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What Was the Temperature of the Universe When a Typical λ\lambda

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What was the temperature of the universe when a typical CMB photon was no longer able to spontaneously create a proton and antiproton pair? Note that a photon has an energy equal to E = hc/ λ\lambda , the CBR at any point in time has a blackbody spectrum that peaks at λ\lambda peak = (2,900 μ\mu m K)/T, and the mass of a single proton is 1.7 *10-27 kg.


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