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  2. Superheavy element - Wikipedia

    en.wikipedia.org/wiki/Superheavy_element

    Superheavy elements, also known as transactinide elements, transactinides, or super-heavy elements, or superheavies for short, are the chemical elements with atomic number greater than 104. [1] The superheavy elements are those beyond the actinides in the periodic table; the last actinide is lawrencium (atomic number 103).

  3. Scientists discovered a method to create element 116 using a titanium beam, paving the way for future synthesis of element 120, ... If we can find stable super heavy elements, scientists may be ...

  4. Island of stability - Wikipedia

    en.wikipedia.org/wiki/Island_of_stability

    The process of slow neutron capture used to produce nuclides as heavy as 257 Fm is blocked by short-lived isotopes of fermium that undergo spontaneous fission (for example, 258 Fm has a half-life of 370 μs); this is known as the "fermium gap" and prevents the synthesis of heavier elements in such a reaction.

  5. Nine elements on periodic table have been discovered using ...

    www.aol.com/nine-elements-periodic-table...

    Carolyn Krause presents the second part of the three-part series on the Oak Ridge National Laboratory's role in the discovery of elements in the periodic table. Many of them have been synthesized ...

  6. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    Synthesis of these elements occurred through nuclear reactions involving the strong and weak interactions among nuclei, and called nuclear fusion (including both rapid and slow multiple neutron capture), and include also nuclear fission and radioactive decays such as beta decay. The stability of atomic nuclei of different sizes and composition ...

  7. Supernova nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Supernova_nucleosynthesis

    Supernova nucleosynthesis is the nucleosynthesis of chemical elements in supernova explosions.. In sufficiently massive stars, the nucleosynthesis by fusion of lighter elements into heavier ones occurs during sequential hydrostatic burning processes called helium burning, carbon burning, oxygen burning, and silicon burning, in which the byproducts of one nuclear fuel become, after ...

  8. File:Apparatus for creation of superheavy elements en.svg

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

    English: Apparatus for creation of superheavy elements, based on the Dubna Gas-Filled Recoil Separator set up in the en:Flerov Laboratory of Nuclear Reactions Date 29 January 2020

  9. Unbihexium - Wikipedia

    en.wikipedia.org/wiki/Unbihexium

    Unbihexium has attracted attention among nuclear physicists, especially in early predictions targeting properties of superheavy elements, for 126 may be a magic number of protons near the center of an island of stability, leading to longer half-lives, especially for 310 Ubh or 354 Ubh which may also have magic numbers of neutrons.