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  2. Helium dimer - Wikipedia

    en.wikipedia.org/wiki/Helium_dimer

    Based on molecular orbital theory, He 2 should not exist, and a chemical bond cannot form between the atoms. However, the van der Waals force exists between helium atoms as shown by the existence of liquid helium, and at a certain range of distances between atoms the attraction exceeds the repulsion.

  3. Isotopes of helium - Wikipedia

    en.wikipedia.org/wiki/Isotopes_of_helium

    In Earth's atmosphere, the ratio of 3 He to 4 He is 1.343(13) × 10 −6. [5] However, the isotopic abundance of helium varies greatly depending on its origin. In the Local Interstellar Cloud , the proportion of 3 He to 4 He is 1.62(29) × 10 −4 , [ 6 ] which is ~121 times higher than in Earth's atmosphere.

  4. Lambda point - Wikipedia

    en.wikipedia.org/wiki/Lambda_point

    The point's name derives from the graph (pictured) that results from plotting the specific heat capacity as a function of temperature (for a given pressure in the above range, in the example shown, at 1 atmosphere), which resembles the Greek letter lambda. The specific heat capacity has a sharp peak as the temperature approaches the lambda point.

  5. Helium - Wikipedia

    en.wikipedia.org/wiki/Helium

    [132] [133] The concentration is low and fairly constant despite the continuous production of new helium because most helium in the Earth's atmosphere escapes into space by several processes. [134] [135] [136] In the Earth's heterosphere, a part of the upper atmosphere, helium and hydrogen are the most abundant elements.

  6. Helium compounds - Wikipedia

    en.wikipedia.org/wiki/Helium_compounds

    Noble gas cluster ions exist for different noble gases. Singly charged cluster ions containing xenon exist with the formula He n Xe + m, where n and m ≥ 1. [74] Many different He n Kr + exist with n between 1 and 17, with higher values possible. He n Kr + 2 and He n Kr + 3 also exist for many values of n.

  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. Molecular orbital - Wikipedia

    en.wikipedia.org/wiki/Molecular_orbital

    The advantage of this approach is that the orbitals will correspond more closely to the "bonds" of a molecule as depicted by a Lewis structure. As a disadvantage, the energy levels of these localized orbitals no longer have physical meaning. (The discussion in the rest of this article will focus on canonical molecular orbitals.

  9. Diatomic molecule - Wikipedia

    en.wikipedia.org/wiki/Diatomic_molecule

    About 99% of the Earth's atmosphere is composed of two species of diatomic molecules: nitrogen (78%) and oxygen (21%). The natural abundance of hydrogen (H 2) in the Earth's atmosphere is only of the order of parts per million, but H 2 is the most abundant diatomic molecule in the universe. The interstellar medium is dominated by hydrogen atoms.