Analytic approach to the polarization of the cosmic microwave background in flat and open universes
We develop an analytic method and approximations to compute the polarization induced in the cosmic microwave background radiation on a wide range of angular scales by anisotropic Thomson scattering in the presence of adiabatic scalar (energy-density) linear fluctuations. The formalism is an extensio...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1995
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
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