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<a accesskey="3" href="page.php?w=Big_Bang_nucleosynthesis&amp;p=2">3.Next</a>
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<p>In <a href="page.php?w=physical_cosmology">physical cosmology</a>, <b>Big Bang nucleosynthesis</b> (also known as <b>primordial nucleosynthesis</b>, and abbreviated as <b>BBN</b>) is a model for the production of light <a href="page.php?w=Atomic_nucleus">nuclei</a> (including, but not limited to, <a href="page.php?w=Deuterium"><sup>2</sup>H</a>, <sup>3</sup>He, <sup>4</sup>He, and <sup>7</sup>Li) during the first ~20 minutes of the evolution of the <a href="page.php?w=universe">universe</a>. The predictions of BBN rely on a combination of thermodynamic</p><p>
<a accesskey="3" href="page.php?w=Big_Bang_nucleosynthesis&amp;p=2">3.Next</a>
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