about quantum wells and quantum barriers
TRANSCRIPT
ABOUT QUANTUM WELLS AND QUANTUM BARRIERS
Flavio Aristone
Institute of Physics – Federal University of South Mato Grosso, Brazil
79070-900 Campo Grande, MS – Brazil
ABSTRACT
A particular discussion of the ground state energy level and the corresponding wave
function shape is discussed for quantum well systems aiming to provide a better
comprehension of such confinement effects for quantum mechanics beginners. The results
have been numerically obtained from the solution of one dimensional time independent
Schrödinger equation for a confined space inside which either a barrier or a quantum well is
grown. The wave function and energy level for the ground state is extensively analyzed in
both scenarios, when the inserted barrier height increases considerably and when the
inserted quantum well becomes extremely thin and deeper simulating a delta-doped
system. The physics interpretations of these results are particularly rich and may become
useful to undergraduate students not only of physics courses but also for other domains
where structural concepts of quantum theory are necessary, required or wanted.
KEYWORDS: Quantum well, quantum barrier, wave function, Eigen state of energy,
confinement effects, delta-doped potential.
I. INTRODUCTION
Quantum wells and quantum barriers are important examples frequently used to
introduce quantum effects before getting into the postulates and the specific mathematics
tolls necessary to develop a more formal discussion of quantum mechanics. Actually,
quantum wells and quantum barriers are routinely discussed during classes of Modern
Physics even if the Schrödinger equation has to be imposed without further explanations.
Students of physics courses normally don’t have enough time to completely absorb the
first ideas introduced by teachers of quantum mechanics or modern physics when they are
presented to quantum effects. Normally quantum mechanics is presented as something
describing effects that are not allowed to occur in the classical world as, e.g. the tunneling
effect. Another startling feature appearing already at the first contact and associated with
quantum effects is the separation of the energy values in discrete levels that a particle is
allowed to assume, separated by inaccessible ranges of values that the particle cannot
access.
Quantum wells and quantum barriers are particularly interesting since the Schrödinger
equation can be analytically solved at every coordinate point due to the flat regions where
the potential energy is constant. Some special careful calculations must be taken at the
interfaces where the potential energy changes abruptly though, implying that the continuity
of the wave function and of its derivative have to be preserved.
The particular interest discussed in this paper is to start with a confined region leading
to confined states, actually a quantum well and slowly grow in the middle of this region
another potential energy, either an attracting well or a scattering barrier, to analyzed the
effect of such structures on the original wave function and ground state energy. The
consequence is clearly to identify the tunneling process occurring through the barrier in the
first case and notice the confinement effect that happens due to the quantum well in the
second case.
II. SCHRÖDINGER EQUATION FOR A CONFINED REGION
The Schrödinger equation may be presented in different ways. Actually the most formal
introduction presents it as the 6th postulate of quantum mechanics theory [1]. However, this
process doesn’t carry any especial understanding for this paper and we prefer to avoid such
a description in order to discuss a more direct approach directly applicable to our interests.
The system we will study is time independent as the involved potentials, the quantum
barrier and/or the quantum well don’t change as a function of time. Therefore the specific
Schrödinger equation is simply:
(1)
where are the Eigen states of the system; are the Eigen energies. is the Hamiltonian
operator describing the total energy of the system given by the sum of kinetic ( ) plus
potential ( ) energies, or:
(2)
Equation (1) looks very similar to the Hamilton-Jacobi formalism of Classical
Mechanics excepted by the presence of the new term described as the quantum state of
the particle / system. The “state” of the system is not discussed in classical theory as
classical particles are simply particles without any further discussion about it. They may be
little spheres, cubes, or simply dots having all necessary physical characteristics treated as
parameters. Equation (1) may therefore be seen as a supplementary discussion wherein the
particle, from now on called quantum system, must be somehow described before any
calculations to consider other mechanical property.
The very first conclusion is that equation (1) is completely equivalent to a problem of
matrix diagonalization since is an operator and is a number. This interpretation is
absolutely correct and is called Heisenberg formalism. Nevertheless it is also possible to
expand equation (1) as a second order differential equation, in which case the process is
called Schrödinger formalism.
It is beyond the scope of this paper to describe how equation (1) transforms into the
usual and most common form of Schrödinger equation represented in equation (3) for a one
dimensional system:
(3)
where is the Planck constant divided by and is the mass of
the particle.
Up to this point everything is plausible even if not entirely justifiable as some critical
mathematical steps have been avoided. Actually, equation (3) is frequently exhibited in
textbooks prior to the introduction of the quantum mechanics theory postulates. The first
postulate determines the meaning of , defining such a function as the mathematical
description of a quantum state. An easier physical picture of is to understand it as a
function whose modulus square represents the density of probability of finding the particle
(or the quantum state). Therefore, given the value of is the probability of
finding the particle around position within the interval .
Equation (3) is easily solved for , i.e., a constant value. An ideal quantum
well is defined by a region of constant potential surrounded by barriers of infinity height
where the wave function must not exist. Realistic quantum wells are limited by barriers of
elevated but finite values wherein the wave function may penetrate even though it must
vanish rapidly. It is this condition of confinement in both cases that imposes the
discretization of the energy levels accessible to the quantum particle.
It is not extremely complicated to solve numerically equation (3). Some typical
results are exhibited and discussed in this paper as examples. Initially we compare the
ground state energy and wave function for both cases: when the barriers of potential
energy of confinement are infinite and when they are limited to fixed values. In the second
case the wave function penetrates the forbidden region and the ground state of quantized
energy is smaller than the values found out previously.
The results expressed in this paper have been obtained through the solution of
Schrödinger equation treated generally. An indisputably confirmed numerical method, the
fourth order Runge-Kutta method [2], is applied to solve the Schrödinger equation of a
confined system limited between 0 (zero) and . Outside these limits the potential energy is
assumed to be infinite, where as a result the wave function is null. Actually, this first analysis
defines exactly a typical infinite quantum well whose width is . Conversely, when the
barriers are not infinite, the wave function is not zero at the edges even though it must
vanish. To find out the Eigen state analytically it is necessary to match the wave function
and its derivative in both edges. Numerically this is not a real concern as the function and its
derivative are continuous by construction.
The numerical processes are not trivial but neither they are of extreme complexity.
However, we opted for presenting the numerical solutions as the results may be more
interesting, easily repeatable and even implemented by any person with minimal computer
skills [3]. Our computer program has been written in FORTRAN 95 and it is accessible to
anyone on demand.
The computational details employed to obtain all present data are not discussed in
this article as the complications involved are quite limited. The main interest is to discuss
the physics interpretation of wave functions and density of probability arising from the
proposed systems. Further questions about the numerical and computational specificities
are encouraged to be sent directly to the author who shall gladly provide all the information
demanded.
To make equation (3) more appropriate to work numerically with, it is convenient to
rewrite it entirely in a units free system. Two parameters of scale are necessary and we opt
to rewrite equation (3) in terms of a dimensionless position variable that is proportional to
, i.e., . The second parameter suitable to be treated in terms of a
dimensionless value is the energy that we write as being proportional to , i.e.,
. Consequently the potential energy ought also to be written as for sake
of direct comparison. Actually, equation (3) becomes entirely units free when it is rewrote in
terms of the dimensionless variable and the dimensionless parameter . Therefore, the
two parametrical values connecting laboratory units and the results presented here are the
system or particle mass and the frequency that is determined once is fixed.
The energy levels of ideal quantum wells for this free of units system units described
previously are:
(4)
The complete values are immediately regained simply taking into consideration that the real
size of the quantum well in units of length is .
0 1 2 3 40,00
0,15
0,30
0,45
0,60
0,75
0()
|0()|²
0=0.30845
Figure 1. Wave function in black and density of probability in red for the ground state of
energy of an ideal quantum well, i.e., when the limiting barriers of confinement are
described as assuming infinite values, which obligates the vanishing of at the edges.
The marked area in the figure represents the infinite energy potential barriers.
In Figure 1 it is represented the normalized wave function and the normalized
density of probability for the lowest energy level, also called the ground state level.
For both and the barrier of potential energy is infinite and therefore the wave
function must be null out there. The discontinuities of
occurring at and are
“authorized” only because the potential is assumed to be infinite for these values. The
energy found in our system of units is indicated in the Figure and corresponds exactly to the
theoretical value obtained in equation (4).
-1 0 1 2 3 4 50,0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,0
1,0
2,0
3,0
4,0
5,0
6,0
7,0
V0(
)
0(
)
0()
|0()|²
0=0.22947
Figure 2. Wave function and density of probability for the ground state of energy of a real
quantum well, i.e., when the limiting barriers of confinement are limited, allowing then the
penetration of the function into the normally forbidden region, represented by the shadow
areas of the figure.
In figure (2) we represent the same ground state: wave function, density of probability
and energy level for a system whose confinement is given by high but finite barriers. These
barriers are considered to exist from to and from to . The Eigen value of energy
decreases when compared to the precedent ideal case. The energy level is considerably
lower than the previous one. The penetration of the wave function is responsible for such
an effect. The infinite barriers raise the energy level by approximately 34% in this particular
example. In this case the wave function must vanish for infinite values, positive and
negative, of , i.e. of . The energy gaps between Eigen levels also decrease and for energies
higher than 5.0 units the spectrum is continuum again, since there is no more confinement.
The limited length represented in the figure from -1.0 to +5.0 provide only a reference as it
can be seen from the fact that the wave function is not yet zero for those values.
III. CONFINEMENT WITH AN INSIDE BARRIER
The first specific case to be discussed is that of a quantum barrier inside a quantum well.
Actually, the “external” quantum well is useful to provide the initial confinement of the
particle physical states resulting in quantized energy levels. Let us give some numbers to the
system in order to get quantitative rather than only qualitative arguments.
The barrier inside the quantum well is located at the center of the well and its length is
measured as a percentage of the well width. Its height is represented by as described in
the precedent paragraph. Two limit situations regarding are easier to analyze, it is the
case when and . When the condition is trivial and simply reports to
the isolated quantum well energy levels and Eigen functions. When the solution is
also trivial as it reports to the situation when there are two separated quantum wells
instead of only one within a barrier inside. The two quantum wells have widths equal the
quantum well width minus the barrier width. As the barrier is initially symmetrically located
at the center of the well, the new quantum wells are also symmetric. The energy levels of
each well are identical and the wave functions get obligatory null values at the both
borders. The energy level values are exactly the same as the values calculated for a single
quantum well having the same width given by the region where the energy is zero.
The interesting analysis arises then when the situation of the introduced barrier is
intermediary. In order to make the results clearer the study ought to be separated in two
parts, the first one considering a constant width barrier and variable potential height. The
second part takes into account a fixed barrier height while its width is modified. It is very
didactic to spend time investigating the energy levels and wave functions that arise from
these calculations.
For sake of simplicity we will keep the width of this new barrier constant and equal to
of the initial quantum well width, which means in our calculation that the inside
barrier width is equal . Nevertheless the barrier height will be augmented from to
a limit considered much higher than the first value of the ground state confined energy,
.
0 1 2 3 40,00
0,15
0,30
0,45
0,60
0,75
V0=0.0
V0=2.0
V0=4.0
V0=8.0
V0=16.0
V0=32.0
V0=56.0
0(
)
0 1 2 3 40
10
20
30
40
50
60
V0(
)
Figure 3. Wave functions of the ground state for different values of the barrier energy height
(a). In part (b) the different barriers are represented in the center of the well
Obviously nothing changes while the new potential energy is null. Conversely, both the
wave function and the energy level are modified as the new barrier height increases. In
figure 3 it is plotted two families of curves, representing the wave functions and the
inserted barrier. The dot-dashed lines are the wave functions and the continuum lines
represent the barriers of potential energy.
The first effect to notice is the deformation of wave functions as the barrier height
increases, reducing the probability of presence of the particle in the barrier region. The
Eigen values of energy increases as a function of the barrier height and the ground state
energy is smaller than all barriers represented in figure 3, which means that for all situations
the particle may be found in the barrier region that is classically forbidden. However, it is
evident that the barrier acts like a scattering center since the probability of finding the
particle is clearly moving away at both left and right directions.
Actually, it becomes also clear another limiting situation, when the new barrier is
extremely high. The wave function in this case almost splits completely in two quasi-
separated parts, each one centered exactly in the middle of the new free regions at left and
right. In fact, the “old” quantum well has been divided in two new quantum wells, limited by
the former infinite barriers and by the new inserted barrier.
The Eigen energy obtained for the highest barrier coincides exactly with the expect value
calculated for an infinite quantum well of width equal to the half of the previous one
diminished by 5%, which is half of the inserted barrier width. In figure 4 we represent the
Eigen energy for the ground state as function of the potential barrier height. The straight
line is the analytical Eigen energy for a quantum well of width limited by infinite
barriers.
0 10 20 30 40 50 600,2
0,4
0,6
0,8
1,0
1,2
1,4
1,6
0
V0
Figure 4. Ground state of energy for a quantum well limited by infinite barriers and width =
4.0 within an inside centered barrier of height = V0 and width = 0.4. The blue line represents
the theoretical value of the ground state energy for a quantum well limited by infinite
barriers and width = 1.8.
IV. A QUANTUM WELL INSIDE A QUANTUM WELL
Our second consideration is to introduce a different quantum well inside the first one
instead of a barrier as in the previous session. This second well is also centered at and
its presence naturally modifies the ground state of energy and the corresponding wave
function that are analyzed as a function of this inserted quantum well deepness and width.
Even though those analyses bring interesting pieces of information of quantum systems, it is
much more interesting to study the effects induced by the presence of the second quantum
well as a function of the product of the well deepness multiplied by the well width
maintained constant. For very small widths this inserted quantum well shall behave like a
delta-doped potential energy. For sake of definition these different wells can be called as
quantum well of confinement and inserted quantum well respectively, which eventually
becomes a delta doped-like system.
Holding a constant value for the inserted quantum well width and increasing the
deepness of the potential energy value the Eigen function for the ground state becomes
more concentrate in the new well region. The ground state of energy decreases and
eventually becomes negative. Therefore, it is like both the energy values and the wave
function enter the new quantum well, even though the probability to find the particle in the
region of the old quantum is still non-negligible.
An equivalent analysis arises when the potential energy of the new quantum well is kept
constant, e.g. , and its width is modified, from to . Both the energy level and the
wave function will end inside the new quantum well at some point. When the system
is absolutely identical to the pervious one and when too except that the bottom line
of energy is no longer but instead. The wave functions and density of probability are
exactly the same for these two cases.
In spite of these transitions described above and all the adjustment suffered by the
wave function, the comprehension of the process is not extremely elaborated.
Nevertheless, the situation changes a bit when a new condition is practiced. Instead of
keeping either the well width constant or its potential energy constant, we investigate what
happens to the ground state of energy and its corresponding wave function when the
product well width multiplied by the potential energy intensity is kept constant, while
varying them both. The different relationship connecting energy and width can be visualized
in figure (5).
0 1 2 3 4
-800
-700
-600
-500
-400
-300
-200
-100
0
V0
(A)
1,95 1,96 1,97 1,98 1,99 2,00 2,01 2,02 2,03 2,04 2,05
V0=-800
V0=-400
V0=-200
V0=-100
(B)
Figure 5. Schematic representation of the potential energy considered to solve the
Schrödinger equation. The system is limited by infinite barriers for and as usual
and it is free in between except these additional quantum wells. The product is kept
constant and equal 4 in our work.
In the part (A) of figure (5) we see all the different quantum wells at once and it is clear
then that the pattern converges to a delta doped – like system. In part (B) it is represented a
magnification of the central part of the well to make clear the meaning of description.
An important analysis arises when is kept small and constant, typically 2%, and gets
deeper until the ground state is located inside this tiny confinement, meaning that the Eigen
energy for is negative. The corresponding wave function is represented in figure (5) and
shows a much localized form. Actually, it is possible to obtain the analytical function when
the potential energy is described as a -function obeying its natural mathematical
properties. The resulting wave function is given by decaying exponential centered at the
origin of the and the energy of confinement is given by:
(5)
where is the parameter characterizing the function, or more appropriately saying, the
distribution. In the system of units assumed here to solve Schrödinger equation the energy
is therefore equal to
.
In order to exhibit some numerical results a quantum well composed of the following
characteristics: energy potential depth and width = has been considered. The
product is kept constant and equal 4.0. Making very small implies to increase
considerably the intensity , which is one particular form of definition of -function.
0 1 2 3 4
0,00
0,25
0,50
0,75
1,00
1,25
1,50
0
1
2
0(x
)|²
Numerical data
Analytical result
0(x
)
x
Figure 6. Wave function and density of probability (in the small frame) for the confined state
of a -doped system. The red line represents the analytical solution of an ideal system while
the dots represent the numerical results for our simulation of a potential.
In figure (6) it is represented the wave function for the ground state of an analytical -
doped potential energy as the straight line. The numerical solution of Schrödinger equation
for a square well potential extremely thin and deep: and respectively
is represented by the sequence of dots. The coincidence of both curves is remarkable, even
though is noticeable the little deviation close to both edges. The numerical solution is
constructed with the obligation that the wave function vanishes at and while
the analytical solution is described by a pure decaying exponential, which may assume very
small values but not zero.
-800 -600 -400 -200 0
-9
-8
-7
-6
-5
-4
-3
-2
-1
0
1
0
V0
Figure (7). Variation of the ground state level of energy as a function of the potential energy
depth for a quantum well whose width is also variable but the product is kept
constant and equal 4, simulating a -doped system. The system is composed of an external
quantum well limited by infinite barriers of potential at 0 and 4 inside which another
quantum well is centered at the middle distance.
In figure (7) the dots represent the ground state of energy as a function of the
potential depth maintaining the product constant and equal 4, which classifies
the -function. The bottom straight line is the level of energy for an analytical -doped
potential while the top straight line is the level of energy for the free quantum well system
limited by infinite barriers at and .
Finally, in figure (8) it is exhibited three different Eigen functions obtained while
calculating the points of figure (7) to exemplify its behavior. The shape of the wave function
changes drastically from the free quantum well to the -doped like system. An intermediary
condition is also shown. The system goes from completely delocalized to very localized as
the potential depth increases.
0 1 2 3 4
0,0
0,5
1,0
1,5
2,0
0,0
0,4
0,8
1,2
1,6
2,0
2,4
2,8
3,2
3,6
4,0
0(x
)|²
V0=0.0
V0=-20.0
V0=-800.0
Figure 8. Three different Eigen functions for different values of the potential depth placed as
a quantum well at the center of the system.
In figure (9) it is shown that the Eigen values are correctly calculated for any value of
parameter that classifies de -doped function, expressed in equation (5).
0 1 2 3 4 5 6
-20
-15
-10
-5
0
0
Numerical
Analytical
Figure 9. Ground state of energy or energy of confinement for a single -doped quantum
well characterized by the parameter . The dependence is expressed in equation (5) and
verified numerically as indicated in the figure by the dots following the straight line.
V. CONCLUSION
In this paper the Schrödinger equation independent of time has been numerically solved
inside a quantum well delimited by confining barriers of infinite potential height. The
common situation is defined by a constant potential inside the well whose analytical
solutions are easily found. The ground state energy has been obtained and the
corresponding wave function and density of probability are exhibited. It has also been
shown the effects of changing the barriers from infinite to limited values. The wave function
then penetrates the forbidden region and the energy level is lowered.
The study is more interesting when a perturbation potential is placed inside the well.
This situation is divided in two different cases. The first study is the analysis of a quantum
barrier placed symmetrically at the center of the precedent well width. The ground state
energy is studied as a function of this new barrier potential energy height. The evolution of
these functions as the potential energy for the inside barriers increases is actually
interesting for a didactical point of view. It is clear visible that the new barrier acts as a new
confining condition, separating the previous wave function in two distinct parts. At the limit
of a very high inside barrier, the ground state converges to the expected value of a single
quantum well for which the width is defined by the distance between the previous infinite
barrier and the inside confinement barrier. For a larger inside barrier the ground state
converges quicker as the tunneling effect is reduced.
The second case studied in this paper is the situation of a confining potential placed
inside the initial quantum well. This confining potential is described as a quantum well
centralized in the middle of the previous well, which is always limited by infinite height
barriers. For this specific case a particular control is observed, the product of the new
quantum well energy depth multiplied by its width is maintained constant. This is an initial
simulation of the so-called delta-doped quantum well, which is an electronic device made,
e.g., of Gallium-Arsenide within a single monolayer of doped Silicon. A potential energy in
the form of a function presents a confined level of energy easily calculated from the
Schrödinger equation. However, the procedure presented in this paper is highly educational
as it is possible to actually “see” the wave function getting inside the new confining
potential, as if it is falling down inside the attractive shape of the potential energy.
The results presented in this paper are not exactly new from any research point of view
but they have been used to teach introductory quantum mechanics to physics students at
two different courses: computational physics 2 and quantum mechanics 1. Apparently the
students appreciate seeing the modification of the wave function as the potential inside the
initial confined quantum well is customized. The simplicity and reliability of the numerical
methods are powerful instruments to facilitate the comprehension of the results.
VI. ACKNOWLEDGMENTS
This work has been financially supported by CNPq under contract 407840/2013-3. CAPES
and Fundect/MS must also be acknowledged. It is very important to thank Ms. Victoria Tangi
for careful English editing and text revision.
VII. REFERENCES
[1]. Claude Cohen-Tannoudji, Bernard Diu and Franck Lalöe. Quantum Mechanics Vol. 1,
1977.
[2]. Milton Abramowitz and Irene Stegun. Handbook of mathematical functions, 1972.
[3]. William H. Press, Saul A. Teukolsky, William T. Vettering and Brian P. Flannery.
Numerical Recipes in Fortran, 1992.