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  2. Helium-4 - Wikipedia

    en.wikipedia.org/wiki/Helium-4

    The stability of helium-4 is the reason that hydrogen is converted to helium-4, and not deuterium (hydrogen-2) or helium-3 or other heavier elements during fusion reactions in the Sun. It is also partly responsible for the alpha particle being by far the most common type of baryonic particle to be ejected from an atomic nucleus; in other words ...

  3. Triple-alpha process - Wikipedia

    en.wikipedia.org/wiki/Triple-alpha_process

    Nuclear fusion reaction of two helium-4 nuclei produces beryllium-8, which is highly unstable, and decays back into smaller nuclei with a half-life of 8.19 × 10 −17 s, unless within that time a third alpha particle fuses with the beryllium-8 nucleus [3] to produce an excited resonance state of carbon-12, [4] called the Hoyle state, which ...

  4. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    An exception to this general trend is the helium-4 nucleus, whose binding energy is higher than that ... Because nuclear reaction rates depend on density as well as ...

  5. Nuclear reaction - Wikipedia

    en.wikipedia.org/wiki/Nuclear_reaction

    In a nuclear reaction, the total (relativistic) energy is conserved. The "missing" rest mass must therefore reappear as kinetic energy released in the reaction; its source is the nuclear binding energy. Using Einstein's mass-energy equivalence formula E = mc 2, the amount of energy released can be determined.

  6. Nuclear binding energy - Wikipedia

    en.wikipedia.org/wiki/Nuclear_binding_energy

    The binding energy of helium is the energy source of the Sun and of most stars. [12] The sun is composed of 74 percent hydrogen (measured by mass), an element having a nucleus consisting of a single proton. Energy is released in the Sun when 4 protons combine into a helium nucleus, a process in which two of them are also converted to neutrons. [11]

  7. Alpha decay - Wikipedia

    en.wikipedia.org/wiki/Alpha_decay

    It has a charge of +2 e and a mass of 4 Da. For example, uranium-238 decays to form thorium-234. While alpha particles have a charge +2 e, this is not usually shown because a nuclear equation describes a nuclear reaction without considering the electrons – a convention that does not imply that the nuclei necessarily occur in neutral atoms.

  8. Big Bang nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Big_Bang_nucleosynthesis

    Almost all neutrons that fused instead of decaying ended up combined into helium-4, due to the fact that helium-4 has the highest binding energy per nucleon among light elements. This predicts that about 8% of all atoms should be helium-4, leading to a mass fraction of helium-4 of about 25%, which is in line with observations.

  9. Beryllium-8 - Wikipedia

    en.wikipedia.org/wiki/Beryllium-8

    The nucleus of helium-4 is particularly stable, having a doubly magic configuration and larger binding energy per nucleon than 8 Be. As the total energy of 8 Be is greater than that of two alpha particles, the decay into two alpha particles is energetically favorable, [5] and the synthesis of 8 Be from two 4 He nuclei is endothermic