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Laserlight that marches in step

An ordinary light bulb shines like a crowd in which everyone walks their own way. A laser is a squad in which billions of photons share the same color, direction and stride. Look inside a laser cavity, compare it with a light bulb, browse laser types from ultraviolet to infrared, and learn the story of the blue diode — the same one that gave us the blue laser and white LED light.

Light Amplification by Stimulated Emission of Radiation — light made stronger by stimulated emission.

Laser cavity

Controls

Population inversion
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Photons in the cavity
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Output power
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Pump threshold (this scheme)
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Simplified model: two rate equations (upper-level population and the number of photons in the cavity) computed in the background; the animation shows only a sample of the photons and atoms. Time is measured in upper-level lifetimes τ (ruby: about 3 ms, Nd:YAG: about 0.23 ms). Power is in arbitrary units (a.u.).

Levels and threshold

Below threshold the cavity only glows faintly with spontaneous emission. Once the gain catches up with the losses, the number of photons grows like an avalanche, and the output power rises linearly with the pump — that's the “knee” in the graph. Right after switch-on you can also see the characteristic relaxation oscillations (spikes).

Where the name comes from, and why 4 levels are easier

Stimulated emission: a photon of just the right energy passes an excited atom and “persuades” it to give up its energy. The new photon is an exact copy of the first — same direction, phase, polarization and wavelength. Each copy can trigger more — hence the avalanche and the gain.

Population inversion: gain beats absorption only when there are more atoms in the upper laser level than in the lower one. That's why the laser has to be pumped — with a flash lamp, a diode or an electrical discharge.

3 levels (ruby): the lower laser level is the ground state, where all the atoms sit at the start. So you have to excite more than half of them before any gain appears. 4 levels (Nd:YAG, He-Ne): the lower laser level lies a little above the ground state and empties almost instantly — a handful of excited atoms is enough for inversion, so the threshold is many times lower.

Mirrors: one reflects almost 100%, the other e.g. 98% — it lets a fraction of the light out. A photon bounces back and forth many times and is amplified on every pass. If the output mirror lets too much through, the losses exceed the gain and the laser goes dark.

A short history

  • Albert Einstein describes stimulated emission (in his work on the quantum theory of radiation, 1916–1917).
  • Charles Townes and his team run the first maser, using ammonia — a “laser” for microwaves. Nikolay Basov and Alexander Prokhorov developed similar ideas independently (they shared the 1964 Nobel Prize).
  • On May 16, Theodore Maiman (Hughes Research Laboratories) runs the first laser — a pulsed ruby laser at 694.3 nm. In December, Ali Javan, William Bennett and Donald Herriott run the first gas laser (He-Ne, initially in the infrared).
  • The first semiconductor lasers (GaAs) — at General Electric and IBM labs, among others.
  • The first lasers built in Poland — including a gas laser at the Military University of Technology in Warsaw, by Zbigniew Puzewicz's team.

Back then people joked that the laser was “a solution looking for a problem.” Today it's hard to find a field of technology without one.

How does it work?

A photon carries a packet of energy

Light is made of photons. The energy of one photon depends only on the frequency ν (or the wavelength λ):

E = h·ν = h·cλh = 6.626·10⁻³⁴ J·s, c ≈ 3·10⁸ m/s

A handy version for electronvolts and nanometers:

λ [nm] ≈ 1240E [eV]e.g. 1240/2.7 ≈ 459 nm — blue

Lasing threshold

A laser “switches on” when the gain per round trip of the cavity equals the losses (light let out through the mirror + absorbed inside). Above threshold, extra pump power is turned almost entirely into output light — that's why the graph has a knee.

The beam spreads too

θ ≈ λπ·w₀w₀ — beam waist radius

Distance from time of flight

d = c·t2divide by 2 because the light goes there and back

The smallest spot

dspot ≈ λ2·NANA — numerical aperture of the objective

Peak power of a pulse

Ppeak ≈ Eτthe same energy in a shorter time = more power

Challenges

  1. Cross the lasing thresholdIn “How a laser works” mode, raise the pump until the laser starts to shine.not completed
  2. Lower the threshold: 4 levels instead of 3Switch from ruby to Nd:YAG and keep it lasing with the pump below the threshold of the 3-level laser.not completed
  3. Tune the gap to blue lightSet Eg so the diode glows blue (450–490 nm).not completed
  4. Fit 25 GB on a discChoose the laser and objective of a Blu-ray drive.not completed
  5. Measure the distance to the MoonIn “Applications,” send a pulse to the Apollo retroreflector and wait for the echo.not completed
  6. Femtosecond pulseIn “Power and pulses,” shorten the pulse below 1 ps and see the peak power.not completed

Did you know…?

  • The first item scanned by a laser barcode reader in a store was a pack of chewing gum — on June 26, 1974, in Ohio.
  • The retroreflectors left on the Moon by Apollo 11, 14 and 15 still work today. Thanks to them, we know the Moon is moving away from Earth by about 3.8 cm a year.
  • The LIGO detector measures changes in the length of its 4-kilometer arms of about 10⁻¹⁸ m — less than a thousandth of a proton's diameter. It does this with a laser.

Keys

Q W E R T Y
switch modes
← →
on the tabs: neighboring mode; on the laser axis: neighboring laser
Space
pause / resume the laser cavity
3 4
3- or 4-level scheme
0
reset the cavity (pump switched on again)
Esc
stop the cavity animation