Gamma emission is a distinctive process in nuclear physics, often occurring alongside alpha or beta decay. During gamma emission, an atom releases gamma rays, which are high-energy photons. A photon, in this context, is a particle of light and a form of energy that is part of the electromagnetic spectrum. Notably, gamma rays have no mass or charge, represented by the symbol γ (gamma).
When an atom is in an excited state, such as thallium-204, it can undergo gamma emission. In this process, the atom does not change its mass number or atomic number; thallium-204 remains thallium-204. Instead, the emission involves the transition of electrons between energy levels or orbitals. As the electrons move from a higher energy shell to a lower one, energy is released in the form of a gamma ray. This transition signifies a return to a more stable, ground state configuration without altering the identity of the isotope.
It is essential to recognize that gamma emission typically occurs in conjunction with alpha or beta decay. Therefore, while gamma emission can happen independently, it often follows these other decay processes, enhancing the complexity of nuclear reactions. Understanding gamma emission is crucial for grasping the behavior of excited nuclei and the energy transformations that occur during radioactive decay.