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One of the major causes of the degradation of VLSI devices is the damage created by high-energy ('hot') electrons as they travel from source to drain along the channel: Some electrons gain from the electric field enough kinetic energy to be injected into the silicon dioxide gate-insulator. This energy then becomes - somehow - the source of degradation: Atomic bonds are broken at the Si-SiO2 interface and/or within the oxide. Ultimately, the electric charge associated with these defects will cause a shift of the threshold voltage of the device, increased Coulomb scattering for electrons in the channel - and so a degradation of the mobility -, or even catastrophic dielectric breakdown of the gate insulator. In any event, bad news.
Understanding the microscopic physics involved is no easy feast:
There are even more problems concerning, for example, the three-dimensional atomic structure of the interface and how
one could treat tunneling in a more realistic fashion than what's usually implied by 'abrupt, square' potential barriers;
the role of inelastic tunneling processes; the effect that the electron gas in the Si channels has on the dielectric properties
of the interfacial region and on electron tunneling and injection, etc.
etc. But those few problems mentioned above are sufficient to give an idea of the complexity of the problem.
Figure 1. Schematic diagram of the Si-SiO2 interfacial region illustrating the issue which must
be resolved in order to understand electron injection into silicon dioxide.
(Adapted from Ref. [5]).
The typical 'testing ground' for models attempting to model electron injection into SiO2 is the
simulation of the devices Ning and co-workers[4] employed to measure the injection probability.
These are long-channel MOSFETs on p-type substrates. By connecting the source and drain contacts together,
negatively biasing the substrate, positively biasing the gate, and shining light on the device, one creates electron-hole
pairs deep in the substrate. While the holes drift away to the substrate, electrons are accelerated towards the
interface, 'falling down' the large substrate-to-channel 'cliff'. Most of the electrons 'bump' against the
Si-SiO2 barrier, thermalize, and are eventually collected by the source or the drain contacts and
contribute to the 'channel current', Ichannel.
But a few electrons (typically, one in a million or billion!) will be lucky
enough to acquire so much energy as to be injected by tunneling at high energy into the oxide, or even jump over
the top of the barrier. These electrons will be measured as 'gate current', Igate.
By varying the substrate bias, Vsub, and the gate bias, Vgate,
from the ratio Ichannel/Igate one extracts the injection probability as a function
of the accelerating potential and field in the oxide. Figure 2 illustrates the situation for a substrate bias of
7.5 V.
DAMOCLES has been used to mimic the experimental scenario and confirm the following answers to the questions raised above
(See Refs. [5]
and [6] for ample discussion of these issues):
The success of a model in predicting (or, in our case, postdicting) experimental results should not be
considered proof that the model is correct. After all, the
Copernican model
[A]
of the solar system, in its original -- if not historically correct-- formulation based on circular orbits,
didn't improve at all the ephemerides computed on the basis of the mathematically -- but not
'psychologically'-- equivalent Tycho Brahe's model
[B], or even of the centuries-old
Ptolemaic system
[C]. (The Prutenic Tables, which replaced the Alfonsine Tables based on the ptolemaic system, did indeed
improve upon the latter ones, but at the expense of complicating the Copernican system with many unaesthetical circles and epicycles,
bringing it almost at the level of the ptolemaic model).
This is an example of an 'incorrect' theory (Thyco's) yielding better agreement with the data ("save the phenomena", in
the jargon of those times) than a 'correct' (Copernicus') one. What really matters is that Copernicus' model planted the seed
of a 'full-band solar-system model'
[D], which finally allowed
predictions
[E] to be made, which is what counts.
Yet, the arguments we have listed above, and the success shown in Fig. 3
are at least suggestive that the gross features of the model are not too far off the mark (...but: Is DAMOCLES like
Ptolemy or is it like Kepler?)
The major problem of the model implemented in DAMOCLES remains its heavy computational cost. For some, this
is a small price to pay for physical correctness. For others, more empirical and faster methods may be preferable.
The abstract
of an article[6] on which this page is based is available from the
IBM Research Division CyberDigest.
The images of models of the solar-system are from:
Some questions about the physics
Ning's experiment and DAMOCLES simulation
Some answers about the physics
Some astronomical conclusions
References
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