It's a tall order. Nevertheless, we at Intel's
Photonics Technology Lab have been working on these
building blocks for several years. One of our latest
achievements, announced last February, is the world's
first continuous all-silicon laser, which is based on
the Raman scattering effect. Named for the Indian
physicist Chandrasekhara Venkata Raman, who first
described it in 1928, this effect causes light to
scatter in certain materials to produce longer or
shorter wavelengths.
Raman scattering is used today, for example, to boost
signals traveling through long stretches of glass fiber.
It allows light energy to be transferred from a strong
pump beam into a weaker data beam. Most long-distance
telephone calls today benefit from Raman amplification.
Typically, a Raman amplifier requires kilometers of
fiber to produce a useful amount of amplification,
because glass exhibits very weak scattering. Silicon,
though, has a crystal structure, so its Raman scattering
is more than 10 000 times as strong as that of ordinary
glass fiber. In other words, you could achieve the same
amplification in a centimeter-square chip that you'd get
in kilometers of glass fiber.
In fact, so intense is the light amplification in
silicon that it sets the stage for creating a laser. To
build a Raman laser in silicon, you first need to create
a conduit, also known as a waveguide, for the light
beam. This can be done using standard CMOS techniques to
etch a ridge or channel into a silicon wafer. In any
waveguide, some light is lost through imperfections,
surface roughness, and absorption by the material. The
trick, of course, is to ensure that the amplification
provided by the Raman effect exceeds the loss in the
waveguide.
In mid-2004, we discovered that increasing the pump
power beyond a certain point failed to increase the
Raman amplification and eventually even reduced it. The
culprit was a process called two-photon absorption,
which caused the silicon to absorb a fraction of the
pump beam's photons and release free electrons. Almost
immediately after we turned on the pump laser, a cloud
of free electrons built up in the waveguide, absorbing
some of the pump and signal beams and killing the
amplification. The stronger the pump beam, the more
electrons created and the more photons lost.
Intel researchers found a way to flush out the extra
electrons by sandwiching the waveguide within a device
called a PIN diode; PIN stands for
p-typeintrinsicn-type. When a voltage is applied, the
free electrons move toward the diode's positively
charged side; the diode effectively acts like a vacuum
and sweeps the free electrons from the path of the
light. Using the PIN waveguide, we demonstrated
continuous amplification of a stream of optical bits,
more than doubling its original power.
Once we had the amplification, we created the silicon
laser by coating the ends of the PIN waveguide with
specially designed mirrors. We make these dielectric
mirrors by carefully stacking alternating layers of
nonconducting materials, so that the reflected light
waves combine and intensify. They can also reflect light
at certain wavelengths while allowing other wavelengths
to pass through.
With the Raman amplifier between the two dielectric
mirrors, we had the basic configuration needed for a
laser. After all, laser stands for "light amplification
by stimulated emission of radiation," and that's what
was going on in our device. Photons that entered were
multiplied in number by the Raman amplifier. Meanwhile,
as the light waves bounced back and forth between the
two mirrors, they stimulated the emission of yet more
photons through Raman scattering.
The photons stimulated in this way were in phase with
the others in the amplifier, so the beam generated was
coherent. Once the round-trip gain of photons in the
cavity exceeded the round-trip loss, we observed a
steady beam of laser light exiting the silicon chip. We
had built the first continuous silicon laser [see
illustration, "Let There Be
Light"].
Beyond building the light source and moving light
through the chip, you need a way to modulate the light
beam with data. The simplest option is switching the
laser on and off, a technique called direct modulation.
An alternative, called external modulation, is analogous
to waving your hand in front of a flashlight beam:
blocking the beam of light represents a logical 0;
letting it pass represents a 1. The only difference is
that in external modulation the beam is always on.
For data rates of 10 Gb/s or higher and traveling
distances greater than tens of kilometers, this
difference is critical. Each time a semiconductor laser
is turned on, it "chirps." The initial surge of current
through the laser changes its optical properties,
causing an undesired shift in wavelength. A similar
phenomenon occurs when you turn on a flashlight: the
light changes quickly from orange to yellow to white as
the bulb filament heats up.
If the chirped beam is sent through an optical fiber,
the different wavelengths will travel at slightly
different speeds, which warps data patterns. When
there's a lot of data traveling quickly, this distortion
causes errors in the data.
With an external modulator, by contrast, the laser
beam remains stable, continuous, and chirp-free. The
light enters the modulator, which shutters the beam
rapidly to produce a data stream; even 10-Gb/s data can
be sent up to about 100 km with no significant
distortion. Fast modulators are typically made from
lithium niobate, which has a strong electro-optic
effect—that is, when an electric field is applied to
it, it changes the speed at which light travels through
the material.
You start by splitting the laser beam in two and then
applying an electric field to one beam. If the speed
changes enough to delay the beam by half of one
wavelength, that beam will be out of phase with its
mate. When the beams recombine, they will interfere with
each other and cancel out [see illustration, "Encoding Photons With
Data"].
If, on the other hand, no voltage is applied, the
beams remain in phase, and they will add constructively
when recombined. Encoding the beam with 1s and 0s, then,
means making the beams interfere (0) or keeping them in
phase (1).
A silicon-based modulator, as mentioned before, has
the disadvantage of lacking this electro-optic effect.
To get around this drawback, we devised a way to
selectively inject charge carriers (electrons or holes)
into the silicon waveguide as the light beam passes
through. Because of a phenomenon known as the free
carrier plasma dispersion effect, the accumulated
charges change the silicon's refractive index and thus
the speed at which light travels through it. The silicon
modulator splits the beam in two, just like the lithium
niobate modulator. However, instead of the electro-optic
effect, it's the presence or absence of electrons and
holes that determines the phases of the beams and
whether they combine to produce a 1 or a 0.
The trick is to get those electrons and holes into
and out of the beam's path fast enough to reach
gigahertz data rates. Previous schemes injected the
electrons and holes into the same region of the
waveguide. When the power was turned off, the free
electrons and holes faded away very slowly; the maximum
speed was about 20 megahertz.
Intel's silicon modulator uses a transistorlike
device rather than a diode both to inject and to remove
the charges. Electrons and holes are inserted on
opposite sides of an oxide layer at the heart of the
waveguide, where the light is most intense. Rather than
waiting for the charges to fade away, the transistor
structure pulls them out as rapidly as they go in. To
date, this silicon modulator has encoded data at speeds
of up to 10 Gb/s—fast enough to rival conventional
optical communications systems in use today.
Once the beam is flowing through the waveguide,
photodetectors are used to collect the photons and
convert them into electrical signals. They can also be
used to monitor the optical beam's properties—power,
wavelength, and so on—and feed this information back to
the transmitter, so that it can optimize the beam.
Silicon absorbs visible light well, which is why it
appears opaque to the naked eye. Infrared, however,
passes through silicon without being absorbed, so
photons at those wavelengths can be neither collected
nor detected.
This problem can be overcome by adding germanium to
the silicon waveguides. Germanium absorbs infrared
radiation at longer wavelengths than does silicon. So
using an alloy of silicon and germanium in part of the
waveguide creates a region where infrared photons can be
absorbed. Our research shows that silicon germanium can
achieve fast and efficient infrared photodetection at
850 nanometers and 1310 nm, the communications
wavelengths most commonly used in enterprise networks
today.