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23 Nov 2019
In the early universe, free electrons and nuclei combined toform nuetral hydrogen and helium when the temperature dropped toapproximately 3,000K. Nuetral matter scatters radiation much lessthan charged particles do; therefore, the then-existing blackbodyradiation could subsequently expand freely, uncoupled to matter (togood approximation). By what factor has the "colume of theuniverse" increased since the ionization in space dropped toessentially zero?
Please help! You'll be a lifesaver!
In the early universe, free electrons and nuclei combined toform nuetral hydrogen and helium when the temperature dropped toapproximately 3,000K. Nuetral matter scatters radiation much lessthan charged particles do; therefore, the then-existing blackbodyradiation could subsequently expand freely, uncoupled to matter (togood approximation). By what factor has the "colume of theuniverse" increased since the ionization in space dropped toessentially zero?
Please help! You'll be a lifesaver!