and are crucial processes in nuclear physics, explaining how excited nuclei release energy. These mechanisms showcase the interplay between nuclear and atomic physics, revealing the complex nature of radioactive decay.
Understanding these processes is essential for grasping the full picture of nuclear decay. They complement alpha and beta decay, providing insights into nuclear structure, energy levels, and the various ways atoms can shed excess energy.
Nuclear Excited States and Deexcitation
Nuclear Energy Levels and Transitions
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Nuclear excited states represent higher energy configurations of nucleons within an atomic nucleus
Excited nuclei possess excess energy above their
Energy levels in nuclei are quantized, similar to electron energy levels in atoms
Transitions between levels involve emission or absorption of energy
Isomeric transition occurs when a nucleus in a metastable state transitions to a lower energy state
Metastable states have longer lifetimes compared to typical excited states (ranging from nanoseconds to years)
Isomers are denoted with an "m" after the mass number (Technetium-99m)
Nuclear deexcitation involves the release of excess energy as the nucleus returns to its ground state
Can occur through various processes (gamma emission, internal conversion, pair production)
Energy conservation dictates that the energy released equals the difference between initial and final nuclear states
Mechanisms of Nuclear Deexcitation
Gamma decay serves as a primary mechanism for nuclear deexcitation
Involves emission of (gamma rays)
Does not change the number of protons or neutrons in the nucleus
Internal conversion offers an alternative deexcitation pathway
Excess nuclear energy transfers directly to an atomic electron
Results in ejection of an electron from the atom without gamma ray emission
Pair production can occur for high-energy transitions (> 1.022 MeV)
Creates an electron-positron pair from the excess energy
Requires sufficient energy to overcome the rest mass of two electrons
Gamma Decay
Characteristics of Gamma Radiation
Gamma rays consist of high-energy photons emitted during nuclear transitions
Typical gamma ray energies range from tens of keV to several MeV