Detailed schematic of LIGO's laser system showing power amplification and frequency stabilization components

LIGO's Laser

The 200 W beam that enters LIGO's interferometers begins inside a laser diode, which uses electricity to generate a 4 W, 808 nm beam of near-infrared laser light. While laser diodes are the kind of devices that one finds in everyday laser pointers, at 4 Watts, LIGO's is 800 times more powerful than most off-the-shelf laser pointers. This beam is first directed into a fingernail-sized crystal of man-made garnet in which it circulates and stimulates the emission of a 2 Watt beam with a wavelength of 1064 nm. This crystal lasing device is called a Non-Planar Ring Oscillator (NPRO) and the resulting 2 W beam is called a “seed” beam because it will eventually grow into a much more powerful laser.

NPRO with Scale Marker

Non-Planar Ring Oscillator where LIGO's laser begins its journey. (Credit: Peter King)

While 1064 nm is the target wavelength for LIGO’s laser, it needs 100 times more power before it can enter the interferometer. To get there, the 2 Watt seed beam undergoes two amplification stages that boost its power up to nearly 200 W.

In the multi-faceted first step of amplification, the seed beam passes through a device called a Master Oscillator-Power Amplifier (MOPA). The MOPA contains four thin laser amplifier rods that begin the power-boosting process. These rods, composed of a glass-like material made of neodymium, yttrium, lithium, and fluoride, are about the size of the graphite inside a pencil: just 3 mm in diameter and 5 cm long.

To amplify the seed beam, the molecules in each rod are first energized by shining separate 808 nm lasers into each rod. When the seed beam then also travels through the first rod, the rod molecules respond by emitting 1064 nm photons with the same properties (phase, wavelength) as the incoming seed beam. These new 1064 nm photons join those from the seed beam traveling in the same direction (more photons means more power). This more powerful beam then travels to the second rod where this amplification process occurs again, then again in the third, and again in the fourth rod. Like tributaries to a river, at each stage of this amplification process, more and more photons of the same wavelength join the seed beam, gradually increasing its power.

LIGOs Laser HPO Cutout

Path of the beam from the MOPA (blue line entering from lower left) through the High Power Oscillator as it is amplified from 35 W to 200 W. (Credit: Caltech/MIT/LIGO Lab)

Labeled MOPA

The 2 W beam exits the NPRO (bottom left) and travels via a series of mirrors and lenses through the amplifier rods. Each rod boosts the power a little bit until it reaches 35 W. (Credit: Caltech/MIT/LIGO Lab)

By the time the seed beam has passed through all four rods, its power has increased from 2 W to 35 W all while maintaining a wavelength of 1064 nm. The path that the beam takes from the NPRO through the 4 rods is shown in the figure at right (click on the image for a larger version).

The final stage of power amplification is achieved in another four-rod device called a high power oscillator (HPO). The HPO uses four more amplifier rods, about the same size as the MOPA rods but made of a different material. As the beam passes through these rods, just like in the MOPA, it gets an additional power boost from laser light funneled through bundles of fiber-optic cables arranged like a flower, and only 3 mm across.

HPO bundle amplifier

7 fiber-optic cables deliver 315 W of power to the rods in the HPO, stimulating them to emit more 1064 nm light.

Each fiber carries 45 Watts of laser power, so each bundle delivers 315 Watts (7 fibers x 45 W each) into each rod to prime it to emit more and more laser light. By the time the beam exits the HPO it has finally achieved its desired power of 200 W. The complexity of this device is revealed in the image below left (click on the image for a larger version).

Frequency and Power Stability


Despite the purity and stability of the initial beam, uponexiting the HPO it is still not stable enough for use. LIGO's laser needs to be 100-million times more stable than it is intrinsically. To achieve this unprecedented level of stability, the beam’s natural frequency variations (i.e. its inability to continually radiate a single, discrete color of light) and power fluctuations are mechanically reduced by about a factor of 100-million through a series of feedback mechanisms before the laser is used in the interferometer. This whole process is akin to tuning the world’s most complex piano.

Power fluctuations are also reduced through feedback control loops, which use photodetector data to sense power fluctuations. To learn more about LIGO's feedback and control systems, visit Feedback and Control Systems.

Labeled Laser Table

LIGO's laser is generated in its laser room by the numerous devices on the table