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  2. Unbinilium - Wikipedia

    en.wikipedia.org/wiki/Unbinilium

    The team studied the nuclear fusion reaction between uranium ions and a target of natural nickel: [91] [92] 238 92 U + nat 28 Ni → 296,298,299,300,302 120 Ubn * → fission. The results indicated that nuclei of unbinilium were produced at high (~70 MeV) excitation energy which underwent fission with measurable half-lives just over 10 −18 s.

  3. Isotopes of unbinilium - Wikipedia

    en.wikipedia.org/wiki/Isotopes_of_unbinilium

    Jens Volker Kratz predicted the actual maximum cross section for producing unbinilium by any of the four reactions 238 U+ 64 Ni, 244 Pu+ 58 Fe, 248 Cm+ 54 Cr, or 249 Cf+ 50 Ti to be around 0.1 fb; [21] in comparison, the world record for the smallest cross section of a successful reaction was 30 fb for the reaction 209 Bi(70 Zn,n) 278 Nh, [11 ...

  4. Unbihexium - Wikipedia

    en.wikipedia.org/wiki/Unbihexium

    It has been suggested that fusion-evaporation will not be feasible to reach unbihexium. As 48 Ca cannot be used for synthesis of elements beyond atomic number 118 or possibly 119, the only alternatives are increasing the atomic number of the projectile or studying symmetric or near-symmetric reactions. [70]

  5. AI solves nuclear fusion puzzle for near-limitless clean energy

    www.aol.com/news/ai-solves-nuclear-fusion-puzzle...

    Nuclear fusion breakthough overcomes key barrier to grid-scale adoption

  6. Explained: What nuclear fusion breakthrough means [Video] - AOL

    www.aol.com/news/nuclear-fusion-could-change...

    Fusion, on the other hand, does not create any long-lived radioactive nuclear waste.” The waste byproduct of a fusion reaction is far less radioactive than in fission, and decays far more ...

  7. Extended periodic table - Wikipedia

    en.wikipedia.org/wiki/Extended_periodic_table

    The reaction between 254 Es and 48 Ca would be superior, but preparing milligram quantities of 254 Es for a target is difficult.) [28] Nevertheless, the necessary change from the "silver bullet" 48 Ca to 50 Ti divides the expected yield of element 119 by about twenty, as the yield is strongly dependent on the asymmetry of the fusion reaction. [28]

  8. The Hope and Hype of Fusion Energy, Explained - AOL

    www.aol.com/news/hope-hype-fusion-energy...

    Fusion power is viewed as more dependable than wind and solar power; relatively clean, as fossil fuel power is certainly not; and lacking the hazardous waste and uncontrolled reaction risks of ...

  9. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The reaction rate density between species A and B, having number densities n A,B, is given by: = where k is the reaction rate constant of each single elementary binary reaction composing the nuclear fusion process: = here, σ(v) is the cross-section at relative velocity v, and averaging is performed over all velocities.