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  2. r-process - Wikipedia

    en.wikipedia.org/wiki/R-process

    The r-process can typically synthesize the heaviest four isotopes of every heavy element; of these, the heavier two are called r-only nuclei because they are created exclusively via the r-process. Abundance peaks for the r -process occur near mass numbers A = 82 (elements Se, Br, and Kr), A = 130 (elements Te, I, and Xe) and A = 196 (elements ...

  3. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    This first process, Big Bang nucleosynthesis, was the first type of nucleogenesis to occur in the universe, creating the so-called primordial elements. A star formed in the early universe produces heavier elements by combining its lighter nuclei – hydrogen , helium , lithium, beryllium , and boron – which were found in the initial ...

  4. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The alpha process; Fusion of heavier elements: Lithium burning: a process found most commonly in brown dwarfs; Carbon-burning process; Neon-burning process; Oxygen-burning process; Silicon-burning process; Production of elements heavier than iron: Neutron capture: The r-process; The s-process; Proton capture: The rp-process; The p-process ...

  5. Scientists discovered a method to create element 116 using a titanium beam, paving the way for future synthesis of element 120, the "holy grail" of chemistry.

  6. 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 ...

  7. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    All of the elements heavier than iron have some potential energy to release, in theory. At the extremely heavy end of element production, these heavier elements can produce energy in the process of being split again back toward the size of iron, in the process of nuclear fission.

  8. Neutron capture - Wikipedia

    en.wikipedia.org/wiki/Neutron_capture

    In this process, the mass number increases by one. This is written as a formula in the form 197 Au + n → 198 Au + γ, or in short form 197 Au(n,γ) 198 Au. If thermal neutrons are used, the process is called thermal capture. The isotope 198 Au is a beta emitter that decays into the mercury isotope 198 Hg. In this process, the atomic number ...

  9. Alpha process - Wikipedia

    en.wikipedia.org/wiki/Alpha_process

    Creation of elements beyond carbon through alpha process. The alpha process, also known as alpha capture or the alpha ladder, is one of two classes of nuclear fusion reactions by which stars convert helium into heavier elements. The other class is a cycle of reactions called the triple-alpha process, which consumes only helium, and produces ...