schrodinger equation

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    Schrodinger Equation

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    Each particleis represented by awave function (x,t) such that *=theprobability of finding the particle at that

    position at that time

    The wave function is used in theSchrodinger equation. The Schrodinger

    equation plays the role of Newtons lawsand conservation of energy in classicalmechanics. It predicts analytically andprecisely the probability of events.

    THE WAVE FUNCTION

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    Wavefunction Properties

    contains all the measurable information aboutthe particle

    * summed over all space=1(if particleexists, probability of finding it somewheremust be one and its derivative is continuous

    allows energy calculations via the Schrodingerequation

    permits calculation of expectation value of agiven variable.

    is finite and single valued

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    ))(/( pxEtiAe

    SCHRODINGERS EQUATION:

    TIME-DEPENDENT FORM

    The wave function for a particle moving freely in

    the +x direction is given by.(1)

    where E is total energy of the particle and p is its

    momentum.Differentiating (1) for twice w r to x gives

    Also differentiating (1) for once w r to tgives

    2

    2

    22

    2

    p

    xor

    .(2)

    iE

    t .(3)or tiE

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    ),(2

    2

    txVm

    pE

    V

    xmt

    i2

    22

    2

    .(4)

    The quantities

    are called operators.

    The total energy E of aparticle is the sum of itskinetic energy and potentialenergy

    Multiply (5) by on bothsides gives

    Substitute for E and p2 to obtain the timedependent form of schrodinger equation:

    .(6)

    ..(5)

    .(7)

    tiE

    and

    Vm

    pE2

    2

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    V

    zyxmti

    2

    2

    2

    2

    2

    22

    2

    In three dimensions the time dependent form ofSchrodingers equation is

    .(8)

    Where the particles potential energy V is some

    function of x,y,z and t. Any restriction that maybe present on the particles motion will affect thepotential energy and once V is knownSchrodinger's equation may be solved to obtain the

    energy, wave function and probability density ofthe particle.

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    EXPECTATION VALUES

    )1...(..................

    .....

    321

    332211

    i

    ii

    N

    xN

    NNN

    xNxNxNX

    )2.....(....................2dxP ii

    The average position of a number of particlesdistributed along the x axis such that N1 particles

    at x1, N2 particles at x2 and so on is given by

    For a single particle the number Ni at xi must bereplaced by the probability

    Where i is the particle wave function evaluatedat x=xi. Making substitution and changing thesummations to integrals, the expectation value ofthe position is given by

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    )3..(..............................2

    2

    dx

    dxx

    x

    If the wave function is normalized

    then )4...(..............................2

    dxxx

    1..2

    dxei

    )5......(2

    dxEE

    dxpp2

    Similarly expectation values of momentum andenergy are given by

    and

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    )1(.......................................... )/(

    )/()/())(/(

    tiE

    xiptiEpxEti

    eei

    eAeAe

    )2(..........2 2

    22

    V

    xmti

    tiEtiEtiE

    eVxemeE

    )/(

    2

    2)/(

    2)/(

    2

    xipAewhere )/(

    SCHRODINGER EQUATION: STEADY-STATE FORM

    The wave function

    of unrestricted particle may bewritten as

    is the product of time dependent and a positiondependent function

    Substituting in time dependent form ofSchrodinger equation

    We get

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    Dividing through by the common exponential factorgives

    is the steady-state form of Schrodinger equation.

    In three dimensions the equation takes the form as

    )4........(0)(2

    22

    2

    2

    2

    2

    2

    VE

    m

    zyx

    )3(....................0)(

    222

    2

    VE

    m

    x

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    EIGENVALUES AND EIGENFUNCTIONS

    The values of energy En for which Schrodingers

    steady-state equation can be solved are calledeigenvalues and corresponding wave functions nare called eigenfunctions.

    The discrete energy levels of the hydrogen atom

    are an example of a set of eigenvalues

    2222

    4 1

    32 n

    meEn

    n = 1,2,3,..

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    )1.(..............................02

    22

    2

    E

    m

    x

    APPLICATION: PARTICLE IN A BOX

    0 L x

    V

    Aim: To show energy quantization

    1.How to solve Schrodingers equation?

    2.Obtain eigenvalues and eigenfunctions

    3.Compare the results with classicalmechanics

    The potential energy of the particle isV=0 inside the box andV= outside the box

    The steady-state form of Schrodingersequation for the particle within the box with aboverestrictions may be written as

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    )2...(2

    sin xmE

    A

    )4......(..............................2 nLmE

    The equation (1) will have the following possiblesolutions

    )3......(2

    cos xmE

    B

    and

    These solutions are subject to the importantboundary condition such that =0 for x=0 and x=LSince cos(0)=1, the second solution cannot

    describe the particle at x=0 implies B=0

    The first solution gives=0 for x=0 but will bezero at x=L only when

    n=1,2,3,..

    From equation (4) the energy of the particle canhave only certain values called eigenvalues givenby

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    )7...(..........)sin(2

    sin xL

    nAx

    mEA

    n

    n

    )5(..............................2 2

    222

    mL

    nEn

    n=1,2,3,..

    A particle confined to a box cannot have an

    arbitrary energy and also n=0 or E=0 is notadmissible

    WAVE FUNCTIONS

    The wave function of a particle in a box whoseenergy is E is

    Substituting for E from equation (5) we get

    )6.....(..........2

    sin xmE

    A

    further )8.........(....................1

    2

    dx

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    )10..(..........sin2

    xL

    n

    Ln

    )9.(..............................2

    LA

    gives

    Therefore the normalized wavefunctions of theparticle are

    The normalized wanefunctions

    1,2, 3 are plotted as shown.

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    Graphical explanation

    A particle in a box with infinitely high

    walls is an application of the Schrodingerequation which yields some insights intoparticle confinement. The wavefunctionmust be zero at the walls and the solution

    for the wavefunction yields just sine waves.

    The longest wavelength is = 2L andthe higher

    modes have wavelengths given by

    =2L/n where n= 1,2,3,.

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    When this is substituted into the DeBroglierelationship it yields momentum p=h/

    =nh/2LThe momentum expression for the particlein a box :

    p=h/ =nh/2L: n= 1,2,3,..is used to calculate the energy associatedwith the particle

    nEmL

    hn

    m

    pmv

    2

    2222

    822

    1

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    Though oversimplified, this indicates someimportant things about bound states for

    particles:

    1. The energies are quantized and can becharacterized by a quantum number n

    2. The energy cannot be exactly zero.

    3. The smaller the confinement, the largerthe energy required.

    If ti l i fi d i t

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    If a particle is confined into arectangular volume, the same kind ofprocess can be applied to a three-

    dimensional "particle in a box", and thesame kind of energy contribution is madefrom each dimension. The energies for athree-dimensional box are

    This gives a more physically realisticexpression for the available energies forcontained particles. This expression is usedin determining the density of possible

    energy states for electrons in solids.

    2

    2

    3

    2

    2

    2

    1

    8mLE

    nnnn

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