Phys Lecture Laplace

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    Laplace and Poissons

    Equations

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    Derivation

    We have the differential form of Gauss law

    Using D = E and E = - in the above equation, we get

    This is the Poissons Equation

    . D

    V

    2D = V =-E V

    2V

    or

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    20V

    In free space , this equation becomes,

    This equation is called the Laplace equation.

    is called the Laplacian operator or simply Laplacian.

    Note that the del operator is defined only in the

    rectangular coordinates only, as

    i j k

    x y z

    2

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    The Laplacian in the three coordinate systems are

    2 2 2

    2

    2 2 2

    = ( )cartesian

    x y z

    2 2

    2

    2 2 2

    1

    1= ( )Cylindrical

    z

    2

    2 2

    2 2 2 2 2

    1 1

    1= sin ( )

    sin sinr Spherical

    r r r r r

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    Applications

    one dimensional solution of Laplace equation

    2 2 2

    2

    2 2 2

    = = 0 ( )V V V

    V cartesian

    x y z

    --- (1)

    V is a function of only one variable and is independent of theother two variables. Under this condition, in rectangular

    coordinate system the Laplace equation reduces to

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    ne dimensional solution of Laplace Equation in rectangular

    coordinate system

    Let V be a function of z only. Then in Rectangular coordinatesystem,the Laplaces Equation reduces to

    2

    2

    20

    VV

    z

    Since V is a function of z only, it is independentof x and y. Therefore,

    Integrating both sides once we get

    --- (2)

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    Equation (3) represents a family of equi potential surfaceswith z taking up constant values

    dVA

    dz

    Integrating both sides once again, we get

    , A is an arbitrary constant --- (3)

    V Az B , B is an arbitrary constant --- (4)

    A and B are arbitrary constants to be evaluated under suitable

    boundary conditions.

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    Consider two such equi potential surfaces one at z = z1 and theother at z = z2. Let V= V1 at z = z1 and V = V2 at z = z2.

    We immediately recognize that this is the case with a parallel

    plate capacitor with a plate separation of z1 - z2 = d and apotential difference V1 - V2 .

    Applying the above two conditions, called boundary conditions,we get,

    1 1

    2 2

    V V Az B

    V V Az B

    --- (5)

    --- (6)

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    Solving equations (5) and (6) we getthe values for A and B as

    2 1

    2 1

    1 2 2 1

    2 1

    V VA

    z z

    V z V z B

    z z

    Substituting the values of A and B in equation (4) we get,

    2 1 1 2 2 1

    2 1 2 1

    2 1 1 2

    2 1

    ( ) ( )

    V V V z V z V zz z z z

    V z z V z z

    z z

    --- ( 7)

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    Further let, for simplicity, V1 = 0 and z1 = 0, V2 = Va

    Then equation (7) reduces to

    aV

    V zd

    We find that V is a linear function of z

    V = V2 = Va

    V = V1 = 0

    d

    z = z2

    z = z1Fig 1 Parallel plate capacitor

    --- (8)

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    1 Given V, Determine E using the formula E = - V

    2 Determine D using D = E

    3 Find D on any one of the plates, D = DS= DS aS = DN aNon the chosen plate, and recognising that DN = S

    4 Determine Q by surface integration of S over the surfacearea of the chosen plate using

    5 Compute the capacitance using the formulaa

    QC

    V

    S

    S

    Q dS

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    Applying these five steps to the parallel plate capacitor we get,

    0;

    a

    az

    a

    z

    aS z S S N N N S

    z

    a a a

    S S

    zV V

    d

    VE V a

    d

    V

    D E adV

    D D a D a D a D d

    V V VQ dS dS S

    d d d

    Therefore the capacitance of the parallel plate capacitor is

    a

    Q SC

    V d

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    We have, in cylindrical coordinates, the Laplace equation as

    2 2

    2

    2 2 21 0

    1V= ( )V V V Cylindricalz

    One dimensional solution of Laplace Equation in cylindrical

    coordinate system

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    We consider that V is a function of only. In this casethe Laplace equation in cylindrical coordinates reduces to

    0

    V

    Integrating this equation once we get,

    10

    V

    V V AA o r

    , , A an arbitrary constant

    Case 1:

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    Integrating once again, we get

    V A l n B, B an arbitrary constant

    From this equation, we observe that equipotential surfaces

    are given by = constant and are cylinders. Example of theproblem is that of a coaxial capacitor or coaxial cable.

    Let us create the boundary conditions by choosing V = Va at = a and V = 0 at = b, b > a.

    Then we get from the above equation,

    BbnlAVV

    BanlAVV

    b

    a

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    Solving these two equations for A and B we get

    b

    a

    bVaVBdna

    b

    a

    VVA abba

    ln

    lnln

    ln

    Substituting these the values of A and B in the generalExpression for V , we get

    b

    a

    bVaV

    b

    a

    VVV abba

    ln

    lnlnln

    ln

    Letting Vb = 0, we get

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    a

    b

    b

    VVa

    ln

    ln

    ab

    a

    bVab

    a

    bVVVE aa ln

    ln

    ln

    ln

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    Therefore

    dnaaDaDa

    a

    ba

    VD

    Then

    Da

    a

    b

    VED

    a

    ab

    VE

    NNNSa

    S

    Sa

    a

    ln

    1

    ln

    1

    ln

    1

    i.e.,

    Hence

    a

    bV

    aD

    aSN

    ln

    1

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    Therefore,

    1

    ln

    12

    ln

    S S

    S of one of S of one of the plates the plates with a with a

    a

    a

    Q dS dS

    V Sbaa

    V a Lba

    a

    over a length L meters of the

    coaxial cable

    a

    b

    L

    V

    QC

    a ln

    2

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    Therefore the capacitance per unit length of the line CL is

    a

    bCL

    ln

    2 F/m

    Next we consider V as a function of only. In this case

    The Laplace equation in cylindrical coordinate systemreduces to

    2

    2

    2 2

    10

    V=

    V

    Case 2:

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    i.e.,

    2

    2 2

    1

    0 d V

    d

    Excluding the value = 0 this equation becomes

    2

    20

    d V

    d

    Integrating both sides we get

    dV

    Ad

    Integrating once again, we get V A B

    This is the general equation for V when V is a function of only.

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    From this equation, we observe that equipotential surfacesare given by = constant and are planes To visualize this, choose twosuch equipotential surfaces, V = Va at = and V = 0 at =0.

    Insulating gap

    V = Vaat =

    V = 0at =0

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    For the chosen boundary condition, we get

    andaVA

    Thus the general expression for V becomes

    0 0 0

    aV V A B

    V A B B

    aV

    V

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    Once again we follow the 5 step procedure to determine

    the capacitance of the system1 1

    aVV

    E V

    Note that E is a function of and not of . But the vector field EIs a function of . Now,

    a

    VD E

    a

    NNSSS

    VaDaDD

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    S

    a

    N

    V

    D

    The surface integration on S gives Q:

    S

    a

    S

    a

    S

    S dSVdsVdSQ

    and we get immediately the value for the capacitance ofthe corner reflector system as

    Sa

    S

    a

    a

    dSV

    dSV

    V

    QC

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    Next we consider the Laplace Equation in spherical coordinates:

    2

    2 2

    2 2 2 2 2

    1 1 1sin 0

    sin sin

    V V VV r

    r r r r

    In this system we consider that V is a function of r only.Then the Laplace equation reduces to

    01 2

    2

    2

    r

    V

    rrV

    Again we exclude r = 0 from our solutions. Multiplying bothSides by r2 we get

    02

    r

    Vr

    --- ( a)

    --- ( b)

    One dimensional solution of Laplace Equation in spherical

    coordinate system

    Case 1:

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    Integrating once again, we get

    2 Vr A

    r

    2

    V Aor

    r r

    Ao r V B

    r

    where A and B are arbitrary constants to be evaluated. This

    equation represents a family of equi potential surfaces forr = constant.

    Let us choose two such equipotential surfaces at r = a andR = b, b > a , such that at r = a, V = Va and at r = b, V = Vb

    --- ( c)

    --- ( d)

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    a

    b

    AV B

    a

    A

    V Bb

    Solving these two equations we get

    --- ( e)

    --- ( f)

    1 1

    a bV VA

    a b

    and

    1 1

    1 1

    a bV Vb aB

    b a

    We immediately recognise that this is the example of concentric

    spheres or Spherical capacitor

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    Substituting the values of A and B in equation (d), we get,

    1 1

    1

    1 1 1 1

    a ba b

    V VV V b a

    Vr

    a b b a

    1 1

    1

    1 1 1 1

    b aa b

    V VV V a b

    o r Vr

    a b a b

    Let Vb = 0 Then equation (g) becomes

    --- (g)

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    1 1

    1 1a

    r b

    V V

    a b

    --- (h)

    2

    1 1

    1

    1 1 1 1

    a

    a

    Vr bE V V r

    r

    a b a b

    2

    1 1

    aV

    D E rr

    a b

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    2

    1 1

    aS S S N N

    VD D D a D a r

    ra b

    21 1

    a

    N S

    VD

    a

    a b

    Therefore the charge Q on the capacitor plate is

    2 21 1 1 1

    a a

    S

    S S S

    V VQ dS dS dS

    a a

    a b a b

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    Therefore we get the expression for the spherical capacitor as

    2

    2

    4 4

    1 1 1 1

    a

    a a

    Q V aC

    V a V

    a b a b

    4

    1 1C

    a b

    For an isolated sphere , i.e., as b we get

    4C a

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    Finally let us consider V as a function of only . In this caseThe Laplaces equation reduces to

    2

    2

    10

    V= sinsin

    V

    r

    We exclude r = 0 and = n/2, n = 0, 1, 2, 3, . . .

    Multiplying both sides of the above equation by r2 sin, we get

    0

    sinV

    Case 2:

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    Integrating the equation with respect to we get,

    or

    sin V A

    sin

    V AA is an arbitrary constant

    Integrating once again, we get,

    2 ln(tan / )V A B

    This equation represents a family of equipotential surfaces forconstant . Let us consider two such equipotential surfaces at =/2 and = and let V = 0 at =/2 and V = Va at =0.

    --- (i)

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    The equipotential surfaces are cones as shown in figure below.Such a system is called a conical antenna

    Insulating gap

    Ground plane

    V = Va at =

    V = 0 at = 0

    Applying these two boundary conditions to the equation (i),Solving for A and B and substituting these values in (i),we get,

    2

    2

    ln(tan / )

    ln(tan / )aV V

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    We have 2

    2

    ln(tan / )

    ln(tan / )aV V

    We use E = -

    V to find the field strength, as1

    2

    sin (tan / )

    aVV

    E V a ar r ln

    Next we determine D using D = 0 E as

    2

    sin (tan / )

    aV

    D E ar ln

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    2

    sin (tan / )

    aS

    V

    r ln

    The total charge Q on the conical surface is therefore,

    2

    0 2

    sinsin (tan / )

    aS

    S o

    VQ ds r d dr

    r ln

    0

    2

    2

    (tan / ) a

    VQ dr

    ln

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    This equation leads to an infinite value of charge and capacitance.

    Therefore we have to consider a cone of finite size.

    Our expression for Q is approximate, since, theoretically, the

    potential surface = extends from r = 0 to r = . But our physicalconical surface extends from r = 0 to say, r = r1 . The approximatecapacitance is

    12

    2

    (cot / ) a

    rC

    ln