Plasmas in Deposition Processes 67
for a number of reasons. Electron ionization processes are obviously important in sustaining
the plasma, while excitation and dissociation produce reactive species that are critically
important in such processes as reactive sputter deposition, plasma-assisted etching, PACVD,
and plasma polymerization. The variety of excited and ionized species, as well as radicals
(reactive dissociation products), in a plasma has a much different chemical reactivity than
those of the parent gas [64, 65]. For example, although He and Ar atoms are inert, He
+
ions
with one valence electron are chemically similar to hydrogen, while Ar
+
ions can react with
H
2
molecules to form ArH
+
ions [64]. Similarly, N
2
is largely inert, but N radicals formed
from the dissociation of N
2
are reactive and important in the formation of metal-nitride thin
films.
2.5.2 Electron–Atom Interactions
As noted, the interaction of energetic electrons with atoms can be either elastic or inelastic.
The former is sufficiently understood classically; that is, a collision of two hard spheres in
which kinetic energy and momentum is conserved. For inelastic collisions, where kinetic
energy is not conserved, the interaction is not sufficiently understood classically. Instead, it is
best understood by recognizing that the atom gains an amount of internal energy equal to the
loss of electron kinetic energy. This internal energy results in the promotion of an electron to a
higher energy level, thereby creating an excited atom. Of course, this transferred energy must
be in discrete amounts since the energy levels are quantized. Excited states are limited in their
lifetimes and will decay by emitting a photon as the electron falls back to its ground state level.
Excited states called metastables, however, can last for very long times and can be significant
in low-pressure discharges (see Section 2.5.4). If there is enough energy transferred, the
electron can be liberated from the atom producing an ion [66]. For large impacting electron
energies, the process could leave the ion in an excited state, the secondary (ejected) electron
could have excess kinetic energy, or the impacting electron could retain a large amount of
energy. All of these are best described by noting that an electron passing close by an atom does
not simply knock an electron to a higher orbit or out of the atom, but produces a perturbation
of the atom leading to either excitation or ionization.
In making plasma calculations, the average energy W
ei
spent by an electron in creating an
electron–ion pair in a given gas or gas mixture is often used. Values of W
ei
for various atoms
and molecules are shown in Table 2.4 along with values for the ionization potential I and first
excited states. Typically, W
ei
/I ≈2–3. It should be noted that W
ei
is determined using
high-energy electrons and the values shown in Table 2.4 are valid for energies above several
keV. At low impacting energies more energy is consumed in excitation and elastic collisions,
thus more energy is required to produce an ion–electron pair. For plasmas with average
electron energies in the range of a few eV, the values of W
ei
will be larger than those given in
Table 2.4 [67].