linkedin post 2022-01-27 05:38:55

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PHOTONS EXCEED BARYONS. “The present day photon number density is nγ,0 = 4.1×10(8) m(-3), which is roughly nine orders of magnitude greater than the present day baryon number density; the fact that there is a huge number of photons for every baryon has consequences for the thermal history of the Universe.” https://lnkd.in/e6ifiQMn View in LinkedIn
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linkedin post 2022-01-28 05:33:52

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“FIGURE 1: Evolution of the log of the density of the universe, ε, with the log of the scale factor, a. The universe starts off radiation dominated (red line), becomes matter dominated (blue) and then at late times is dominated by the cosmological constant (burgundy).” https://lnkd.in/e6ifiQMn View in LinkedIn
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linkedin post 2022-01-28 05:37:27

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Early cosmos. “The Universe is composed of nuclei and electrons, and photons scatter frequently off these charged particles. As the Universe expands and cools the energy of the photons drops and atoms form. This process is known as recombination and occurs at t ∼ 0.25 Myr.” https://lnkd.in/e6ifiQMn View in LinkedIn
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linkedin post 2022-01-28 05:39:13

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A LITTLE LATER. “The Universe becomes neutral and photons stop scattering and subsequently free-stream through the Universe. This process is known as decoupling and occurs at t ∼ 0.37Myr. The resulting Cosmic Microwave Background has a black body spectrum with present day temperature.” https://lnkd.in/e6ifiQMn View in LinkedIn
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