Synonyms
Definition
The nucleosynthetic process that took place within the first 20 min after the big bang is called big bang nucleosynthesis (BBN) or primordial nucleosynthesis. At this early epoch, the Universe was dense and hot enough to allow for nuclear reactions to take place, producing the “light elements,” 4He, 2H (≡D, i.e., deuterium), 3He, and 7Li, starting from neutrons and protons. The comparison between the primordial abundances of these isotopes deduced on one hand from observations and on the other hand from model calculations is one of the main support of the big bang model.
History
Prominent landmarks in the development of the big bang nucleosynthesis theory include works by Gamow in the 1940s (out of equilibrium nucleosynthesis in an expanding Universe dominated by radiation), Peebles in 1966 (big bang nucleosynthesis calculations up to 4He), and Wagoner in 1973 (big bang nucleosynthesis calculations including 7Li).
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References and Further Reading
Aghanim N et al (2020) Planck 2018 results. VI. Cosmological parameters. Astron Astrophys 641:A6. https://doi.org/10.1051/0004-6361/201833910
Aver E, Olive KA, Skillman ED (2015) The effects of He I λ10830 on helium abundance determinations. JCAP 7:011. https://doi.org/10.1088/1475-7516/2015/07/011
Bania TM, Rood RT, Balser DS (2002) The cosmological density of baryons from observations of 3He+ in the Milky Way. Nature 415:54–57. https://doi.org/10.1038/415054a
Coc A, Descouvemont P, Olive KA, Uzan JP, Vangioni E (2012) Variation of fundamental constants and the role of A = 5 and A = 8 nuclei on primordial nucleosynthesis. Phys Rev D 86:043529. https://doi.org/10.1103/PhysRevD.86.043529
Coc A, Uzan JP, Vangioni E (2014) Standard big bang nucleosynthesis and primordial CNO Abundances after Planck. JCAP 10:050. https://doi.org/10.1088/1475-7516/2014/10/050
Cooke RJ, Pettini M, Steidel CC (2018) One percent determination of the primordial deuterium abundance. Astrophys J 855:102. https://doi.org/10.3847/1538-4357/aaab53
Fields BD (2011) Annu Rev Nucl Part Sci 61:47–68. https://doi.org/10.1146/annurev-nucl-102010-130445
Fields BD, Olive KA, Yeh TH, Young C (2020) Big-Bang Nucleosynthesis after Planck. JCAP 03:010. https://doi.org/10.1088/1475-7516/2020/03/010
Iocco F, Mangano G, Miele G, Pisanti O, Serpico PD (2009) Primordial nucleosynthesis: from precision cosmology to fundamental physics. Phys Rep 472:1–76
Mossa V et al (2020) The baryon density of the Universe from an improved rate of deuterium burning. Nature 587:210–213. https://doi.org/10.1038/s41586-020-2878-4
Pitrou C, Coc A, Uzan JP, Vangioni E (2018) Precision big bang nucleosynthesis with improved Helium-4 predictions. Phys Rep 75:1–66. https://doi.org/10.1016/j.physrep.2018.04.005
Sbordone L et al (2010) The metal-poor end of the Spite plateau. I. Stellar parameters, metallicities, and lithium abundances. Astron Astrophys 522:A26. https://doi.org/10.1051/0004-6361/200913282
Further Reading
Gamow G (1948) The evolution of the universe. Nature 162:680–682. https://doi.org/10.1038/162680a0
Kolb EW & Turner MS (1994) Westview Press, Nashville, ISBN-13: 978-0201626742
Peebles PJE, Page LA Jr, Partrige RB (2009) Finding the Big Bang. Cambridge University Press, Cambridge, ISBN-13: 978-0521519823
Peebles PJE (1966) Primordial helium abundance and the primordial fireball. Astrophys J 146:542–552. https://doi.org/10.1086/148918
Wagoner RV (1973) Big-bang nucleosynthesis revisited. Astrophys J 179:343–360. https://doi.org/10.1086/151873
Weinberg S (2008) Cosmology. Oxford University Press, Oxford. ISBN-13: 978-0198526827
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Coc, A. (2021). Big Bang Nucleosynthesis. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_160-7
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DOI: https://doi.org/10.1007/978-3-642-27833-4_160-7
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DOI: https://doi.org/10.1007/978-3-642-27833-4_160-8
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