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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. Magic number (physics) - Wikipedia

    en.wikipedia.org/wiki/Magic_number_(physics)

    Alpha decay (the emission of a 4 He nucleus – also known as an alpha particle – by a heavy element undergoing radioactive decay) is common in part due to the extraordinary stability of helium-4, which makes this type of decay energetically favored in most heavy nuclei over neutron emission, proton emission or any other type of cluster decay.

  4. Roton - Wikipedia

    en.wikipedia.org/wiki/Roton

    In theoretical physics, a roton is an elementary excitation, or quasiparticle, seen in superfluid helium-4 and Bose–Einstein condensates with long-range dipolar interactions or spin-orbit coupling. The dispersion relation of elementary excitations in this superfluid shows a linear increase from the origin, but exhibits first a maximum and ...

  5. Helion (chemistry) - Wikipedia

    en.wikipedia.org/wiki/Helion_(chemistry)

    The term helion is a portmanteau of helium and ion, and in practice refers specifically to the nucleus of the helium-3 isotope, consisting of two protons and one neutron. The nucleus of the other (and far more common) stable isotope of helium, helium-4, consisting of two protons and two neutrons, is called an alpha particle or an alpha for short.

  6. Proton–proton chain - Wikipedia

    en.wikipedia.org/wiki/Proton–proton_chain

    Once the helium-3 has been produced, there are four possible paths to generate 4 He. In p–p I, helium-4 is produced by fusing two helium-3 nuclei; the p–p II and p–p III branches fuse 3 He with pre-existing 4 He to form beryllium-7, which undergoes further reactions to produce two helium-4 nuclei. About 99% of the energy output of the sun ...

  7. Superfluid helium-4 - Wikipedia

    en.wikipedia.org/wiki/Superfluid_helium-4

    This condensation occurs in liquid helium-4 at a far higher temperature (2.17 K) than it does in helium-3 (2.5 mK) because each atom of helium-4 is a boson particle, by virtue of its zero spin. Helium-3, however, is a fermion particle, which can form bosons only by pairing with itself at much lower temperatures, in a weaker process that is ...

  8. File:Phase diagram of Helium-4-en.svg - Wikipedia

    en.wikipedia.org/wiki/File:Phase_diagram_of...

    This file contains additional information, probably added from the digital camera or scanner used to create or digitize it. If the file has been modified from its original state, some details may not fully reflect the modified file.

  9. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    Helium-4 is produced by alpha-decay, and the helium trapped in Earth's crust is also mostly non-primordial. In other types of radioactive decay, such as cluster decay , larger species of nuclei are ejected (for example, neon-20), and these eventually become newly formed stable atoms.