CMB anisotropies induced by seeds versus inflationary perturbations: Comparing theoretical predictions to observational data

Details CMB anisotropies induced by seeds versus inflationary perturbations: Comparing theoretical predictions to observational data CMB anisotropies induced by seeds versus inflationary perturbations: Comparing theoretical predictions to observational data

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.577s&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We calculate the angular power spectra of cosmic microwave background anisotropies induced by active perturbations and compare them to perturbations of quantum origin generated during an inflationary era. We confront the theoretical predictions to current measurements of the CMB, in order to discriminate among the various models which could address the origin of the large scale structure in the universe.

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