Polarization of the microwave background in inflationary cosmology
We evaluate the large scale polarization of the cosmic microwave background induced, via Thomson scattering prior to decoupling, by nearly scale-invariant spectra of scalar and tensor metric perturbations, such as those predicted by most inflationary models of the early Universe. We solve the radiat...
| Autores principales: | Harari, D.D., Zaldarriaga, M. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03702693_v319_n1-3_p96_Harari |
| Aporte de: |
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