472 F.M. Ross
generates point defects which deform the graphitic sheets, forming
new structures (Ugarte, 1992; Banhart, 1997), while irradiation of mate-
rials such as Cu implanted with C causes graphitic onions to grow (Abe
et al., 2002). Familiar or new C and BN structures, and even formation
of diamond from graphite, can thus be observed in situ (Ugarte, 1992;
Ru et al., 1996; Niihara et al., 1996; Banhart, 1997, 1999, 2003; Bengu and
Marks, 2000; Roddatis et al., 2002; Troiani et al., 2003; Gloter et al., 2004;
Wang et al., 2005).
Carbon nanotubes are of particular interest, and can be grown in situ
by introducing a precursor gas such as methane, propylene, or acety-
lene over a catalyst (Sharma and Iqbal, 2004; Sharma et al., 2005).
During growth, individual catalyst particles change their shape, and
nucleation sites can be identifi ed (Helveg et al., 2004). Once grown,
carbon nanotubes can be modifi ed with the beam (Terrones et al., 2000,
2002) to produce more complex structures.
3.5 Epitaxial and Polycrystalline Thin Film Growth
The experiments in Section 3.4 have shown the exciting possibilities
for controlled environment growth of nanostructures. Continuous thin
fi lms can also be grown in situ, and this allows important processes
such as nucleation, development of surface morphology, and relaxation
to be observed. Although some studies describe polycrystalline fi lm
growth (for example Al; Drucker et al., 1995), most systems examined
in situ have been epitaxial. These include Au on MgO (Kizuka and
Tanaka, 1997a, b), Ge on Si (see below), and silicides on Si (Section 2).
These experiments can provide detailed and quantitative information
if growth conditions such as fl ux and temperature are calibrated
carefully.
The most detailed studies have examined Ge and SiGe epitaxy on
Si. This is a “test system” for studying epitaxial growth phenomena
which also has great relevance to the development of microelectronic
devices. A true UHV environment is required for the experiments, as
the Si substrate foil is cleaned by heating in UHV to above the oxide
desorption temperature. Growth is then carried out by UHV-CVD
using gases such as disilane or digermane. Growth was observed by
Krishnamurthy et al. (1991) in STEM, and by Minoda and Yagi (1996)
and Ichikawa et al. (1998) in REM. But most work in this system has
been carried out using conventional weak beam imaging in plan view,
giving the highest sensitivity to strain fi elds (Figure 6–17). LeGoues et
al. (1996) and Hammar et al. (1996) grew Ge on Si(111) and (001) in situ,
clearly imaging the initial surface reconstruction, the nucleation of Ge
islands, and later their growth and coalescence. The structures pro-
duced depend strongly on growth conditions. By varying the parame-
ters, a range of fascinating phenomena now known to be common in
other epitaxial systems was observed, such as the change in island
shape during the introduction of stress-relieving dislocations (LeGoues
et al., 1994, 1995). The range of structures observed in these studies
would have been tedious to capture ex situ, and dynamic phenomena