Theoretical Work on the Resolution of AFM
One of the most
potent achievments in AFM (atomic force microscopy) in the recent
years was the use of a new type of cantilever called the qPlus
sensor[1]. This much stiffer sensor allowed to image the surface
in distances of a view tenth of a nanometer. With this amazing
new technology
Giessibl
et. al. succeeded to obtain "subatomic resolution"[2]. This
signifies that the images resolved substructures within an atomic
dimension. The questions now to be raised are: how to understand
these subatomic features? How is it possible that with a tip,
extended on the scale of several nanometer, such small features
can be resolved?
Figure
1
 |
An important clue to understand the substructures is the
observation that the sample-tip distance is of the order of some
angstroems. This is the regime of atomic orbitals, so the
structures may be ascribed to orbital overlap and the formation of
covalent bonds between tip and sample. If, for simplicity, we
assume the tip to have one front atom with two dangling sp3-bonds
(we are talking about a silicon 100-tip) one can imagine that
these two dangling bonds participate in creating such
substructures in the atomic image. The images were taken on a
silicon 111(7x7) surface. This surface is well investigated and
it is considered to have one dangling sp3 bond perpendicular to
the surface per surface atom. For our theoretical treatment we
focus, in a first step, just on one atom of this complicated
surface and correspondingly take the one perpendicular dangling
bond into account. Our model tip also consists of only one atom
namely the front atom with the two dangling bonds. So our problem
is reduced to the overlap of two imaging tip orbitals and one
imaged surface orbital. The actual geome try is shown in figure 1.
Figure
2 |
With this extremely
simplified model we can easily perform a LCAO calculation to get
the energy profile of this configuration. From the profile we
deduce the forces between the tip and the sample atom which are
due to covalent binding of the considered atoms. In a final step,
the frequency shift is compared to experiments. Indeed it is
possible to reproduce some aspects of the measured substructures.
We find a doublepeak (figure 2) like in the experimental data
and, moreover, this structures emerges within a reasonable
distance and energy range.
This proves within a
simple microscopic modelling that we have to deal with the
orbital configuration of both tip and sample to understand
subatomic structures in AFM and STM measurements. Actually, in
the case considered the substructures are an image of the tip.
One could think of imaging the tip with known surfaces.
Beyond this basic
approach we started to investigate the tip-sample interactions
with the LDA-method (Local Density Approximation). This state of
the art technique shows very good results in predicting bulk
properties of weakly correlated systems. It is also suitable for
more complicated situations like our tip-sample problem. We
expect to get more accurate results this way but we pay for it
with considerable more complexity in the calculations.
References
| [1] | Franz J. Giessibl, App. Phys. Lett.
76, 1470 (2000) |
| [2] | Franz J. Giessibl, S. Hembacher, H.
Bielefeldt and J. Mannhart, Science 289, 422
(2000) |