. Nuclei in this "iron peak" (notably and Nickel-62 ) are the most tightly bound and stable in the universe.
), indicating that nuclear forces are "saturated" in mid-sized nuclei.
) . It illustrates the stability of atomic nuclei and explains why certain nuclear reactions—like fusion and fission—release energy. Peak Stability: The curve peaks around a mass number of to
. Nuclei in this "iron peak" (notably and Nickel-62 ) are the most tightly bound and stable in the universe.
), indicating that nuclear forces are "saturated" in mid-sized nuclei.
) . It illustrates the stability of atomic nuclei and explains why certain nuclear reactions—like fusion and fission—release energy. Peak Stability: The curve peaks around a mass number of to
