Doppler peaks from active perturbations
We examine how the qualitative structure of the Doppler peaks in the angular power spectrum of the cosmic microwave anisotropy depends on the fundamental nature of the perturbations which produced them. The formalism of Hu and Sugiyama is extended to treat models with cosmic defects. We discuss how...
| Main Authors: | , , , |
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| Format: | Journal article |
| Published: |
1995
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