Spontaneous emission

In optics, spontaneous emission is the process by which matter may lose energy, resulting in the creation of a photon. A simple model of spontaneous emission consists of an atom which may be in two electronic energy states, the ground state (1) and the excited state (2), with energies E₁ and E₂ respectively. If the atom is in the excited state, it may spontaneously decay into the ground state, releasing the difference in energies between the two states as a photon. The photon will have frequency ν and energy hν, given by: :$E\_2\; -\; E\_1\; =\; h\; \backslash \; u$, where h is Planck's constant. The phase of the photon in spontaneous emission is random as is the direction the photon propagates in. This is not true for stimulated emission. An energy level diagram illustrating the process is shown below:

   Before emission              After emission

  --------O---------          ------------------ E2
          |  Atom in
          |  excited state               
          |                              ~~~>
          |                          Photon hν
          |                                              
          V                            
  ------------------          ---------O-------- E1
                                     Atom in ground state

In a group of such atoms, if the number of atoms in the excited state is given by N, the rate at which spontaneous emission occurs is given by: :$\backslash \backslash frac\{\backslash \backslash partial\; N\}\{\backslash \backslash partial\; t\}\; =\; -A\_\{21\}\; N$, where A₂₁ is a proportionality constant for this particular transition in this particular atom. (The constant is referred to as an Einstein A co-efficient.) The rate of emission is thus proportional to the number of atoms in the excited state, N. The above equation can be solved to give: :$N(t)\; =\; N(0)\; e^\{\; -\; \backslash \backslash frac\{t\}\{\backslash \backslash tau\_\{21\}\; \}\; \}$, where N(0) is the initial number of atoms in the excited state, and τ₂₁ is the lifetime of the transition, τ₂₁ = (''A''₂₁)^-1. It can be seen that spontaneous emission occurs in a way rather similar to the decay of radioactive particles, in particular that the lifetime is analogous to a half-life. There are two different ways in which decay or relaxation can occur: radiative and nonradiative. In nonradiative relaxation, the energy is absorbed as phonons, more commonly known as heat. Nonradiative relaxation is nearly impossible to measure and cannot be inferred except in very small particles because the difference in the temperature before and after a relaxation is so small that it is in the noise of any measurement for practical systems. Nonradiative relaxations occur when the energy difference between the levels is very small, and these typically occur on a much faster time scale than radiative transitions. For many materials (for instance, semiconductors), electrons move quickly from a high energy level to a meta-stable level via small nonradiative transitions and then make the final move down to the bottom level via an optical or radiative transition (This final transition is the transition over the bandgap in semiconductors.). Large nonradiative transitions do not occur frequently because the crystal structure generally can not support large vibrations without destroying bonds (which generally doesn't happen for relaxation). Meta-stable states form a very important feature that is exploited in the construction of lasers. Specifically, since electrons decay slowly from them, they can be piled up in this state without too much loss and then stimulated emission can be used to boost an optical signal. See also absorption, stimulated emission, laser science. Category:Exponentials Category:Optics

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