13.2
Ultracold atoms and optical lattices
The coldest place on Earth is a laboratory: lasers slow atoms down to nanokelvin, then a standing-wave light field assembles an artificial crystal whose every parameter is yours to tune.
Recommended first
After this section you should be able to
- Use momentum conservation and the Doppler effect to explain why lasers can cool atoms, and estimate the relevant scales
- Explain how an optical lattice acts as an "artificial crystal" and the physical meaning of the two Hubbard-model parameters
- Explain why the superfluid–Mott insulator transition is a tug-of-war between kinetic energy and interactions
At room temperature, a rubidium atom zips around at about 300 m/s — faster than a high-speed train. In today’s cold-atom laboratories, the same atom is cooled to a few tens of nanokelvin: its speed drops to a few millimetres per second, a hundred million times colder than the cosmic microwave background (2.7 K). Nothing this cold has ever appeared in the observable history of the universe — it exists only inside vacuum chambers on Earth.
Why go this cold? Recall the de Broglie wavelength : the slower the atom, the longer its matter wave. Around microkelvin temperatures reaches the scale of an optical wavelength and the atoms’ wave natures begin to “overlap”; colder still, bosons pile en masse into a single quantum state — Bose–Einstein condensation (BEC, achieved in 1995), a million atoms sharing one macroscopic wavefunction. From that moment on, an atomic gas is no longer a bit-player in the thermodynamic background: it becomes a piece of macroscopic quantum matter you can see, photograph, and tune.
And the first step of it all sounds the most implausible: cooling atoms with light.
How a laser can possibly be a refrigerator
Light heats what it shines on — that is everyday experience. The trick of laser cooling is to make only the atoms coming towards you absorb the light.
The mechanism is Doppler cooling: tune the laser frequency slightly below the atomic transition (red detuning).
- An atom running into the laser sees the light blue-shifted by the Doppler effect in its own frame — right into resonance, so it absorbs photons copiously. Every absorbed photon delivers a head-on momentum kick of .
- An atom running with the laser sees the light shifted further to the red, further from resonance, and absorbs almost nothing.
After each absorption the atom spontaneously re-emits the photon, but in a random direction, so on average the emission carries away no momentum. Net effect: whoever runs into the beam gets kicked — a damping force proportional to velocity and opposed to it. With six beams in three counter-propagating pairs covering all directions, the atoms swim as if through syrup, which is why the arrangement is called “optical molasses”.
Order of magnitude: how many photons to stop an atom? How cold does it get?basic~8 min
How hard is one kick? A rubidium atom (mass ) absorbing a 780 nm photon recoils at
How many kicks are needed? To stop from a room-temperature speed of 300 m/s takes
How long does the kicking take? The absorption–emission cycle rate is capped by the excited-state lifetime; rubidium’s spontaneous emission rate is , giving a saturated scattering rate of about per second. So the stopping time is , over a stopping distance of about 1 metre — which is exactly the length of the “Zeeman slower” tube in the lab. A tabletop-scale apparatus, just right.
How cold can it get? The damping cannot go on forever: each spontaneous emission delivers a random recoil, a continuous “heating noise”. Balancing cooling against heating leaves the atom with a residual energy of order the excited state’s energy width (velocity differences within the linewidth are invisible to the Doppler mechanism). The careful calculation gives the Doppler limit
From 300 K to 150 μK — six orders of magnitude — in a few milliseconds with a few laser beams. Getting lower needs new tricks: polarisation-gradient cooling reaches a few microkelvin, and the final step, evaporative cooling (repeatedly skimming off the hottest atoms and letting the rest rethermalise — the same principle as blowing on a bowl of soup), delivers the gas into the nanokelvin regime and BEC.
Optical lattices: building a crystal out of standing waves
Two counter-propagating laser beams form a standing wave with intensity profile . A detuned light field shifts the atomic energy levels by an amount proportional to the intensity (the AC Stark shift — you met its mechanism in the second-order perturbation theory of section 7.5), so the atom feels a spatially periodic potential
Three beam pairs make a three-dimensional simple-cubic “lattice” with spacing half an optical wavelength. Cold atoms loaded into these wells are in exactly the situation of electrons in the ionic lattice of a solid — except that this “crystal”:
- has no impurities, no defects, no lattice vibrations — the potential is printed by laser light, perfectly periodic;
- has adjustable depth — turning the laser-power knob changes the barrier height;
- runs ten orders of magnitude slower — electrons hop between sites in femtoseconds, atoms in milliseconds, slow enough to photograph the atoms site by site through a microscope (the quantum gas microscope, mature since 2009).
In a deep lattice each site is approximately a harmonic-oscillator well (section 2.9), the atoms occupy only the lowest orbital, and the physics of the whole system reduces to two ingredients: tunnelling to the neighbouring site (amplitude — the barrier penetration of section 2.11) and the repulsion energy of two atoms on the same site. Written in the language of section 8.5, this is the celebrated Bose–Hubbard model:
The first term lets atoms delocalise and lower their kinetic energy; the second penalises two atoms crowding onto one site.
The superfluid–Mott transition: kinetic energy versus interactions, in a tug-of-war
Imagine exactly one atom per site on average, and tune :
- Shallow lattice (): tunnelling wins. Each atom spreads its wavefunction over the whole lattice, and the whole gas condenses into a single phase-coherent entity — the superfluid phase. The price: large fluctuations in the atom number on each site.
- Deep lattice (): repulsion wins. Squeezing an extra atom onto a site costs , so the system simply locks exactly one atom onto every site, and nobody moves — the Mott insulator phase. With the number pinned down, the phase becomes completely uncertain (number and phase are a conjugate pair, bound by the uncertainty principle just like and ).
In 2002, Greiner and colleagues filmed this tug-of-war: switch the lattice off suddenly and let the atoms fly free, and the interference pattern their wavefunctions form reveals the coherence — the superfluid phase gives sharp interference peaks; ramp the lattice deeper and the peaks vanish (into the Mott phase); ramp it back down and the peaks come back to life. A quantum phase transition, demonstrated reversibly, back and forth.
Key formulas
Photon recoil velocity
Stopping a room-temperature atom takes ~5×10⁴ photons and a few milliseconds
Doppler limit
Balance point between cooling and random spontaneous-emission recoils
Optical lattice potential
AC Stark shift; the depth V₀ is set directly by laser power
Bose–Hubbard model
Large t/U: superfluid; small t/U (integer filling): Mott insulator
Self-check3 questions
- 1.
In Doppler cooling, why is the laser tuned slightly below the atomic resonance (red detuning)?
- 2.
The excited-state spontaneous emission rate of rubidium is Γ = 2π × 6.07 MHz. Find the Doppler limit temperature T_D = ħΓ/(2k_B) in μK. (ħ = 1.055×10⁻³⁴ J·s, k_B = 1.381×10⁻²³ J/K)
μK1000% relative tolerance - 3.
Which of the following statements about the superfluid–Mott insulator transition are correct? (Select all that apply.)
Select all that apply
What comes next
Cold atoms scale “artificial quantum matter” to a million atoms, but each atom’s energy levels come pre-set by nature. The next section goes the opposite way: build a single “atom” out of a circuit board — energy levels, transition frequency, and coupling to photons all decided by the lithography mask.
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