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บรรทัด 38:
* Jedamzik, Karsten, "''[https://arxiv.org/abs/astro-ph/9805156v1 Non-Standard Big Bang Nucleosynthesis Scenarios]''". [[Max-Planck-Institut für Astrophysik]], Garching.
* Steigman, Gary, Primordial Nucleosynthesis: Successes And Challenges {{arxiv|astro-ph/0511534}}; Forensic Cosmology: Probing Baryons and Neutrinos With BBN and the CBR {{arxiv|hep-ph/0309347}}; and Big Bang Nucleosynthesis: Probing the First 20 Minutes {{arxiv|astro-ph/0307244}}
* R. A. Alpher, H. A. Bethe, G. Gamow, ''[http://prola.aps.org/abstract/PR/v73/i7/p803_1 The Origin of Chemical Elements] {{Webarchive|url=https://web.archive.org/web/20130207022355/http://prola.aps.org/abstract/PR/v73/i7/p803_1 |date=2013-02-07 }}'', ''Physical Review'' '''73''' (1948), 803. The so-called [[Alpher-Bethe-Gamow Paper|αβγ paper]], in which Alpher and Gamow suggested that the light elements were created by hydrogen ions capturing neutrons in the hot, dense early universe. Bethe's name was added for symmetry
* {{cite journal | last1 = Gamow | first1 = G. | year = 1948 | title = The Origin of Elements and the Separation of Galaxies | journal = Physical Review | volume = 74 | issue = 4| pages = 505–506 | doi=10.1103/physrev.74.505.2|bibcode = 1948PhRv...74..505G }} These two 1948 papers of Gamow laid the foundation for our present understanding of big-bang nucleosynthesis
* {{cite journal | last1 = Gamow | first1 = G. | year = 1948 | title = The Evolution of the Universe | journal = Nature | volume = 162 | issue = 4122| pages = 680–2 | doi=10.1038/162680a0|bibcode = 1948Natur.162..680G | pmid=18893719| s2cid = 4793163 }}
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