Cosmologists refer to the time period when neutral atoms first formed as the recombination epoch, and the event shortly afterwards when photons started to travel freely through space is referred to as photon decoupling. Unlike the plasma, these newly conceived atoms could not scatter the thermal radiation by Thomson scattering, and so the universe became transparent. When the temperature had dropped enough, protons and electrons combined to form neutral hydrogen atoms. As the universe expanded the plasma grew cooler and the radiation filling it expanded to longer wavelengths. When the universe was young, before the formation of stars and planets, it was denser, much hotter, and filled with an opaque fog of hydrogen plasma. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s, and earned the discoverers the 1978 Nobel Prize in Physics.ĬMB is landmark evidence of the Big Bang origin of the universe.
This glow is strongest in the microwave region of the radio spectrum. However, a sufficiently sensitive radio telescope shows a faint background brightness, or glow, almost uniform, that is not associated with any star, galaxy, or other object. With a traditional optical telescope, the space between stars and galaxies (the background) is completely dark (see: Olbers' paradox).
It is an important source of data on the early universe because it is the oldest electromagnetic radiation in the universe, dating to the epoch of recombination when the first atoms were formed. The CMB is faint cosmic background radiation filling all space. In Big Bang cosmology the cosmic microwave background ( CMB, CMBR) is electromagnetic radiation that is a remnant from an early stage of the universe, also known as "relic radiation".
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