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  2. Syncytium - Wikipedia

    en.wikipedia.org/wiki/Syncytium

    A classic example of a syncytium is the formation of skeletal muscle.Large skeletal muscle fibers form by the fusion of thousands of individual muscle cells. The multinucleated arrangement is important in pathologic states such as myopathy, where focal necrosis (death) of a portion of a skeletal muscle fiber does not result in necrosis of the adjacent sections of that same skeletal muscle ...

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

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

    Advances in the potential energy source may not be about electricity, at least at first.

  4. To-day and To-morrow - Wikipedia

    en.wikipedia.org/wiki/To-day_and_To-morrow

    To-day and To-morrow (sometimes written Today and Tomorrow) was a series of 110 [citation needed] speculative essays published as short books by the London publishers Kegan Paul between 1923 and 1931 (and published in the United States by E. P. Dutton, New York). [1] As Fredric Warburg proudly recalled in 1959: It was a unique publishing event.

  5. Cell fusion - Wikipedia

    en.wikipedia.org/wiki/Cell_fusion

    Cell fusion is an important cellular process in which several uninucleate cells (cells with a single nucleus) combine to form a multinucleate cell, known as a syncytium.Cell fusion occurs during differentiation of myoblasts, osteoclasts and trophoblasts, during embryogenesis, and morphogenesis. [1]

  6. Muon-catalyzed fusion - Wikipedia

    en.wikipedia.org/wiki/Muon-catalyzed_fusion

    Muon-catalyzed fusion (abbreviated as μCF or MCF) is a process allowing nuclear fusion to take place at temperatures significantly lower than the temperatures required for thermonuclear fusion, even at room temperature or lower. It is one of the few known ways of catalyzing nuclear fusion reactions.

  7. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released. A nuclear fusion process that produces atomic nuclei lighter than iron-56 or nickel-62 will generally release energy.

  8. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    The CNO cycle (for carbon–nitrogen–oxygen; sometimes called Bethe–Weizsäcker cycle after Hans Albrecht Bethe and Carl Friedrich von Weizsäcker) is one of the two known sets of fusion reactions by which stars convert hydrogen to helium, the other being the proton–proton chain reaction (p–p cycle), which is more efficient at the Sun's ...

  9. Superheavy element - Wikipedia

    en.wikipedia.org/wiki/Superheavy_element

    Large changes are expected to occur in the subshell structure in going from element 120 to element 121: for example, the radius of the 5g orbitals should drop drastically, from 25 Bohr units in element 120 in the excited [Og] 5g 1 8s 1 configuration to 0.8 Bohr units in element 121 in the excited [Og] 5g 1 7d 1 8s 1 configuration, in a ...

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