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Progress of Theoretical Physics
Vol. 16 No. 6 (1956) pp. 613-624
URL : http://ptp.ipap.jp/link?PTP/16/613/
DOI : 10.1143/PTP.16.613

Formation of Light Nuclei in the Expanding Universe

Chushiro Hayashi and Minoru Nishida

Department of Physics, Kyoto University, Kyoto

(Received September 4, 1956)

The building up of light nuclei up to Ne20 out of intial protons and neutrons in the early stage of the expanding universe is studied, taking account of the α-capture reactions. If we take the matter density ρm=106∼107 g/cm3 at T=1010 °K, we can obtain the relative abundance of hydrogen, helium and oxygen, consistent with present observation. The possibility of forming heavier nuclei is discussed.


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References:

  1. See, for example, R. A. Alpher and R. C. Herman, Rev. Mod. Phys. 22 (1950), 153[APS].
  2. E. Fermi and A. Turkevich, see ref. (1).
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  11. V. L. Ginzburg, Dokl. Akad. Nauk U.S.S.R. 92 (1953), 727; Usp. Fiz. Nauk. 51 (1953), 343; Izv. Acad. Nauk. U.S.S.R. 20 (1955), 5.
  12. S. Hayakawa and Y. Terashima, private communication.

Citing Article(s) :

  1. Progress of Theoretical Physics Vol. 38 No. 5 (1967) pp. 1083-1094 :
    Formation of Li, Be, B in the Expanding Hot Universe
    Humitaka Satō

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