Recombination (cosmology)

In cosmology, recombination refers to the epoch during which charged electrons and protons first became bound to form electrically neutral hydrogen atoms. Recombination occurred about 378000 years after the Big Bang (at a redshift of z = 1100).

Source: Wikipedia — Recombination (cosmology) (CC BY-SA 4.0)

Recombination (cosmology)

In cosmology, recombination refers to the epoch during which charged electrons and protons first became bound to form electrically neutral hydrogen atoms. Recombination occurred about 378000 years after the Big Bang (at a redshift of z = 1100).

Source: Wikipedia "Recombination (cosmology)" · CC BY-SA 4.0

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