The deserts of Arizona are home to Intel’s Fab 32, a
$3billion factory that’s performing one of the most complicated electrical
engineering feats of our time. It’s here that processors with components
measuring just 45 millionths of a millimetre across are manufactured, ready to
be shipped out to motherboard manufacturers all over the world. Creating these
complicated miniature systems is impressive enough, but it’s not the
processors’ diminutive size that’s the most startling or impressive part of the
process.
It may seem an impossible transformation, but
these fiendishly complex components are made from nothing more glamorous than
sand. Such a transformative feat isn’t simple. The production process requires
more than 300 individual steps. However, they can be neatly summed up in just
ten...
Before get started
though, if you’re fascinated by all things silicon, don’t forget to check out
our article revealing the amazing history of computer memoryNow I want all of you to see this video-
1. Converting sand to silicon
Sand is composed of silica (also known as silicon
dioxide), and is the starting point for making a processor. Sand used in the
building industry is often yellow, orange or red due to impurities, but the
type chosen in the manufacture of silicon is a purer form known as silica sand,
which is usually recovered by quarrying. To extract the element silicon from
the silica, it must be reduced (in other words, have the oxygen removed from
it). This is accomplished by heating a mixture of silica and carbon in an
electric arc furnace to a temperature in excess of 2,000°C. The carbon reacts
with the oxygen in the molten silica to produce carbon dioxide (a by-product)
and silicon, which settles in the bottom of the furnace. The remaining silicon
is then treated with oxygen to reduce any calcium and aluminium impurities. The
end result of this process is a substance referred to as metallurgical-grade
silicon, which is up to 99 per cent pure.
This is not nearly pure enough for semiconductor
manufacture, however, so the next job is to refine the metallurgical-grade
silicon further. The silicon is ground to a fine powder and reacted with
gaseous hydrogen chloride in a fluidised bed reactor at 300°C to give a liquid
compound of silicon called trichlorosilane. Impurities such as iron, aluminium,
boron and phosphorous also react to give their chlorides, which are then
removed by fractional distillation. The purified trichlorosilane is vaporised
and reacted with hydrogen gas at 1,100°C so that the elemental silicon is
retrieved.
During the reaction, silicon is deposited on the
surface of an electrically heated ultra-pure silicon rod to produce a silicon
ingot. The end result is referred to as electronic-grade silicon, and has a
purity of 99.999999 per cent.
2. Creating a cylindrical crystal
Although pure to a very high degree, raw
electronic-grade silicon has a polycrystalline structure. In other words, it’s
made up of lots of small silicon crystals, with defects called grain boundaries
between them. Because these anomalies affect local electronic behaviour,
polycrystalline silicon is unsuitable for semiconductor manufacturing. To turn
it into a usable material, the silicon must be turned into single crystals that
have a regular atomic structure. This transformation is achieved through the
Czochralski Process.
Electronic-grade silicon is melted in a rotating
quartz crucible and held at just above its melting point of 1,414°C. A tiny
crystal of silicon is then dipped into the molten silicon and slowly withdrawn
while being continuously rotated in the opposite direction to the rotation of
the crucible. The crystal acts as a seed, causing silicon from the crucible to
crystallise around it. This builds up a rod – called a boule – that comprises a
single silicon crystal. The diameter of the boule depends on the temperature in
the crucible, the rate at which the crystal is ‘pulled’ (which is measured in
millimetres per hour) and the speed of rotation. A typical boule measures 300mm
in diameter.
3. Slicing the crystal into wafers
Integrated circuits are approximately linear,
which is to say that they’re formed on the surface of the silicon. To maximise
the surface area of silicon available for making chips, the boule is sliced up
into discs called wafers. The wafers are just thick enough to allow them to be
handled safely during semiconductor fabrication. 300mm wafers are typically
0.775mm thick. Sawing is carried out using a wire saw that cuts multiple slices
simultaneously, in the same way that some kitchen gadgets cut an egg into
several slices in a single operation. Silicon saws differ from these kitchen
tools in that the wire is constantly moving and also carries with it a slurry of
silicon carbide, the same abrasive material that forms the surface of ‘wet-dry’
sandpaper. The sharp edges of each wafer are then smoothed down to prevent the
wafers from chipping during later processes. Next, in a procedure called
‘lapping’, the surfaces are polished using an abrasive slurry until the wafers
are flat to within an astonishing 2µm (two thousandths of a millimetre).
The wafer is then etched in a mixture of nitric,
hydrofluoric and acetic acids. The nitric acid oxides the surfaces to give a
thin layer of silicon dioxide – which the hydrofluoric acid immediately
dissolves away to leave a clean silicon surface – and the acetic acid controls
the reaction rate. The result of all this refining and treating is an even
smoother and cleaner surface.
4. Making a patterned oxide layer
In many of the subsequent steps, the electrical
properties of the wafer will be modified through exposure to ion beams, hot gasses
and chemicals. But this needs to be done selectively to specific areas of the
wafer in order to build up the circuit. In some cases, this procedure can be
achieved using ‘photoresist’, a photosensitive chemical not dissimilar to that
used in making photographic film (just as described in steps B, C and D,
below). Where hot gasses are involved, however, the photoresist would be
destroyed, making another, more complicated, method of masking the wafer
necessary. To overcome the problem, a patterned oxide layer is applied to the
wafer so that the hot gasses only reach the silicon in those areas where the
oxide layer is missing. Applying the oxide layer mask to the wafer is a
multistage process, as illustrated to the left.
(A) The wafer is heated to a high temperature in
a furnace. The surface layer of silicon reacts with the oxygen present to
create a layer of silicon dioxide.
(B) A layer of photoresist is applied. The wafer
is spun in a vacuum so that the photoresist spreads out evenly over the surface
before being baked dry.
(C) The wafer is exposed to ultraviolet light
through a photographic mask or film. This mask defines the required pattern of
circuit features. This process has to be carried out many times, once for each
chip or rectangular cluster of chips on the wafer. The film is moved between
each exposure using a machine called a ‘stepper’.
(D) The next stage is to develop the latent
circuit image. This process is carried out using an alkaline solution. During
this process, those parts of the photoresist that were exposed to the
ultraviolet soften in the solution and are washed away.
(E) The photoresist isn’t sufficiently durable to
withstand the hot gasses used in some steps, but it is able to withstand
hydrofluoric acid, which is now used to dissolve those parts of the silicon
oxide layer where the photoresist has been washed away.
(F) Finally, a solvent is used to remove the
remaining photoresist, leaving a patterned oxide layer in the shape of the
required circuit features.
5. Creating n-type and p-type regions
The fundamental building block of a processor is
a type of transistor called a MOSFET – you can see how they work in the box
above. The type of device illustrated there is a ‘p-channel’ MOSFET (so-called
because it uses p-type material). Processors also use ‘n-channel’ MOSFETs,
which use n-type material. The first step in creating a circuit is to create
n-type and p-type regions. Below is the method Intel uses for its 90nm process
and beyond:
(A) The wafer is exposed to a beam of boron ions.
These implant themselves into the silicon through the gaps in a layer of
photoresist to create areas called ‘p-wells’. These are, confusingly enough,
used in the n-channel MOSFETs. A boron ion is a boron atom that has had an
electron removed, thereby giving it a positive charge. This charge allows the
ions to be accelerated electrostatically in much the same way that electrons
are accelerated towards the front of a CRT television, giving them enough
energy to become implanted into the silicon.
(B) A different photoresist pattern is now
applied, and a beam of phosphorous ions is used in the same way to create
‘n-wells’ for the p-channel MOSFETs.
(C) In the final ion implantation stage,
following the application of yet another photoresist, another beam of
phosphorous ions is used to create the n-type regions in the p-wells that will
act as the source and drain of the n-channel MOSFETs. This has to be carried
out separately from the creation of the n-wells because it needs a greater
concentration of phosphorous ions to create n-type regions in p-type silicon
than it takes to create n-type regions in pure, un-doped silicon.
(D) Next, following the deposition of a patterned
oxide layer (because, once again, the photoresist would be destroyed by the hot
gas used here), a layer of silicon-germanium doped with boron (which is a
p-type material) is applied.
6: Adding gates to complete the MOSFETs
With the n-type and p-type regions in place, all
that is needed to complete the MOSFETs is the gate. As with many of these
steps, the first job is to produce a patterned oxide layer as described in Step
4. In this case, the oxide layer will have gaps only in the gate regions of the
MOSFETs. Again, there are different ways of making the gates, but the method
described here is typical.
The first part of the gate is a very thin
insulating layer of silicon dioxide, deposited on the surface of the silicon
between the source and the drain. This is done using chemical vapour deposition
(CVD), a process that takes place in a furnace filled with various gases that
cause a chemical reaction to take place on the surface of the silicon. To
complete the MOSFET, a layer of silicon is applied over the top of the thin
oxide layer to act as a conductor. Again, CVD is used, and the silicon is
applied via an oxidation reaction in which gaseous silicon hydride reacts with
oxygen to give silicon and water as products.
Silicon is a poor electrical conductor, but it
can be made more conductive by adding impurities, a process known as 'doping'.
Phosphorous has one more electron in its outer shell than silicon, so doping
with it introduces extra electrons that are free to move within the crystal
matrix. This is called 'n-type' (for negative) material and is more conductive
than pure silicon because of its negative charge carriers. Conversely, boron has
one fewer electron in its outer shell, so doping with this element creates
'p-type' (for positive) material that can conduct via positive charge carriers
called 'holes'.
A MOSFET can act as an electronic switch,
controlling the flow of current in one circuit by applying a voltage on
another. This is a requirement of all digital electronic circuits. If a voltage
is applied between the source and the drain, no current will flow, and the
MOSFET is turned off. This is because like charges repel each other, so
electrons can't flow from the p-type into the negative n-type material.
However, if a negative voltage is applied to the gate (which is insulated from
the p-type material because of the silicon dioxide layer), the electrostatic
charge repels electrons from the n-type material and draws in holes from the
p-type regions. This causes a p-type channel to be created just below the gate,
and accordingly a conductive path exists between the source and the drain. The
MOSFET has, therefore, been turned on. </p>
7. Connecting the MOSFETs with copper tracks
Once all of this has been done, the wafer will
contain billions of MOSFETs. In order for them to work together as circuits,
they need to be connected together to produce lots of individual chips, each of
them still containing millions of MOSFETs. The process used by Intel is as
follows:
(A) The initial state of the MOSFETs on the
wafer.
(B) Before the addition of copper circuitry can
be carried out, a layer of insulation has to be applied to the wafer so that
the interconnecting tracks don’t short all the MOSFETs. Silicon dioxide is used
as the insulator, and this layer is built up on the surface of the wafer either
by oxidising it in a furnace or by a process of chemical vapour deposition.
With the entire surface of the wafer covered in
an insulating layer of silicon dioxide, it’s no longer possible to make
connections to the source, drain and gate of the MOSFETs. There are a number of
ways of restoring connections, but for simplicity’s sake we’re going to
describe an up-and-coming method called ‘double damascene’. This method
involves two damascene steps – one to create tungsten connecting pins and the
second to make copper interconnects.
(C) Hydroflouric acid is used to etch holes in
the silicon dioxide insulation (through a layer of photoresist).
(D) After that, trenches in the pattern of the
required interconnection tracks are etched into the silicon dioxide through
another photoresist layer.
(E) A top layer of copper is then applied by
electro-plating. This fills the trenches and holes to make contact with the
underlying MOSFETs. The resultant metallic pins that protrude through the
insulating layer are called ‘vias’.
(F) The wafer is now covered in a layer of
copper. The final stage is to take this off. In a process called
chemical-mechanical polishing, the excess copper is removed so that the desired
amount is left to form tracks in the trenches and holes.
8. Completing the circuit
It’s not always feasible to wire up a circuit
without wires crossing. If there was just one rogue interconnection, any tracks
that crossed would short. To avoid this, MOSFETs have more than one metallic
layer, each insulated by another layer of silicon dioxide and connected using vias.
9. Sorting the good chips from the bad
All being well, the wafer should now contain a
couple of hundred dies (the official name for chips), but in reality, not all
of them will work correctly. Semiconductor manufacturers tend not to publish
these figures, but industry experts consider a typical yield (the percentage of
working dies on a wafer) to be about 60 per cent. The next job is therefore to
find out which dies are working, a task that is carried out by a wafer probe.
This piece of hardware uses pins that line up with the contacts on a die,
through which electrical signals can be passed to put the processor through its
paces. To sort the wheat from the chaff, dies are categorised as ‘functional’
or ‘non-functional’, but there might also be several examples of partially
functional dies. Processors in which only some of the dies are working can
still be sold as a lower-specification product.
After all of the dies have been tested, the wafer
is sawn up into individual dies that are sorted and deployed according to the
results of the wafer test.
10. Packaging to survive the real world
We might have a fully working die now, but, as it
stands, it’s much too fragile to ship to a motherboard manufacturer.
Furthermore, the die has hundreds or thousands of connections to the outside
world, but it’s only a few millimetres square, making it far too fiddly for an
electronics company to make connectors for it. The final step, therefore, is to
encase the bare chip into a package that most people would think of as a
‘processor’. Several methods are available for this process. Whichever one is
used, the end result is that the die is firmly attached to the package, and
electrical connections are made between the contacts on the die and the
contacts on the package. A final test on the finished assembly is all that’s
needed before the processor can be shipped to a manufacturer and ultimately
used to power a computer.
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