The key-ingredient to surface science experiments is ultra-high vacuum.
This means pressures in the 10
mbar range and below. Only such a low
pressure will assure that a surface stays clean for a time
long enough to do some experiments (we
will see later how to obtain a clean surface). In the following, some
important parts of UHV technology are described. To get a feel for it
we will go down to the lab during the exercise and look at the
hardware!
We can quickly estimate the vacuum requirements for surface science. Let's imagine a surface in the vacuum. The number of gas molecules impinging on the surface is
where m is the molecular mass in kg and M is the molecular mass in
units of the atomic mass constant.
The usual units for the pressure in vacuum technology are torr or
mbar (1 torr = 1.3332 mbar = 133.32 Pascal). For a pressure of
mbar and a temperature of 300K we find
As an order of magnitude value a surface has
atoms per
square centimetre. This means that if every rest-gas
molecule at the above conditions sticks to the surface the latter will only
stay clean for a second or so. If we are not willing to tolerate more
than, say, a percent of contaminating rest-gas molecules on the
surface then the pressure has to be in the UHV region.
It is also interesting to calculate the mean free path of the molecules at a given pressure, i.e. the mean distance before hitting another molecule. It is
where
is the molecular diameter. For typical UHV pressures the
mean free path of the molecules is many meters. This means that it is
much more likely that the molecule hits the walls of the vacuum vessel
than another molecule. We come back to this later.
In order to achieve UHV conditions two stages of pumping are needed
(see Fig
).

Figure: Pumping of a UHV system.
A roughing pump is used to pump the system down in the
mbar
region. A typical pump is an oil-sealed rotary vane pump
as shown in
Fig.
.

Figure: A oil-sealed rotary vane pump. Principle of operation:
(a) gas from the vacuum system is expanded into the pump
and (b) the gas is pushed through the pump exhaust.
The pump of choice for the second stage is a so-called turbomolecular
pump (see Fig.
).

Figure: A turbomolecular pump. Picture: Leybold Vacuum GmbH, used with permisssion.
Once the low pressure has been achieved it can also be maintained by
another type of pump, the so-called ion pump
shown in Fig.
.

and 10
mbar.
In order to reach a low pressure in a short time it is necessary to
perform a so-called bakeout of the whole vacuum system. During the
bakeout the system is heated to at least 100-200
C for an
extended period of time (24h or so). The heating causes a fast removal
of the impurities adsorbed on the walls of the vacuum system (mostly
water). The need
for baking systems renders working with UHV chambers rather
time-consuming. It also requires that the system is build only of
components which can withstand high temperatures for a long
period of time.
For the roughing pump stage one can use a so-called Pirani gauge
to
measure the pressure. The idea of this instrument is to measure the
resistance of a heated wire placed into the vacuum system. The
resistance depends on the temperature of the wire. At high pressures
the wire will be cooled by collisions with the rest gas molecules,
i.e. by warming up the rest gas. As the pressure is reduced this
cooling mechanism gets less effective and the temperature of the wire
rises. The resistance of the wire can be calibrated as function of
the pressure. Pirani gauges work from ambient pressure down to about
10
mbar.
For lower pressures, a so-called ion gauge
can be used. It is shown in
Fig.
.

and 10
mbar. The low pressure limit is given by an
unwanted effect: when an electron hits the cage it produces a photon
which then can cause the emission of an electron from the centre
wire. While this effect sounds extremely unlikely it becomes the
dominant contribution to the current at very low pressures.
We have already seen above that all materials in the vacuum system have to be able to withstand high temperatures during the bakeout. Another important criterion is that the vapour pressure of the materials has to be very low at the normal operating temperature of the vacuum system. The following table gives the temperatures in K to generate a certain vapour pressure.
Obviously, the first materials in the table are very undesirable in a vacuum chamber! The last two are important for the actual construction: most chambers are made of stainless steel and almost all the filaments (for example in the ion gauges ) are made of W. Electrical insulators are made of ceramics with a low vapour pressure.
A vacuum vessel has many circular flanges where windows or equipment with the same flange type can be bolted on. These flanges have sharp knife-edges profiled on their operating sides. A leak-tight seal between the two flanges is achieved by placing a copper gasket between the knife edges and pressing it until it is tight. It is necessary to use copper (instead of simply ``rubber'') because of the bakeout.
When putting the pumps on the chamber one has to consider the concept of conductance. Keep in mind that in the low pressure region the mean free path of the molecules is much longer than the dimensions of the vacuum system. It is therefore clear that it does not make sense to connect a very powerful pump to the vacuum system via a small diameter tube with many right angles. The rest-gas molecules will never find their way to the pump.
Another important requirement is to linearly move items inside the vacuum or to rotate them. Most of the motions are transferred from outside via stainless steel bellows. We will look at some linear and rotational feedthroughs in the lab.
Finally, it is desirable to measure the chemical compositions of the rest gas in the system. This can be used to see if there is a leak in the vacuum chamber, to check the purity of gases used for the experiment and to leak-test the system. To do this, one directs a stream of He gas on the suspected leak from outside the system. If one observes a increase in the partial pressure of He inside, the leak has been found.
A so-called quadrupole mass spectrometer
is shown in Fig.
. It consists of three sections. In the first, rest-gas
atoms are ionized just as in the ion gauge. These ions are then
accelerated and focused into the second section, the actual mass
filter. It consists of four bars which set up an electrical
quadrupole field, driven by the superposition of a DC and a radio
frequency AC voltage. The filter works such that only ions with the
same m/e can pass it. The last element of the spectrometer is the
ion detector which contains an electron multiplier leading to an
amplification of the signal by a factor 10
-10
. The
lower limit of the partial pressures which can be detected with such a
spectrometer is about 10
mbar.

Figure: A quadrupole mass spectrometer
A typical mass spectrum is shown in Fig.
. The main
residual gases in the vacuum are hydrogen, water, carbon monoxide and
some carbon dioxide. It is important to note that the criterion
is m/e and not simply m! It means that doubly charged ions appear
as particles with half the mass in the spectrum. CO does for example
not only give a peak at m=28 but also one at m=14 due to double
ionization. The gases are also dissociated in the spectrometer such
that one does not only find one peak for single-ionized water at m=18
but also peaks at m=16, 17 and 2 for the fragments.

Figure: A typical mass spectrum.
After the bakeout of the system, the partial pressure of water will be strongly reduced and the total pressure will be determined by CO and atomic hydrogen. If there is an air leak in the system this would show up as peaks of 28 and 32.