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...

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Detalles Bibliográficos
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
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