Change of an electron between energy levels within an atom
An electron in aBohr model atom, moving fromquantum leveln = 3 ton = 2 and releasing aphoton. The energy of an electron is determined by its orbit around the atom, The n = 0 orbit, commonly referred to as theground state, has the lowest energy of all states in the system.
Electrons canrelax into states of lower energy by emittingelectromagnetic radiation in the form of a photon. Electrons can also absorb passing photons, whichexcites the electron into a state of higher energy. The larger the energy separation between the electron's initial and final state, the shorter the photons'wavelength.[4]
with amplitude, angular frequency, and polarization vector.[7] Note that the actual phase is. However, in many cases, the variation of is small over the atom (or equivalently, the radiation wavelength is much greater than the size of an atom) and this term can be ignored. This is called the dipole approximation. The atom can also interact with the oscillatingmagnetic field produced by the radiation, although much more weakly.
The Hamiltonian for this interaction, analogous to the energy of a classical dipole in an electric field, is. The stimulated transition rate can be calculated usingtime-dependent perturbation theory; however, the result can be summarized usingFermi's golden rule:The dipole matrix element can be decomposed into the product of the radial integral and the angular integral. The angular integral is zero unless theselection rules for the atomic transition are satisfied.
In 2019, it was demonstrated in an experiment with a superconductingartificial atom consisting of two strongly-hybridizedtransmon qubits placed inside a readout resonator cavity at 15 mK, that the evolution of some jumps is continuous, coherent, deterministic, and reversible.[8] On the other hand, other quantum jumps are inherently unpredictable.[9]