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matter era
(recombination era, decoupling era)
subjectfact 
matter erahas duration > 1010 years2001-09-27 09:29:58.0
has synonym recombination era2001-09-27 09:29:58.0
has synonym decoupling era2001-09-27 09:29:58.0
is preceded by radiation era2001-09-27 09:29:58.0
has start time 1012 s2001-09-27 09:29:58.0
has temperature 3 K to 3000 K2001-09-27 09:29:58.0
has definition The Big Bang era when the temperature had dropped to 3000 K, at which time the recombination of hydrogen became possible. The plasma of free electrons and nuclei condensed to form a neutral gas. Matter and radiation consequently decouple from one another because no further scattering of the radiation occurs.has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:58.0
has definition Separation of classes of particles from regular interaction with one another, as in the decoupling of photons from particles of matter that produced the cosmic background radiation.has source: Ferris, T. 1988 Coming of Age in the Milky Way, Morrow, 2001-09-27 09:29:58.0
has definition The rapid transition from an ionized state at a redshift of 1000, when the blackbody radiation is scattered by the free electrons, to an unionized state, when the matter is predominantly in the form of hydrogen atoms that do not scatter the radiation appreciably. Radiation subsequently does not interact with matter unless the matter becomes reionized at a later epoch by radiation from quasars or forming galaxies.has source: Silk, J. 1990 The Big Bang, W. H. Publishers, New York, 2001-09-27 09:29:58.0
has definition The epoch at t ≈ 1013 s after the big bang (T ≈ 3000 K) when matter and radiation decoupled.has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:58.0
has definition The era some 3 × 105 years after the Big Bang when the cosmic blackbody radiation was last scattered by the matter. At this era, at a redshift of about 1,000 and a temperature of about 3,000 K, the protons and electrons combined to form hydrogen atoms, which are effectively transparent to the radiation.has source: Silk, J. 1990 The Big Bang, W. H. Publishers, New York, 2001-09-27 09:29:58.0
has definition A cosmic epoch during which the matter content of the Universe ceased to be ionized. This led to a decrease in the optical depth of the Universe, and the photons of radiation (which we now observe as the cosmic microwave background) became able to travel large distances without interacting with matter.has source: Clark, S. 1997 Towards the Edge of the Universe, Wiley, 2001-09-27 09:29:58.0
has definition The release of photons from constant collisions with massive particles as the universe expanded and its matter density diminished. See decoupling.has source: Ferris, T. 1988 Coming of Age in the Milky Way, Morrow, 2001-09-27 09:29:58.0
is a kind of Big Bang era2001-09-27 09:29:58.0
Big Bang erais followed by2001-09-27 09:29:57.0
eventhas time of occurrence2001-09-27 09:29:57.0

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