Recoil temperature

In laser cooling, the Boltzmann constant times the recoil temperature is equal to the recoil energy deposited in a single atom initially at rest by the spontaneous emission of a single photon.[1] It is defined as

T_{recoil}=\frac{\hbar^2k^2}{2mk_B}

where k is the wavevector of the light, m is the mass of an atom, k_B is Boltzmann's Constant and \hbar is Planck's Constant. It is typically on the order of 1 μK, and thus lower than the Doppler temperature. An example of a process where the recoil temperature can be reached is Sisyphus cooling.

References

  1. Metcalf and van der Straten (1999). Laser Cooling and Trapping. New York: Spinger-Verlag. ISBN 0-387-98728-2.