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Take a single isolated optical transition of angular frequency ${\omega }_0$. Both beams have laboratory angular frequency ${\omega }_L$, with laser detuning $\delta ={\omega }_L-{\omega }_0$. Let the pump travel along $+z$, the probe along $-z$, $v$ denote an atom's $z$-velocity, and $k={\omega }_0/c$ be the approximate vacuum wavenumber; $c$ is the speed of light. To first order in $v/c$, the laser detunings in the atom's frame areThe pump addresses atoms near $v=\delta /k$, while the probe addresses atoms near $v=-\delta /k$. For the same transition, simultaneous exact resonance requires both expressions to vanish: adding and subtracting gives $\delta =0$ and $v=0$. The selected atoms can still have substantial transverse velocity. Finite natural linewidth admits a narrow interval of longitudinal velocities; a warm gas has not been cooled.

This is velocity selection, not cancellation of each atom's Doppler shift within a single absorption event. Changing laser detuning selects different atoms for ordinary photon absorption, but only near line centre do these two selected classes overlap. Laser cooling instead changes the distribution of the atoms' velocities through repeated momentum transfer.

Consider equal opposing laser beams along the $x$ axis and an atom with velocity $v$. Let ${\omega }_L$ be their angular frequency, ${\omega }_0$ the atomic resonance angular frequency, $k=2\pi /\lambda >0$ their wavenumber, and $\delta ={\omega }_L-{\omega }_0$ the laser detuning. Red detuning means $\delta <0$. To first order in $v/c$, the atom seesFor small positive $v$, the beam travelling towards negative $x$ is closer to resonance and causes more photon absorption; its momentum kicks point against $v$. The beam travelling towards positive $x$ is further from resonance. Reversing $v$ exchanges the roles of the two beams. This is a Doppler effect on the absorption rates, rather than a need to follow each atom with a moving beam.

An absorbed photon gives the atom momentum $\pm \hslash k$, where $\hslash =h/(2\pi )$ is the reduced Planck constant. Subsequent spontaneous emission gives a recoil opposite to the emitted photon. For an emission pattern symmetric under reversal of direction, that recoil has zero expected value, but nonzero variance. Its mean therefore leaves the directional absorption force intact, while its randomness adds recoil energy. Random absorption times and choices of beam add further momentum fluctuations. Zero mean recoil does not mean zero heating.

Use a closed two-level system with spontaneous emission population decay $P_e(t)=P_e(0)e^{-\Gamma t}$. Here $\Gamma$ is a decay rate in inverse seconds and also the full width at half maximum of the natural linewidth expressed in angular frequency. The corresponding full width in hertz is $\Gamma /(2\pi )$; the angular half width is $\Gamma /2$. These conventions determine every factor of two and $2\pi$ below.

Let $s$ be the on-resonance saturation parameter of each beam, with total excitation weak enough that saturation and coherent coupling between beams can be neglected. The independent-beam scattering rates and net force areThe force is the photon momentum per absorption multiplied by the difference in absorption rates. With dimensionless laser detuning $d=\delta /\Gamma$ and dimensionless velocity $u=kv/\Gamma$, writeFor the example $d=-0.5$ and $u=0.25$, the positive and negative beam factors are respectively $4/13$ and $4/5$. Thus $F(0.25)=-32/65\simeq -0.4923$: the atom is moving right and the net force points left. All values in this example are dimensionless.

Subtracting the two fractions gives an especially useful sign check:For red detuning, the force opposes nonzero $v$ throughout this ideal model; its useful magnitude eventually falls at large $|u|$. Near zero, a Taylor series gives dampingAt $d=-0.5$, $F^{\prime }(0)=-2$ and $\alpha =\hslash k^{2}s$. For blue detuning the sign reverses and the small-velocity motion is amplified; at exact resonance the opposing mean forces cancel in this symmetric model. Its derivation assumes weak excitation, a closed two-level system, equal beam intensities and nonrelativistic velocities; real multilevel atoms need additional physics.

Laser detuning is the difference between a laser angular frequency and a specified atomic resonance angular frequency. Red detuning has $\delta <0$; blue detuning has $\delta >0$. The sign matters in laser cooling: a moving atom can see a red-detuned laser closer to resonance because of the Doppler effect.

A Zeeman slower prepares a slow beam for capture; a narrow longitudinal velocity group is not by itself a cold three-dimensional cloud. The historical apparatus measured slowed-beam velocities with a separate fluorescence probe scanned in frequency, just after switching off the slowing beam. This avoided simultaneous-beam complications.^[ref]

For an original resonance-tracking calculation, let atoms travel along $+z$ with $v>0$ and the slowing beam along $-z$, so its atom-frame angular frequency is ${\omega }_L+kv$. Approximate the selected cycling transition by ${\omega }_{eg}(B)={\omega }_0+\zeta B$ on one field branch; $\zeta$ is its signed angular frequency shift per unit magnetic field. A multilevel atom may require a nonlinear ${\omega }_{eg}(B)$ outside that branch. Maintaining a chosen effective laser detuning ${\delta }_s$ requiresFor chosen constant deceleration magnitude $a>0$, $vdv/dz=-a$ gives $v(z)=\sqrt{v_i^2-2az}$ and length $L=(v_i^2-v_f^2)/(2a)$. Substitution supplies a square-root magnetic field profile, plus a constant offset. The signs follow from the specified directions; reversing the selected transition's magnetic slope reverses the required field variation.

As a hypothetical design, take $v_i=300\mathrm{m}{\mathrm{s}}^{-1}$, $v_f=30\mathrm{m}{\mathrm{s}}^{-1}$ and $a=5.0\times 10^4\mathrm{m}{\mathrm{s}}^{-2}$. The required length is $0.891\mathrm{m}$ and flight time $(v_i-v_f)/a=5.4\mathrm{ms}$. For chosen $\lambda =589\mathrm{nm}$ and $m=3.82\times 10^{-26}\mathrm{kg}$, photon recoil velocity $\hslash k/m\simeq 0.0294\mathrm{m}{\mathrm{s}}^{-1}$ implies roughly $9.17\times 10^3$ directed absorption events. The mean required scattering rate is about $1.70\times 10^6{\mathrm{s}}^{-1}$. This budget must lie below the available scattering rate, with margin for capture and intensity variation. Optical pumping into unwanted hyperfine structure or magnetic sublevels can interrupt the cycle. Longitudinal slowing, transverse recoil heating and final cloud temperature are separate quantities.