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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