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Chapter 41
Quantum Mechanics
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Probability A Particle
Interpretation From the particle point of view, the
probability per unit volume of finding a
photon in a given region of space at aninstant of time is proportional to the
numberNof photons per unit volume at
that time and to the intensityProbability
IN
V V
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Probability A Wave
Interpretation From the point of view of a wave, the
intensity of electromagnetic radiation is
proportional to the square of the electricfield amplitude, E
Combining the points of view gives
2Probability EV
2I E
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Probability Interpretation
Summary For electromagnetic radiation, the probability
per unit volume of finding a particle
associated with this radiation is proportionalto the square of the amplitude of theassociated em wave The particle is the photon
The amplitude of the wave associated withthe particle is called the probabilityamplitudeor the wave function The symbol is
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Wave Function, cont. The wave function is often complex-valued The absolute square ||2 = is always real
and positive * is the complete conjugate of It is proportional to the probability per unit volume
of finding a particle at a given point at someinstant
The wave function contains within it all theinformation that can be known about theparticle
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Wave Function, General
Comments, Final The probabilistic interpretation of the
wave function was first suggested by
Max Born Erwin Schrdinger proposed a wave
equation that describes the manner inwhich the wave function changes inspace and time This Schrdinger wave equation represents a
key element in quantum mechanics
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Wave Function of a Free
Particle The wave function of a free particle moving
along the x-axis can be written as (x) =Aeikx
k= 2/ is the angular wave number of the waverepresenting the particle
A is the constant amplitude
If represents a single particle, ||2 is the
relative probability per unit volume that theparticle will be found at any given point in thevolume ||2 is called the probability density
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Wave Function of a Free
Particle, Final Because the particle must be
somewhere along thexaxis, the sum of
all the probabilities over all values ofxmust be 1
Any wave function satisfying this equationis said to be normalized
Normalization is simply a statement that
the particle exists at some point in space
21abP dx
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Expectation Values is not a measurable quantity
Measurable quantities of a particle can
be derived from
The average position is called the
expectation value ofxand is defined
as* x xdx
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Expectation Values, cont. The expectation value of any function of
xcan also be found
The expectation values are analogous to
weighted averages
*f x f x dx
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Summary of Mathematical
Features of a Wave Function (x) may be a complex function or a
real function, depending on the system
(x) must be defined at all points inspace and be single-valued
(x) must be normalized
(x) must be continuous in space There must be no discontinuous jumps in
the value of the wave function at any point
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Particle in a Box A particle is confined
to a one-dimensionalregion of space The box is one-
dimensional
The particle isbouncing elasticallyback and forthbetween twoimpenetrable wallsseparated by L
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Potential Energy for a Particle
in a Box As long as the particle
is inside the box, thepotential energy does
not depend on itslocation We can choose this
energy value to be zero
The energy is infinitely
large if the particle isoutside the box This ensures that the
wave function is zerooutside the box
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Wave Function for the Particle
in a Box Since the walls are impenetrable, there
is zero probability of finding the particle
outside the box (x) = 0 forx< 0 andx> L
The wave function must also be 0 at thewalls The function must be continuous (0) = 0 and (L) = 0
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Wave Function of a Particle in
a Box Mathematical The wave function can be expressed as
a real, sinusoidal function
Applying the boundary conditions and
using the de Broglie wavelength
2( ) sin
x x A
( ) sinnx
x AL
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Graphical Representations for
a Particle in a Box
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Active Figure 41.4
(SLIDESHOW MODE ONLY)
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Wave Function of the Particle
in a Box, cont. Only certain wavelengths for the particle
are allowed
||2 is zero at the boundaries ||2 is zero at other locations as well,
depending on the values ofn
The number of zero points increases byone each time the quantum numberincreases by one
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Energy of a Particle in a Box We chose the potential energy of the
particle to be zero inside the box
Therefore, the energy of the particle is
just its kinetic energy
The energy of the particle is quantized
22
2 1 2 38 , , ,
n
h
E n nmL
K
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Energy Level Diagram
Particle in a Box The lowest allowed
energy correspondsto the ground state
En = n2E1 are called
excited states E= 0 is not an
allowed state The particle can
never be at rest
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Active Figure 41.5
(SLIDESHOW MODE ONLY)
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Boundary Conditions Boundary conditions are applied to determine
the allowed states of the system
In the model of a particle under boundaryconditions, an interaction of a particle with itsenvironment represents one or moreboundary conditions and, if the interactionrestricts the particle to a finite region ofspace, results in quantization of the energy ofthe system
In general, boundary conditions are related tothe coordinates describing the problem
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Erwin Schrdinger 1887 1961 Best known as one of
the creators of quantum
mechanics His approach was
shown to be equivalentto Heisenbergs
Also worked with: statistical mechanics color vision general relativity
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Schrdinger Equation The Schrdinger equation as it applies
to a particle of mass m confined to
moving along thexaxis and interactingwith its environment through a potentialenergy function U(x) is
This is called the time-independentSchrdinger equation
2 2
22
d
U Em dx h
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Schrdinger Equation, cont. Both for a free particle and a particle in
a box, the first term in the Schrdinger
equation reduces to the kinetic energyof the particle multiplied by the wave
function
Solutions to the Schrdinger equation indifferent regions must join smoothly at
the boundaries
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Schrdinger Equation, final (x) must be continuous
(x) must approach zero asx
approaches This is needed so that (x) obeys the
normalization condition
d/dxmust also be continuous for finitevalues of the potential energy
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Solutions of the Schrdinger
Equation Solutions of the Schrdinger equation may be
very difficult
The Schrdinger equation has beenextremely successful in explaining thebehavior of atomic and nuclear systems Classical physics failed to explain this behavior
When quantum mechanics is applied tomacroscopic objects, the results agree withclassical physics
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Schrdinger Equation Applied
to a Particle in a Box In the region 0
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Finite Potential Well
Region II U= 0
The allowed wave functions are sinusoidal
The boundary conditions no longer requirethat be zero at the ends of the well
The general solution will be
II(x) = Fsin kx+ G cos kx where Fand G are constants
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Finite Potential Well
Regions I and III The Schrdinger equation for these
regions may be written as
The general solution of this equation is
A and B are constants
2 22 2
2m U Ed C
dx
h
Cx Cx Ae Be
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Finite Potential Well
Regions I and III, cont. In region I, B = 0
This is necessary to avoid an infinite value
for for large negative values ofx In region III,A = 0
This is necessary to avoid an infinite value
for for large positive values ofx
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Finite Potential Well
Graphical Results for The wave functions for
various states areshown
Outside the potentialwell, classical physicsforbids the presence ofthe particle
Quantum mechanicsshows the wavefunction decaysexponentially toapproach zero
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Finite Potential Well
Graphical Results for2
The probability
densities for the
lowest three statesare shown
The functions are
smooth at the
boundaries
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Active Figure 41.8
(SLIDESHOW MODE ONLY)
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Finite Potential Well
Determining the Constants The constants in the equations can be
determined by the boundary conditions
and the normalization condition The boundary conditions are
I II
I II
II IIIII III
and at 0
and at
d d
xdx dx
d d x L
dx dx
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Application Nanotechnology Nanotechnology refers to the design and
application of devices having dimensions
ranging from 1 to 100 nm Nanotechnology uses the idea of trapping
particles in potential wells
One area of nanotechnology of interest to
researchers is the quantum dot A quantum dot is a small region that is grown in a
silicon crystal that acts as a potential well
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Tunneling, cont. Classically, the particle is reflected by the
barrier Regions II and III would be forbidden
According to quantum mechanics, all regionsare accessible to the particle The probability of the particle being in a classically
forbidden region is low, but not zero According to the uncertainty principle, the particle
can be inside the barrier as long as the timeinterval is short and consistent with the principle
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Tunneling, final The curve in the diagram represents a full
solution to the Schrdinger equation
Movement of the particle to the far side of thebarrier is called tunneling orbarrier
penetration
The probability of tunneling can be described
with a transmission coefficient, T, and a
reflection coefficient, R
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Tunneling Coefficients The transmission coefficient represents the
probability that the particle penetrates to theother side of the barrier
The reflection coefficient represents theprobability that the particle is reflected by thebarrier
T+ R= 1 The particle must be either transmitted or reflected T e-2CL and can be nonzero
Tunneling is observed and provides evidence
of the principles of quantum mechanics
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Applications of Tunneling Alpha decay
In order for the alpha particle to escape
from the nucleus, it must penetrate abarrier whose energy is several timesgreater than the energy of the nucleus-alpha particle system
Nuclear fusion Protons can tunnel through the barrier
caused by their mutual electrostaticrepulsion
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More Applications of Tunneling
Resonant Tunneling Device
Electrons travel in the gallium arsenide
semiconductor They strike the barrier of the quantum dot from
the left The electrons can tunnel through the barrier
and produce a current in the device
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More Applications of Tunneling
Scanning Tunneling Microscope An electrically
conducting probe with avery sharp edge is
brought near thesurface to be studied The empty space
between the tip and thesurface represents the
barrier The tip and the surface
are two walls of thepotential well
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Scanning Tunneling
Microscope The STM allows
highly detailedimages of surfaces
with resolutionscomparable to thesize of a single atom
At right is thesurface of graphiteviewed with theSTM
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Scanning Tunneling
Microscope, final The STM is very sensitive to the distance
from the tip to the surface This is the thickness of the barrier
STM has one very serious limitation Its operation is dependent on the electrical
conductivity of the sample and the tip Most materials are not electrically conductive at
their surfaces The atomic force microscope overcomes this
limitation
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Simple Harmonic Oscillator Reconsider black body radiation as
vibrating charges acting as simple
harmonic oscillators The potential energy is
U= kx2 = m2x2
Its total energy is
K+ U= kA2 = m2A2
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Simple Harmonic Oscillator, 2 The Schrdinger equation for this
problem is
The solution of this equation gives the
wave function of the ground state as
2 22 2
2
1
2 2
dm x E
m dx h
22m x Be h
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Simple Harmonic Oscillator, 3 The remaining solutions that describe the
excited states all include the exponential
function
The energy levels of the oscillator are
quantized
The energy for an arbitrary quantum number
n is En = (n + ) where n = 0, 1, 2,
2Cxe
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Energy Levels in the
Harmonic Oscillator The state n = 0 corresponds to the ground
state The energy is Eo =
The state n = 1 is the first excited state The separations between adjacent levels are
equal and are given by E=
As n increases, the agreement between theclassical and the quantum-mechanical resultsimprove