decoupling vâjafsari, vâjofteš Fr.: découplage Cosmology: In the early history of the Universe, separation of matter
and radiation due to their non-interaction. At a redshift of 1000, that is about 400,000
years after the Big Bang, the temperature would have cooled to the point (4000 degrees Kelvin)
where electrons and nuclei can recombine and form neutral hydrogen atoms. Since atoms do not
scatter the radiation appreciably, free electrons were lacking, and the Universe became
transparent to radiation. Same as → recombination. See also: Verbal noun of decouple, from → de- + → couple + → -ing. |