 |
In this
subchapter we will give an outline of how to progress from the simple version
of Ohms
"Law", which is a kind of
"electrical" definition for a black box, to a formulation of the same
law from a materials point of view
employing (almost) first principles. |
|
|
|
 |
In other words: The electrical engineering point of view is: If a
"black box" exhibits a linear relation between the (dc) current
I flowing through it and the voltage U
applied to it, it is an ohmic
resistor. |
|
|
 |
That is illustrated in the picture: As long as the
voltage-current characteristic you measure between two terminals of the black
box is linear, the black box is called an (ohmic) resistor. |
|
|
 |
Neither the slope of the I-U-characteristics
matters, nor what's in the box or what materials are involved. |
|
 |
The Materials Science point of view is quite different,
it is essentially the reverse of the electrical engineering point of view.
Taken to the extreme, the Materials Science point of view is simply: |
|
|
 |
Tell me what kind of material is in the black box, and I tell
you:
- If it really is an ohmic resistor, i.e.
if the current relates linearly to the
voltage for reasonable voltages and both
polarities.
- What its (specific) resistance will be, including its temperature
dependence.
- And everything else of interest.
|
|
|
|
|
|
|
 |
In what follows we will see, what we
have to do for this approach. We will proceed in 3 steps. |
|
|
|
 |
In step one
and two, contained in this sub-chapter we
simply reformulate Ohms law in physical
quantities that are related to material properties. |
|
 |
In other words, we look at the properties of the
moving charges that produce an electrical current. But we only define the necessary quantities; we do not calculate
their numerical values from basic
principles. We will, however, calculate some numbers, based on experimental
input. |
|
 |
In the third
step - which is the content of many chapters - we will find ways to actually
calculate (some of) the important
quantities, in particular for semiconductors. |
 |
As it will turn out, this is not just
difficult with classical physics, but simply impossible. We will need a good dose of quantum
mechanics and statistical thermodynamics to get results. |
|
|
|
|
 |
First we switch from current I and
voltage U to the current
density j
and the field
strength
E, which are not only independent of the (uninteresting)
size and shape of the body, but, since they are
vectors, carry far more information about the
system of interest. |
|
 |
This is easily seen in the schematic drawing
below. |
|
|
|
|
|
|
 |
Current
density j and field
strength E may depend on the coordinates,
because U (taken as the local potential) and I
depend on the coordinates, e.g. in the way schematically shown in the picture
to the left. However, for a homogeneous material with constant cross section,
we may write |
|
|
|
|
|
|
 |
with F = cross sectional area of the reference
plane considered. The direction of the vector j is parallel to the
normal vector f of the reference area considered; it also
may differ locally. So in full splendor we must write |
| |
| j(x,y,z) = |
I(x,y,z)
F |
· f |
|
|
|
|
|
|
|
 |
The "global" field strength is |
|
|
|
|
|
|
|
|
|
|
With l = length of the body. If we
want the local field strength
E(x,y,z) as a vector, we have, in
principle, to solve the
Poisson
equation |
|
|
|
|
| Ñ ·
E(x,y,z) = |
r(x,y,z)
ee0 |
|
|
|
|
|
|
 |
With r(x,y,z) = charge density. For a
homogeneous material with constant cross section, however,
E is parallel to f and constant
everywhere, again something that is clear without calculation. |
 |
In order to make things easy, we realize that for
a homogenous material of length l with constant cross-sectional
area F, the field strength E and the current
density j do not depend on position - they have the same
numerical value everywhere. |
|
 |
For this case we can now write down Ohms law with
the new quantities and obtain |
|
|
|
|
|
| j · F = I =
|
1
R |
· U |
= |
1
R |
· E · l |
|
|
|
|
|
 |
The fraction l/ F ·
R obviously (think about
it!) has the same numerical value for
any homogeneous cube (or homogeneous
whatever) of a given material; it is, of course, the
specific
conductivity s |
|
|
|
|
|
|
|
|
|
|
 |
In the equation above we have also defined the
specific
resistivity
r with the unit [r]
= Wm, or - more frequently used - Wcm. |
|
 |
The specific
resistivity obtained in this way is necessarily identical to what
you would define as specific resistivity by looking at some rectangular body
with cross-sectional area F and length l. You would
assume that R is proprotional to l, and inversely
proportional to F, and the proportionality constant you would
call "specific resistivity". |
|
 |
A 1 cm3 cube of homogeneous
material having the specific resistivity r
has the resistance R = r, if r is given in Wcm. |
|
 |
Of course, we will never mix up
the specific resistivity r with the charge density
r or general densities r, because we know from the context what is
meant! |
 |
The specific conductivity has the dimension [s] = W1cm1 and is the
quantity one uses if looking at conduction mechanisms etc. |
 |
The specific
resistivity is more prominent in technological terms and for
charcaterizing materials and you should at least have a feeling for some
representative numbers by remembering: |
|
|
|
|
|
| r (metal) |
» |
2 µWcm |
| |
|
|
| r (semicoductor) |
» |
1 Wcm |
| |
|
|
| r (insulator) |
» |
1 GWcm |
|
|
|
|
|
 |
Restricting ourselves to
isotropic and homogenoeus materials, restricts s and r to being
scalars with the same numerical value everywhere, and Ohms law now
can be formulated for any material with weird shapes and being quite
inhomogeneous; we "simply" have |
|
|
|
|
|
|
|
|
 |
Ohms law in this vector
form is now valid at any point
of a body, since we do not have to make assumptions about the shape of the
body. |
|
 |
To appreciate this, take an arbitrarily shaped
body with current flowing through it, cut out a little cube (with your
"mathematical" knife) at the coordinates (x,y,z)
without changing the flow of current, and you must find that the local current density and the
local field strength obey the equation given above
locally. |
|
|
|
|
|
|
|
|
|
|
 |
Of course, obtaining the external current
I flowing for the external voltage U now needs
summing up the contributions of all the little cubes, i.e. integration over the
whole volume, which may not be an easy thing to do. |
 |
Still, we have now a much more powerful version of
Ohms law! But we should now harbor a certain suspicion: |
|
 |
There is no good reason why
j must always be parallel to E. This means that
for the most general case s is not a scalar quantity, but a
tensor; s =
sij.
(There is no good way to write tensors in html; we use
the ij index to indicate tensor properties. |
|
 |
Ohms law then writes |
|
|
|
|
|
jx = sxx
· Ex + sxy · Ey +
sxz ·
Ez
jy = syx
· Ex + syy · Ey +
syz ·
Ez
jz = szx
· Ex + szy · Ey +
szz ·
Ez |
|
|
|
|
|
 |
For anisotropic inhomogeneous materials you have
to take the tensor, and its components will all depend on the coordinates -
that is the most general version of Ohms law. |
|
 |
Note that this is not so general as to be meaningless: We still have
the basic property of Ohms law: The local current density is directly
proprotional to the local field strength (and not, for example, to
exp [const. · E] ). |
 |
Our goal now is to find a relation that allows to
calculate sij for a given material
(or material composite); i.e. we are looking for |
|
|
|
|
|
| sij =
sij(material, temperature, pressure,
defects... ) |
|
|
|
|
 |
Electrical current needs charged and mobile "things", or charge carriers that are mobile. Note that we do not automatically assume
that the charged "things" are always electrons. Anything charged and mobile will do. |
 |
What we want to do now is to express sij in terms of the properties of the carriers present in the material
under investigation. |
|
 |
To do this, we will express an electrical current as a
"mechanical" stream or current of (charged) particles, and compare
the result we get with Ohms law. If you have problems visualizing this, check
this Basic module. |
 |
First, lets define an electrical current in a wire
in terms of the carriers flowing through that wire. There are three crucial points to consider: |
 |
1. The external electrical current as
measured in an Ampèremeter is the result of the net current flow through any cross section of an
(uniform) wire. |
|
 |
In other words, the measured current is proportional to the
difference of the number of carriers of the
same charge sign moving from the left to
right through a given cross sectional area minus the number of carriers moving from the
right to the left. |
|
 |
In short: the net current
is the difference of two partial currents
flowing in opposite directions: |
|
|
|
|
|
|
|
|
|
|
 |
Do not take this point as something simple! We
will encounter cases where we have to sum up 8 partial currents to
arrive at the externally flowing current, so keep this in mind! |
 |
2. In summing up the individual
current contributions, make sure the signs are
correct. The rule is simple: |
|
 |
The electrical current is (for historical reasons)
defined as flowing from the + pole to the pole. For a
particle current this means: |
|
|
|
|
|
|
|
|
|
|
 |
In words: A technical current I flowing from
+ to may be obtained by negatively charged carriers flowing in the opposite direction (from to +),
by positively charged carriers flowing in
the same direction, or from both kinds of
carriers flowing at the same time in the proper directions. |
|
 |
The particle currents of differently charged particles then must be added! Conversely, if negatively charged carriers
flow in the same directions as positively charged carriers, the value of the
partial current flowing in the "wrong" direction must be subtracted
to obtain the external current. |
 |
3. The flow of
particles through a reference surface as symbolized by one of arrows above, say
the arrow in the +x -direction, must be seen as an average
over the x -component of the velocity of the individual particles
in the wire. |
|
 |
Instead of one arrow, we
must consider as many arrows as there are particles and take their average. A more detailed picture of a wire at
a given instant thus looks like this |
|
|
|
|
|
|
|
|
|
|
 |
An instant later it looks entirely different in detail, but exactly the same on average! |
|
 |
If we want to obtain the net flow of particles through the wire (which is obviously
proportional to the net current flow), we
could take the average of the velocity components <v+x>
pointing in the +x direction (to the right) on the left hand
side, and subtract from this the average <vx>
of the velocity components pointing in the x direction (to
the left) on the right hand side. |
|
 |
We call this difference in
velocities the drift
velocity vD
of the ensemble of carriers. |
|
 |
If there is no driving force, e.g. an electrical field, the
velocity vectors are randomly distributed and <v+x> =
<vx>; the drift velocity and thus net current is zero
as it should be. |
 |
Average properties of ensembles
can be a bit tricky. Lets
look at some properties by considering the analogy to a localized
swarm of summer flies
"circling" around like crazy, so that the ensemble looks like a small
cloud of smoke. A more detailed treatment can be found in the
advanced section. |
|
 |
First we notice that while the individual fly moves around quite fast, its vector velocity vi averaged
over time t, <vi>t, must be zero as long as the swarm as
an ensemble doesn't move. |
|
 |
In other words, the individual flies, on average, move just as often to the left as to the
right, etc. The net current produced by all
flies at any given instance
or by
one individual fly after sufficient time is
obviously zero for any reference
surface. |
 |
In real life, however, the fly swarm
"cloud" often moves slowly around
- it has a finite drift velocity which must
be just the difference between the average movement in drift direction minus
the average movement in the opposite direction. |
|
 |
The drift velocity thus
can be identified as the proper average that gives the net current through a
reference plane perpendicular to the direction of the drift velocity. |
|
 |
This drift velocity is usually much smaller than the average
magnitude of the velocity <v> of the individual flies. Its value is the
difference of two large numbers - the average velocity of the individual flies in the drift direction minus the
average velocity of the individual flies in
the direction opposite to the drift direction. |
 |
Since we are only interested in the drift velocity
of the ensemble of flies (or in our case, carriers) we may now simplify our
picture as follows: |
|
|
|
|
|
|
|
|
 |
We now equate the current density with the particle flux density by the basic law of current
flow: |
|
 |
Current density j = Number
N of particles carrying the charge q flowing
through the cross sectional area F (with the normal vector
f and |f| = 1) during the time
interval t, or |
|
|
|
|
|
|
|
|
|
|
 |
If the charge q is negative (e.g. for electrons
we have q = e; e = elementary charge), the direction of the
electrical current is opposite to the
particle current, as it should be. In
scalar notation, because the direction of the current flow is clear, we
have |
|
|
|
|
|
|
|
|
|
 |
The problem with this formula is N,
the number of carriers flowing through the cross section F every
second. |
|
 |
A number N
of carriers is not a basic property of the material; we certainly would much
prefer the carrier density n =
N/V of carriers. In going from numbers to densities, we have
to chose the volume V = F · l in such a
way that it contains just the right number N of carriers. |
|
 |
Since the cross section F is given, this means
that we have to pick the length l in such a way, that all
carriers contained in that length of material will have moved across the
internal interface after 1 second. |
|
 |
This is easy! The trick is to give l just that
particular length that allows every carrier
in the defined portion of the wire to reach the reference plane, i.e. |
|
|
|
|
|
|
|
|
|
|
 |
This makes sure that all
carriers contained in this length, will have reached F after the
time t has passed, and thus all carriers contained in the volume
V = F · vD ·
t will contribute to the current density. We can now
write the current equation as follows: |
|
|
|
|
|
| j |
= |
q · N
F · t |
= |
q · n · V
F · t |
= |
q · n · F · l
F · t |
= |
q · n · F · vD · t
F · t |
|
|
|
|
|
 |
This was shown in excessive
detail because now we have the fundamental law of
electrical conductivity (in obvious vector form) |
|
|
|
|
|
|
|
|
|
 |
This is a very general equation relating a particle current (density) via its drift velocity to an electrical current (density) via the charge
q carried by the particles. |
|
 |
Note that it does not matter at all, why an ensemble of charged particles moves on
average. You do not need an electrical field as
driving force anymore. If, for example, a concentration gradient
induces a particle flow via diffusion, you
have an electrical current too, if the particles are charged. |
|
 |
Note also that electrical current flow
without an electrical field as primary
driving force as outlined above is not some
odd special case, but at the root of most electronic devices that are more
sophisticated than a simple resistor. |
|
 |
Of course, if you have different particles numbered
i, with different densities, drift velocities, and charges, you
simply sum up the individual contributions as pointed out above: j =
Si (qi ·
ni · vi) |
 |
All we have to do now is to compare our equation
from above to Ohms law in its general form from
above: |
|
|
|
|
|
|
|
|
|
|
 |
We then obtain |
|
|
|
|
|
| s |
= |
q · n · vD
E |
:= |
constant |
|
|
|
|
|
 |
If
Ohms law holds, s must be a
constant, and this implies by necessity
|
|
|
|
|
|
|
|
|
|
|
 |
This is a simple but far reaching equation, saying something
about the driving force of electrical currents (= electrical field strength
E) and the drift velocity of the particles in the material. |
|
 |
What this means is that if
vD/E = const. holds for any (reasonable) field E, the material
will show ohmic behavior. We have a first condition
for ohmic behavior expressed in terms of material properties. |
|
 |
If, however, vD/E is constant (in
time) for a given field, but with a value
that depends on E, we have s =
s(E); the behavior will not be ohmic! |
 |
The requirement vD/E =
const. for any electrical field thus
requires a drift velocity in field direction for the particle, which is
directly proportional to E. This leads to a simple
conclusion: |
|
 |
This is actually a rather strange result! A charged particle
in an electrical field experiences a constant force, and Newtons first law
tells us that this will induce a constant accelerations, i.e. its velocity
should increase all the time! Its velocity therefore would grow to infinity -
if there wouldn't be some kind of friction. |
|
 |
We thus conclude that there must exist some mechanism that acts like a
frictional force on all accelerated particles, and that this frictional force
in the case of ohmic behavior must be in a form where the average drift velocity obtained is proportional to the
driving force. |
 |
Since vD/E =
constant must obtain for all (ohmic) materials under investigation, we may
give it a name: |
|
|
|
|
|
vD
E |
= |
µ |
= Mobility = |
Material constant |
|
|
|
|
|
|
 |
The mobility
µ of the carriers
has the unit [µ] = (m/s)/(V/m) = m2/V · s. |
|
 |
The
mobility µ
(Deutsch: Beweglichkeit) then is
a material constant; it is determined by
the "friction", i.e. the processes that determine the average
velocity for carriers in different materials subjected to the same force
q · E. |
|
 |
Friction,
as we (should) know, is a rather
unspecified
term, but always describing energy transfer from some moving body to the
environment. |
|
 |
Thinking ahead a little
bit, we might realize that µ is a basic material constant even in the absence of electrical fields. Since it
is tied to the "friction" a moving carrier experiences in its
environment - the material under consideration - it simply expresses how fast
carriers give up surplus energy to the lattice; and it must not matter how they
got the surplus energy. It is therefore no suprise that µ pops up
in all kinds of relations, e.g. in the famous
Einstein -
Smoluchowski equation linking
diffusion coefficients and mobility of particles. |
|
|
Thinking ahead a little
bit more, we realize that the mobility of carriers is an extremely important
material parameter because it describes "somehow" how quickly
carriers can respond to an electrical field and therefore if they can follow
rapidly changing electrical fields - e.g. in a micorpocessor running at 4
GHz. Very large amounts of money are spend right now (2006) to
increase the carrier mobility in Si - see the
link for a taste treat of what
that means. |
 |
We now can write down the
most general form of Ohms law applicable to
all materials meeting the two requirements: n = const. and
µ = const. everywhere. It is expressed completely in particle (=
material) properties. |
|
|
|
|
|
|
|
|
|
 |
The task is now to calculate n and
µ from first priciples, i.e. from only knowing what atoms we are
dealing with in what kind of structure (e.g. crystal + crystal defects) |
|
 |
This is a rather formidable task since s variies over a extremely wide range, cf. a
short table with some
relevant numbers. |
 |
In order to get acquainted with the new entity
"mobility", we do a little exercise: |
|
|
|
|
|
|
|
|
|
|
|
|
 |
Since we like to give s as a positive number, we always take only the
magnitude of the charge q carried by a particle. |
|
 |
However, if we keep the sign, e.g. write
s = e · n ·
µe for electrons carrying the charge q =
e; e = elementary charge, we now have an indication if the particle
current and the electrical current have the same direction (s >
0) or opposite directions (s < 0)
as in the case of electrons. |
|
 |
But it is entirely a matter of taste if you like to schlepp1) along the signs all the time, or
if you like to fill 'em in at the end. |
 |
Everything more detailed then this is no longer
universal but specific for certain materials. The remaining task is to
calculate n and µ for given materials (or groups of
materials). |
|
 |
This is not too difficult for simple
materials like metals, where we know that there is one (or a few) free
electrons per atom in the sample - so we know n to a sufficient
approximation. Only µ needs to be determined. |
|
 |
This is fairly easily done with classical physics; the
results, however, are flawed beyond repair: They just do not match the
observations and the unavoidable conclusion is that classical physics must not
be applied when looking at the behavior of electrons in simple metal crystals
or in any other structure - we will show this in the immediately following
subchapter 2.1.3. |
 |
We obviously need to resort to
quantum theory and solve the Schrödinger
equation for the
problem. |
|
 |
This, surprisingly, is also fairly easy in a simple
approximation. The math is not too complicated; the really difficult part is to
figure out what the (mathematical) solutions actually mean. This will occupy us for quite some
time. |
|
|
|
|
|
|
|
|
|
© H. Föll (MaWi 2 Skript)