A change in a quantum system's energy state, here the nuclear excitation and emission.In quantum physics, a transition is the change of a system from one energy state to another, typically involving the absorption or emission of a photon. Here, the focus is on nuclear transitions, where the nucleus of an atom jumps between energy levels, releasing or absorbing gamma rays. These transitions are fundamental to understanding nuclear structure and have applications in fields like astrophysics and quantum technology.
The concept of quantum transitions was developed in the early 20th century with the Bohr model of the atom (1913) and later formalized in quantum mechanics by Dirac and others in the 1920s. Nuclear transitions were studied extensively after the discovery of the nucleus in 1911.
A nucleus in an excited state can decay to a lower energy state by emitting a gamma-ray photon, a process known as gamma decay. The energy of the photon equals the difference between the two nuclear energy levels. Transitions can also be induced by absorbing a photon of the right energy, a process used in Mössbauer spectroscopy. The probability of a transition depends on selection rules, such as changes in angular momentum and parity, and is described by Fermi's golden rule.
Nuclear transitions are used in Mössbauer spectroscopy to study chemical environments, in nuclear medicine for imaging and therapy, and in the design of nuclear clocks, which are ultra-precise timekeepers based on nuclear energy levels.
The Mössbauer effect, which relies on recoil-free nuclear transitions, is so precise that it can measure the gravitational redshift of gamma rays over a vertical distance of just a few meters in the Earth's field.













