In atomic, molecular, and optical physics, resonance fluorescence is the process in which a two-level atom system interacts with the quantum electromagnetic field if the field is driven at a frequency near to the natural frequency of the atom. When discussing nuclear physics and gamma rays, it is known as nuclear resonance fluorescence.
General theory Typically the electromagnetic field is applied to the two-level atom through the use of a monochromatic laser. A two-level atom is a specific type of two-state system in which the atom can be found in two possible states: where an electron is either in its ground state or in its excited state. In many experiments a lithium atom is used because it can be modeled as a two-level atom, since the excited states of its singular valence electron are far enough apart that the possibility of the electron jumping to a higher excited state can be ignored. Thus it allows for easier frequency tuning of the applied laser as frequencies further from resonance can be used while still driving the electron to jump to only the first excited state. Once the atom is excited, it will release a photon with the same energy as the energy difference between the excited and ground state. The mechanism for this release is the spontaneous decay of the atom. The emitted photon is released in an arbitrary direction. While the transition between two specific energy levels is the dominant mechanism in resonance fluorescence, experimentally other transitions will play a very small role and thus must be taken into account when analyzing results. The other transitions will lead to emission of a photon of a different atomic transition with much lower energy which will lead to "dark" periods of resonance fluorescence. The dynamics of the electromagnetic field of the monochromatic laser can be derived by first treating the two-level atom as a spin-1/2 system with two energy eigenstates which have energy separation of ħω0. The dynamics of the atom can then be described by the three rotation operators, R i ^ ( t ) {\displaystyle {\hat {R_{i}}}(t)} , R j ^ ( t ) {\displaystyle {\hat {R_{j}}}(t)} , R k ^ ( t ) {\displaystyle {\hat {R_{k}}}(t)} , acting upon the Bloch sphere. Thus the energy of the system is described entirely through an electric dipole interaction between the atom and field with the resulting hamiltonian being described by
H ^ = 1 2 ∫ ( ϵ 0 E → ^ 2 ( r → , t ) + 1 μ 0 B → ^ 2 ( r → , t ) ) d 3 x + ℏ ω 0 R k ^ ( t ) + 2 ω 0 μ → ⋅ A → ^ ( 0 , t ) R j ^ ( t ) {\displaystyle {\hat {H}}={\frac {1}{2}}\int (\epsilon _{0}{\hat {\vec {E}}}^{2}({\vec {r}},t)+{\frac {1}{\mu _{0}}}{\hat {\vec {B}}}^{2}({\vec {r}},t))d^{3}x+\hbar \omega _{0}{\hat {R_{k}}}(t)+2\omega _{0}{\vec {\mu }}\cdot {\hat {\vec {A}}}(0,t){\hat {R_{j}}}(t)} . After quantizing the electromagnetic field, the Heisenberg equation and Maxwell's equations can be used to find the resulting equations of motion for R k ^ ( t ) {\displaystyle {\hat {R_{k}}}(t)} as well as for b ^ ( t ) {\displaystyle {\hat {b}}(t)} , the annihilation operator of the field,
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