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Recombination of the Primeval Plasma

Peebles, P. J. E.·1968·The Astrophysical Journal

Abstract

A theory is presented for the plasma recombination that would have taken place when the Universe had expanded and cooled to a Primeval Fireball temperature of about 4000° K. The computed residual ionization of the hydrogen following this recombination is in the range of 2 X 1O~ to 2 X 10~, depend- ing on the assumed cosmological model. In the closed cosmological model the matter temperature would have effectively decoupled from the radiation at a temperature of 12000 K, while in the lowest density model the matter temperature would not have fallen much below the radiation temperature before the galaxies formed. Also computed is the effect of the recombination radiation on the spectrum of the Prime- val Fireball

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Metadata

Authors
Peebles, P. J. E.
Venue
The Astrophysical Journal
Published
1968-07
Volume
153
Pages
1
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1995962607
Cited by
672
References
0
FWCI
8.88
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Recombination of the Primeval Plasma. https://app.cochat.ai/papers/10.1086/149628
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Peebles, P. J. E. (1968). Recombination of the Primeval Plasma. The Astrophysical Journal. https://doi.org/10.1086/149628

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.