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  2. Fermium - Wikipedia

    en.wikipedia.org/wiki/Fermium

    Fermium is produced by the bombardment of lighter actinides with neutrons in a nuclear reactor. Fermium-257 is the heaviest isotope that is obtained via neutron capture, and can only be produced in picogram quantities.

  3. List of radioactive nuclides by half-life - Wikipedia

    en.wikipedia.org/wiki/List_of_radioactive...

    This is a list of radioactive nuclides (sometimes also called isotopes), ordered by half-life from shortest to longest, in seconds, minutes, hours, days and years. Current methods make it difficult to measure half-lives between approximately 10 −19 and 10 −10 seconds.

  4. Fermion - Wikipedia

    en.wikipedia.org/wiki/Fermion

    Suppose multiple fermions have the same spatial probability distribution, then, at least one property of each fermion, such as its spin, must be different. Fermions are usually associated with matter, whereas bosons are generally force carrier particles. However, in the current state of particle physics, the distinction between the two concepts ...

  5. r-process - Wikipedia

    en.wikipedia.org/wiki/R-process

    In nuclear astrophysics, the rapid neutron-capture process, also known as the r-process, is a set of nuclear reactions that is responsible for the creation of approximately half of the atomic nuclei heavier than iron, the "heavy elements", with the other half produced by the p-process and s-process.

  6. Francium - Wikipedia

    en.wikipedia.org/wiki/Francium

    Francium-223 is the most stable isotope, with a half-life of 21.8 minutes, [8] and it is highly unlikely that an isotope of francium with a longer half-life will ever be discovered or synthesized. [22] Francium-223 is a fifth product of the uranium-235 decay series as a daughter isotope of actinium-227; thorium-227 is the more common daughter. [23]

  7. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    That fusion process essentially shut down at about 20 minutes, due to drops in temperature and density as the universe continued to expand. This first process, Big Bang nucleosynthesis, was the first type of nucleogenesis to occur in the universe, creating the so-called primordial elements.

  8. Majorana fermion - Wikipedia

    en.wikipedia.org/wiki/Majorana_fermion

    [54] [55] This process is done by creating so called 'twist defects' in codes such as the toric code [56] which carry unpaired Majorana modes. [57] The Majoranas are then "braided" by being physically moved around each other in 2D sheets or networks of nanowires. [58] This braiding process forms a projective representation of the braid group. [59]

  9. Fermi gas - Wikipedia

    en.wikipedia.org/wiki/Fermi_gas

    The two particles of the same energy have spin 1 ⁄ 2 (spin up) or − 1 ⁄ 2 (spin down), leading to two states for each energy level. In the configuration for which the total energy is lowest (the ground state), all the energy levels up to n = N /2 are occupied and all the higher levels are empty.