How is Thomson scattering responsible for the CMB polarization?
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Due to Thomson scatterings in the early Universe, the CMB is predicted to be polarized at the level of roughly 5%5% of its temperature anisotropies.
Physically, how did the Thomson scattering of photons with the thermal plasma (consisting of charged particles such as electrons and protons) polarized the CMB
Physically, how did the Thomson scattering of photons with the thermal plasma (consisting of charged particles such as electrons and protons) polarized the CMB
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scalar field is responsible for the exponential expansion of the universe at the very early ...... CMB polarization via Thomson scattering of the local quadrupole of the
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