Minimum temperature The
Doppler temperature is the minimum temperature achievable with Doppler cooling. When a
photon is
absorbed by an atom counter-propagating to the light source, its velocity is decreased by
momentum conservation. When the absorbed photon is spontaneously emitted by the
excited atom, the atom receives a momentum kick in a random direction. The spontaneous emissions are
isotropic and therefore these momentum kicks average to zero for the mean velocity. On the other hand, the mean squared velocity, \langle v^2\rangle, is not zero in the random process, and thus heat is supplied to the atom. At equilibrium, the heating and cooling rates are equal, which sets a limit on the amount by which the atom can be cooled. As the transitions used for Doppler cooling have broad
natural linewidths \gamma (measured in
radians per second), this sets the lower limit to the temperature of the atoms after cooling to be T_{\mathrm{Doppler}} = \hbar \gamma /(2k_\text{B}) , where k_\text{B} is the
Boltzmann constant and \hbar is the
reduced Planck constant. This is usually much higher than the
recoil temperature, which is the temperature associated with the momentum gained from the spontaneous emission of a photon. The Doppler limit has been verified with a gas of metastable helium.
Sub-Doppler cooling Temperatures well below the Doppler limit have been achieved with various laser cooling methods, including
Sisyphus cooling,
evaporative cooling, and
resolved sideband cooling. The theory of Doppler cooling assumes an atom with a simple two level structure, whereas most atomic species which are laser cooled have complicated hyperfine structure. Mechanisms such as Sisyphus cooling due to multiple ground states lead to temperatures lower than the Doppler limit.
Maximum concentration The concentration must be minimal to prevent the absorption of the photons into the gas in the form of heat. This absorption happens when two atoms collide with each other while one of them has an excited electron. There is then a possibility of the excited electron dropping back to the ground state with its extra energy liberated in additional kinetic energy to the colliding atoms—which heats the atoms. This works against the cooling process and therefore limits the maximum concentration of gas that can be cooled using this method.
Atomic structure Only certain atoms and ions have optical transitions amenable to laser cooling, since it is extremely difficult to generate the amounts of laser power needed at wavelengths much shorter than 300 nm. Furthermore, the more
hyperfine structure an atom has, the more ways there are for it to emit a photon from the upper state and
not return to its original state, putting it in a
dark state and removing it from the cooling process. It is possible to use other lasers to
optically pump those atoms back into the excited state and try again, but the more complex the hyperfine structure is, the more (narrow-band, frequency locked) lasers are required. Since frequency-locked lasers are both complex and expensive, atoms which need more than one extra
repump laser are rarely cooled; the common
rubidium magneto-optical trap, for example, requires one repump laser. This is also the reason why molecules are in general difficult to laser cool: in addition to hyperfine structure, molecules also have
rovibronic couplings and so can also decay into excited rotational or vibrational states. However, laser cooling of molecules has been demonstrated, first with SrF molecules, and subsequently with other diatomics such as CaF and YO. == Configurations ==