br />
(<strong>the</strong> Cl’s) is matched by linear predictions<br />
The observable Universe to <strong>the</strong><br />
CMB last scattering surface<br />
The Large-Scale Structure is <strong>the</strong> result<br />
of a highly nonlinear evolution, with<br />
different sources of non-Gaussianity<br />
How can we distinguish and detect<br />
<strong>the</strong> primordial component?<br />
Why bo<strong>the</strong>r at all?!<br />
The Sloan Digital Sky Survey<br />
(white dots are galaxies)
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