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- W2964154920 abstract "We present a brief review of the polarization properties of the cosmic microwave background in dark matter models for structure formation. Quite independently of the model parameters, the polarization level is expected to be similar to 10% Of the anisotropy signal at angular scales less than or equal to 1 degrees. Detections of polarization at larger angular scales would provide strong evidence in favour of an early reionization of the intergalactic medium." @default.
- W2964154920 created "2019-07-30" @default.
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- W2964154920 date "1996-01-01" @default.
- W2964154920 modified "2023-09-28" @default.
- W2964154920 title "Polarization of the microwave background: Theoretical framework" @default.
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