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    Contents

    1 One Dimensional Wave and Heat Equations 51.1 One Dimensional Wave Equation . . . . . . . . . . . . . . . . . 5

    1.1.1 Laplace transform formulae . . . . . . . . . . . . . . . . 51.1.2 Solution of Wave Equation by variable separable method 51.1.3 D Alemberts solution of the wave equation . . . . . . . 71.1.4 Fourier Transform Formulae . . . . . . . . . . . . . . . . 67

    2 Elliptic Equations 932.1 Laplace Equation . . . . . . . . . . . . . . . . . . . . . . . . . . 93

    3 Calculus of Variations 1073.1 Calculus of Variations . . . . . . . . . . . . . . . . . . . . . . . 1073.2 The variational problem: . . . . . . . . . . . . . . . . . . . . . . 107

    3.2.1 Euler-Lagrange Equation . . . . . . . . . . . . . . . . . 1073.2.2 Other forms of Euler Equation . . . . . . . . . . . . . . 1103.3 Variational Problems involving several unknown functions . . . 1383.4 Functionals involving Higher Order Derivatives . . . . . . . . . 141

    3.4.1 Euler Equation . . . . . . . . . . . . . . . . . . . . . . . 1413.5 The Raleigh Ritz method . . . . . . . . . . . . . . . . . . . . . 1473.6 Variational Problems involving several independent variables . 1543.7 Constraints and Lagrange multipliers . . . . . . . . . . . . . . . 155

    3.7.1 Working Rule . . . . . . . . . . . . . . . . . . . . . . . . 1553.8 Variational problems with moving boundaries . . . . . . . . . . 159

    4 Eigen Value Problems 171

    4.1 Faddeev-Leverrier Method for Eigenvalues . . . . . . . . . . . . 1714.1.1 Faddeev-Leverrier Method . . . . . . . . . . . . . . . . . 1714.2 Power Method with deflation . . . . . . . . . . . . . . . . . . . 1804.3 Rayleigh-Ritz method . . . . . . . . . . . . . . . . . . . . . . . 187

    5 Numerical Integration 1895.1 Introduc tion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1895.2 Gaussian Quadrature . . . . . . . . . . . . . . . . . . . . . . . . 189

    5.2.1 Two Point Gaussian Quadrature Formulae . . . . . . . . 1895.2.2 Higher Point Gaussian Quadrature Formulae . . . . . . 1955.2.3 Gauss-Hermite Quadrature Formulae . . . . . . . . . . . 200

    1

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    MA 9203 APPLIED MATHEMATICS(ME STRUCTURAL ENGINEERING)

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    2

    MA 9203 APPLIED MATHEMATICS L T P C3 1 0 4

    OBJECTIVE:

    . To familiarize the students in the field of differential and elliptic equa-tions to solve boundary value problems associated with engineering ap-plications.

    . To expose the students to variational formulation and numerical integra-tion techniques and their applications to obtain solutions for buckling,dynamic response, heat and flow problems of one and two dimensionalconditions.

    UNIT I ONE DIMENSIONAL WAVE AND HEAT EQUATIONS10+3

    Laplace transform methods for one-dimensional wave equation Displace-ments in a long string longitudinal vibration of an elastic bar Fourier trans-form methods for one-dimensional heat conduction problems in infinite andsemi-infinite rods.UNIT - II ELLIPTIC EQUATION 9+3

    Laplace equation Properties of harmonic functions Solution of Laplacesequation by means of Fourier transforms in a half plane, in an infinite stripand in a semiinfinite strip Solution of Poisson equation by Fourier transformmethod.UNIT - III CALCULUS OF VARIATIONS 9+3

    Concept of variation and its properties Eulers equation Functional depen-dant on first and higher order derivatives Functionals dependant on functionsof several independent variables Variational problems with moving boundariesDirect methods Ritz and Kantorovich methods.

    UNIT - IV EIGEN VALUE PROBLEMS 9+3Methods of solutions: Faddeev Leverrier Method, Power Method with

    deflation Approximate Methods: Rayleigh Ritz Method

    UNIT - V NUMERICAL INTEGRATION 8+3

    Gaussian Quadrature One and Two Dimensions Gauss Hermite Quadra-ture Monte Carlo Method Multiple Integration by using mapping function

    TOTAL (L:30+T:15) : 45 PERIODS

    REFERENCES:

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    3

    1. Sankara Rao, K., Introduction to Partial Differential Equations, PrenticeHall of India Pvt. Ltd., New Delhi, 1997.

    2. Rajasekaran.S, Numerical Methods in Science and Engineering A Prac-tical Approach, A.H.Wheeler and Company Private Limited, 1986.

    3. Gupta, A.S., Calculus of Variations with Applications, Prentice Hall ofIndia Pvt. Ltd., New Delhi, 1997.

    4. Andrews, L.C. and Shivamoggi, B.K., Integral Transforms for Engineers,Prentice Hall of India Pvt. Ltd., New Delhi, 2003.

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    Chapter 1One Dimensional Wave and Heat

    Equations1.1 One Dimensional Wave Equation

    1.1.1 Laplace transform formulae

    (1) L [u(x, t)] = U(x, s)

    (2) Lx u(x, t)

    = d

    dxU(x, s)

    (3) L

    2

    x2 u(x, t)

    = d2

    dx2 U(x, s)

    (4) L t u(x, t)

    = sL[u(x, t)] su(x, 0) = sU(x, s) su(x, 0)

    (5) L2

    t2 u(x, t)

    = s2L[u(x, t)] su(x, 0) ut(x, 0) = s2U(x, s) su(x, 0) ut(x, 0)

    (6) L1 [F(s)] = 12i

    + i i

    estF(s)ds = sum of residues of estF(s)

    1.1.2 Solution of Wave Equation by variable separablemethod

    Let the one dimensional wave equation be

    2y

    t2= a2

    2y

    x2or ytt = a

    2yxx (1.1.1)

    Clearly the solution y is in terms of x and t.Assume that the solution of equation (1.1.1) is y(x, t) = X(x)T(t) or simply y= XT.Then

    y

    x= yx = X

    T,y

    t= yt = XT

    2y

    x2

    = yxx = XT, and

    2y

    t2

    = ytt = XT.

    5

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    Therefore, equation (1.1.1) becomes

    XT = a2XT

    X

    X=

    T

    a2T= k say

    X

    X= k and

    T

    a2T= k

    X = kX and T = ka2T

    2X

    x2 kX = 0 and

    2T

    t2 ka2T = 0

    d2X

    dx2 kX = 0 and d

    2T

    dt2 ka2T = 0

    D2X kX = 0 and D2T ka2T = 0 (D2 k)X = 0 and (D2 ka2)T = 0

    Case i: Suppose that k is positiveThen k = 2 for some .Therefore, (D2 2)X = 0 and (D2 2a2)T = 0Hence the auxiliary equation is

    m2 2 = 0 and m2 2a2 = 0 m2 = 2 and m2 = 2a2 m2 = and m = a

    Consequently, X = Aex + Bex and T = Ceat + Beat

    Therefore, the solution isy(x, t) =

    Aex + Bex

    Ceat + Beat

    Case ii: Suppose that k is negativeThen k = 2 for some .Therefore, (D2 + 2)X = 0 and (D2 + 2a2)T = 0Hence the auxiliary equation is

    m2 + 2 = 0 and m2 + 2a2 = 0

    m2 = 2 and m2 = 2a2

    m2 =

    i and m =

    ai

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    7

    Consequently, X = Acos(x) + Bsin(x) and T = Ccos(at) + Bsin(at)Therefore, the solution isy(x, t) = [Acos(x) + Bsin(x)] [Ccos(at) + Bsin(at)]Case iii: Suppose that k = 0Then,

    D2X = 0 and D2T = 0

    d2X

    dx2= 0 and

    d2T

    dt2= 0

    ddx

    dX

    dx

    = 0 and

    d

    dt

    dT

    dt

    = 0

    dXdx

    = A anddT

    dt= C

    X = Ax + B and T = Ct + D

    Therefore, the solution isy(x, t) = (Ax + B)(Ct + D)

    1.1.3 D Alemberts solution of the wave equation

    Let the one dimensional wave equation be

    2y

    t2= a2

    2y

    x2or ytt = a

    2yxx (1.1.2)

    Let yt = D and yx = D. Then equation (1.1.2) becomes

    D2y = a2D2y

    D2 a2D2

    y = 0

    Therefore, the auxiliary equation is

    m2 a2 = 0 m2 = a2 m = a

    Therefore, the solution is

    y(x, t) = f(x + at) + g(x at) (1.1.3)

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    where f and g are arbitrary functions.Assume that at time t = 0, initial displacement is y(x, 0) = (x) and initialvelocity is y

    t(x, 0) = v(x).

    At time t = 0, equation (1.1.3) becomes y(x, 0) = f(x) + g(x)

    (x) = f(x) + g(x) (1.1.4)Also differentiating equation partially with r. to t, we get yt(x, t) = af

    (x +at) ag(x at)When t = 0, we have yt(x, 0) = af(x) ag(x)

    v(x) = af(x) ag(x) (1.1.5)Integrating (1.1.5) between ( c, x ) w.r.t. x, we have

    x

    c

    v(x)dx =x

    c

    [af(x)

    ag(x)] dx

    xc

    v()d = axc

    f(x)dx axc

    g(x)dx

    xc

    v()d = af(x) ag(x)

    Hence

    f(x) g(x) = 1a

    x

    c

    v()d (1.1.6)

    Adding (1.1.4) and (1.1.6), we have

    2f(x) = (x) +1

    a

    xc

    v()d

    f(x) = (x)2

    +1

    2a

    xc

    v()d

    f(x + at) = (x + at)2

    +1

    2a

    x + at

    cv()d

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    Hence

    f(x + at) =

    (x + at)

    2 +

    1

    2a

    x + atc v()d (1.1.7)

    Subtracting (1.1.4) and (1.1.6), we have

    2g(x) = (x) 1a

    xc

    v()d

    g(x) = (x)2

    12a

    xc

    v()d

    g(x at) = (x at)2

    12a

    x atc

    v()d

    Hence

    g(x at) = (x at)2

    12a

    x atc

    v()d (1.1.8)

    Substituting the values of f(x + at) and g(x at) in (1.1.3), we have

    y(x, t) =(x + at)

    2 +1

    2a

    x + atc

    v()d +(x

    at)

    2 1

    2a

    x

    at

    cv()d

    =1

    2[(x + at) + (x at)] + 1

    2a

    x + atc

    v()d x at

    c

    v()d

    =1

    2[(x + at) + (x at)] + 1

    2a

    x + atc

    v()d +c

    x atv()d

    =1

    2[(x + at) + (x at)] + 1

    2a

    x + at

    x atv()d

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    10

    Hence the D Alemberts solution of the one dimensional wave equation is givenby

    y(x, t) = 12

    [(x + at) + (x at)] + 12a

    x + atx at

    v()d (1.1.9)

    Remark 1.1.1 If the string is at rest at t = 0, then initial velocity = 0.Therefore, v(x) = 0. Hence y(x, t) = 12 [(x + at) + (x at)]Example 1.1.2 A tightly stretched string of length with its fixed ends at x= 0, x = executes transverse vibrations. Motion is started with zero initialvelocity by displacing the string into the form f(x) = k(x2 x3). Find thedeflection at any time t.

    SolutionGiven that the ends x = 0, x = of a given tightly stretched string of length

    are fixed. Therefore, there is no displacement at its end at any time. Hence,y(0, t) = 0, y(, t) = 0. Also the initial displacement is f(x) = k(x2 x3).Hence y(x, 0) = (x) = f(x) = k(x2 x3). Initial velocity is zero. Therefore,yt(x, 0) = v(x) = 0.

    Therefore, the D Alemberts solution of the one dimensional wave equationis given by

    y(x, t) =1

    2[(x + at) + (x at)]

    =1

    2

    k

    (x + at)2 (x + at)3 + k (x at)2 (x at)3=

    k

    2 x2 + 2xat + (at)2 (x3 + 3x2(at) + 3x(at)2 + (at)3

    +

    x2 2xat + (at)2 (x3 3x2(at) + 3x(at)2 (at)3

    =k

    2

    x2 + 2xat + (at)2 x3 3x2(at) 3x(at)2 (at)3

    +x2 2xat + (at)2 x3 + 3x2(at) 3x(at)2 + (at)3

    =k

    2

    2x2 + 2(at)2 2x3 6x(at)2

    =2k

    2

    x2 + (at)2 x3 3x(at)2

    = k

    x2 + (at)2 x3 3x(at)2

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    11

    Example 1.1.3 Using laplace transform method, solve the initial value prob-lem ytt = yxx, 0 < x < 1 and t > 0 with the boundary conditions y(0, t) = 0,y(1, t) = 0, y(x, 0) = sin x and yt(x, 0) =

    sin x.

    SolutionLet the given equation be

    ytt = yxx (1.1.10)

    Taking laplace transform in equation (1.1.10), we have

    L [ytt] = L [yxx]

    s2y(x, s) sy(x, 0) yt(x, 0) = d2 [y(x, s)]

    dx2where y(x,s) = L[y(x,t)]

    s2y(x, s)

    (s)sinx

    {sinx

    }=

    d2 [y(x, s)]

    dx2

    d2 [y(x, s)]

    dx2 s2y(x, s) = sinx (s)sinx

    D2 [y(x, s)] s2y(x, s) = (1 s)sinx (D2 s2) [y(x, s)] = (1 s)sinx

    Now, the auxiliary equation is

    m2 s2 = 0

    m2 = s2

    m = s

    Therefore, the complementary function isC.F = Aesx + Besx

    Now, Particular integral

    P.I =1

    D2 s2 (1 s)sinx

    =1

    2 s2 (1 s)sinx

    =1

    2

    + s2

    (s

    1)sinx

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    12

    Therefore, the solution is Hence the solution isy(x, s) = Aesx + Besx + 12+s2 (s 1)sinx.Now, taking laplace transforms to the first two conditions, we have

    L [y(0, t)] = L[0] and L [y(1, t)] = L[0]

    y(0, s) = 0 and y(1, s) = 0

    y(0, s) = 0 Ae0 + Be0 + 12 + s2

    (s 1)sin(0) = 0 A + B = 0 A = B

    y(1, s) = 0 Aes + Bes + 12 + s2

    (s 1)sin() = 0

    Aes + Bes = 0 Aes Aes = 0 A(es es) = 0 A = 0 B = 0

    Hence the solution is

    y(x, s) =1

    2 + s2(s 1)sinx

    L [y(x, t)] =1

    2 + s2 (s 1)sinx

    y(x, t) = L1

    1

    2 + s2(s 1)sinx

    y(x, t) = sinx

    L1

    s

    2 + s2

    L1

    1

    2 + s2

    y(x, t) = sinx

    L1

    s

    2 + s2

    1

    L1

    2 + s2

    y(x, t) = sinx

    cost

    1

    sint

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    13

    Example 1.1.4 A string is stretched and fixed between two points (0,0) and(, 0). Motion is started by displacing the string in the form ksin

    x

    andreleased from rest at time t = 0. Find the displacement of any point of thestring at any time t using laplace transform.

    SolutionLet the one dimensional wave equation be

    ytt = a2yxx (1.1.11)

    Given that the ends x = 0, x = of a given tightly stretched string of length are fixed. Therefore, there is no displacement at its end at any time. Hence,y(0, t) = 0, y(, t) = 0. Also the initial displacement is y(x, 0) = ksin

    x

    .

    Also the string is released from rest at time t = 0. Therefore, Initial velocityis zero. Therefore, yt(x, 0) = 0.

    Taking laplace transform in equation (1.1.11), we have

    L [ytt] = L

    a2yxx

    s2y(x, s) sy(x, 0) yt(x, 0) = a2 d2 [y(x, s)]

    dx2where y(x,s) = L[y(x,t)]

    s2y(x, s) (s)ksinx

    = a2

    d2 [y(x, s)]

    dx2

    a2 d2 [y(x, s)]

    dx2 s2y(x, s) = (s)ksin

    x

    a2D2y(x, s) s2y(x, s) = (s)ksin

    x

    D2y(x, s)

    s2

    a2y(x, s) =

    ks

    a2sinx

    D2 s2

    a2

    y(x, s) = ks

    a2sin

    x

    Now, the auxiliary equation is

    m2 s2

    a2= 0

    m2 = s2

    a2

    m =

    s

    a

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    14

    Therefore, the complementary function isC.F = Ae

    s

    ax + Be

    s

    ax

    Now, Particular integral

    P.I =1

    D2 s2a2

    ksa2

    sinx

    =ksa2

    2 s2a2

    sin

    x

    =ksa2

    2+ s

    2

    a2

    sin

    x

    Hence the solution is

    y(x, s) = Aes

    ax + Be

    s

    ax +

    ks

    a2

    ( )2+ s

    2

    a2 sinx .

    Now, taking laplace transforms to the first two conditions, we have

    L [y(0, t)] = L[0] and L [y(, t)] = L[0]

    y(0, s) = 0 and y(, s) = 0

    y(0, s) = 0 Ae0 + Be0 +ksa2

    2+ s

    2

    a2

    sin(0) = 0

    A + B = 0 A = B

    y(, s) = 0 Ae sa + Be sa +ksa2

    2+ s

    2

    a2

    sin

    = 0

    Ae sa + Be sa +ksa2

    2+ s

    2

    a2

    sin() = 0

    Ae sa + Be sa = 0 Ae sa Ae sa = 0 A(e sa e sa ) = 0 A = 0

    B = 0

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    15

    Hence the solution is

    y(x, s) =ksa2

    2+ s

    2

    a2

    sin

    x

    L [y(x, t)] =ksa2

    1a2

    a

    2+ s2

    sinx

    y(x, t) = L1

    ksa2

    a2

    a

    2+ s2

    sin

    x

    y(x, t) = L1

    ks

    a

    2+ s2

    sin

    x

    y(x, t) = k sin

    x

    L1

    s

    a

    2+ s2

    y(x, t) = k sinx

    cos

    at

    Example 1.1.5 Solve using laplace transform method uxx =1c2 utt cost,

    0 < x < , t > 0 u(x, 0) = ut(x, 0) = u(0, t) = 0 and u is bounded as x ..

    SolutionThe given equation is

    uxx =1

    c2utt cost uxx = 1

    c2

    utt c2cost

    c2uxx = utt c2cost utt = c2uxx + c2cost

    Therefore,utt = c

    2uxx + c2cost (1.1.12)

    Also the initial and boundary conditions are given by

    (i) u(x, 0) = 0

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    (ii) ut(x, 0) = 0

    (iii) u(0, t) = 0

    (iv) u is bounded as x

    Taking laplace transform in equation (??), we have

    L [utt] = L

    c2uxx + c2cost

    L [utt] = L

    c2uxx+ L

    c2cost

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]dx2

    + c2 ss2 + 2

    where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2+ c2

    s

    s2 + 2{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = c2 s

    s2 + 2

    d2 [U(x, s)]

    dx2 s

    2

    c2U(x, s) =

    ss2 + 2

    D2 s2

    c2

    U(x, s) =

    ss2 + 2

    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = sc

    Therefore, the complementary function is

    C.F = Ae

    s

    cx

    + Bes

    cx

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    Now, Particular integral

    P.I = 1D2 s2c2

    ss2 + 2

    =

    1

    s2c2

    1 c2

    s2(D2)

    ss2 + 2

    =

    c2

    s2

    1 c

    2

    s2(D2)

    1s

    s2 + 2

    =

    c2

    s(s2 + 2)

    1 +

    c2

    s2(D2) + ...

    (1)

    =c2

    s(s2 + 2)(1)

    =c2

    s(s2 + 2)

    Hence the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx + c

    2

    s(s2+2) .

    Now,taking laplace transforms to the remaining two conditions, we have

    L [u(0, t)] = L[0] and Lu(x, t) is bounded as x u(0, s) = 0 and u(x, s) is bounded as x

    u(0, s) = 0 Ae0 + Be0 + c2

    s(s2 + 2)= 0

    A + B + c2

    s(s2 + 2)= 0

    A + B = c2

    s(s2 + 2)

    Also u(x, s) is bounded as x A = 0

    B = c2

    s(s2+2) .

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    18

    Therefore, the solution is

    U(x, s) =

    c2s(s2 + 2)

    e

    s

    cx +

    c2

    s(s2 + 2)

    L [U(x, t)] = c2

    s(s2 + 2)

    e

    s

    cx +

    c2

    s(s2 + 2)

    U(x, t) = L1 c2

    s(s2 + 2)

    e

    s

    cx +

    c2

    s(s2 + 2)

    U(x, t) =

    c2L1

    1

    s(s2

    + 2

    ) e

    s

    cx + c2L1

    1

    s(s2

    + 2

    )

    Now,

    L1

    1

    s(s2 + 2)

    =

    1

    2L1

    2

    s(s2 + 2)

    =1

    2L1

    s2 + 2 s2

    s(s2 + 2)

    =1

    2

    L1

    s2 + 2

    s(s2 + 2)

    L1

    s2

    s(s2 + 2)

    =1

    2

    L1

    1

    s

    L1

    s

    s2 + 2

    =1

    2

    {1

    cost

    }

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    19

    Also we know that

    L1

    eas

    F(s)

    = L1

    [F(s)]tta H(t a) where H(t a)= 1 if t > a

    = 0 if t < a

    L1

    es

    cx

    1

    s(s2 + 2)

    = L1

    1

    s(s2 + 2)

    tt s

    c

    H

    t sc

    L1

    es

    cx

    1

    s(s2 + 2)

    =

    1

    2{1 cost}tt s

    c

    H

    t sc

    L1

    es

    cx

    1

    s(s2 + 2)

    =

    1

    2

    1 cos

    t s

    c

    H(t a)

    L1

    es

    cx

    1

    s(s2 + 2)

    = 1

    2

    1 cos t sc if t > a

    = 0 if t < a

    Therefore, the solution isU(x, t) = c2

    12

    1 cos t sc if t > a

    0 if t < a

    + c2 12 {1 cost}

    Example 1.1.6 Using laplace transform method, solve the initial value prob-lem utt = uxx, 0 < x < and t > 0 with the boundary conditions ux(0, t) =0, u(x, 0) = ex, ut(x, 0) = 0 and u(x, t) 0 as x .

    SolutionLet the given equation be

    utt = uxx (1.1.13)

    Taking laplace transform in equation (1.1.13), we have

    L [utt] = L [uxx]

    s2U(x, s) su(x, 0) ut(x, 0) = d2 [U(x, s)]

    dx2where U(x,s) = L[u(x,t)]

    s2U(x, s) (s)ex = d2 [U(x, s)]

    dx2

    d2 [U(x, s)]

    dx2 s2U(x, s) = sex

    D2 [U(x, s)] s2U(x, s) = sex

    (D2

    s2) [U(x, s)] =

    sex

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    Now, the auxiliary equation is

    m2

    s2 = 0

    m2 = s2 m = s

    Therefore, the complementary function isC.F = Aesx + Besx

    Now, Particular integral

    P.I =1

    D2 s2 (s)ex

    =1

    (1)2 s2 (s)ex

    = 11 s2 (s)e

    x

    =sex

    s2 1

    Therefore, the solution is U(x, s) = Aesx + Besx + sex

    s21 .Now,taking laplace transforms to the remaining two conditions, we have

    L [ux(0, t)] = L [0] and L [u(x, t)] 0 as x Ux(0, s) = 0 and U(x, s) 0 as x

    Now, Ux(x, s) = Asesx + B(

    s)esx + se

    x

    s2

    1

    Ux(0, s) = 0 Ase0 Bse0 + se0

    s2 1 = 0

    As Bs ss2 1 = 0

    A B 1s2 1 = 0

    A B = 1s2 1

    Also U(x, s) 0 as x A = 0

    B

    = 1

    s21 .

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    Therefore, the solution is

    U(x, s) =1

    s2 1(

    s)esx +sexs2 1

    U(x, s) =s

    s2 1 esx +

    sexs2 1

    L [u(x, t)] = ss2 1 e

    sx +sexs2 1

    u(x, t) = L1

    s

    s2 1 esx +

    sexs2 1

    u(x, t) = L1

    s

    s2 1 esx

    exL1

    s

    s2 1

    u(x, t) = L1 s

    s2

    1esx

    excosht

    Also we know that

    L1

    easF(s)

    = L1 [F(s)]tta H(t a) where H(t a)= 1 if t > a= 0 if t < a

    L1

    esxs

    s2 1

    = L1

    s

    s2 1ttx

    H(t x)

    = [cosht]ttx H(t x)

    = cosh(t x) 1 if t > x0 if t < x= cosh(t x) if t > x

    0 if t < x

    Therefore, the solution is

    u(x, t) =cosh(t x) if t > x

    0 if t < x excosht

    u(x, t) = cosh(t x) excosht if t > x

    excosht if t < xExample 1.1.7 Solve using laplace transform method uxx =

    1c2 utt, 0 < x 0 u(x, 0) = u

    t(x, 0) = u(0, t) = f(t) and u(x, t)

    0 as x

    . .

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    SolutionThe given equation is

    uxx = 1c2 utt

    c2uxx = uttTherefore,

    utt = c2uxx (1.1.14)

    Also the initial and boundary conditions are given by

    (i) u(x, 0) = 0

    (ii) ut(x, 0) = 0

    (iii) u(0, t) = f(t)

    (iv) u(x, t) 0 as x Taking laplace transform in equation (??), we have

    L [utt] = L

    c2uxx

    L [utt] = c2L [uxx]

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]

    dx2where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = 0

    d2 [U(x, s)]dx2

    s2c2

    U(x, s) = 0

    D2 s2

    c2

    U(x, s) = 0

    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = sc

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    Therefore, the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx

    Now,taking laplace transforms to the remaining two conditions, we have

    L [u(0, t)] = L [f(t)] and L [u(x, t)] 0 as x u(0, s) = F(s) and u(x, s) 0 as x

    u(0, s) = F(s) Ae0 + Be0 = F(s) A + B = F(s)

    Also u(x, s) 0 as x A = 0 B = F(s).Therefore, the solution is

    U(x, s) = F(s)es

    cx

    L [u(x, t)] = F(s)e scx u(x, t) = L1 F(s)e scx

    Also we know that

    L1

    easF(s)

    = L1 [F(s)]tta H(t a) where H(t a)= 1 if t > a= 0 if t < a

    L1 e scxF(s) = L1 [F(s)]tt sc

    H

    t sc

    Therefore, the solution is

    U(x, t) = L1 [F(s)]tt sc

    H

    t sc

    = [f(t)]tt s

    c

    H

    t sc

    = f

    t s

    c

    H

    t sc

    Example 1.1.8 Using laplace transform, solve a2yxx = ytt , 0 < x < ,t > 0subject to y = 0 at x = 0, t0 and Eyx = p at x = , y = yt(x, 0) = 0, 0 < x < .

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    SolutionLet the given equation be

    ytt = a2yxx (1.1.15)

    Also the initial and boundary conditions are given by

    (i) y(x, 0) = 0 , 0 < x <

    (ii) yt(x, 0) = 0 , 0 < x <

    (iii) y(0, t) = 0, t > 0

    (iv) yx(, t) =pE

    Taking laplace transform in equation (1.1.15), we have

    L [ytt] = L

    a2yxx

    s2Y(x, s) sy(x, 0) yt(x, 0) = a2 d2 [Y(x, s)]

    dx2where Y(x,s) = L[y(x,t)]

    s2Y(x, s) = a2 d2 [Y(x, s)]

    dx2

    a2 d2 [Y(x, s)]

    dx2 s2Y(x, s) = 0

    a2D2Y(x, s) s2Y(x, s) = 0

    D2Y(x, s) s2

    a2Y(x, s) = 0

    D2 s2a2

    Y(x, s) = 0

    Now, the auxiliary equation is

    m2 s2

    a2= 0

    m2 = s2

    a2

    m = sa

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    Therefore, the solution isY(x, s) = Ae

    s

    ax + Be

    s

    ax

    Now, taking laplace transforms to the remaining two conditions, we have

    L [y(0, t)] = L[0] and L [yx(, t)] = L p

    E

    Y(0, s) = 0 and Yx(, s) = p

    Es

    y(0, s) = 0 Ae0 + Be0 = 0 A + B = 0 A = B

    Now, Yx(x, s) = Asa

    es

    ax + B

    sa

    e

    s

    ax

    yx(, s) =p

    Es A

    sa

    es

    a + B

    sa

    e

    s

    a =

    p

    Es

    sa

    Ae

    s

    a Be sa = p

    Es

    Ae sa Be sa = paEs2

    Ae sa + Ae sa = paEs2

    A e sa + e sa = paEs2

    A2cosh s

    a

    =pa

    Es2

    A =paEs2

    2coshsa

    A = pa2Es2cosh

    sa

    B = pa2Es2cosh

    sa

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    Hence the solution is

    Y(x, s) =pa

    2Es2coshsae sax + pa

    2Es2coshsa e sax

    pa2Es2cosh

    sa e sax e sax

    pa2Es2cosh

    sa 2sinh s

    ax

    y(x, t) = L1

    pa

    2Es2coshsa 2sinh s

    ax

    y(x, t) =pa

    EL1 sinh sax

    s2coshsa

    Let F(s) =sinh( sax)s2cosh( sa )

    Then the poles of F(s) are given by

    s2cosh s

    a

    = 0

    s = 0 and cosh sa = 0 s = 0 and cos

    is

    a

    = 0

    s = 0 and isa

    =(2n + 1)

    2, n is any integer

    s = 0 and s = (2n + 1)a2i

    s = 0 and s = (2n + 1)ia2i2

    s = 0 and s = (2n + 1)ia2

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    Clearly s = 0 is a pole of order 2 and s = (2n+1)ic2 are the poles of orderone. Now,

    Res

    estF(s)

    s=0

    =Lim

    s 01

    1!

    d

    ds

    (s 0)2estF(s)

    =Lim

    s 0d

    ds

    s2

    est

    sinhsax

    s2coshsa

    =Lim

    s 0d

    ds

    est

    sinhsa

    x

    coshsa

    =Lim

    s 0cosh

    sa

    estxa

    cosh

    sa

    x

    + testsinhsa

    x estsinh s

    ax

    a

    sinh

    sa

    cosh

    sa2

    =cosh(0)

    e0xa

    cosh(0) + te0sinh(0)

    e0sinh(0) a

    sinh(0)

    [cosh(0)]2

    =(1)

    (1)

    xa

    (1) + t(1)(0)

    [(1)(0)] a

    (0)

    12

    =x

    a

    Now, take estF(s) =estsinh( sax)s2[cosh( sa )]

    = G(s)H(s) where G(s) = e

    stsinhsax

    and H(s)

    = s2coshsa

    Res

    estF(s)

    (2n+1)ia

    2

    =Lim

    s (2n+1)ia2G(s)

    H(s)

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    =Lim

    s (2n+1)ia2estsinh

    sax

    (s2)

    a

    sinh

    sa

    + (2s)cosh

    sa

    =e

    (2n+1)iat

    2 sinh(2n+1)ix2

    (2n+1)ia

    2

    2 a

    sinh

    (2n+1)i

    2

    +2

    (2n+1)ia

    2

    cosh

    (2n+1)i

    2

    =e(2n+1)iat

    2

    1i

    sin

    (2n+1)i2x

    2

    1i

    (2n+1)i2a22

    42

    a

    sin

    (2n+1)i2

    2

    +2

    (2n+1)ia

    2

    cos

    (2n+1)i2

    2

    =e(2n+1)iat

    2 sin(2n+1)x

    2 (2n+1)a24

    sin

    (2n+1)

    2

    + 2

    (2n+1)ia2

    cos

    (2n+1)

    2

    =e(2n+1)iat

    2 sin(2n+1)x

    2

    (2n+1)a2

    4

    (1)n + 2

    (2n+1)ia

    2

    (0)

    =e(2n+1)iat

    2 sin(2n+1)x

    2

    (2n+1)a2

    4

    (1)n

    =e(

    (2n+1)iat2 )sin

    (2n+1)x

    2

    (1)n

    (2n+1)2a24

    (1)n(1)n=

    4e((2n+1)iat2 )sin(2n+1)x

    2

    (1)n

    (2n + 1)2a2(1)2n

    =4e((2n+1)iat2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2a2

    Now,

    Res

    estF(s)

    (2n+1)ia

    2

    =Lim

    s (2n+1)ia2G(s)

    H(s)

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    =Lim

    s (2n+1)ia2estsinh

    sax

    (s2)

    a

    sinh

    sa

    + (2s)cosh

    sa

    =e

    (2n+1)iat

    2 sinh (2n+1)ix

    2

    (2n+1)ia

    2

    2 a

    sinh

    (2n+1)i

    2

    +2

    (2n+1)ia

    2

    cosh

    (2n+1)i

    2

    =e(2n+1)iat

    2

    1i

    sin

    (2n+1)i2x

    2

    1i

    (2n+1)i2a22

    42

    a

    sin

    (2n+1)i2

    2

    +2

    (2n+1)ia

    2

    cos

    (2n+1)i2

    2

    =e(2n+1)iat

    2 sin(2n+1)x

    2 (2n+1)a24

    sin

    (2n+1)2

    + 2

    (2n+1)ia

    2

    cos

    (2n+1)2

    =e (2n+1)iat2 sin

    (2n+1)x

    2

    (2n+1)a2

    4

    sin

    (2n+1)

    2

    + 2

    (2n+1)ia

    2

    cos

    (2n+1)

    2

    =e (2n+1)iat2 sin

    (2n+1)x

    2

    (2n+1)a2

    4

    (1)n + 2

    (2n+1)ia

    2

    (0)

    =e (2n+1)iat2 sin

    (2n+1)x

    2

    (2n+1)a2

    4 (1)n

    =e( (2n+1)iat2 )sin

    (2n+1)x

    2

    (1)n

    (2n+1)2a2

    4

    (1)n(1)n

    =4e( (2n+1)iat2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2a2(1)2n

    =4e( (2n+1)iat2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2a2

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    Now, L1 [F(s)] = Sum of the residues of estF(s) at its poles

    L1

    sinh sax

    s2

    coshsa

    = n = 0

    4e((2n+1)iat

    2 )sin[ (2n+1)x2 ](1)n

    (2n+1)2a2

    +4e(

    (2n+1)iat2 )sin[ (2n+1)x2 ](1)n

    (2n+1)2a2

    =4

    a2

    n = 0

    (1)nsin(2n+1)x

    2

    (2n + 1)2

    e(

    (2n+1)iat2 ) + e(

    (2n+1)iat2 )

    =8

    a2

    n = 0

    (1)ncosh(2n+1)iat

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    Hence the solution is

    u(x, t) =pa

    EL1

    sinh

    sax

    s2

    coshsa

    =pa

    E

    8

    a2

    n = 0

    (1)ncosh(2n+1)iat

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    =

    8p

    E2

    n = 0

    (1)ncosh (2n+1)iat

    2 sin(2n+1)x

    2 (2n + 1)2

    =8a

    2

    n = 0

    (1)ncosh(2n+1)ict

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    Example 1.1.9 Prove that the solution of the wave equation uxx =1c2 utt

    in the strip |x| ,t > 0 satisfying the boundary conditions u(,t)x = 0 ,t > 0 and the initial condition u(x, 0) = ax,

    u(x,0)t = 0 , |x| < is ax

    acL1 s2sinh xsc sech s

    c.

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    SolutionThe given equation is

    uxx =1

    c2utt

    c2uxx = utt

    Therefore,

    utt = c2uxx (1.1.16)

    Also the initial and boundary conditions are given by

    (i) u(x, 0) = ax

    (ii) u(x,0)t

    = 0 , |x| <

    (iii)u(,t)x = 0 , t > 0

    (iv) u(,t)x

    = 0 , t > 0

    Taking laplace transform in equation (??), we have

    L [utt] = L c2uxx L [utt] = c2L [uxx]

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]

    dx2where U(x,s) = L[u(x,t)]

    s2U(x, s) sax = c2 d2 [U(x, s)]

    dx2{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = sax

    d2 [U(x, s)]

    dx2 s

    2

    c2U(x, s) =

    saxc2

    D2 s2

    c2 U(x, s) =sax

    c2

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    Now, the auxiliary equation is

    m2

    s2

    c2 = 0

    m2 = s2

    c2

    m = sc

    Therefore, the complementary function isC.F = Ae

    s

    cx + Be

    s

    cx

    Now, Particular integral

    P.I =1

    D2 s2

    c2

    saxc2

    =1

    s2c2

    1 c2D2

    s2

    saxc2

    =

    axc2

    c2s2

    1 c2D2s2

    (s)=

    ax

    s2

    1 c

    2D2

    s2

    1(s)

    =ax

    s2

    1 +

    c2D2

    s2+ ...

    (s)

    =

    ax

    s2 (s)

    =ax

    s

    Hence the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx + ax

    s.

    Now,taking laplace transforms to the remaining two conditions, we have

    L [ux(, t)] = L [0] and L [ux(, t)] = L [0]

    Ux(, s) = 0 and Ux(

    , s) = 0

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    Now, Ux(x, s) = Asc

    e(

    s

    c)x + Bs

    c

    e(

    s

    c)x + as

    Ux(, s) = 0 A

    sc

    es + B

    sc

    es + a

    s= 0

    As

    c

    e(

    s

    c ) Bs

    c

    e(

    s

    c) =a

    s

    s

    c

    Ae(

    s

    c) Be( sc)

    =a

    s

    Ae( sc) Be( sc ) = acs2

    Ae( sc)e( sc) Be(sc)e( sc ) = esac

    s2

    Ae2( sc ) B = e( sc)ac

    s2

    (1.1.17)

    Ux(, s) = 0 As

    c

    e(

    s

    c ) + B

    sc

    e(

    s

    c ) +a

    s= 0

    As

    c e( sc ) B

    s

    c e( sc ) = a

    s

    sc

    Ae(

    s

    c) Be(sc)

    =a

    s

    Ae( sc ) Be( sc ) = acs2

    Ae( sc )e( sc) Be( sc )e( sc ) = e( sc )ac

    s2

    Ae2(

    s

    c )

    B = e(

    s

    c )ac

    s2 (1.1.18)

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    Subtracting equations (5.2.16) and (5.2.12), we get,

    Ae2(s

    c )

    Ae2(

    s

    c ) = e(s

    c )acs2 e

    ( sc )acs2

    A

    e2(s

    c) e2( sc )

    =

    acs2

    e(

    s

    c) e( sc)

    A

    2sinh

    2s

    c

    =

    acs2

    2sinh

    s

    c

    A =ac

    s2

    2sinh

    sc

    2sinh

    2sc

    A =

    acs2

    sinh

    sc

    2sinh

    sc

    cosh

    sc

    A = acs

    2 2cosh

    sc

    A =

    ac2s2

    sech

    s

    c

    From equation (5.2.16), we have

    Ae2(s

    c ) B = e( sc )ac

    s2

    B = Ae2( sc) e( sc )ac

    s2

    B = ac2s2 sechsc e2(s

    c )

    e( sc )acs2

    B =ac

    s2

    e(

    s

    c )

    1

    2

    sech

    s

    c

    e(

    s

    c) 1

    B =ac

    s2

    e(

    s

    c )

    1

    2

    2

    e(s

    c ) + e(s

    c )e(

    s

    c) 1

    B =ac

    s2

    e(

    s

    c )

    e(

    s

    c)

    e(s

    c ) + e(s

    c ) 1

    B =ac

    s2

    e(

    s

    c )

    e(

    s

    c ) e(sc ) e(sc )e(

    s

    c ) + e(s

    c )

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    B =ac

    s2

    e(

    s

    c)

    e(sc )

    e(s

    c ) + e(s

    c )

    B = acs2

    1e(

    s

    c ) + e(s

    c )

    B =

    ac2s2

    2e(

    s

    c ) + e(s

    c )

    B = ac

    2s2

    sech

    s

    c

    Hence the solution is

    U(x, s) =ac

    2s2

    sech

    sc

    escx +

    ac

    2s2

    sech

    sc

    e

    scx + ax

    s

    =

    ac2s2

    sech

    s

    c

    es

    cx e scx + ax

    s

    =

    ac2s2

    sech

    s

    c

    2sinh

    sc

    x

    +ax

    s

    =ax

    sac

    s2

    sech

    s

    c

    sinh

    sc

    x

    L [u(x, t)] = axs

    ac

    s2

    sech

    s

    c

    sinh

    sc

    x

    u(x, t) = L1

    ax

    sac

    s2

    sech

    s

    c

    sinh

    sc

    x

    u(x, t) = (ax)L1

    1

    s

    (ac)L1

    sinh

    sc

    x

    s2

    coshsc

    u(x, t) = (ax) (ac)L1

    sinhscx

    s2 cosh sc

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    Let F(s) =sinh( scx)

    s2[cosh( sc )]Then the poles of estF(s) are given by

    s2coshs

    c

    = 0

    s = 0 and coshs

    c

    = 0

    s = 0 and cos

    is

    c

    = 0

    s = 0 and isc

    = (2n + 1)2

    s = 0 and s = (2n + 1)c2i

    s = 0 and s = (2n + 1)ic2i2

    s = 0 and s = (2n + 1)ic2

    s = 0 and s = (2n + 1)ic2

    Clearly s = 0 is a pole of order 2 and s = (2n+1)ic2 are the poles of orderone. Now,

    Res

    estF(s)

    s=0

    =Lim

    s 01

    1!

    d

    ds

    (s 0)2estF(s)

    =Lim

    s 0d

    ds

    s2

    est

    sinhsa

    x

    s2coshsc

    =Lim

    s 0d

    ds

    est

    sinhsax

    cosh sc

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    =Lim

    s 0cosh

    sc

    estxc

    cosh

    scx

    + testsinhscx estsinh scx c sinh sc

    cosh

    sc

    2

    = cosh(0)

    e0 x

    c

    cosh(0) + te0

    sinh(0) e0sinh(0) c sinh(0)

    [cosh(0)]2

    =(1)

    (1)

    xc

    (1) + t(1)(0)

    [(1)(0)] c (0)12

    =x

    c

    Now, take estF(s) =estsinh( scx)s2[cosh( sc )]

    =G(s)H(s) where G(s) = e

    stsinhsc

    x

    and H(s)

    = s2coshsc

    Res

    estF(s)

    (2n+1)ic

    2

    =Lim

    s (2n+1)ic2G(s)

    H(s)

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    =Lim

    s (2n+1)ic2estsinh

    scx

    (s2)

    c

    sinh

    sc

    + (2s)cosh

    sc

    = e

    (2n+1)ict

    2

    sinh(2n+1)ix2

    (2n+1)ic

    2

    2 c

    sinh

    (2n+1)i

    2

    +2

    (2n+1)ic

    2

    cosh

    (2n+1)i

    2

    =e(2n+1)ict

    2

    1i

    sin

    (2n+1)i2x

    2

    1i

    (2n+1)i2c22

    42

    c

    sin

    (2n+1)i2

    2

    +2

    (2n+1)ic

    2

    cos

    (2n+1)i2

    2

    =e(2n+1)ict

    2 sin

    (2n+1)x

    2 (2n+1)c24

    sin

    (2n+1)

    2

    + 2(2n+1)ic

    2

    cos(2n+1)

    2

    =e(2n+1)ict

    2 sin(2n+1)x

    2

    (2n+1)c2

    4

    (1)n + 2

    (2n+1)ic

    2

    (0)

    =e(2n+1)ict

    2 sin(2n+1)x

    2

    (2n+1)c2

    4

    (1)n

    =e(

    (2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n+1)2c24 (1)n(

    1)n

    =4e((2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2c2(1)2n

    =4e((2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2c2

    Now,

    Res

    estF(s)

    (2n+1)ic

    2

    =Lim

    s (2n+1)ic2G(s)

    H(s)

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    =Lim

    s (2n+1)ic2estsinh

    scx

    (s2)

    c

    sinh

    sc

    + (2s)cosh

    sc

    = e

    (2n+1)ict

    2

    sinh (2n+1)ix

    2

    (2n+1)ic

    2

    2 c

    sinh

    (2n+1)i

    2

    +2

    (2n+1)ic

    2

    cosh

    (2n+1)i

    2

    =e(2n+1)ict

    2

    1i

    sin

    (2n+1)i2x

    2

    1i

    (2n+1)i2c22

    42

    c

    sin

    (2n+1)i2

    2

    +2

    (2n+1)ic

    2

    cos

    (2n+1)i2

    2

    =e(2n+1)ict

    2 sin

    (2n+1)x

    2 (2n+1)c24 sin(2n+1)2 + 2 (2n+1)ic2 cos(2n+1)2 =

    e (2n+1)ict2 sin(2n+1)x

    2

    (2n+1)c2

    4

    sin

    (2n+1)

    2

    + 2

    (2n+1)ic

    2

    cos

    (2n+1)

    2

    =e (2n+1)ict2 sin

    (2n+1)x

    2

    (2n+1)c2

    4

    (1)n + 2

    (2n+1)ic

    2

    (0)

    =e (2n+1)ict2 sin

    (2n+1)x

    2

    (2n+1)c24 (1)n

    =e( (2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n+1)2c2

    4

    (1)n(1)n

    =4e( (2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2c2(1)2n

    =4e( (2n+1)ict2 )sin

    (2n+1)x

    2

    (1)n

    (2n + 1)2c2

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    Now, L1 [F(s)] = Sum of the residues of estF(s) at its poles

    L1 sinh scxs2 cosh sc =x

    c +

    n = 0

    4e(

    (2n+1)ict2 )sin[ (2n+1)x2 ](1)n

    (2n+1)2

    c2

    +4e(

    (2n+1)ict2 )sin[ (2n+1)x2 ](1)n

    (2n+1)2c2

    =x

    c 4

    c2

    n = 0

    (1)nsin(2n+1)x

    2

    (2n + 1)2

    e(

    (2n+1)ict2 ) + e(

    (2n+1)ict2 )

    =x

    c 8

    c2

    n = 0

    (1)ncosh(2n+1)ict

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    Hence the solution is

    u(x, t) = (ax) (ac)L1

    sinhscx

    s2

    coshsc

    = ax (ac)xc 8c2

    n = 0

    (1)ncosh(2n+1)ict

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    = ax ax + 8a2

    n = 0(1)ncosh

    (2n+1)ict

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    =8a

    2

    n = 0

    (1)ncosh(2n+1)ict

    2

    sin

    (2n+1)x

    2

    (2n + 1)2

    Example 1.1.10 An infinitely long string having one end at x = 0 is initiallyat rest on the x-axis and the end x = 0 undergoes a periodic transverse dis-placement described by A0sint, t > 0. Find the displacement of any point onthe string at any time t.

    SolutionThe transverse displacement of the string is described by the partial differential

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    equation

    uxx =1

    c2utt

    c2uxx = uttTherefore,

    utt = c2uxx (1.1.19)

    Also the initial and boundary conditions are given by

    (i) u(x, 0) = 0

    (ii) ut(x, 0) = 0

    (iii) u(0, t) = A0sint, t > 0

    (iv) u is bounded as x

    Taking laplace transform in equation (??), we haveL [utt] = L

    c2uxx

    L [utt] = c2L [uxx]

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]

    dx2where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = 0

    d2 [U(x, s)]

    dx2 s2

    c2 U(x, s) = 0

    D2 s2

    c2

    U(x, s) = 0

    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = sc

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    Therefore, the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx.

    Now,taking laplace transforms to the remaining two conditions, we have

    L [u(x, t)] = bounded and L [u(0, t)] = L [A0sint]

    U(x, s) = bounded and U(0, s) = A0 s2 + 2

    Since U(x, s) is bounded as x , we have A = 0Therefore, U(x, s) = Be

    s

    cx

    U(0, s) = A0

    s2 + 2 Be0 = A0

    s2 + 2

    B = A0 s2 + 2

    Therefore, the solution is

    U(x, s) = A0

    s2 + 2e

    s

    cx

    L [u(x, t)] = A0 s2 + 2

    es

    cx

    u(x, t) = L1

    A0

    s2 + 2e

    s

    cx

    u(x, t) = A0L1

    s2 + 2e

    s

    cx

    Also we know that

    L1

    eas

    F(s)

    = L1

    [F(s)]tta H(t a) where H(t a)= 1 if t > a= 0 if t < a

    L1

    s2 + 2e

    s

    cx

    = L1

    s2 + 2

    tt x

    c

    H

    t xc

    = [sint]tt xc

    H

    t xc

    = sin

    t x

    c

    1 if t > xc0 if t < x

    c

    = sin

    t xc

    if t > xc0 if t < xc

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    Therefore, the solution is

    u(x, t) =sin

    t xc

    if t > xc

    0 if t < xc

    Example 1.1.11 If the function u(x,t) satisfies the following PDE uxx =1c2 utt + k, 0 < x < , t > 0 subject to the boundary conditions u(0, t) =0 and ux(, t) = 0, t > 0 and the initial conditions u(x, 0) = ut(x, 0) = 0,0 < x < . .

    SolutionThe given equation is

    uxx =

    1

    c2 utt + k uxx =1

    c2

    utt + c2

    k

    c2uxx = utt + c2k utt = c2uxx c2k

    Therefore,

    utt = c2uxx c2k (1.1.20)

    Also the initial and boundary conditions are given by

    (i) u(x, 0) = 0, 0 < x <

    (ii) ut(x, 0) = 0, 0 < x <

    (iii) u(0, t) = 0

    (iv) ux(, t) = 0, t > 0

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    Taking laplace transform in equation (??), we have

    L [utt] = L

    c2uxx c2k L [utt] = L

    c2uxx

    c2kL[1] s2U(x, s) su(x, 0) ut(x, 0) = c2 d

    2 [U(x, s)]

    dx2 c2k

    1

    s

    where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2 c

    2k

    s{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = c

    2k

    s

    d2 [U(x, s)]

    dx2 s

    2

    c2U(x, s) =

    k

    s

    D2 s2c2

    U(x, s) = ks

    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = s

    c

    Therefore, the complementary function isC.F = Ae

    s

    cx + Be

    s

    cx

    Now, Particular integral

    P.I =1

    D2 s2c2 k

    s

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    P.I =1

    D2 s2c2

    k

    s

    =

    1s2c2

    1 c2D2s2

    ks

    =

    c2s2

    1 c2D2s2

    ks

    =kc2

    s3

    1 c

    2D2

    s2

    1(1)

    =kc2

    s3

    1 +

    c2D2

    s2+ ...

    (1)

    =kc2

    s3

    Hence the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx kc2

    s3.

    Now,taking laplace transforms to the remaining two conditions, we have

    L [ux(, t)] = L [0] and L [u(0, t)] = L [0]

    Ux(, s) = 0 and U(0, s) = 0

    Now, Ux(x, s) = A sc

    e

    ( sc)x

    + Bsc e(

    s

    c)x

    U(0, s) = 0 A + B kc2

    s3= 0

    A + B = kc2

    s3

    A + B =

    kc2

    s

    3(1.1.21)

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    Ux(, s) = 0 As

    c

    e(

    s

    c) + B

    sc

    e(

    s

    c ) = 0

    As

    c e( sc) B

    s

    c e( sc ) = 0

    s

    c

    Ae(

    s

    c ) Be( sc)

    = 0

    Ae( sc) Be( sc) = 0 Ae( sc)e( sc) Be( sc)e( sc) = 0 Ae( 2sc ) B = 0

    Ae(2sc ) B = 0 (1.1.22)

    adding equations (1.1.21) and (1.1.22), we get,

    Ae2(s

    c ) + A =kc2

    s3

    Ae(sc)

    e(s

    c) + e2(s

    c )

    =kc2

    s3

    A = kc2

    s3e(s

    c )

    e(s

    c ) + e2(s

    c)

    A = kc2e(

    s

    c )

    2s3coshsc

    From equation (1.1.22), we have

    Ae2(s

    c) B = 0 B = Ae2( sc )

    B =

    kc2e(s

    c )

    2s3coshsc

    e2(

    s

    c )

    B =

    kc2e(s

    c)

    2s3coshsc

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    Hence the solution is

    U(x, s) = Aes

    cx + Be

    s

    cx

    kc2

    s3

    =kc2e(

    s

    c )

    2s3coshsc

    es

    cx +

    kc2e(s

    c)

    2s3coshsc

    es

    cx kc

    2

    s3

    =kc2

    2s3coshsc

    e(

    (x)sc ) + e(

    (x)sc )

    kc

    2

    s3

    =kc2

    2s3coshsc

    2cosh

    ( x)s

    c

    kc

    2

    s3

    =kc2

    s3cosh

    sc

    cosh

    ( x)s

    c

    kc

    2

    s3

    L [u(x, t)] = kc2

    s3coshsc

    cosh

    ( x)s

    c

    kc

    2

    s3

    u(x, t) = L1

    kc2

    s3coshsc

    cosh

    ( x)s

    c

    kc

    2

    s3

    u(x, t) = kc2

    L1

    cosh

    (x)s

    c

    s3cosh sc

    L1

    1

    s3

    u(x, t) = kc2L1

    cosh

    (x)s

    c

    s3coshsc

    1

    2L1

    2!

    s3

    u(x, t) = kc2L1

    cosh

    (x)s

    c

    s3coshsc

    1

    2t2

    Let F(s) =cosh( (x)sc )s3cosh(sc)

    Then estF(s) =estcosh( (x)sc )

    s3cosh(sc)

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    Then the poles of estF(s) are given by

    s3cosh

    sc

    = 0

    s = 0 and coshs

    c

    = 0

    s = 0 and cos

    is

    c

    = 0

    s = 0 and isc

    = (2n + 1)2

    s = 0 and s = (2n + 1)c2i

    s = 0 and s = (2n + 1)ic2i2

    s = 0 and s = (2n + 1)ic2

    s = 0 and s = (2n + 1)ic2

    Clearly s = 0 is a pole of order 3 and s = (2n+1)ic2 are the poles of orderone. Now,

    Res

    estF(s)

    s=0

    =Lim

    s 01

    2!

    d2

    ds2

    (s 0)3estF(s)

    =1

    2

    Lim

    s 0d2

    ds2

    s3

    est cosh

    (x)s

    c

    s3coshsc

    =1

    2

    Lim

    s 0d2

    ds2

    estcosh

    (x)s

    c

    cosh

    sc

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    =1

    2

    Lim

    s 0d

    ds

    coshsc

    est

    (x)c sinh

    (x)s

    c

    + testcosh

    (x)s

    c

    estcosh

    (x)s

    c

    c

    sinh

    sc

    cosh sc

    2

    =1

    2

    Lim

    s 0

    cosh

    sc

    2

    coshsc

    test (x)c sinh

    (x)s

    c

    + est

    xc

    2 cos

    (x)s

    c

    + t2estcosh

    (x)s

    c

    + t

    xc

    estsinh

    (x)s

    c

    +c

    sinh

    sc

    est

    (x)c sinh

    (x)s

    c

    + testcosh

    (x)s

    c

    testcosh

    (x)s

    c

    c

    sinh

    sc

    est xc sinh (x)sc c sinh sc estcosh (x)sc c2 cosh sc

    coshsc

    est

    (x)c sinh

    (x)s

    c

    + testcosh

    (x)s

    c

    estcosh

    (x)s

    c

    c

    sinh

    sc

    2c

    cosh

    sc

    sinh

    sc

    coshsc

    4

    =1

    2

    [cosh(0)]2

    cosh(0)

    te0(x)

    c sinh(0) + e0xc

    2cos(0) + t2e0cosh(0) + t

    xc

    e0sinh(0)

    +c

    sinh(0)

    e0

    (x)c sinh(0) + te

    0cosh(0)

    te0cosh(0) c sinh(0) e0 xc sinh(0) c sinh(0) e0cosh(0) c2 cosh(0)

    cosh(0)

    e0(x)

    csinh(0) + te0cosh(0)

    e0cosh(0)

    c

    sinh(0)

    2c

    cosh(0)sinh(0)

    [cosh(0)]4

    =1

    2

    0 +

    x

    c

    2+ t2 + 0 + 0 0 0

    c

    2 {0 + t 0} 2(0)

    =1

    2

    2 + x2 2x + c2t2 2

    c2

    =x2 2x + c2t2

    2c2

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    Now, take estF(s) =estcosh( (x)sc )

    s3cosh( sc )= G(s)

    H(s) where G(s) = estcosh

    (x)s

    c

    and H(s) = s3cosh sc

    Res

    estF(s)

    (2n+1)ic

    2

    =Lim

    s (2n+1)ic2G(s)

    H(s)

    =Lim

    s (2n+1)ic

    2

    estcosh

    (x)s

    c

    3s2

    cosh sc

    + s3

    c

    sinh sc

    =

    e[(2n+1)ic

    2 ]tcosh

    (x)[(2n+1)ic2 ]

    c

    3(2n+1)ic

    2

    2cosh

    [(2n+1)ic2 ]

    c

    +

    (2n+1)ic

    2

    3 c

    sinh

    [(2n+1)ic2 ]

    c

    =e[

    (2n+1)ic2 ]tcos

    (x)(2n+1)i2

    2

    3(2n+1)ic

    2

    2cos

    (2n+1)i2

    2

    +(2n+1)ic

    2

    3 ic

    sin

    (2n+1)i2

    2

    =e[

    (2n+1)ict2 ]cos

    (x)(2n+1)

    2

    3(2n+1)2c2242 cos (2n+1)2 + (2n+1)3ic3383 ic sin (2n+1)2

    =e[

    (2n+1)ict2 ]cos

    (x)(2n+1)

    2

    (2n+1)3ic23

    8i2

    sin

    (2n+1)

    2

    =82

    cos

    (2n+1)ct

    2

    isin

    (2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23] (1)n

    =82(1)n

    cos

    (2n+1)ct

    2

    isin

    (2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23]

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    51Res

    estF(s)

    (2n+1)ic

    2

    =Lim

    s (2n+1)ic2G(s)

    H(s)

    = Lims (2n+1)ic2

    estcosh (x)sc

    3s2cosh

    sc

    + s3

    c

    sinh

    sc

    =

    e[(2n+1)ic

    2 ]tcosh

    (x)[ (2n+1)ic2 ]

    c

    3(2n+1)ic

    2

    2cosh

    [ (2n+1)ic2 ]

    c

    +

    (2n+1)ic

    2

    3 c

    sinh

    [ (2n+1)ic2 ]

    c

    =e[

    (2n+1)ic2 ]tcos

    (x)(2n+1)i2

    2

    3(2n+1)ic

    2

    2cos

    (2n+1)i2

    2

    +(2n+1)ic

    2

    3 ic

    sin

    (2n+1)i2

    2

    =

    e[(2n+1)ict

    2 ]cos(x)(2n+1)2 3(2n+1)2c22

    42

    cos

    (2n+1)

    2

    +(2n+1)3ic33

    83

    ic

    sin

    (2n+1)

    2

    =e[

    (2n+1)ict2 ]cos

    (x)(2n+1)

    2

    (2n+1)3ic23

    8i2

    sin

    (2n+1)

    2

    =82

    cos

    (2n+1)ct

    2

    + isin

    (2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23] (1)n

    =82(1)n

    cos

    (2n+1)ct

    2

    + isin

    (2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23]

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    Now,L1 [F(s)] = sum of residues of estF(s) at its polesHence,

    L1cosh (x)sc

    s3coshsc

    = sum of residues of est cosh(

    x)s

    c

    s3cosh

    sc

    =

    x22x+c2t22c2

    +

    n = 0

    82(1)n{cos( (2n+1)ct2 )+isin( (2n+1)ct2 )}cos( (x)(2n+1)2 )

    [(2n+1)3c23]

    +

    n = 0

    82(1)n{cos( (2n+1)ct2 )isin( (2n+1)ct2 )}cos( (x)(2n+1)2 )

    [(2n+1)3c23]

    =x2

    2x + c2t2

    2c2 +

    n = 0

    162(

    1)ncos (2n+1)ct2 cos (x)(2n+1)2

    [(2n + 1)3c23]

    The solution is

    u(x, t) = kc2

    L1

    cosh

    (x)s

    c

    s3coshsc

    1

    2t2

    = kc2

    x2 2x + c2t22c2

    +

    n = 0

    162(1)ncos(2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23]

    t2

    2

    = kc2

    x

    2 2x2c2

    +

    n = 0

    162(1)ncos(2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    [(2n + 1)3c23]

    =kx(x 2)

    2+

    8k2

    3

    n = 0

    (1)ncos(2n+1)ct

    2

    cos

    (x)(2n+1)

    2

    (2n + 1)3

    Example 1.1.12 The end x = 0 of an elastic bar is free while a constantlongitudinal force F0 per unit area acts longitudinally at length x = . Thebar is initially at rest and it is unstrained. Find the displacement u(x, t) in thebar.

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    SolutionThe initial and boundary conditions are given by

    (i) u(x, 0) = 0

    (ii) ut(x, 0) = 0

    (iii) ux(0, t) = 0

    (iv) Eux(, t) = F0.

    The transverse displacement of the string is described by the partial differentialequation

    uxx = 1c2

    utt

    c2uxx = utt

    Therefore,

    utt = c2uxx (1.1.23)

    Taking laplace transform in equation (1.1.23), we have

    L [utt] = L

    c2uxx

    L [utt] = c2L [uxx]

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]

    dx2where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = 0

    d2 [U(x, s)]

    dx2 s

    2

    c2U(x, s) = 0

    D2 s2

    c2

    U(x, s) = 0

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    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = sc

    Therefore, the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx.

    Now, taking laplace transforms to the remaining two conditions, we have

    L [ux(0, t)] = L[0] and L [ux(, t)] = L

    F0

    E

    Ux(0, s) = 0 and Ux(, s) = F0Es

    Now, Ux(x, s) = A sc

    es

    cx + B

    sc

    es

    cx

    Ux(0, s) = 0 As

    c

    e0 + B

    sc

    e0 = 0

    As

    c

    B

    sc

    = 0

    s

    c

    (A B) = 0

    A B = 0 A = B.

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    Ux(, s) =F0

    Es A

    sc

    es

    c + B

    sc

    e

    s

    c =

    F0

    Es

    s

    cAesc Be

    sc = F0

    Es

    Ae sc Be sc = F0cEs2

    Ae sc Ae sc = F0cEs2

    A e sc e sc = F0cEs2

    A2sinhs

    c

    =F0c

    Es2

    A =F0cEs2

    2sinh sc

    A = F0c2Es2sinh

    sc

    B = F0c2Es2sinh

    sc

    Hence the solution is

    U(x, s) =F0c

    2Es2sinhsc e scx + F0c

    2Es2sinhsc e scx

    F0c2Es2sinh

    sc e scx + e scx

    pa2Es2sinh

    sa 2cosh s

    ax

    u(x, t) = L1

    F0c

    2Es2sinhsc

    2coshs

    cx

    u(x, t) = F0cE

    L1

    coshscx

    s2sinh sc

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    Let F(s) =cosh( scx)s2sinh( sc )

    Then the poles of F(s) are given by

    s2coshs

    c

    = 0

    s = 0 and sinhs

    c

    = 0

    s = 0 and 1i

    sin

    is

    c

    = 0

    s = 0 and sin isc = 0 s = 0 and is

    c= n, n is any integer

    s = 0 and s = nci

    s = 0 and s = nici2

    s = 0 and s = nic

    s = 0 and s = nic

    , n is any integer

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    Clearly s = 0 is a pole of order 2 and s = nic are poles of order 1 where n isany integer.

    estcosh

    scx

    s2sinhsc =

    1 + st1! +

    (st)2

    2! + ...

    1 +( scx)

    2

    2! +( scx)

    4

    4! + ...

    s2

    ( sc )1! +

    ( sc )3

    3! +( scx)

    5

    5! + ...

    =

    1 + st + s

    2t2

    2 +s3t3

    6 ...

    1 + s2x2

    2c2 + ...

    s3c

    1 + s

    22

    6c2 + ...

    =c

    s3

    1 +

    s2x2

    2c2+ st +

    s3x2t

    2c2+

    s2t2

    2+

    s3t3

    6+ ...

    1 +

    s22

    6c2+ ...

    1

    = c

    s3 +x2

    2cs +ct

    s2 +x2t

    2c +ct2

    2s +ct3

    6 + ...

    1 s22

    6c2 + ...

    =c

    s3+

    x2

    2cs+

    ct

    s2+

    x2t

    2c+

    ct2

    2s+

    ct3

    6

    6cs sx

    2

    12c3 t

    6c s

    2x2t

    6c3 st

    2

    12c s

    2t3

    36c ...

    Res

    estF(s)

    s=0

    = coefficient of1

    sin the expansion of Laurent series of estF(s)

    =

    x2

    2c +

    ct2

    2

    6c

    Now, take estF(s) =estcosh( scx)s2[sinh( sc )]

    =G(s)H(s) where G(s) = e

    stcoshscx

    and H(s)

    = s2sinhsc

    Res

    estF(s)

    nic

    =Lim

    s nicG(s)

    H(s)

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    =Lim

    s nicestcosh

    scx

    (s2)c

    cosh

    sc

    + (2s)sinhsc

    =

    enict

    cosh nix

    nic

    2 c

    cosh (ni)

    +2nic

    sinh (ni)

    =enict

    cosni2x

    n2i2c22

    2

    c

    cos

    ni2+2

    nic

    1i sin

    ni2

    =enict

    cosnx

    n2c22

    2

    c

    cos (n)

    +2 nc sin (n)

    =enict

    cosnx

    n2c2

    (1)n + 2 nc

    (0)

    =enict

    cos(nx

    n2c2

    (1)n

    =e(

    nict

    )cosnx

    (1)nn2c2

    (1)n(1)n

    =e(nict )cos nx (1)n

    n2c2(1)2n

    =e(

    nict

    )cosnx

    (1)n

    n2c2

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    Now,

    =Lim

    s nicestcosh

    scx

    (s2)c

    cosh

    sc

    + (2s)sinhsc

    =

    enict

    coshnix

    nic

    2 c

    cosh (ni)

    +2nic

    sinh (ni)

    =enict

    cosni2x

    n2i2c22

    2 c cos ni

    2+2

    nic 1

    i sin

    ni2

    =enict

    cosnx

    n2c22

    2

    c

    cos (n)

    +2nc

    sin (n)

    =enict

    cosnx

    n2c22

    2

    c

    cos (n)

    2 nc sin (n)

    =enict

    cos

    nx

    n2c2 (1)n

    2 nc (0)

    =enict

    cos(nx

    n2c2

    (1)n

    =e(

    nict

    )cosnx

    (1)nn2c2

    (1)n(1)n

    =e(nict )cos nx (1)n

    n2c2(1)2n

    =e(nict )cos nx (1)n

    n2c2

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    Now, L1 [F(s)] = Sum of the residues of estF(s) at its poles

    L1 cosh scx

    s2

    sinhsc

    =

    x2

    2c +

    ct2

    2

    6c +

    n = 0

    e(

    nict )cos[nx ](1)n

    n2c2

    +e(

    nict )cos[nx ](1)n

    n2c2

    =x2

    2c+

    ct2

    2

    6c

    c2

    n = 0

    (1)ncos nx

    n2

    e(

    nict

    ) + e(nict

    )

    =x2

    2c+

    ct2

    2

    6c 2

    c2

    n = 0

    (1)ncos nct cos nx n2

    Hence the solution is

    u(x, t) =F0c

    EL1

    cosh

    scx

    s2

    sinhsc

    =F0c

    E

    x

    2

    2c+

    ct2

    2

    6c 2

    c2

    n = 0

    (1)ncos nct cos nx n2

    Example 1.1.13 A semi infinite string is stretched along the positive half ofa horizontal x-axis with its end x = 0 ties at the origin and with its end x = 0ties at the origin and with its distant end looped around a vertical support that

    exerts no vertical force on the loop. The string is initially supported at restalong the x-axis. At time t = 0, the support is removed and the string movesunder the action of gravity. Obtain the displacement u(x, t) at any position x,at any time t.

    SolutionWe know that the wave equation for a long string under its weight is

    utt = c2uxx g (1.1.24)

    where g is the gravitational force.Also the initial and boundary conditions are given by

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    (i) u(x, 0) = 0

    (ii) ut(x, 0) = 0

    (iii) u(0, t) = 0

    (iv) ux 0 as x

    Taking laplace transform in equation (1.1.24), we have

    L [utt] = L

    c2uxx g

    L [utt] = L c2uxx L[g]

    s2U(x, s) su(x, 0) ut(x, 0) = c2 d2 [U(x, s)]dx2

    gs

    where U(x,s) = L[u(x,t)]

    s2U(x, s) = c2 d2 [U(x, s)]

    dx2 g

    s{by using the initial conditions (i) and (ii)}

    c2 d2 [U(x, s)]

    dx2 s2U(x, s) = g

    s

    d2 [U(x, s)]

    dx2 s

    2

    c2U(x, s) =

    g

    sc2

    D2 s2

    c2

    U(x, s) =

    g

    sc2

    Now, the auxiliary equation is

    m2 s2

    c2= 0

    m2 = s2

    c2

    m = sc

    Therefore, the complementary function isC.F = Ae

    s

    cx + Be

    s

    cx

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    Now, Particular integral

    P.I =1

    D2 s2

    c2

    g

    sc2

    =1

    D2 s2c2 g

    sc2e0x

    =1 s2c2

    gsc2

    e0x

    =c2s2

    g

    sc2

    =gs3

    Hence the solution isU(x, s) = Ae

    s

    cx + Be

    s

    cx

    g

    s3 .

    Now,taking laplace transforms to the remaining condition u(0, t) = 0, we have

    L [u(0, t)] = L[0]

    u(0, s) = 0

    u(0, s) = 0 Ae0 + Be0 gs3

    = 0

    A + B gs3

    = 0

    A + B = gs3

    Also, Ux(x, s) = Asc

    e scx + B

    sc

    e scx

    Now, by (iv), ux 0 as x Hence A = 0. B = g

    s3.

    Therefore, the solution is

    U(x, s) = g

    s3

    e

    s

    cx g

    s3

    U(x, s) = g

    s3

    e

    s

    cx 1

    L [U(x, t)] =

    g

    s3 e

    s

    cx 1

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    U(x, t) = L1 g

    s3

    e

    s

    cx 1

    = L1 ge

    s

    cx

    s

    3

    g

    s

    3 = gL1

    e

    s

    cx

    s3

    g

    2!L1

    2!

    s3

    = gu xc

    (t)L1

    1

    s3

    g

    2!L1

    2!

    s3

    = gu xc

    (t)1

    2!L1

    2!

    s3

    ttx

    c

    g2!

    t2

    = g

    0 if t < xc1 if t > xc

    t2

    2 ttxc

    gt2

    2

    = g 0 if t < xc

    1 if t > xc t

    xc 2

    2 gt2

    2

    = g

    0 if t < xc

    (txc )2

    2 if t >xc

    gt

    2

    2

    Example 1.1.14 A tightly stretched string has ends fixed at x = 0 and x =. At time t = 0, the string is given a shape defined by y = x( x) and thenreleased. Find the displacement at any time t.

    SolutionLet the one dimensional wave equation be

    ytt = a2yxx (1.1.25)

    Also the initial and boundary conditions are given by

    (i) y(0, t) = 0, t > 0

    (ii) y(, t) = 0

    (iii) yt(x, 0) = 0 , 0 < x <

    (iv) y(x, 0) = x( x) , 0 < x <

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    Taking laplace transform in equation (1.1.25), we have

    L [ytt] = L

    a2yxx

    s2Y(x, s) sy(x, 0) yt(x, 0) = a2 d2 [Y(x, s)]

    dx2where Y(x,s) = L[y(x,t)]

    s2Y(x, s) sx( x) = a2 d2 [Y(x, s)]

    dx2

    a2 d2 [Y(x, s)]

    dx2 s2Y(x, s) = sx( x)

    a2D2Y(x, s) s2Y(x, s) = sx( x)

    D2Y(x, s)

    s2

    a2

    Y(x, s) =

    sx(

    x)

    D2 s2

    a2

    Y(x, s) =

    sxa2

    ( x)

    Now, the auxiliary equation is

    m2 s2a2

    = 0

    m2 = s2

    a2

    m = sa

    Therefore, the complementary function isC.F = Ae

    s

    ax + Be

    s

    ax

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    Now, Particular integral

    P.I = 1D2 s2a2

    sxa2

    ( x)

    =1

    s2a2

    1 D2a2s2

    sxa2

    ( x)

    =a2

    s2

    1 D

    2a2

    s2

    1 sa2

    (x x2)

    =a2

    s2

    1 +

    D2a2

    s2+ ...

    sa2

    (x x2)

    =a2

    s2 s

    a2(x x2) + a

    2

    s2s

    a2(2)

    =

    s(x x2) 2a

    2

    s3

    Therefore, the solution is

    Y(x, s) = Aes

    ax + Be

    s

    ax + s (x x2) 2a

    2

    s3

    Now, taking laplace transforms to the remaining two conditions, we have

    L [y(0, t)] = L[0] and L [y(, t)] = 0 Y(0, s) = 0 and Y(, s) = 0

    y(0, s) = 0 Ae0 + Be0 2a2

    s3= 0

    A + B = 2a2

    s3

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    y(, s) = Aes

    a + Be

    s

    a +

    s(2 2) 2a

    2

    s3

    Ae

    s

    a + Be

    s

    a

    2a2

    s3

    = 0

    Ae sa + Be sa = 2a2

    s3

    Ae 2sa + B = 2a2e

    s

    a

    s3

    Ae 2sa A = 2a2e

    s

    a

    s3 2a

    2

    s3

    Ae sa Aesa = 2a2

    s3 2a

    2es

    a

    s3

    A es

    a esa =

    2a2

    s3 1 es

    a

    2Asinh

    sa

    = 2a2

    s3

    1 esa

    Asinh

    sa

    =a2

    s3

    1 esa

    A = a

    2

    s3sinhsa

    1 esa

    a2

    s3sinhsa 1 esa + B = 2a2

    s3

    B = 2a2

    s3 a

    2

    s3sinh sa 1 esa

    Therefore, the solution is

    Y(x, s) =a2

    s3sinhsa

    1 esa e sax + 2a2

    s3 a

    2

    s3sinhsa

    1 esa e sax +

    s(x x2) 2a

    2

    s3

    L [y(x, t)] = a2

    s3sinhsa 1 esa e sax + 2a2

    s3 a

    2

    s3sinhsa 1 esa e sax +

    s(x x2) 2a

    2

    s3

    y(x, t) = L1

    a2

    s3sinh

    sa

    1 esa

    es

    ax +

    2a2

    s3 a

    2

    s3sinh

    sa

    1 esa

    e

    s

    ax +

    s(x x2) 2a

    2

    s3

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    1.1.4 Fourier Transform Formulae

    (1) Fourier Transform of f(x) is F[f(x)] = 1

    2

    f(x)e

    isx d x = F(s).

    (2) Inverse Fourier Transform of F[f(x)] is f(x) = 12

    F[f(x)]eisx d

    s.

    (3) Fourier Cosine Transform of f(x) is FC[f(x)] =

    2

    0

    f(x)cossx d x.

    (4) Inverse Fourier Cosine Transform ofFC[f(x)] is f(x) = 20

    FC[f(x)]cossx

    d s.

    (5) Fourier Sine Transform of f(x) is FS[f(x)] =

    2

    0

    f(x)sinsx d x.

    (6) Inverse Fourier Sine Transform ofFS[f(x)] is f(x) =

    2

    0

    FS[f(x)]sinsx

    d s.

    (7) FS[f(x)] = sFC[f(x)]

    (8) FC[f(x)] = sFS[f(x)] f(0)(9) FS[f

    (x)] = s2FS[f(x)] + sf(0)

    (10) FC[f(x)] = s2FC[f(x)] f(0)(11) F [u(x, t)] = U(s, t)

    (12) Fdnfdxn

    = (is)nF(s) if f, f,...,fn1 0 as x where F(s) =

    F[f(x)].

    (13) Fx u(x, t) = (is)U(s, t)

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    (14) F

    2

    x2 u(x, t)

    = (is)2U(s, t)

    (15) F t u(x, t)

    = Ut(s, t)

    (16) FC

    x u(x, t)

    =

    (17) FC

    2

    x2 u(x, t)

    = s2FC[u(x, t)], if ux(0, t) = 0.

    (18) FS

    x u(x, t)

    =

    (19) FS 2x2 u(x, t)

    = s

    2

    FS[u(x, t)], if u(0, t) = 0.

    Remark 1.1.15 If u at x = 0 is given, then take Fourier sine transform andif u

    xat x = 0 is given, then take Fourier cosine transform.

    Example 1.1.16 Solve the diffusion equation ut

    = K2u

    x2, < x < ,

    t > 0 with the conditions u(x, 0) = f(x) and ux , u tend to zero as x tend to.

    SolutionLet the given equation be

    u

    t= K

    2u

    x2, < x < , t > 0 (1.1.26)

    Here u = u(x, t). We know that the Fourier transform of u(x, t) = u(s, t) =

    12

    u(x, t)eisx d x. Hence taking Fourier transform of the given differ-

    ential equation, we get KF[uxx] = F[ut]

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    K[(is)2u(s, t)] = 12

    u

    teisxdx

    =d

    dt

    12

    u(x, t)eisxdx

    =d

    dtF[u(x, t)]

    =du(s, t)

    dt

    Ks2u(s, t) = du(s, t)dt

    du(s, t)u(s, t)

    = Ks2dt

    log[u(s, t)] = Ks2t + logA log[u(s, t)] logA = Ks2t

    log

    u(s, t)

    A

    = Ks2t

    u(s, t)A

    = eKs2t

    u(s, t) = AeKs2t

    u(s, 0) = Ae0 = ANow,

    u(x, 0) = f(x) F[u(x, 0)] = F[f(x)] u(s, 0) = F(s) A = F(s)

    Hence

    u(s, t) = F(s)eKs2t

    F[u(x, t) = F(s)eKs2t

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    u(x, t) = F1

    F(s)eKs2t

    = F1 [F(s)] F1 eKs2t

    = f(x)

    ex24Kt2Kt

    =12

    f()

    e(x)2

    4Kt2Kt

    d

    Take = x2Kt

    . Then

    (2

    Kt) = x

    = x 2Kt

    Also,

    d

    d=

    12

    Kt

    d = 2

    Ktd

    Hence

    u(x, t) = 12

    f(x 2Kt)e

    2

    (2Kt)d

    =2Kt

    f(x 2

    Kt)e2

    d

    This is the required solution.

    Example 1.1.17 Solve ut = K2ux2 , t > 0 with the conditions u(x, 0) =

    { 1if |x| < a0if |x| > a .

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    SolutionLet the given equation be

    u

    t = K

    2u

    x2 , t > 0 (1.1.27)

    Here u = u(x, t). We know that the Fourier transform of u(x, t) = u(s, t) =

    12

    u(x, t)eisx d x. Hence taking Fourier transform of the given differ-

    ential equation, we get KF[uxx] = F[ut]

    K[(is)2u(s, t)] = 12

    u

    teisxdx

    =d

    dt

    12

    u(x, t)eisxdx

    =d

    dtF[u(x, t)]

    =du(s, t)

    dt

    Ks2u(s, t) = du(s, t)dt

    du(s, t)

    u(s, t) = Ks2

    dt

    log[u(s, t)] = Ks2t + logA log[u(s, t)] logA = Ks2t

    log

    u(s, t)

    A

    = Ks2t

    u(s, t)A

    = eKs2t

    u(s, t) = AeKs2t

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    u(s, 0) = Ae0 = ANow,

    u(x, 0) = { 1if |x| < a0if |x| > a F[u(x, 0)] =

    12

    u(x, 0)eisxdx

    F[u(x, 0)] = 12

    aa

    eisxdx

    u(s, 0) = 12

    eisx

    is

    aa

    u(s, 0) = 12

    eisa eisa

    is

    u(s, 0) = 12

    2isin(as)

    is

    u(s, 0) =

    2

    sin(as)

    s

    A =

    2

    sin(as)

    s

    Hence

    u(s, t) =

    2

    sin(as)

    s

    eKs

    2t

    F[u(x, t)] =

    2

    sin(as)

    s

    eKs

    2t

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    u(x, t) = F1

    2

    sin(as)

    s

    eKs

    2t

    = 12

    2

    sin(as)

    s

    eKs2teisxds

    =1

    sin(as)

    s

    eKs

    2t[cos(sx) isin(sx)]ds

    =1

    sin(as)

    s

    eKs

    2tcos(sx)ds i

    sin(as)

    s

    eKs

    2tsin(sx)ds

    =2

    0

    sin(as)

    s eKs2tcos(sx)ds

    Example 1.1.18 Solve ut

    = K2u

    x2, x > 0 with the conditions u(x, 0) = ex,

    u(0, t) = 0.

    SolutionLet the given equation be

    u

    t= K

    2u

    x2, x > 0 (1.1.28)

    Here u = u(x, t). We know that the Fourier sine transform of u(x, t) = uS(s, t)

    =2

    0

    u(x, t)sin(sx) d x. Hence taking Fourier sine transform of the given

    differential equation, we get KFS[uxx] = FS[ut]

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    K[(is)2uS(s, t)] = 12

    0

    u

    tsin(sx)dx

    =d

    dt

    12

    0

    u(x, t)sin(sx)dx

    =d

    dtFS[u(x, t)]

    =duS(s, t)

    dt

    Ks2uS(s, t) = duS(s, t)dt

    duS(s, t)

    uS(s, t) = Ks2

    dt

    log[uS(s, t)] = Ks2t + logA log[uS(s, t)] logA = Ks2t

    log

    uS(s, t)

    A

    = Ks2t

    uS(s, t)A

    = eKs2t

    uS(s, t) = AeKs2t

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    uS(s, 0) = Ae0 = ANow,

    u(x, 0) = ex

    FS[u(x, 0)] = FS[e

    x]

    FS[u(x, 0)] =

    2

    0

    u(x, 0)sin(sx)dx

    FS[u(x, 0)] =

    2

    0

    exsin(sx)dx

    FS[u(x, 0)] =

    2

    ex

    1 + s2[(1)sin(sx) scos(sx)]

    0

    FS[u(x, 0)] =

    2

    0 e0

    1 + s2[(1)sin(0) scos(0)]

    FS[u(x, 0)] = 2

    0 1

    1 + s2(s)

    uS(s, 0) =

    2

    s

    1 + s2

    A =

    2

    s

    1 + s2

    Hence

    uS(s, t) = AeKs2t

    F[u(x, t)] =

    2

    s

    1 + s2 eKs2t

    u(x, t) = F1S

    2

    s

    1 + s2

    eKs

    2t

    =

    2

    0

    2

    s

    1 + s2

    eKs

    2tsin(sx)ds

    =2

    0

    s

    1 + s2

    eKs

    2tsin(sx)ds

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    Example 1.1.19 Solve ut =2ux2 , for x > 0, t > 0 with the conditions u(0, t)

    = 0 for t > 0, u(x, 0) = { 1if 0 < x < 10if x 1

    and u(x, t) is bounded.

    SolutionLet the given equation be

    u

    t=

    2u

    x2, t > 0 (1.1.29)

    Here u = u(x, t). We know that the Fourier sine transform of u(x, t) = uS(s, t)

    =2

    0

    u(x, t)sin(sx) d x. Hence taking Fourier sine transform of the given

    differential equation, we get FS[uxx] = FS[ut]

    (s2)uS(s, t) =

    2

    0

    u

    tsin(sx)dx

    =d

    dt

    2

    0

    u(x, t)sin(sx)dx

    =d

    dtFS[u(x, t)]

    =duS(s, t)

    dt

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    s2uS(s, t) = duS(s, t)dt

    duS(s, t)

    uS

    (s, t)=

    s2dt

    log[uS(s, t)] = s2t + logA log[uS(s, t)] logA = s2t

    log

    uS(s, t)

    A

    = s2t

    uS(s, t)A

    = es2t

    uS(s, t) = Aes2t

    uS(s, 0) = Ae0 = A

    Now,

    u(x, 0) = { 1if 0 < x < 10if x 1

    FS[u(x, 0)] =

    2

    0

    u(x, 0)sin(sx)dx

    FS[u(x, 0)] =

    2

    10

    sin(sx)dx

    uS(s, 0) =

    2

    cos(sx)s

    10

    uS(s, 0) = 2

    cos(s) + 1s

    A =

    2

    1 cos(s)

    s

    Hence

    uS(s, t) =

    2

    1 cos(s)

    s

    es

    2t

    FS[u(x, t)] =

    2

    1 cos(s)

    s

    es

    2t

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    u(x, t) = F1S

    2

    1 cos(s)

    s

    es

    2t

    = 2

    0

    2

    1 cos(s)

    s

    es

    2

    tsin(sx)ds

    =2

    0

    1 cos(s)

    s

    es

    2tsin(sx)ds

    Example 1.1.20 Solve ut

    = K2u

    x2, 0 < x < , t > 0 with the conditions

    u(x, 0) = 0, x 0, ux (0, t) = a, is a constant and u(x, t) is bounded.

    SolutionLet the given equation be

    u

    t= K

    2u

    x2, 0 < x < , t > 0. (1.1.30)

    Here u = u(x, t). We know that the Fourier cosine transform of u(x, t) =

    uC(s, t) =2

    0

    u(x, t)cos(sx) d x. Hence taking Fourier cosine transform of

    the given differential equation, we get KFC[uxx] = FC[ut]

    Ks2uC(s, t)

    2

    xu(0, t)

    =

    2

    0

    u

    tcos(sx)dx

    =d

    dt

    2

    0

    u(x, t)cos(sx)dx

    =d

    dtFC[u(x, t)]

    =duC(s, t)

    dt

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    Ks2uC(s, t)

    2

    (a)

    =

    duC(s, t)

    dt

    Ks2uC(s, t) + 2 Ka = duC(s, t)dt duC(s, t)

    dt+ Ks2uC(s, t) =

    2

    Ka

    This is linear equation in uC(s, t). Here P = Ks2 and Q =

    2Ka

    .

    Hence the integrating factor

    I.F = ePdt

    = eKs2dt

    = eKs2t

    Hence the solution is

    uC(s, t)ePdt =

    Qe

    Pdt

    dt + C

    uC(s, t)eKs2t =

    2

    (Ka)eKs

    2t

    dt + C

    uC(s, t)eKs2t =

    2

    (Ka)

    eKs

    2t

    Ks2

    + C

    uC(s, t) =

    2

    as2

    + CeKs

    2t

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    uC(s, 0) =

    2

    as2

    + Ce0 =

    2

    as2

    + C

    Now,

    u(x, 0) = 0

    FC[u(x, 0)] = 0

    uC(s, 0) = 0

    2

    as2

    + C = 0

    C =

    2

    as2

    Hence

    uC(s, t) =

    2

    as2

    + CeKs

    2t

    FC[u(x, t)] = 2 as2 + 2 as2 eKs2t

    FC[u(x, t)] =

    2

    as2

    2

    as2

    eKs

    2t

    FC[u(x, t)] =

    2

    as2

    1 eKs2t

    u(x, t) = F1C

    2

    a

    s2 1 eKs2t

    =

    2

    0

    2

    as2

    1 eKs2t

    cos(sx)ds

    =2a

    0

    1

    s2

    1 eKs2t

    cos(sx)ds

    Example 1.1.21 Find the temperature distribution in semi-infinite bar withits end point and the lateral surface insulated and with initial temperaturedistribution in the bar is prescribed by f(x). Deduce the solution when f(x)= eax.

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    SolutionThis problem is represented by one dimensional heat equation

    u

    t= c2

    2u

    x2, 0 < x < , t > 0. (1.1.31)

    with boundary condition ux(0, t) = 0 (insulated end) and with the initial con-

    dition u(x, 0) = f(x) (given) for 0 < x < . Here u = u(x, t). We know thatthe Fourier cosine transform of u(x, t) = uC(s, t) =

    2

    0

    u(x, t)cos(sx) d x.

    Hence taking Fourier cosine transform of the given differential equation, we getc2FC[uxx] = FC[ut]

    c2s2uC(s, t)

    2

    xu(0, t)

    =

    2

    0

    u

    tcos(sx)dx

    =d

    dt

    2

    0

    u(x, t)cos(sx)dx

    =d

    dtFC[u(x, t)]

    =duC(s, t)

    dt

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    c2s2uC(s, t)

    2

    (0)

    =

    duC(s, t)

    dt

    duC(s, t)

    uC(s, t) = c2

    s

    2

    dt

    log[uC(s, t)] = c2s2t + logA log[uC(s, t)] logA = c2s2t

    log

    uC(s, t)

    A

    = c2s2t

    uC(s, t)A

    = ec2s2t

    uC(s, t) = Aec2s2t

    uC(s, 0) = Ae0 = ANow,

    u(x, 0) = f(x) FC[u(x, 0)] = FC[f(x)]

    FC[u(x, 0)] =

    2

    0

    f(x)cos(sx)dx

    uC(s, 0) =

    2

    0f(x)cos(sx)dx

    A =

    2

    0

    f(x)cos(sx)dx

    uC(s, t) = Aec2s2t F[u(x, t)] =

    2

    0

    f(x)cos(sx)dx

    ec2s2t

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    u(x, t) = F1C

    2

    0

    f(x)cos(sx)dx

    ec2s2t

    = 2

    0

    2

    0

    f(x)cos(sx)dx ec2s2tcos(sx)ds

    =2

    0

    0f(x)cos(sx)dx

    ec2s2tcos(sx)ds

    Suppose f(x) = eax. Then,

    u(x, t) =2

    0

    0eaxcos(sx)dx

    ec

    2s2tcos(sx)ds

    =2

    0

    eax

    a2 + s2[(a)cos(sx) + ssin(sx)]

    0

    ec

    2s2tcos(sx)ds

    =2

    0

    0

    e0

    a2 + s2[(a)cos(0) + ssin(0)]

    ec

    2s2tcos(sx)ds

    =2

    0

    1a2 + s2

    (a)

    ec2s2tcos(sx)ds

    =

    2

    0

    aa2 + s2

    e

    c2s2t

    cos(sx)ds

    Example 1.1.22 Solve ut = K2ux2 , 0 < x < , t > 0 under the conditions u

    = u0 at x = 0, t > 0 with the initial condition u(x, 0) = 0, for x 0.SolutionLet the given equation be

    u

    t= K

    2u

    x2, x > 0 (1.1.32)

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    84

    Here u = u(x, t). We know that the Fourier sine transform of u(x, t) = uS(s, t)

    =2

    0u(x, t)sin(sx) d x. Hence taking Fourier sine transform of the given

    differential equation, we get KFS[uxx] = FS[ut]

    Ks2uS(s, t) +

    2

    su(0, t)

    =

    2

    0

    u

    tsin(sx)dx

    =d

    dt

    2

    0

    u(x, t)sin(sx)dx

    =d

    dtFS[u(x, t)]

    =duS(s, t)

    dt

    Ks2uS(s, t) +

    2

    su0

    =

    duC(s, t)

    dt

    Ks2uS(s, t) +

    2

    Ksu0

    =

    duS(s, t)

    dt

    duS(s, t)

    dt

    + Ks2uS(s, t) = 2

    Ksu0

    This is linear equation in uS(s, t). Here P = Ks2 and Q =

    2 Ksu0.

    Hence the integrating factor

    I.F = ePdt

    = eKs2dt

    = eKs2t

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    Hence the solution is

    uS(s, t)ePdt =

    Qe

    Pdt

    dt + C

    uS(s, t)eKs2t =

    2

    (Ksu0)e

    Ks2t

    dt + C

    uS(s, t)eKs2t =

    2

    (Ksu0)

    eKs

    2t

    Ks2

    + C

    uS(s, t)eKs2t =

    2

    (u0)

    eKs

    2t

    s

    + C

    uS(s, t) =

    2

    u0s

    + CeKs2t

    uS(s, 0) =

    2

    u0s

    + Ce0

    uS(s, 0) =

    2

    u0s

    + C

    Now,

    u(x, 0) = 0 FS[u(x, 0)] = 0 uS(s, 0) = 0

    2

    u0s

    + C = 0

    C =

    2

    u0s

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    Hence

    uS(s, t) =

    2

    u0

    s + CeKs2t

    FS[u(x, t)] =

    2

    u0s

    +

    2

    u0s

    eKs

    2t

    FS[u(x, t)] =

    2

    u0s

    2

    u0s

    eKs

    2t

    FS[u(x, t)] =

    2

    u0s

    1 eKs2t

    u(x, t) = F1

    S2

    u0

    s

    1 eKs2t

    =

    2

    0

    2

    u0s

    1 eKs2t

    sin(sx)ds

    =2u0

    0

    1

    s

    1 eKs2t

    sin(sx)ds

    Example 1.1.23 Solve ut

    = K2u

    x2, 0 < x < , t > 0 under the conditions

    u(x, 0) = eax, a > 0, ux(0, t) = 0, ux(x, t) = 0, t 0.

    SolutionLet the given equation be

    u

    t= K

    2u

    x2, 0 < x < , t > 0. (1.1.33)

    under the conditions u(x, 0) = eax, a > 0, ux(0, t) = 0, Ux(x, t) = 0, t 0.Here u = u(x, t). In this problem, the ends of the bar have been insulated andkept at zero temperature. We know that the Fourier cosine transform ofu(x, t)

    = uC(s, t) =2

    0

    u(x, t)cos(sx) d x. Hence taking Fourier cosine transform

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    of the given differential equation, we get KFC[uxx] = FC[ut]

    Ks2uC(s, t)

    2

    xu(0, t)

    =

    2

    0

    u

    tcos(sx)dx

    =d

    dt

    2

    0

    u(x, t)cos(sx)dx

    =d

    dtFC[u(x, t)]

    =duC(s, t)

    dt

    Ks2uC(s, t)

    2

    (0)

    =

    duC(s, t)

    dt

    duC(s, t)

    uC(s, t)=

    Ks2dt

    log[uC(s, t)] = Ks2t + logA log[uC(s, t)] logA = Ks2t

    log

    uC(s, t)

    A

    = Ks2t

    uC(s, t)A

    = eKs2t

    uC(s, t) = AeKs2t

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    uC(s, 0) = Ae0 = ANow,

    u(x, 0) = eax

    FC[u(x, 0)] = FC[e

    ax]

    FC[u(x, 0)] =

    2

    0

    eaxcos(sx)dx

    uC(s, 0) =

    2

    eax

    a2 + s2[(a)cos(sx) + ssin(sx)]

    0

    A =

    2

    0 e

    0

    a2 + s2[(a)cos(0) + ssin(0)]

    A =

    2

    1

    a2 + s2(a)

    A =

    2

    aa2 + s2

    uC(s, t) = AeKs2t F[u(x, t)] =

    2

    a

    a2 + s2

    eKs

    2t

    u(x, t) = F1C

    2

    a

    a2 + s2

    eKs

    2t

    = 2

    0

    2

    a

    a2 + s2

    eKs

    2tcos(sx)ds

    =2a

    0

    1

    a2 + s2

    eKs

    2tcos(sx)ds

    Example 1.1.24 Determine the temperature distribution in semi-infinite mediumx 0 when the end x = 0 is maintained at zero temperature and the initialtemperature distribution is f(x).

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    SolutionThis problem is represented by one dimensional heat equation

    u

    t= K

    2u

    x2, 0 < x < , t > 0. (1.1.34)

    under the conditions u(x, 0) = f(x) (given) for 0 < x 0, described by the partial differential equation uxx+uyy = 0, < x < , y > 0 with the boundary conditions u(x, 0) = f(x), < x < , u isbounded as y , u and ux both vanishes as |x| .

    SolutionLet the given the partial differential equation be

    uxx + uyy = 0, < x < , y > 0

    Since x has an infinite range of values, we take Fourier transform on both sidesto the given partial differential equation in the variable x. Therefore, we have

    F[uxx] + [uyy ] = 0

    1

    2

    uxxe

    isxdx +1

    2

    uyye

    isxdx = 0

    12

    eisxd[ux] +12

    2u

    y2

    eisxdx = 0

    12

    eisxux

    ux

    eisx(is)

    dx

    +

    d2

    dy2

    12

    ueisxdx

    = 0

    93

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    12

    0 (is)

    ux

    eisx

    dx

    + d2dy

    2F[u(x, y)] = 0 1

    2(is)

    eisx

    d(u)

    +

    d2

    dy2

    F[u(x, y)] = 0

    12

    (is)eisxu

    u

    eisx(is)

    dx

    +

    d2

    dy2

    F[u(x, y)] = 0

    12 (is)[0 0] (is) ueisxdx+

    d2

    dy2

    F[u(x, y)] = 0

    (is)2 12

    ueisxdx +

    d2

    dy2

    F[u(x, y)] = 0

    s2F[u(x, y)] +

    d2

    dy2

    F[u(x, y)] = 0

    d2

    dy2

    U(s, y) s2

    U(s, y) = 0

    D2 s2U(s, y) = 0where U(s, y) = F[u(x, y)].Therefore, the auxiliary equation is

    m2 s2 = 0 m2 = s2 m = s

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    Hence the solution isU(s, y) = A(s)esy + B(s)esy .Since u must be bounded as y , its Fourier transform U(s, y) also shouldbe bounded. Hence we have A(s) = 0 for s > 0 and B(s) = 0 for s < 0.

    Therefore, U(s, y) = B(s)esy for s > 0 and U(s, y) = A(s)esy for s < 0.Consequently, U(s, y) = Ke|s|y. U(s, 0) = Ke0 = KNow,

    u(x, 0) = f(x) F[u(x, 0)] = F[f(x)] U(s, 0)] = F[F(x)] K = F[f(x)]

    U(s, y) = F[f(x)]e|s|y

    Hence,

    U(s, y) =

    1

    2

    f(x)eisxdx

    e|s|y

    F[u(x, y)] = 12

    f(x)e|s|y e

    isxdx

    u(x, y) = F1 12

    f(x)e|s|y

    eisxdx

    u(x, y) = 12

    12

    f()e|s|y

    eisd

    eisxds

    u(x, y) = 12

    f()d

    eis(x)|s|yds

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    Now,

    eis(x)|s|yds =

    0

    eis(x)|s|yds +

    0

    eis(x)|s|yds

    =0

    eis(x)+syds +

    0

    eis(x)syds

    =0

    es[i(x)+y]ds +

    0

    es[i(x)+y]ds

    =

    es[i(x)+y]

    i( x) + y0

    +

    es[i(x)+y]

    [i(x ) + y]0

    =1

    i( x) + y 0 + 0

    1

    [i(x ) + y]=

    1

    i( x) + y +1

    i(x ) + y=

    i(x ) + y + i( x) + y[i( x) + y][i(x ) + y]

    =ix i+ y + i ix + y

    [y + i( x)][y i( x)}]=

    2y

    y2 + ( x)2

    Therefore,

    u(x, y) =1

    2

    f()d

    2y

    y2 + ( x)2

    =y

    f()

    y2 + ( x)2

    d

    Example 2.1.2 Solve uxx + uyy = 0, y > 0 subject to the conditions u and

    ux 0 as x2 + y2 , u(x, 0) = { 1if|x|