k Triple alpha nuclear fusion The triplealpha process is a set of nuclear fusion reactions by which three helium4 nuclei alpha particles are transformed into carbon. The triple alpha process is highly dependent on carbon12 and beryllium8 having resonances with the same energy as helium4, and before 1952, no such energy levels were known. Because the triplealpha process is unlikely, it needs a long time to produce much carbon. One consequence of this is that no significant amount of carbon was produced in the Big Bang because within minutes after the Big Bang, the temperature fell below the critical point for nuclear fusion. This creates a situation in which stellar nucleosynthesis produces large amounts of carbon and oxygen but only a small fraction of these elements is converted into neon and heavier elements. Stock Photo - Afloimages
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Triple alpha nuclear fusion The triple alpha process is a set of nuclear fusion reactions by which three helium 4 nuclei  alpha particles  are transformed into carbon. The triple alpha process is highly dependent on carbon 12 and beryllium 8 having resonances with the same energy as helium 4, and before 1952, no such energy levels were known. Because the triple alpha process is unlikely, it needs a long time to produce much carbon. One consequence of this is that no significant amount of carbon was produced in the Big Bang because within minutes after the Big Bang, the temperature fell below the critical point for nuclear fusion. This creates a situation in which stellar nucleosynthesis produces large amounts of carbon and oxygen but only a small fraction of these elements is converted into neon and heavier elements.
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Triple alpha nuclear fusion

The triple-alpha process is a set of nuclear fusion reactions by which three helium-4 nuclei (alpha particles) are transformed into carbon. The triple alpha process is highly dependent on carbon-12 and beryllium-8 having resonances with the same energy as helium-4, and before 1952, no such energy levels were known. Because the triple-alpha process is unlikely, it needs a long time to produce much carbon. One consequence of this is that no significant amount of carbon was produced in the Big Bang because within minutes after the Big Bang, the temperature fell below the critical point for nuclear fusion. This creates a situation in which stellar nucleosynthesis produces large amounts of carbon and oxygen but only a small fraction of these elements is converted into neon and heavier elements.

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