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PART 1

ELECTROSTATICS
ELECTROSTATICS

2.1   COULUMB’S LAW
2.2   ELECTRIC FIELD INTENSITY
2.3   LINE, SURFACE & VOLUME CHARGES
2.4   ELECTRIC FLUX DENSITY
2.5   GAUSS’S LAW
2.6   ELECTRIC POTENTIAL
2.7   BOUNDARY CONDITIONS
2.8   CAPACITANCE


                                       2
INTRODUCTION

   Electromagnetics is the study of the effect of
    charges at rest and charges in motion.


   Some special cases of electromagnetics:
       Electrostatics: charges at rest
       Magnetostatics: charges in steady motion (DC)
       Electromagnetic waves: waves excited by
        charges in time-varying motion


                                              3
INTRODUCTION (Cont’d)

  Fundamental laws of
                                 Maxwell’s
  classical electromagnetics
                                 equations


Special      Electro-             Magneto-       Electro-             Geometric
cases         statics              statics       magnetic              Optics
                                                  waves
                               
                    Statics:      0             Transmission
                               t                    Line
                                                    Theory
           Input from                  Circuit
              other                    Theory      Kirchoff’s
           disciplines                                          d  
                                                     Laws

                                                                  4
INTRODUCTION (Cont’d)


• Electrical phenomena caused by friction
  are part of our everyday lives, and can be
  understood in terms of electrical charge.

• The effects of electrical charge can be
  observed in the attraction/repulsion of
  various objects when “charged.”


                                        5
INTRODUCTION (Cont’d)

• Charge comes in two varieties called “positive”
  and “negative.”
• Objects carrying a net positive charge attract
  those carrying a net negative charge and repel
  those carrying a net positive charge.
• Objects carrying a net negative charge attract
  those carrying a net positive charge and repel
  those carrying a net negative charge.
• On an atomic scale, electrons are negatively
  charged and nuclei are positively charged.
                                         6
INTRODUCTION (Cont’d)

• Electric charge is inherently quantized such
  that the charge on any object is an integer
  multiple of the smallest unit of charge which
  is the magnitude of the electron charge
  e = 1.602  10-19 C.
• On the macroscopic level, we can assume
  that charge is “continuous.”


                                        7
COULUMB’S LAW


In the late 18th century, Colonel Charles
Augustus Coulomb invented a sensitive
torsion   balance     that   he    used       to
experimentally      determine     the       force
exerted in one charge by another.



                                        8
COULUMB’S LAW (Cont’d)

He found that the force is proportional to the
product of two charges, inversely proportional
to the square of the distance between the
charges and acts in a line containing the two
charges.

                 Q1Q 2
            F k    2
                  R
                                        9
COULUMB’S LAW (Cont’d)


  The proportional constant, k is:

                 1
          k           ,             r 0
                4 
  Where the free space permittivity with
  a value given by:
                                           9
                            12   F 10     F
        0  8 . 85  10            
                                  m   36  m
                                                10
COULUMB’S LAW (Cont’d)

 Charge Q1 exerts a vector force F12 in Newton's (N)
 on charge Q2,




                          Q1Q 2
               F12                      a 12
                       4  0 R 12
                                     2

                                                11
COULUMB’S LAW (Cont’d)

  If more than two charges, use the principle of
  superposition to determine the force on a
  particular charge.

  If there are N charges, Q1,Q2...QN located
  respectively at point with position vectors
  r1,r2...rN the resultant force F on a charge Q
  located at point r is the vector sum of the forces
  exerted on Q by each charges Q1,Q2...QN


                                           12
COULUMB’S LAW (Cont’d)


  F
               QQ 1         r  r1            QQ 2           r  r2 
       4  0 r  r1
                        2
                            r  r1        4  0 r  r2
                                                            2
                                                                r  r2

       ... 
                   QQ N             r  r N 
               4  0 r  r N
                                2
                                    r  rN

  Or generally,

                            Q         N   Q k r  rk 
                F             
                        4  0 k  1                    3
                                             r  rk
                                                                  13
COULUMB’S LAW (Cont’d)

 For example,

 FTOTAL  F12  F32 ,
            Q1Q 2
 F12                      a 12
         4  0 R 12
                       2


            Q 3Q 2
 F32                      a 32
         4  0 R 32
                       2



         F12  F21
                                  14
EXAMPLE 1

 Suppose 10nC charge Q1 located at (0.0, 0.0, 4.0m)
 and a 10nC charge Q2 located at (0.0, 4.0m, 0.0). Find
 the force acting on Q2 from Q1.




                                               15
SOLUTION TO EXAMPLE 1


  To employ Coulomb’s Law, first find vector    R12
        R12  r2  r1
               
             4a y  4a z 
             4a y  4a z
   Magnitude of   R12

        R12  42  42
              32  4 2
                                           16
SOLUTION TO EXAMPLE 1 (Cont’d)

            R12 4a y  4a z   1       1
  And a12                     ay     az
            R12    4 2         2       2
  Then
             Q1Q 2
  F12                      a 12
          4  0 R 12
                        2



     
          10  10 10  10 
                        9            9
                                                1
                                                  ay 
                                                        1     
                                                           az 
       4  8 . 854  10  4 2 
                                12             2            
                                           2
                                                         2
      4 . 0 a y  4 . 0 a z nN
                                                      17
2.2 ELECTRIC FIELD INTENSITY


 If Q1 is fixed to be at origin, a second charge
 Q2 will have force acting on Q1 and can be
 calculated using Coulomb’s Law. We also
 could calculate the force vector that would
 act on Q2 at every point in space to generate
 a field of such predicted force values.


                                           18
ELECTRIC FIELD INTENSITY (Cont’d)


  It becomes convenient to define electric field
  intensity E1 or force per unit charge as:

                        F12
                   E1 
                        Q2
  This field from charge Q1 fixed at origin results
  from the force vector F12 for any arbitrarily
  chosen value of Q2

                                              19
ELECTRIC FIELD INTENSITY (Cont’d)


   Coulomb’s law can be rewritten as

                          Q
              E                    aR
                     4  0 R
                                2



   to find the electric field intensity at any point in
   space resulting from a fixed charge Q.


                                              20
EXAMPLE 2



  Let a point charge Q1 = 25nC be located

  at P1 (4,-2,7). If ε = ε0, find electric field

  intensity at P2 (1,2,3).




                                           21
SOLUTION TO EXAMPLE 2


   By using the electric field intensity,

               Q
     E                   aR
           4  0 R
                      2


    This field will be:

                   9
        25  10
     E           a12
        4 0 R12

                                            22
SOLUTION TO EXAMPLE 2 (Cont’d)

  Where,    R12  r2  r1  3a x  4a y  4a z

  and      R12  41
               Q                      Q
   E                 a
                     2 12
                                                    R12
        4 0 R12                 4 0 R12
                                                 3

                             9
                   25  10
                                              3a x  4a y  4a z 
           
        4 8.854  1012 41        3
                                          2

    
                                                            23
ELECTRIC FIELD INTENSITY (Cont’d)

  If   there    are        N    charges,       Q1,Q2...QN         located
  respectively        at       point    with      position        vectors
  r1,r2...rN the electric field intensity at point r is:

  E
               Q1           r  r1   ..         QN             r  r N 
        4  0 r  r1
                        2
                               r  r1        4  0 r  r N
                                                              2
                                                                  r  rN


                            1       N   Q k r  rk 
               E            
                      4  0 k  1                      3
                                             r  rk
                                                                  24
FIELD LINES

  The behavior of the fields can be visualized using
  field lines:


  Field vectors plotted
  within a regular grid in
  2D space surrounding
  a point charge.




                                           25
FIELD LINES (Cont’d)

  Some    of   these   field
  vectors can easily be
  joined by field lines that
  emanate      from     the
  positive point charge.

  The direction of the arrow
  indicates the direction of
  electric fields

      The magnitude is given by density of the lines

                                             26
FIELD LINES (Cont’d)



  The field lines terminated
  at a negative point charge




  The field lines for a pair
  of opposite charges



                               27
2.3 LINE,SURFACE &
    VOLUME CHARGES

  Electric fields due to continuous charge
  distributions:




                                        28
LINE,SURFACE &
VOLUME CHARGES (Cont’d)

 To determine the charge for each distributions:

  Line charge:          Surface charge:
      dQ   L dl              dQ   S dS
      Q    L dl             Q    S dS
           L                       S

  Volume charge:
                     dQ  V dV
                     Q   V dV
                         V

                                              29
LINE CHARGE


 Infinite Length of Line Charge:

 To derive the electric field intensity at any
 point in space resulting from an infinite
 length line of charge placed conveniently
 along the z-axis




                                        30
LINE CHARGE (Cont’d)

 Place an amount of charge in
 coulombs along the z axis.
 The linear charge density is
 coulombs of charge per meter
 length,
             
         L C m

 Choose an arbitrary point P
 where we want to find the
 electric field intensity.

       P  , , z 
                                31
LINE CHARGE (Cont’d)

  The electric field intensity is:

  E   E a   E a  Ez a z
  But, the field is only vary with
  the radial distance from the
  line.

  There is no segment of charge
  dQ anywhere on the z-axis
  that will give us E . So,
        E   E a   E z a z
                                     32
LINE CHARGE (Cont’d)

  Consider a dQ segment a
  distance z above radial axis,
  which will add the field
  components for the second
  charge element dQ.


  The E z components cancel
  each other (by symmetry) ,
  and the E adds, will give:
       E   E a 
                                  33
LINE CHARGE (Cont’d)

  Recall for point charge,
                 Q
      E                    aR
            4  0 R
                        2


  For continuous charge distribution, the
  summation of vector field for each charges
  becomes an integral,

                   dQ
       E                      aR
                4  0 R
                            2


                                         34
LINE CHARGE (Cont’d)


 The differential charge,

   dQ   L dl
         L dz
  The vector from source
  to test point P,

   R  Ra R
      a   za z

                            35
LINE CHARGE (Cont’d)


  Which has magnitude, R                      2  z 2 and a
  unit vector,
                              a   za z
                  aR 
                                    2  z2
   So, the equation for integral of continuous
   charge distribution becomes:

                           L dz               a   za z   
                                                             
    E   
             4  0        z
                              2      2
                                         
                                         2     2  z2
                                             
                                                              
                                                              
                                                          36
LINE CHARGE (Cont’d)

  Since there is no   az    component,

                        L dz
       E                                       a 
                      
                4  0  2  z 2        3
                                             2

                      
            L                     dz
                                                       a
            4  0          2
                                     z2        3
                                                     2




                                                              37
LINE CHARGE (Cont’d)


  Hence, the electric field intensity at any point ρ
  away from an infinite length is:

                       L
                 E          a
                    2  0 

  For any finite length, use the limits on the integral.




                                              38
EXAMPLE 3


 Use Coulomb’s Law to
 find electric field
 intensity at (0,0,h) for
 the ring of charge, of
 charge density,  L
 centered at the origin in
 the x-y plane.


                             39
SOLUTION TO EXAMPLE 3


 By inspection, the ring
 charges delivers only   dE 
 and   dE z contribution
 to the field.


 dE  component will be
 cancelled by symmetry.




                                40
SOLUTION TO EXAMPLE 3 (Cont’d)

 Each term need to be
 determined:
              dQ
  E                     aR
           4  0 R
                      2


 The differential charge,

   dQ   L dl
         L ad

                               41
SOLUTION TO EXAMPLE 3 (Cont’d)

  The vector from source to test point,

       R  Ra R
          aa   ha z

  Which has magnitude, R          a 2  h 2 and a
  unit vector,
                          aa   ha z
                  aR 
                            a 2  h2

                                               42
SOLUTION TO EXAMPLE 3 (Cont’d)


  The integral of continuous charge distribution
  becomes:

                       L ad              aa   ha z   
    E                                                   
             4  0      a h
                          2      2
                                     
                                     2   
                                             a2  h2
                                                           
                                                           

                       L ad 
    E   
                                    
                                     3
                                             ha z
             4  0
                                         2
                          a h
                          2      2



                                                      43
SOLUTION TO EXAMPLE 3 (Cont’d)


   Rearranging,
                                    2
                L ah
    E                                da z
               
         4  0 a 2  h 2     
                              3
                                  2  0


   Easily solved,

                            L ah
          E                                  az
                       
                   2 0 a 2  h 2    3
                                          2


                                                   44
EXAMPLE 4



                                             nC
 An infinite length line of charge  L  4.0
                                              m
 exists at x = 2m and z = 4m. Find the
 electric field intensity at the origin.




                                           45
SOLUTION TO EXAMPLE 4

 Sketch in three dimensions and the cross section:




                                           46
SOLUTION TO EXAMPLE 4 (Cont’d)


  The vector from line charge to the origin:

            R  a   2a x  4a z
  Which has magnitude, R       20   and a unit
  vector,
                  2       4
        aR  a      ax     az
                   20      20

                                               47
SOLUTION TO EXAMPLE 4 (Cont’d)


 Inserting into the infinite line charge equation:

        L
  E          a
     2  0 
                          9
                4  10                     2a x  4a z 
    
           
      2  8 . 854  10  12
                                       
                                         
                                      20        20
                                                         
                                                         
                                  V
      7 . 2 a x  14 . 4 a z
                                  m
                                                 48
SURFACE CHARGE


 Infinite Sheet of Surface Charge:

 To derive the electric field intensity at point
 P at a height h above a charge sheet of
 infinite area (x-y plane).

 The charge distribution,      S is in   C
                                              m2


                                                   49
SURFACE CHARGE (Cont’d)




                          50
SURFACE CHARGE (Cont’d)


 Consider a differential charge,

    dQ   S dS
          S dd
 The vector from surface charge to the origin:

           R    a    ha z


                                            51
SURFACE CHARGE (Cont’d)


 Which has magnitude, R                 2  h 2 and a
 unit vector,
                        a   ha z
                aR 
                            2  h2
 Where, for continuous charge distribution:

                            dQ
                E                     aR
                         4  0 R
                                    2


                                                     52
SURFACE CHARGE (Cont’d)

  The equation becomes:

                S  dd                a   ha z   
  E                                                   
           4  0       2  h2   
                                   2   
                                           a2  h2
                                                         
                                                         

  Since only z components exists,

                 S  dd 
  E   
                                  
                                   3
                                           ha z
           4  0        h
                         2     2       2



                                                     53
SURFACE CHARGE (Cont’d)
                 2        
         S                              h dd
     E            
                                                        
                                                                 az
        4  0    0  0
                                                         3
                                          h2       2       2



                                              
                           
         Sh                                   2  2
                                                  3
               2                   2
                                            h           da z
         4  0            0
                                                     
       
         Sh
         2 0
                 
                     
                    2             h 2  2
                                          1
                                                    
                                                      az
                                                    0
          S
     E       az
          2 0
                                                                  54
SURFACE CHARGE (Cont’d)


  A general expression for the field from a sheet
  charge is:

                      S
                   E      aN
                      2 0

   Where   aN   is the unit vector normal from the
   sheet to the test point.


                                            55
EXAMPLE 5



                                            nC
 An infinite extent sheet of charge  S  10 2
                                            m
 exists at the plane y = -2m. Find the electric
 field intensity at point P (0, 2m, 1m).




                                       56
SOLUTION TO EXAMPLE 5


  Sketch the figure:




                        57
SOLUTION TO EXAMPLE 5 (Cont’d)

  The unit vector directed away from the sheet
  and toward the point P is   ay
      S
   E      aN
      2 0
           10  10  9
     
          
       2 8 . 854  10   12
                            ay
                              
                V
      565 a y
                 m
                                          58
VOLUME CHARGE


  A volume charge is distributed over a
  volume and is characterized by its volume
  charge density, V in C 3
                         m

  The total charge in a volume containing a
  charge    distribution, V is found by
  integrating over the volume: Q   dV
                                     V
                                  V

                                          59
EXAMPLE 6



  Find the total charge
  over the volume with
  volume charge density,

             10 5 z
  V  5e              C       3
                             m


                                     60
SOLUTION TO EXAMPLE 6

 The total charge,    Q   V dV             with volume:
                             V
   dV  dddz
  Thus,   Q   V dV
                V
                0.01 2      0.04
                                          10 5 z
                             5e                 dddz
                  0   0 z  0.02
                                    14
             7.854  10                   C
                                                           61
VOLUME CHARGE (Cont’d)

  To find the electric field intensity resulting from
  a volume charge, we use:

                   dQ                       V dV
       E                     aR                      aR
                4  0 R                  4  0 R
                           2                         2


  Since the vector R and        V    will vary over the
  volume, this triple integral can be difficult. It can
  be much simpler to determine E using Gauss’s
  Law.

                                                         62
2.4 ELECTRIC FLUX DENSITY


 Consider an amount of charge
 +Q is applied to a metallic
 sphere of radius a.

 Enclosed this charged sphere
 using   a   pair   of   connecting
 hemispheres with bigger radius.


                                      63
ELECTRIC FLUX DENSITY (Cont’d)

  The outer shell is grounded. Remove the ground
  then we could find that –Q of charge has
  accumulated on the outer sphere, meaning the
  +Q charge of the inner sphere has induced the –Q
  charge on the outer sphere.




                                             64
ELECTRIC FLUX DENSITY (Cont’d)


  Electric flux,  psi  extends from the positive
  charge and casts about for a negative charge. It
  begins at the +Q charge and terminates at the
  –Q charge.

   The electric flux density, D in C       2   is:
                                       m
                
       D
            4  0 R
                       2
                           a R where   D  E
                                                     65
ELECTRIC FLUX DENSITY (Cont’d)

  This is the relation between D and E, where         is
  the material permittivity. The advantage of using
  electric flux density rather than using electric
  field intensity is that the number of flux lines
  emanating from one set of charge and terminating
  on the other, independent from the media.

  We can find the total flux over a surface as:

                D  dS
                                              66
ELECTRIC FLUX DENSITY (Cont’d)


  We could also find the electric flux density, D
  for:

         Infinite line of charge:

         Where
               L                        L
         E          a       So,    D      a
            2  0                     2 


                                             67
ELECTRIC FLUX DENSITY (Cont’d)

     Infinite sheet of charge:

      Where
         S                               S
      E      aN           So,      D         aN
         2 0                              2
     Volume charge distribution:

                  V dV                             V dV
      E                      aR   So,   D                   aR
                                                   4 R
                                                            2
                4  0 R
                           2



                                                      68
EXAMPLE 7


 Find the amount of electric flux through the
 surface at z = 0 with 0  x  5m , 0  y  3m
 and
       
       D  3 xya x  4 xa z C m      2




                                         69
SOLUTION TO EXAMPLE 7


  The differential surface vector is

             dS  dxdya z
  We could have chosen     dS  dxdy a z     but the

  positive differential surface vector is pointing in

  the same direction as the flux, which give us a

  positive answer.


                                               70
SOLUTION TO EXAMPLE 7 (Cont’d)


  Therefore,

       D  dS
            3 xy a x    4 x a z   dxdy a z
               5   3
                4 xdxdy        Why?!
            x0 y0
         150 C
                                              71
EXAMPLE 8



 Determine D at (4,0,3) if there is a point

 charge    5 mC at (4,0,0) and a line
 charge   3 m C m along the y axis.




                                       72
SOLUTION TO EXAMPLE 8

  How to visualize ?!




                        73
SOLUTION TO EXAMPLE 8 (Cont’d)

  Let total flux,
                                  
                    DTOTAL    DQ  D L
  Where DQ is flux densities due to point charge
  and DL is flux densities due to line charge.
                                    
          DQ   0 E   0         aR 
  Thus,                         Q
                            4 R 2 
                               0      
                   Q
                       a
                      2 R
                4 R
                                            74
SOLUTION TO EXAMPLE 8 (Cont’d)


  Where,
     
     R  4,0,3  4,0,0   0,0,3
          3a z
  Which has magnitude, R  3 and a unit vector,

          3a z
     aR        az
           3

                                         75
SOLUTION TO EXAMPLE 8 (Cont’d)


  So,
               Q
        DQ               aR
               4 R
                      2


               5  103
                         az
                 4 9 
             0.138a m C  z
                               m2


                                    76
SOLUTION TO EXAMPLE 8 (Cont’d)

             L
  And   DL      a
             2
  Where,    a 
                   4,0,3  0,0,0  4a x  3a z
                   4,0,3  0,0,0        5

  So,
             3  4a x  3a z 
        DL                   
             2 5    5      
            0.24a  0.18a m C
                      x         z
                                      m2
                                                77
SOLUTION TO EXAMPLE 8 (Cont’d)


  Therefore, total flux:

                   
   DTOTAL    DQ  D L
              0.318a z   0.24a x  0.18a z 
             240a x  42a z  C
                                   m2


                                            78
2.5 GAUSS’S LAW

 If a charge is enclosed, the net flux passing
 through the enclosing surface must be equal to
 the charge enclosed, Qenc.

 Gauss’s Law states that:
  The net electric flux through any closed surface is
  equal to the total charge enclosed by that surface


               D  dS  Qenc
                                             79
GAUSS’S LAW (Cont’d)


  It can be rearranged so that we have relation
  between the Gauss’s Law and the electric flux.

                D  d S  Q enc
             Q enc      V dV
                       V

        Q   D  dS   V dV
                 S                V
                                            80
GAUSS’S LAW (Cont’d)

    Gauss’s Law is useful in finding the fields for
    problems that have high degree of symmetry.

    • Determine variables influence D and what
    components D present

    • Select an enclosing surface, called Gaussian
    Surface, whose differential surface is directed
    outward from the enclosed volume and is
    everywhere (either tangent or normal to D)

                                            81
GAUSS’S LAW APPLICATION (Cont’d)


  Use Gauss’s Law to determine electric
  field intensity for each cases below:

       Point Charge

       Infinite length of Line Charge

       Infinite extent Sheet of Charge


                                          82
POINT CHARGE

 • Point Charge:

  It has spherical coordinate
  symmetry, where the field
  is everywhere directed
  radially away from the
  origin. Thus,

     D  Dr a r

                                83
POINT CHARGE (Cont’d)


  For a gaussian surface, we could find the
  differential surface vector is:

           dS  r sin dda r
                    2

   So,

     D  d S   D r a r  r sin  d  d  a r
                               2


                D r r sin  d  d 
                         2



                                            84
POINT CHARGE (Cont’d)


  Since the gaussian surface has a fixed radius,
  Dr will be constant and can be taken from
  integration to yield
                                 2
    D  dS                    sin  d  d 
                         2
                 Dr r
                              0 0

                4 r 2 D r

                                                  85
POINT CHARGE (Cont’d)


  By using Gauss’s Law, where:

             D  dS  Qenc
            Dr 4r  Q
                     2

              Q
  So,   Dr              which leads to expected result:
             4r 2

                         Q
            E                   ar   See page 16!
                 4  0 r    2

                                                86
INFINITE LENGTH LINE OF CHARGE

 • Infinite length line of charge:

   Find D and then E at any
   point   P  , , z 
      A Gaussian surface
      containing the point P is
      placed around a section
      of an infinite length line
      of charge density L
      occupying the z-axis.

                                     87
LINE CHARGE (Cont’d)

  An element of charge dQ along the line will give
  Dρ and Dz. But second element of dQ will result
  in cancellation of Dz. Thus,

                 D  D a 
   The flux through the closed surface is:

    D  d S   D  d S top   D  d S bottom
                 D  d S side
                                             88
LINE CHARGE (Cont’d)

  Where,
    dStop  dda z ,
    dSbottom  dd  a z  , dS side  ddza 
  Then, we know that Dρ is constant on the side
  of gaussian surface

      D  d S side       D  a    d  dz a 
                                 2    h
                       D         d  dz     2 h  D 
                                  0 z0
                                                     89
LINE CHARGE (Cont’d)

  The charge enclosed by the gaussian surface:
                  h
          Qenc    L dz   L h
                   0
   We know that,

     D  d S  2 h  D      L h  Q enc
   So,         L      Thus, as          L
         D                        E         a
              2      expected:
                                       2 0 

                                               90
INFINITE EXTENT SHEET OF CHARGE

 • Infinite extent sheet of charge:


   Determine the field everywhere resulting
   from an infinite extent sheet of charge ρS
   placed on the x-y plane at z = 0.


    Locate a point at which we want to find the
    field along the z axis at height h.


                                                91
SHEET OF CHARGE (Cont’d)

 Gaussian surface must contain this point
 and surround some portion of the charged
 sheet.

  A rectangular box is
  employed as the
  Gaussian surface
  surrounding a section
  of sheet charge with
  sides 2x, 2y and 2z

                                        92
SHEET OF CHARGE (Cont’d)

  Only a DZ component will be present, and the
  charge enclosed is simply:
                               x   y
          Q    S dS   S  dx  dy
                            x     y
              4  S xy
   No flux through the side of the box, so find
   the flux through the top and bottom surface

                                            93
SHEET OF CHARGE (Cont’d)

   D  d S   D  d S top   D  d S bottom
                   D z a z  dxdy a z
                  top

                        D z  a z   dxdy  a z 
                      bottom
               2 4 xy D z
  Notice that the answer is independent of the
  height of the box.

                                                 94
SHEET OF CHARGE (Cont’d)

  Then we have:

           D  dS  Q
          2 4 xy D z  4  S xy
                    S              S
           Dz           or   D        az
                     2              2
   And electric field intensity, as expected:
                     S
                  E      aN
                     2 0
                                                95
GAUSS’S LAW (Cont’d)

  Related to Gauss’s Law, where net flux is
  evaluated exiting a closed surface, is the
  concept of divergence.

  Expression for divergence by applying Gauss’s
  Law might be too lengthy to derive, but it can be
  described as:

                    D  V
                                           96
GAUSS’S LAW (Cont’d)

  The expression is also called the point form of
  Gauss’s Law, since it occurs at some particular
  point in space. For instance,
      Plunger stationary – no net
      movement of molecules
      Plunger moves up – net
      movement where air molecules
      diverging  air is expanding
      Plunger pushes in – net flux is
      negative and molecules diverging
       air is compressing
                                             97
EXAMPLE 9


  Suppose:     
               D   a
                      2


   Find the flux through the surface of a cylinder
   with   0 zh    and    a   by evaluating the
   left side and the right side of the divergence
   theorem.



                                             98
SOLUTION TO EXAMPLE 9

  Remember the divergence theorem?

             D  dS     DdV
                       V
  We can first evaluate the left side of the
  divergence theorem by considering:

      D  d S   D  d S top   D  d S bottom
                       D  d S side

                                               99
SOLUTION TO EXAMPLE 9 (Cont’d)

 A sketch of this cylinder is shown with
 differential vectors.

  The integrals over
  the top and bottom
  surfaces are each
  zero, since:

     a  az  0

                                   100
SOLUTION TO EXAMPLE 9 (Cont’d)

  Thus,


     D  d S   D  d S side
                     2   h
                                a    d  dz
                                2

                      0 z0

                  2  ha   3



                                            101
SOLUTION TO EXAMPLE 9 (Cont’d)

  For evaluation of the right side of the divergence
  theorem, first find the divergence in cylindrical
  coordinate:
                 1 
            D
                  
                      D 
               
                 1  3
                  
                         3  
                                             102
SOLUTION TO EXAMPLE 9 (Cont’d)

 Performing a volume integration on this divergence,

           DdV
           V
           3 dddz
               2   a   h
         3             2dddz
             0  0 z 0

          2ha     3
                        This is the same!
                                            103
2.6 ELECTRIC POTENTIAL

  To develop the concept of electric potential and
  show its relationship to electric field intensity.

  In moving the object from point a to b, the
  work can be expressed by:
                       b
                  W   F  dL
                       a
     dL is differential length vector along some
     portion of the path between a and b

                                               104
ELECTRIC POTENTIAL (Cont’d)

 The work done by the field in moving the charge
 from a to b is
                            b
             WE  field  Q  E  dL
                            a
  If an external force moves the charge against the
  field, the work done is negative:
                        b
               W  Q  E  dL
                        a

                                            105
ELECTRIC POTENTIAL (Cont’d)


  We can defined the electric potential difference, Vba
  as the work done by an external source to move a
  charge from point a to point b as:

                             b
                    W
               Vba     E  dL
                    Q    a

   Where,
             Vba  Vb  Va

                                              106
ELECTRIC POTENTIAL (Cont’d)


  Consider the potential difference between two
  points in space resulting from the field of a
  point charge located at origin, where the
  electric field intensity is radially directed, then
  move from point a to b to have:

              b            b
                                Q
      Vba    E  dL                  a r  dra r
                           a 4 0 r
                                       2
              a


                                                         107
ELECTRIC POTENTIAL (Cont’d)

                          r b
                    Q
  Thus,   Vba 
                  4 0r r  a
                Q 1 1
                        Vb  Va
               4 0  b a 
   The absolute potential at some finite radius
   from a point charge fixed at the origin:
                             Q
                    V
                          4 0 r
                                           108
ELECTRIC POTENTIAL (Cont’d)

  If the collection of charges becomes a continuous
  distribution, we could find:
                                  dQ
                       V 
                                 4 0 r
                       L dL
   Where,   V       4  0 r     Line charge

                       S dS
            V       4  0 r     Surface charge

                       V dV
            V       4  0 r     Volume charge

                                                    109
ELECTRIC POTENTIAL (Cont’d)

  The principle of superposition, where applied to
  electric field also applies to potential difference.
                      Q1              Q2
             V                
                 4  0 r  r1   4  0 r  r2
                             QN
                  ... 
                        4  0 r  r N

  Or generally,              1       N
                                    Qk
                   V          rr
                       4  0 k  1    k
                                                 110
ELECTRIC POTENTIAL (Cont’d)


  Three different paths to
  calculate work moving
  from the origin to point
  P against an electric
  field.

  Based on figure, if a closed path is chosen, the
  integral will return zero potential:

                     E  dL  0
                                             111
EXAMPLE 10



  Two point charges -4 μC and 5 μC are
  located    at   (2,1-,3)   and   (0,4,-2)
  respectively. Find the potential at
  (1,0,1).




                                       112
SOLUTION TO EXAMPLE 10


  Let   Q1  4 C and Q2  5C

  So,
                  Q1              Q2
         V                
             4  0 r  r1   4  0 r  r2
  Where,

   r  r1  1, 0 ,1  2 ,  1,3    1,1,  2         6
   r  r2  1, 0 ,1  0 , 4 ,  2   1,  4 ,  2     26

                                                      113
SOLUTION TO EXAMPLE 10 (Cont’d)


  Therefore,
                      Q1              Q2
  V 1, 0 ,1                 
                 4  0 r  r1   4  0 r  r2
                         6               6
                  4  10     5  10
                         
                       
                 4  0 6   4  0 26         
   V 1,0,1  5.872 kV

                                           114
ELECTRIC POTENTIAL (Cont’d)

 The    electrostatic   potential
 contours from a point charge
 form equipotential surfaces
 surrounding the point charge.
 The   surfaces     are    always
 orthogonal to the field lines.
 The electric field can be
 determined by finding the max.
 rate and direction of spatial
 change of the potential field.


                                    115
ELECTRIC POTENTIAL (Cont’d)

  Therefore,

               E  V
  The negative sign indicates that the field is
  pointing in the direction of decreasing potential.

  By applying to the potential field:

                    Q              Q
       E  V             ar          a
                   r 4 0r      4 0r 2 r


                                              116
IMPORTANT!!
Three ways to calculate E:

      If sufficient symmetry, employ Gauss’s Law.

      Use the Coulomb’s Law approach.

      Use the gradient equation.




                                           117
EXAMPLE 11

Consider a disk of charge ρS, find the
potential at point (0,0,h) on the z-axis and
then find E at that point.




                                         118
SOLUTION TO EXAMPLE 11

Find that,

dQ   S dS
                    and    r  h2   2
      S dd
               dQ
With   V              then,
              4 0 r
       S a 2 dd
  V           r
     4 0   0   0

                                          119
SOLUTION TO EXAMPLE
                          11 (Cont’d)
How to calculate the integral?

Let   u  h 2   2 and du  2 d leads to
integral
             u 1 2 du then,
                                  a
         S
      V      h 
               2   2
         2 0                     0

           
             S
             2 0
                    h   2
                              a2  h   
                                            120
SOLUTION TO EXAMPLE
                         11 (Cont’d)
To find E, need to know how V is changing with
position. In this case E varies along the z-axis, so
simply replace h with z in the answer for V, then
proceed with the gradient equation.
              V
E  V         az
              z
    S  1 2 z                 S         z    
                     1a z       1  2      a z
    2 0  2 z 2  a 2         2 0     z  a2 

                                             121
BOUNDARY CONDITIONS

So far we have considered the existence of electric
field in a region consisting of two different media,
the condition that the field must satisfy at the
interfacing separating the media called “boundary
condition”. Thus, we could see how the fields
behave at the boundary between a pair of
dielectrics or between a dielectric and a conductor.



                                             122
BOUNDARY CONDITIONS

First boundary condition can be determined by
performing a line integral of E around a closed
rectangular path,




                                          123
BOUNDARY CONDITIONS

Fields are shown in each medium along with
normal and tangential components. For static
fields,
           E  dL  0
Integrate in the loop clockwise starting from a,

  b          c           d        a
   E  dL   E  dL   E  dL   E  dL  0
  a         b            c        d


                                           124
BOUNDARY CONDITIONS

Evaluate each segment,
 b         w
  E  dL   ET 1aT  dLaT     ET 1w
 a          0
 c           0                      h 2
  E  dL   EN1a N  dLa N   EN 2a N  dLa N
 b         h 2                       0

                               h
            E N 1  E N 2 
                                2

                                            125
BOUNDARY CONDITIONS
d          0
 E  dL   ET 2aT  dLaT        ET 2 w
c         w
a              0                    h 2
 E  dL   EN 2a N  dLa N   EN1a N  dLa N
d         h 2                      0

                           h
         E N 1  E N 2 
                            2
Summing for each segment, then we have the first
boundary condition:         ET 1  ET 2
                                              126
BOUNDARY CONDITIONS

Second boundary condition can be determined by
applying Gauss’s Law over a small pillbox shaped
Gaussian surface,




                                        127
BOUNDARY CONDITIONS

The Gauss’s Law,

          D  dS  Qenc
Where,

  D  dS   D  dS   D  dS   D  dS
          top         bottom      side

The pillbox is short enough, so the flux
passes through the side is negligible.

                                           128
BOUNDARY CONDITIONS

So, only top and bottom where:

 D  dS   DN1a N  dSa N  DN1S
top

   D  dS   DN 2a N  dS  a N    DN 2S
bottom

Which sums to:

         DN1  DN 2 S  Qenc
                                            129
BOUNDARY CONDITIONS

And the right side of Gauss’s Law,

   Qenc    S dS   S S

Thus, it leads to the second boundary condition:

          DN 1  DN 2   S
This is when the normal direction from
medium 2 to medium 1.

                                         130
BOUNDARY CONDITIONS

If the normal direction is from medium 1 to
medium 2,

              DN 2  DN 1   S
 Generally,

          a 21  D1  D2    S


                                         131
BOUNDARY CONDITIONS

For a boundary conditions between a dielectric
and a good conductor,

                 ET  0
Because in a good conductor, E = 0. And since
the electric flux density is zero inside the
conductor,

               DN  S

                                         132
EXAMPLE 12



Consider that the field E1 is known as:

     E1  3a x  4a y  5a z V m

Find the field E2 in the other dielectrics.




                                      133
SOLUTION TO EXAMPLE 12




              134
BOUNDARY CONDITIONS

We   can   employ    Poisson’s   and   Laplace’s
equations to help find the potential function
when conditions at the boundaries are specified.

 From divergence theorem expression,

                    D  V
 By considering   D  E ,
                        V
                  E 
                        
                                         135
BOUNDARY CONDITIONS

From the gradient expression,

               E  V
Which gives us Poisson’s equation,

                     V
               V 
                 2
                     
In charge free medium in which V  0 , it
becomes Laplace’s equation:
                                 V 0
                                 2

                                         136
EXAMPLE 13

Determine the electric
potential in the dielectric
region between a pair of
concentric spheres that
have a potential
difference Vab.




                                     137
SOLUTION TO EXAMPLE 13
                                   0 C
The charge distribution is:   V             3
                                   r      m
This employs Poisson’s equation and the potential
is only a function of r,
              V    0
        V 
         2
                 
                   r
         1   2 V (r )      0
        2 r            
        r r     r        r  r 0

                                                  138
SOLUTION TO EXAMPLE 13

Multiply with r2 and integrate to obtain,

            V (r )    0r 2
         r2                  A
             r        2 r 0
Dividing both sides with r2 and integrate again,

                    0r    A
        V (r )           B
                   2 r 0 r


                                            139
SOLUTION TO EXAMPLE 13 (Cont’d)

 Assume that the Vab consists of a voltage Va on
 the inner conductor and the outer conductor is
 grounded. So,

                      0a A
  V (r  a)  Va           B         1
                     2 r 0 a
                           0b A
  V (r  b)  Vb  0           B     2
                         2 r 0 b


                                           140
SOLUTION TO EXAMPLE 13

                 0 a         A         0b       A 
Vab  Va  Vb   
                 2   a  B     2   b  B 
                                                     
                       r 0                    r 0   
                   0                b  a  
           Va           b  a    A         (3)
                 2 r 0                ab 
                            Va ab 0 ab
 From (3) you can get: A         
                            a  b 2 r 0
      Thus, B  0
                  a  b  Va ab
                           
                   2 r 0   a b
                                             141
SOLUTION TO EXAMPLE 13


Then, the potential between the spheres is
given by:

                 0  a  Va a
       V (r )            r 
                2 r 0  r     r



                                         142
CAPACITANCE

The amount of charge that accumulates as a
function of potential difference is called the
capacitance.

                     Q
                  C
                     V
The unit is the farad (F) or coulomb per volt.



                                            143
CAPACITANCE (Cont’d)

Two methods for determining capacitance:
     Q Method
      •Assume a charge +Q on plate a and a charge
      –Q on plate b.
      • Solve for E using the appropriate method
      (Coulomb’s Law, Gauss’s Law, boundary
      conditions)
      •Solve for the potential difference Vab between
      the plates (The assumed Q will divide out)
                                            144
CAPACITANCE (Cont’d)

   V Method

       •   Assume Vab between the plates.

       •   Find E , then D using Laplace’s equation.

       •Find ρS, and then Q at each plate using
       conductor dielectric boundary condition
       (DN = ρS )

       •   C = Q/Vab (the assumed Vab will divide out)


                                               145
EXAMPLE 14

Use Q method to find the capacitance for
the parallel plate capacitor as shown.




                                         146
SOLUTION TO EXAMPLE 14

Place charge +Q on the inner surface of the top
plate, and –Q charge on the upper surface of the
bottom plate, where the charge density,

      S  Q        from    Q    S dS
               S
Use conductor dielectric boundary, to obtain:

    D Q
            S
               a z    from   DN  S
                                           147
SOLUTION TO EXAMPLE 14

We could find the electric field intensity, E
                    Q
                E          az
                    0 r S
The potential difference across the plates is:
            a
    Vab    E  dL
            b
            d
              Q                      Qd
                   a z  dza z 
           0  0 r S                0 r S
                                               148
SOLUTION TO EXAMPLE 14


Finally, to get the capacitance:

          Q          Q
      C     
         Vab              Qd
                          0 r S

              0 r S
     C 
                d
                                    149
EXAMPLE 15

Use V method to find the capacitance for a length L
of coaxial line of inner conductor radius a and
outer radius b, filled with dielectric permittivity as
shown.




                                              150
SOLUTION TO EXAMPLE 15

Employ Laplace’s equation to find the potential
field everywhere in the dielectric. Assume that
fringing fields are neglected and the field is only
in function of ρ.

Laplace’s equation becomes:

                 V 
                    0
                 
                                            151
SOLUTION TO EXAMPLE 15

Integrating twice to obtain:

                V    A ln   B

Apply boundary condition to determine A and
B. Let V(b) = 0 and V(a) = Vab to get:

                     Vab                  Vab ln b 
B   A ln b,   A           So, V   
                   ln b a                 lnb a 


                                               152
SOLUTION TO EXAMPLE 15

Apply the gradient to obtain E:

                            V  
             E  V  
                             
                    Vab
             E             a
                  lnb a 
and also..
                 r 0Vab
             D            a
                 lnb a 
                                      153
SOLUTION TO EXAMPLE 15 (Cont’d)

  At inner conductor, the flux is directed outward
  indicating a positive surface charge density,

                         r 0Vab
                 S 
                        a ln b a 
  We can find Q on the inner conductor with:

                r 0Vab          2L r 0Vab
   Q  S S             2aL   lnb a 
               a lnb a 

                                             154
SOLUTION TO EXAMPLE 15 (Cont’d)


  Thus, we can find the capacitance:

            Q 2L r  0
          C 
            V  ln b a 




                                       155
EXAMPLE 16

Conducting spherical shells with radius a =10cm
and b = 30cm are maintained at a potential
difference of 100V, such that V(r = a) = 100V and
V(r = b) = 0V. Determine:

• The V and E in the region between the shells.

• If εr = 2.5 in the shells, determine the total
charges induced on the shells and the capacitance
of the capacitor.

                                          156
EXAMPLE 16 (Cont’d)


With:

a  0.1m
b  0.3m
 r  2.5



                         157
SOLUTION TO EXAMPLE 16

Employ Laplace’s equation to find the potential
field and the field is only in function of r.

Laplace’s equation becomes:

              1   2 V 
         V  2 r
          2
                         0
             r r  r 
Multiply by r2,      2 V    
                      r       0
                   r  r     
                                                158
SOLUTION TO EXAMPLE 16 (Cont’d)

  Integrating once gives

          V      V A
        r 2
             A     2
          r      r r
   Integrating again gives

                  A
              V  B
                  r


                             159
SOLUTION TO EXAMPLE 16 (Cont’d)


  To obtain the value of constant A and B, use
  boundary conditions, where:
                                   A
      When,   r  b, V  0  0    B
                                   b
                                 A
                           B 
                                 b
      Thus,
                   1 1
              V  A  
                   b r 
                                          160
SOLUTION TO EXAMPLE 16 (Cont’d)


   When, r  a, V  V0 :

                      1 1
           V  V0  A  
                      b r 
                1 1 
          V0  A  
                b a 
                 V0
          A
                1 1
                  
                b a
                               161
SOLUTION TO EXAMPLE 16 (Cont’d)



   Therefore, the potential difference V

                      1 1
                        
               V  V0 b r 
                      1 1
                        
                      b a


                                           162
SOLUTION TO EXAMPLE 16 (Cont’d)

  Apply the gradient to obtain E:

                   V        A
       E  V      ar   2 ar
                   r       r
  So, the electric field intensity E

                            
                     1  V0 
                 E 2      a r
                    r 1  1 
                       b a 
                                       163
SOLUTION TO EXAMPLE 16 (Cont’d)


  The total charges Q is:


   Q   D  dS   E  dS
                               
         2 
                  0 rV0  1  2
                  2    1 1 r sin dd
         0  0 r         
                          b a 

                                         164
SOLUTION TO EXAMPLE 16 (Cont’d)


  This yields to:

                    2   
         0 rV0
    Q             d  sin d
        1 1  0  0
           
        b a
        4 0 rV0
     
           1 1
             
           b a
                                   165
SOLUTION TO EXAMPLE 16 (Cont’d)


  Thus, substituting the values of a, b and V0
  to get the total charges, Q


    Q
               
        4 8.854  10 2.5100
                            12
                                  
                 1    1
                    
                0.3 0.1
      4.1723 nC

                                           166
SOLUTION TO EXAMPLE 16 (Cont’d)


   And for the potential difference V = V0.

   So, the capacitance, C


      Q 4.1723 nC
    C            41.723 pF
      V   100 V


                                              167
PART 1

 END
PRACTICAL APPLICATION


 Laser Printer

 Electret Microphone

 Electrolytic Capacitors



                            169
LASER PRINTER




           170
LASER PRINTER (Cont’d)

• OPC drum : Organic Photoconductive Cartridge –
has a special coating will hold electrostatic charge.
• The surface is photoconductive – will discharge if
surface hit by light.
 i.    A portion of drum passes under a negative
      charged wire large negative charges induces a
      positive charge on the drum.
 ii. Image to be printed is delivered to this charged
     region by laser and spinning mirror combination.
 iii. Wherever the laser light strikes the drum, the
      photoconductive material is discharged.

                                                171
LASER PRINTER (Cont’d)

iv. The drum rolls past a toner The toner is black
   powder and positive charge drawn to those
   portions of the charge that have been discharged
   by the laser.
v. Paper is fed through same speed as drum it
   passes over positively charged wire that gives the
   paper a strong negative charge.
vi. The positively charged toner drum is transferred to
    the stronger negative charged on the paper then
    it passes near a negatively charged wire that
    removes the negative charge from the paper,
    prevents it from statically clinging to the drum

                                              172
LASER PRINTER (Cont’d)

vii.The paper and loose toner powder passed through
    heated fuser rollers powder melts into the paper
    fiber the warm paper exits the printer.

• The drum continues rolling, passing through high
intensity light discharges all the photoconductors
to erase the image from the drum, and ready for
application of positive charge again from corona
wire.




                                             173
SUMMARY (1)

•The force exerted on a charge Q1 on charge Q2 in a
medium of permittivity ε is given by Coulomb’s Law:

                       Q1Q 2
             F12                     a 12
                     4  R 12
                                  2


Where R12  R12a12 is a vector from charge Q1 to Q2

•Electric field intensity E1 is related to force F12 by:

                            F12
                       E1 
                            Q2
                                                 174
SUMMARY (2)

The Coulomb’s Law can be rewritten as:
                          Q
              E                       aR
                    4  0 R
                                   2

 For a continuous charge distribution:
                           dQ
              E       4  0 R
                                  a
                                 2 R

 •For a point charge at origin:
                           Q
                E                     ar
                        4  0 r   2

                                            175
SUMMARY (3)

•For an infinite length line charge ρL on the z axis
                      L
                 E       a
                    2 
•For an infinite extent sheet of charge ρS
                     S
                  E    aN
                     2
•Electric flux density related to field intensity by:
                   D   r 0E
 Where εr is the relative permittivity in a linear, isotropic
 and homogeneous material.

                                                 176
SUMMARY (4)

• Electric flux passing through a surface is given by:

                    D  dS
• Gauss’s Law states that the net electric flux through
any closed surface is equal to the total charge enclosed
by that surface:
                   D  dS  Qenc
 Point form of Gauss’s Law is

                     D  V
                                                177
SUMMARY (5)

• The electric potential difference Vab between a pair
of points a and b in an electric field is given by:
                  b
          Vba    E  dL  Vb  Va
                  a
 Where Va and Vb are the electrostatics potentials at a
 and b respectively.
 For a distribution of charge in the vicinity of the
 origin, where a zero reference voltage is taken at
 infinite radius:
                            dQ
                      V 
                           4r
                                                 178
SUMMARY (6)

• E is related to V by the gradient equation:

                   E  V
Which for Cartesian coordinates is:
            V      V      V
       V     ax     ay     az
            x      y      z
• The conditions for the fields at the boundary between
a pair of dielectrics is given by:

     ET 1  ET 2   and    a 21  D1  D2    S


                                                    179
SUMMARY (7)

Where ET1 and ET2 are the electric field components
tangential to the boundary, a21 is a unit vector from
medium 2 to 1 and ρS is the surface charge at the
boundary. If no surface charge is present, the
components of D normal to the boundary are equal:

                 D N1  D N 2
At the boundary between a conductor and a dielectric,
the conditions are:

       ET  0    and   DN  S

                                               180
SUMMARY (8)

• Poisson’s equation is:

                     V
               V 
                2
                     
 Where the Laplacian of V in Cartesian coordinates is
 given by:
                 V V V
                     2       2      2
              V 2  2  2
                2
                 x  y  z
 In a charge free medium, Poisson’s equation reduces to
 Laplace’s equation
                        V 0
                       2


                                             181
SUMMARY (9)

• Capacitance is a measure of charge storage capability
and is given by:
                         Q
                      C
                         V
 For coaxial cable:
             L                        2L
      Vab      ln b a     So,   C
            2                       ln b a 
 For two concentric spheres:
            Q 1 1                     4
     Vab                 So,   C
           4  a b                 1 a 1 b
                                                  182

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Part 1:Electrostatics

  • 2. ELECTROSTATICS 2.1 COULUMB’S LAW 2.2 ELECTRIC FIELD INTENSITY 2.3 LINE, SURFACE & VOLUME CHARGES 2.4 ELECTRIC FLUX DENSITY 2.5 GAUSS’S LAW 2.6 ELECTRIC POTENTIAL 2.7 BOUNDARY CONDITIONS 2.8 CAPACITANCE 2
  • 3. INTRODUCTION  Electromagnetics is the study of the effect of charges at rest and charges in motion.  Some special cases of electromagnetics:  Electrostatics: charges at rest  Magnetostatics: charges in steady motion (DC)  Electromagnetic waves: waves excited by charges in time-varying motion 3
  • 4. INTRODUCTION (Cont’d) Fundamental laws of Maxwell’s classical electromagnetics equations Special Electro- Magneto- Electro- Geometric cases statics statics magnetic Optics waves  Statics: 0 Transmission t Line Theory Input from Circuit other Theory Kirchoff’s disciplines d   Laws 4
  • 5. INTRODUCTION (Cont’d) • Electrical phenomena caused by friction are part of our everyday lives, and can be understood in terms of electrical charge. • The effects of electrical charge can be observed in the attraction/repulsion of various objects when “charged.” 5
  • 6. INTRODUCTION (Cont’d) • Charge comes in two varieties called “positive” and “negative.” • Objects carrying a net positive charge attract those carrying a net negative charge and repel those carrying a net positive charge. • Objects carrying a net negative charge attract those carrying a net positive charge and repel those carrying a net negative charge. • On an atomic scale, electrons are negatively charged and nuclei are positively charged. 6
  • 7. INTRODUCTION (Cont’d) • Electric charge is inherently quantized such that the charge on any object is an integer multiple of the smallest unit of charge which is the magnitude of the electron charge e = 1.602  10-19 C. • On the macroscopic level, we can assume that charge is “continuous.” 7
  • 8. COULUMB’S LAW In the late 18th century, Colonel Charles Augustus Coulomb invented a sensitive torsion balance that he used to experimentally determine the force exerted in one charge by another. 8
  • 9. COULUMB’S LAW (Cont’d) He found that the force is proportional to the product of two charges, inversely proportional to the square of the distance between the charges and acts in a line containing the two charges. Q1Q 2 F k 2 R 9
  • 10. COULUMB’S LAW (Cont’d) The proportional constant, k is: 1 k  ,    r 0 4  Where the free space permittivity with a value given by: 9  12 F 10 F  0  8 . 85  10  m 36  m 10
  • 11. COULUMB’S LAW (Cont’d) Charge Q1 exerts a vector force F12 in Newton's (N) on charge Q2, Q1Q 2 F12  a 12 4  0 R 12 2 11
  • 12. COULUMB’S LAW (Cont’d) If more than two charges, use the principle of superposition to determine the force on a particular charge. If there are N charges, Q1,Q2...QN located respectively at point with position vectors r1,r2...rN the resultant force F on a charge Q located at point r is the vector sum of the forces exerted on Q by each charges Q1,Q2...QN 12
  • 13. COULUMB’S LAW (Cont’d) F QQ 1 r  r1   QQ 2 r  r2  4  0 r  r1 2 r  r1 4  0 r  r2 2 r  r2 ...  QQ N r  r N  4  0 r  r N 2 r  rN Or generally, Q N Q k r  rk  F  4  0 k  1 3 r  rk 13
  • 14. COULUMB’S LAW (Cont’d) For example, FTOTAL  F12  F32 , Q1Q 2 F12  a 12 4  0 R 12 2 Q 3Q 2 F32  a 32 4  0 R 32 2 F12  F21 14
  • 15. EXAMPLE 1 Suppose 10nC charge Q1 located at (0.0, 0.0, 4.0m) and a 10nC charge Q2 located at (0.0, 4.0m, 0.0). Find the force acting on Q2 from Q1. 15
  • 16. SOLUTION TO EXAMPLE 1 To employ Coulomb’s Law, first find vector R12 R12  r2  r1    4a y  4a z   4a y  4a z Magnitude of R12 R12  42  42  32  4 2 16
  • 17. SOLUTION TO EXAMPLE 1 (Cont’d) R12 4a y  4a z 1 1 And a12    ay  az R12 4 2 2 2 Then Q1Q 2 F12  a 12 4  0 R 12 2  10  10 10  10  9 9  1  ay  1  az  4  8 . 854  10 4 2   12  2  2 2  4 . 0 a y  4 . 0 a z nN 17
  • 18. 2.2 ELECTRIC FIELD INTENSITY If Q1 is fixed to be at origin, a second charge Q2 will have force acting on Q1 and can be calculated using Coulomb’s Law. We also could calculate the force vector that would act on Q2 at every point in space to generate a field of such predicted force values. 18
  • 19. ELECTRIC FIELD INTENSITY (Cont’d) It becomes convenient to define electric field intensity E1 or force per unit charge as: F12 E1  Q2 This field from charge Q1 fixed at origin results from the force vector F12 for any arbitrarily chosen value of Q2 19
  • 20. ELECTRIC FIELD INTENSITY (Cont’d) Coulomb’s law can be rewritten as Q E aR 4  0 R 2 to find the electric field intensity at any point in space resulting from a fixed charge Q. 20
  • 21. EXAMPLE 2 Let a point charge Q1 = 25nC be located at P1 (4,-2,7). If ε = ε0, find electric field intensity at P2 (1,2,3). 21
  • 22. SOLUTION TO EXAMPLE 2 By using the electric field intensity, Q E aR 4  0 R 2 This field will be: 9 25  10 E a12 4 0 R12 22
  • 23. SOLUTION TO EXAMPLE 2 (Cont’d) Where, R12  r2  r1  3a x  4a y  4a z and R12  41 Q Q E a 2 12  R12 4 0 R12 4 0 R12 3 9 25  10   3a x  4a y  4a z   4 8.854  1012 41  3 2  23
  • 24. ELECTRIC FIELD INTENSITY (Cont’d) If there are N charges, Q1,Q2...QN located respectively at point with position vectors r1,r2...rN the electric field intensity at point r is: E Q1 r  r1   .. QN r  r N  4  0 r  r1 2 r  r1 4  0 r  r N 2 r  rN 1 N Q k r  rk  E  4  0 k  1 3 r  rk 24
  • 25. FIELD LINES The behavior of the fields can be visualized using field lines: Field vectors plotted within a regular grid in 2D space surrounding a point charge. 25
  • 26. FIELD LINES (Cont’d) Some of these field vectors can easily be joined by field lines that emanate from the positive point charge. The direction of the arrow indicates the direction of electric fields The magnitude is given by density of the lines 26
  • 27. FIELD LINES (Cont’d) The field lines terminated at a negative point charge The field lines for a pair of opposite charges 27
  • 28. 2.3 LINE,SURFACE & VOLUME CHARGES Electric fields due to continuous charge distributions: 28
  • 29. LINE,SURFACE & VOLUME CHARGES (Cont’d) To determine the charge for each distributions: Line charge: Surface charge: dQ   L dl dQ   S dS Q    L dl Q    S dS L S Volume charge: dQ  V dV Q   V dV V 29
  • 30. LINE CHARGE Infinite Length of Line Charge: To derive the electric field intensity at any point in space resulting from an infinite length line of charge placed conveniently along the z-axis 30
  • 31. LINE CHARGE (Cont’d) Place an amount of charge in coulombs along the z axis. The linear charge density is coulombs of charge per meter length,   L C m Choose an arbitrary point P where we want to find the electric field intensity. P  , , z  31
  • 32. LINE CHARGE (Cont’d) The electric field intensity is: E   E a   E a  Ez a z But, the field is only vary with the radial distance from the line. There is no segment of charge dQ anywhere on the z-axis that will give us E . So, E   E a   E z a z 32
  • 33. LINE CHARGE (Cont’d) Consider a dQ segment a distance z above radial axis, which will add the field components for the second charge element dQ. The E z components cancel each other (by symmetry) , and the E adds, will give: E   E a  33
  • 34. LINE CHARGE (Cont’d) Recall for point charge, Q E aR 4  0 R 2 For continuous charge distribution, the summation of vector field for each charges becomes an integral, dQ E  aR 4  0 R 2 34
  • 35. LINE CHARGE (Cont’d) The differential charge, dQ   L dl   L dz The vector from source to test point P, R  Ra R  a   za z 35
  • 36. LINE CHARGE (Cont’d) Which has magnitude, R   2  z 2 and a unit vector, a   za z aR   2  z2 So, the equation for integral of continuous charge distribution becomes:  L dz   a   za z    E  4  0   z 2 2  2   2  z2    36
  • 37. LINE CHARGE (Cont’d) Since there is no az component,  L dz E  a   4  0  2  z 2  3 2  L dz   a 4  0   2  z2  3 2 37
  • 38. LINE CHARGE (Cont’d) Hence, the electric field intensity at any point ρ away from an infinite length is: L E a 2  0  For any finite length, use the limits on the integral. 38
  • 39. EXAMPLE 3 Use Coulomb’s Law to find electric field intensity at (0,0,h) for the ring of charge, of charge density,  L centered at the origin in the x-y plane. 39
  • 40. SOLUTION TO EXAMPLE 3 By inspection, the ring charges delivers only dE  and dE z contribution to the field. dE  component will be cancelled by symmetry. 40
  • 41. SOLUTION TO EXAMPLE 3 (Cont’d) Each term need to be determined: dQ E  aR 4  0 R 2 The differential charge, dQ   L dl   L ad 41
  • 42. SOLUTION TO EXAMPLE 3 (Cont’d) The vector from source to test point, R  Ra R  aa   ha z Which has magnitude, R  a 2  h 2 and a unit vector,  aa   ha z aR  a 2  h2 42
  • 43. SOLUTION TO EXAMPLE 3 (Cont’d) The integral of continuous charge distribution becomes:  L ad    aa   ha z  E    4  0  a h 2 2  2   a2  h2    L ad  E    3 ha z 4  0 2 a h 2 2 43
  • 44. SOLUTION TO EXAMPLE 3 (Cont’d) Rearranging, 2  L ah E  da z  4  0 a 2  h 2  3 2  0 Easily solved,  L ah E az  2 0 a 2  h 2 3 2 44
  • 45. EXAMPLE 4 nC An infinite length line of charge  L  4.0 m exists at x = 2m and z = 4m. Find the electric field intensity at the origin. 45
  • 46. SOLUTION TO EXAMPLE 4 Sketch in three dimensions and the cross section: 46
  • 47. SOLUTION TO EXAMPLE 4 (Cont’d) The vector from line charge to the origin: R  a   2a x  4a z Which has magnitude, R  20 and a unit vector, 2 4 aR  a  ax  az 20 20 47
  • 48. SOLUTION TO EXAMPLE 4 (Cont’d) Inserting into the infinite line charge equation: L E a 2  0  9 4  10   2a x  4a z    2  8 . 854  10  12    20  20   V   7 . 2 a x  14 . 4 a z m 48
  • 49. SURFACE CHARGE Infinite Sheet of Surface Charge: To derive the electric field intensity at point P at a height h above a charge sheet of infinite area (x-y plane). The charge distribution,  S is in C m2 49
  • 51. SURFACE CHARGE (Cont’d) Consider a differential charge, dQ   S dS   S dd The vector from surface charge to the origin: R    a    ha z 51
  • 52. SURFACE CHARGE (Cont’d) Which has magnitude, R   2  h 2 and a unit vector,  a   ha z aR   2  h2 Where, for continuous charge distribution: dQ E  aR 4  0 R 2 52
  • 53. SURFACE CHARGE (Cont’d) The equation becomes:  S  dd    a   ha z  E    4  0   2  h2  2   a2  h2   Since only z components exists,  S  dd  E    3 ha z 4  0  h 2 2 2 53
  • 54. SURFACE CHARGE (Cont’d) 2  S h dd E     az 4  0  0  0 3  h2 2 2     Sh 2  2 3  2 2  h da z 4  0  0   Sh 2 0     2  h 2  2 1    az  0 S E  az 2 0 54
  • 55. SURFACE CHARGE (Cont’d) A general expression for the field from a sheet charge is: S E aN 2 0 Where aN is the unit vector normal from the sheet to the test point. 55
  • 56. EXAMPLE 5 nC An infinite extent sheet of charge  S  10 2 m exists at the plane y = -2m. Find the electric field intensity at point P (0, 2m, 1m). 56
  • 57. SOLUTION TO EXAMPLE 5 Sketch the figure: 57
  • 58. SOLUTION TO EXAMPLE 5 (Cont’d) The unit vector directed away from the sheet and toward the point P is ay S E aN 2 0 10  10  9   2 8 . 854  10  12 ay  V  565 a y m 58
  • 59. VOLUME CHARGE A volume charge is distributed over a volume and is characterized by its volume charge density, V in C 3 m The total charge in a volume containing a charge distribution, V is found by integrating over the volume: Q   dV  V V 59
  • 60. EXAMPLE 6 Find the total charge over the volume with volume charge density, 10 5 z V  5e C 3 m 60
  • 61. SOLUTION TO EXAMPLE 6 The total charge, Q   V dV with volume: V dV  dddz Thus, Q   V dV V 0.01 2 0.04 10 5 z      5e dddz   0   0 z  0.02 14  7.854  10 C 61
  • 62. VOLUME CHARGE (Cont’d) To find the electric field intensity resulting from a volume charge, we use: dQ  V dV E  aR   aR 4  0 R 4  0 R 2 2 Since the vector R and V will vary over the volume, this triple integral can be difficult. It can be much simpler to determine E using Gauss’s Law. 62
  • 63. 2.4 ELECTRIC FLUX DENSITY Consider an amount of charge +Q is applied to a metallic sphere of radius a. Enclosed this charged sphere using a pair of connecting hemispheres with bigger radius. 63
  • 64. ELECTRIC FLUX DENSITY (Cont’d) The outer shell is grounded. Remove the ground then we could find that –Q of charge has accumulated on the outer sphere, meaning the +Q charge of the inner sphere has induced the –Q charge on the outer sphere. 64
  • 65. ELECTRIC FLUX DENSITY (Cont’d) Electric flux,  psi  extends from the positive charge and casts about for a negative charge. It begins at the +Q charge and terminates at the –Q charge. The electric flux density, D in C 2 is: m  D 4  0 R 2 a R where D  E 65
  • 66. ELECTRIC FLUX DENSITY (Cont’d) This is the relation between D and E, where  is the material permittivity. The advantage of using electric flux density rather than using electric field intensity is that the number of flux lines emanating from one set of charge and terminating on the other, independent from the media. We can find the total flux over a surface as:    D  dS 66
  • 67. ELECTRIC FLUX DENSITY (Cont’d) We could also find the electric flux density, D for:  Infinite line of charge: Where L L E a So, D a 2  0  2  67
  • 68. ELECTRIC FLUX DENSITY (Cont’d)  Infinite sheet of charge: Where S S E aN So, D aN 2 0 2  Volume charge distribution:  V dV  V dV E  aR So, D  aR 4 R 2 4  0 R 2 68
  • 69. EXAMPLE 7 Find the amount of electric flux through the surface at z = 0 with 0  x  5m , 0  y  3m and  D  3 xya x  4 xa z C m 2 69
  • 70. SOLUTION TO EXAMPLE 7 The differential surface vector is dS  dxdya z We could have chosen dS  dxdy a z  but the positive differential surface vector is pointing in the same direction as the flux, which give us a positive answer. 70
  • 71. SOLUTION TO EXAMPLE 7 (Cont’d) Therefore,    D  dS   3 xy a x  4 x a z   dxdy a z 5 3    4 xdxdy Why?! x0 y0  150 C 71
  • 72. EXAMPLE 8 Determine D at (4,0,3) if there is a point charge  5 mC at (4,0,0) and a line charge 3 m C m along the y axis. 72
  • 73. SOLUTION TO EXAMPLE 8 How to visualize ?! 73
  • 74. SOLUTION TO EXAMPLE 8 (Cont’d) Let total flux,    DTOTAL  DQ  D L Where DQ is flux densities due to point charge and DL is flux densities due to line charge.     DQ   0 E   0  aR  Thus, Q  4 R 2   0  Q  a 2 R 4 R 74
  • 75. SOLUTION TO EXAMPLE 8 (Cont’d) Where,  R  4,0,3  4,0,0   0,0,3  3a z Which has magnitude, R  3 and a unit vector, 3a z aR   az 3 75
  • 76. SOLUTION TO EXAMPLE 8 (Cont’d) So,  Q DQ  aR 4 R 2  5  103  az 4 9   0.138a m C z m2 76
  • 77. SOLUTION TO EXAMPLE 8 (Cont’d)  L And DL  a 2 Where, a  4,0,3  0,0,0  4a x  3a z 4,0,3  0,0,0 5 So,  3  4a x  3a z  DL    2 5  5   0.24a  0.18a m C x z m2 77
  • 78. SOLUTION TO EXAMPLE 8 (Cont’d) Therefore, total flux:    DTOTAL  DQ  D L   0.318a z   0.24a x  0.18a z   240a x  42a z  C m2 78
  • 79. 2.5 GAUSS’S LAW If a charge is enclosed, the net flux passing through the enclosing surface must be equal to the charge enclosed, Qenc. Gauss’s Law states that: The net electric flux through any closed surface is equal to the total charge enclosed by that surface  D  dS  Qenc 79
  • 80. GAUSS’S LAW (Cont’d) It can be rearranged so that we have relation between the Gauss’s Law and the electric flux.    D  d S  Q enc Q enc    V dV V  Q   D  dS   V dV S V 80
  • 81. GAUSS’S LAW (Cont’d) Gauss’s Law is useful in finding the fields for problems that have high degree of symmetry. • Determine variables influence D and what components D present • Select an enclosing surface, called Gaussian Surface, whose differential surface is directed outward from the enclosed volume and is everywhere (either tangent or normal to D) 81
  • 82. GAUSS’S LAW APPLICATION (Cont’d) Use Gauss’s Law to determine electric field intensity for each cases below:  Point Charge  Infinite length of Line Charge  Infinite extent Sheet of Charge 82
  • 83. POINT CHARGE • Point Charge: It has spherical coordinate symmetry, where the field is everywhere directed radially away from the origin. Thus, D  Dr a r 83
  • 84. POINT CHARGE (Cont’d) For a gaussian surface, we could find the differential surface vector is: dS  r sin dda r 2 So,  D  d S   D r a r  r sin  d  d  a r 2   D r r sin  d  d  2 84
  • 85. POINT CHARGE (Cont’d) Since the gaussian surface has a fixed radius, Dr will be constant and can be taken from integration to yield  2  D  dS    sin  d  d  2 Dr r  0 0  4 r 2 D r 85
  • 86. POINT CHARGE (Cont’d) By using Gauss’s Law, where:  D  dS  Qenc Dr 4r  Q 2 Q So, Dr  which leads to expected result: 4r 2 Q E ar See page 16! 4  0 r 2 86
  • 87. INFINITE LENGTH LINE OF CHARGE • Infinite length line of charge: Find D and then E at any point P  , , z  A Gaussian surface containing the point P is placed around a section of an infinite length line of charge density L occupying the z-axis. 87
  • 88. LINE CHARGE (Cont’d) An element of charge dQ along the line will give Dρ and Dz. But second element of dQ will result in cancellation of Dz. Thus, D  D a  The flux through the closed surface is:  D  d S   D  d S top   D  d S bottom   D  d S side 88
  • 89. LINE CHARGE (Cont’d) Where, dStop  dda z , dSbottom  dd  a z  , dS side  ddza  Then, we know that Dρ is constant on the side of gaussian surface  D  d S side   D  a    d  dz a  2 h  D    d  dz  2 h  D   0 z0 89
  • 90. LINE CHARGE (Cont’d) The charge enclosed by the gaussian surface: h Qenc    L dz   L h 0 We know that,  D  d S  2 h  D    L h  Q enc So, L Thus, as L D  E a 2 expected: 2 0  90
  • 91. INFINITE EXTENT SHEET OF CHARGE • Infinite extent sheet of charge: Determine the field everywhere resulting from an infinite extent sheet of charge ρS placed on the x-y plane at z = 0. Locate a point at which we want to find the field along the z axis at height h. 91
  • 92. SHEET OF CHARGE (Cont’d) Gaussian surface must contain this point and surround some portion of the charged sheet. A rectangular box is employed as the Gaussian surface surrounding a section of sheet charge with sides 2x, 2y and 2z 92
  • 93. SHEET OF CHARGE (Cont’d) Only a DZ component will be present, and the charge enclosed is simply: x y Q    S dS   S  dx  dy x y  4  S xy No flux through the side of the box, so find the flux through the top and bottom surface 93
  • 94. SHEET OF CHARGE (Cont’d)   D  d S   D  d S top   D  d S bottom   D z a z  dxdy a z top   D z  a z   dxdy  a z  bottom  2 4 xy D z Notice that the answer is independent of the height of the box. 94
  • 95. SHEET OF CHARGE (Cont’d) Then we have:  D  dS  Q 2 4 xy D z  4  S xy S S  Dz  or D az 2 2 And electric field intensity, as expected: S E aN 2 0 95
  • 96. GAUSS’S LAW (Cont’d) Related to Gauss’s Law, where net flux is evaluated exiting a closed surface, is the concept of divergence. Expression for divergence by applying Gauss’s Law might be too lengthy to derive, but it can be described as:   D  V 96
  • 97. GAUSS’S LAW (Cont’d) The expression is also called the point form of Gauss’s Law, since it occurs at some particular point in space. For instance, Plunger stationary – no net movement of molecules Plunger moves up – net movement where air molecules diverging  air is expanding Plunger pushes in – net flux is negative and molecules diverging  air is compressing 97
  • 98. EXAMPLE 9 Suppose:  D   a 2 Find the flux through the surface of a cylinder with 0 zh and  a by evaluating the left side and the right side of the divergence theorem. 98
  • 99. SOLUTION TO EXAMPLE 9 Remember the divergence theorem?  D  dS     DdV V We can first evaluate the left side of the divergence theorem by considering:    D  d S   D  d S top   D  d S bottom   D  d S side 99
  • 100. SOLUTION TO EXAMPLE 9 (Cont’d) A sketch of this cylinder is shown with differential vectors. The integrals over the top and bottom surfaces are each zero, since: a  az  0 100
  • 101. SOLUTION TO EXAMPLE 9 (Cont’d) Thus,    D  d S   D  d S side 2 h    a    d  dz 2  0 z0  2  ha 3 101
  • 102. SOLUTION TO EXAMPLE 9 (Cont’d) For evaluation of the right side of the divergence theorem, first find the divergence in cylindrical coordinate: 1  D   D   1  3     3   102
  • 103. SOLUTION TO EXAMPLE 9 (Cont’d) Performing a volume integration on this divergence,      DdV V   3 dddz 2 a h 3     2dddz  0  0 z 0  2ha 3 This is the same! 103
  • 104. 2.6 ELECTRIC POTENTIAL To develop the concept of electric potential and show its relationship to electric field intensity. In moving the object from point a to b, the work can be expressed by: b W   F  dL a dL is differential length vector along some portion of the path between a and b 104
  • 105. ELECTRIC POTENTIAL (Cont’d) The work done by the field in moving the charge from a to b is b WE  field  Q  E  dL a If an external force moves the charge against the field, the work done is negative: b W  Q  E  dL a 105
  • 106. ELECTRIC POTENTIAL (Cont’d) We can defined the electric potential difference, Vba as the work done by an external source to move a charge from point a to point b as: b W Vba     E  dL Q a Where, Vba  Vb  Va 106
  • 107. ELECTRIC POTENTIAL (Cont’d) Consider the potential difference between two points in space resulting from the field of a point charge located at origin, where the electric field intensity is radially directed, then move from point a to b to have: b b Q Vba    E  dL    a r  dra r a 4 0 r 2 a 107
  • 108. ELECTRIC POTENTIAL (Cont’d) r b Q Thus, Vba  4 0r r  a Q 1 1      Vb  Va 4 0  b a  The absolute potential at some finite radius from a point charge fixed at the origin: Q V 4 0 r 108
  • 109. ELECTRIC POTENTIAL (Cont’d) If the collection of charges becomes a continuous distribution, we could find: dQ V  4 0 r  L dL Where, V   4  0 r Line charge  S dS V   4  0 r Surface charge  V dV V   4  0 r Volume charge 109
  • 110. ELECTRIC POTENTIAL (Cont’d) The principle of superposition, where applied to electric field also applies to potential difference. Q1 Q2 V   4  0 r  r1 4  0 r  r2 QN ...  4  0 r  r N Or generally, 1 N Qk V   rr 4  0 k  1 k 110
  • 111. ELECTRIC POTENTIAL (Cont’d) Three different paths to calculate work moving from the origin to point P against an electric field. Based on figure, if a closed path is chosen, the integral will return zero potential:  E  dL  0 111
  • 112. EXAMPLE 10 Two point charges -4 μC and 5 μC are located at (2,1-,3) and (0,4,-2) respectively. Find the potential at (1,0,1). 112
  • 113. SOLUTION TO EXAMPLE 10 Let Q1  4 C and Q2  5C So, Q1 Q2 V   4  0 r  r1 4  0 r  r2 Where, r  r1  1, 0 ,1  2 ,  1,3    1,1,  2   6 r  r2  1, 0 ,1  0 , 4 ,  2   1,  4 ,  2   26 113
  • 114. SOLUTION TO EXAMPLE 10 (Cont’d) Therefore, Q1 Q2 V 1, 0 ,1    4  0 r  r1 4  0 r  r2 6 6  4  10 5  10     4  0 6 4  0 26   V 1,0,1  5.872 kV 114
  • 115. ELECTRIC POTENTIAL (Cont’d) The electrostatic potential contours from a point charge form equipotential surfaces surrounding the point charge. The surfaces are always orthogonal to the field lines. The electric field can be determined by finding the max. rate and direction of spatial change of the potential field. 115
  • 116. ELECTRIC POTENTIAL (Cont’d) Therefore, E  V The negative sign indicates that the field is pointing in the direction of decreasing potential. By applying to the potential field:  Q Q E  V   ar  a r 4 0r 4 0r 2 r 116
  • 117. IMPORTANT!! Three ways to calculate E:  If sufficient symmetry, employ Gauss’s Law.  Use the Coulomb’s Law approach.  Use the gradient equation. 117
  • 118. EXAMPLE 11 Consider a disk of charge ρS, find the potential at point (0,0,h) on the z-axis and then find E at that point. 118
  • 119. SOLUTION TO EXAMPLE 11 Find that, dQ   S dS and r  h2   2   S dd dQ With V  then, 4 0 r  S a 2 dd V   r 4 0   0   0 119
  • 120. SOLUTION TO EXAMPLE 11 (Cont’d) How to calculate the integral? Let u  h 2   2 and du  2 d leads to integral  u 1 2 du then,  a S V h  2 2 2 0  0  S 2 0 h 2  a2  h  120
  • 121. SOLUTION TO EXAMPLE 11 (Cont’d) To find E, need to know how V is changing with position. In this case E varies along the z-axis, so simply replace h with z in the answer for V, then proceed with the gradient equation. V E  V   az z S  1 2 z  S  z     1a z  1  2 a z 2 0  2 z 2  a 2  2 0  z  a2  121
  • 122. BOUNDARY CONDITIONS So far we have considered the existence of electric field in a region consisting of two different media, the condition that the field must satisfy at the interfacing separating the media called “boundary condition”. Thus, we could see how the fields behave at the boundary between a pair of dielectrics or between a dielectric and a conductor. 122
  • 123. BOUNDARY CONDITIONS First boundary condition can be determined by performing a line integral of E around a closed rectangular path, 123
  • 124. BOUNDARY CONDITIONS Fields are shown in each medium along with normal and tangential components. For static fields,  E  dL  0 Integrate in the loop clockwise starting from a, b c d a  E  dL   E  dL   E  dL   E  dL  0 a b c d 124
  • 125. BOUNDARY CONDITIONS Evaluate each segment, b w  E  dL   ET 1aT  dLaT  ET 1w a 0 c 0 h 2  E  dL   EN1a N  dLa N   EN 2a N  dLa N b h 2 0 h   E N 1  E N 2  2 125
  • 126. BOUNDARY CONDITIONS d 0  E  dL   ET 2aT  dLaT   ET 2 w c w a 0 h 2  E  dL   EN 2a N  dLa N   EN1a N  dLa N d h 2 0 h  E N 1  E N 2  2 Summing for each segment, then we have the first boundary condition: ET 1  ET 2 126
  • 127. BOUNDARY CONDITIONS Second boundary condition can be determined by applying Gauss’s Law over a small pillbox shaped Gaussian surface, 127
  • 128. BOUNDARY CONDITIONS The Gauss’s Law,  D  dS  Qenc Where,  D  dS   D  dS   D  dS   D  dS top bottom side The pillbox is short enough, so the flux passes through the side is negligible. 128
  • 129. BOUNDARY CONDITIONS So, only top and bottom where:  D  dS   DN1a N  dSa N  DN1S top  D  dS   DN 2a N  dS  a N    DN 2S bottom Which sums to: DN1  DN 2 S  Qenc 129
  • 130. BOUNDARY CONDITIONS And the right side of Gauss’s Law, Qenc    S dS   S S Thus, it leads to the second boundary condition: DN 1  DN 2   S This is when the normal direction from medium 2 to medium 1. 130
  • 131. BOUNDARY CONDITIONS If the normal direction is from medium 1 to medium 2, DN 2  DN 1   S Generally, a 21  D1  D2    S 131
  • 132. BOUNDARY CONDITIONS For a boundary conditions between a dielectric and a good conductor, ET  0 Because in a good conductor, E = 0. And since the electric flux density is zero inside the conductor, DN  S 132
  • 133. EXAMPLE 12 Consider that the field E1 is known as: E1  3a x  4a y  5a z V m Find the field E2 in the other dielectrics. 133
  • 135. BOUNDARY CONDITIONS We can employ Poisson’s and Laplace’s equations to help find the potential function when conditions at the boundaries are specified. From divergence theorem expression,   D  V By considering D  E , V E   135
  • 136. BOUNDARY CONDITIONS From the gradient expression, E  V Which gives us Poisson’s equation, V  V  2  In charge free medium in which V  0 , it becomes Laplace’s equation:  V 0 2 136
  • 137. EXAMPLE 13 Determine the electric potential in the dielectric region between a pair of concentric spheres that have a potential difference Vab. 137
  • 138. SOLUTION TO EXAMPLE 13 0 C The charge distribution is: V  3 r m This employs Poisson’s equation and the potential is only a function of r, V 0  V  2   r 1   2 V (r )  0  2 r  r r  r  r  r 0 138
  • 139. SOLUTION TO EXAMPLE 13 Multiply with r2 and integrate to obtain, V (r ) 0r 2 r2  A r 2 r 0 Dividing both sides with r2 and integrate again, 0r A V (r )    B 2 r 0 r 139
  • 140. SOLUTION TO EXAMPLE 13 (Cont’d) Assume that the Vab consists of a voltage Va on the inner conductor and the outer conductor is grounded. So, 0a A V (r  a)  Va    B 1 2 r 0 a 0b A V (r  b)  Vb  0    B 2 2 r 0 b 140
  • 141. SOLUTION TO EXAMPLE 13  0 a A   0b A  Vab  Va  Vb     2   a  B     2   b  B      r 0   r 0  0  b  a   Va  b  a    A  (3) 2 r 0  ab  Va ab 0 ab From (3) you can get: A   a  b 2 r 0 Thus, B  0  a  b  Va ab  2 r 0 a b 141
  • 142. SOLUTION TO EXAMPLE 13 Then, the potential between the spheres is given by: 0  a  Va a V (r )    r  2 r 0  r  r 142
  • 143. CAPACITANCE The amount of charge that accumulates as a function of potential difference is called the capacitance. Q C V The unit is the farad (F) or coulomb per volt. 143
  • 144. CAPACITANCE (Cont’d) Two methods for determining capacitance:  Q Method •Assume a charge +Q on plate a and a charge –Q on plate b. • Solve for E using the appropriate method (Coulomb’s Law, Gauss’s Law, boundary conditions) •Solve for the potential difference Vab between the plates (The assumed Q will divide out) 144
  • 145. CAPACITANCE (Cont’d)  V Method • Assume Vab between the plates. • Find E , then D using Laplace’s equation. •Find ρS, and then Q at each plate using conductor dielectric boundary condition (DN = ρS ) • C = Q/Vab (the assumed Vab will divide out) 145
  • 146. EXAMPLE 14 Use Q method to find the capacitance for the parallel plate capacitor as shown. 146
  • 147. SOLUTION TO EXAMPLE 14 Place charge +Q on the inner surface of the top plate, and –Q charge on the upper surface of the bottom plate, where the charge density, S  Q from Q    S dS S Use conductor dielectric boundary, to obtain: D Q S  a z  from DN  S 147
  • 148. SOLUTION TO EXAMPLE 14 We could find the electric field intensity, E Q E az  0 r S The potential difference across the plates is: a Vab    E  dL b d Q Qd   a z  dza z  0  0 r S  0 r S 148
  • 149. SOLUTION TO EXAMPLE 14 Finally, to get the capacitance: Q Q C  Vab Qd  0 r S  0 r S C  d 149
  • 150. EXAMPLE 15 Use V method to find the capacitance for a length L of coaxial line of inner conductor radius a and outer radius b, filled with dielectric permittivity as shown. 150
  • 151. SOLUTION TO EXAMPLE 15 Employ Laplace’s equation to find the potential field everywhere in the dielectric. Assume that fringing fields are neglected and the field is only in function of ρ. Laplace’s equation becomes:   V   0     151
  • 152. SOLUTION TO EXAMPLE 15 Integrating twice to obtain: V    A ln   B Apply boundary condition to determine A and B. Let V(b) = 0 and V(a) = Vab to get:  Vab  Vab ln b  B   A ln b, A So, V    ln b a  lnb a  152
  • 153. SOLUTION TO EXAMPLE 15 Apply the gradient to obtain E: V   E  V    Vab E a  lnb a  and also..  r 0Vab D a  lnb a  153
  • 154. SOLUTION TO EXAMPLE 15 (Cont’d) At inner conductor, the flux is directed outward indicating a positive surface charge density,  r 0Vab S  a ln b a  We can find Q on the inner conductor with:   r 0Vab  2L r 0Vab Q  S S   2aL   lnb a   a lnb a  154
  • 155. SOLUTION TO EXAMPLE 15 (Cont’d) Thus, we can find the capacitance: Q 2L r  0 C  V ln b a  155
  • 156. EXAMPLE 16 Conducting spherical shells with radius a =10cm and b = 30cm are maintained at a potential difference of 100V, such that V(r = a) = 100V and V(r = b) = 0V. Determine: • The V and E in the region between the shells. • If εr = 2.5 in the shells, determine the total charges induced on the shells and the capacitance of the capacitor. 156
  • 157. EXAMPLE 16 (Cont’d) With: a  0.1m b  0.3m  r  2.5 157
  • 158. SOLUTION TO EXAMPLE 16 Employ Laplace’s equation to find the potential field and the field is only in function of r. Laplace’s equation becomes: 1   2 V   V  2 r 2 0 r r  r  Multiply by r2,   2 V  r 0 r  r  158
  • 159. SOLUTION TO EXAMPLE 16 (Cont’d) Integrating once gives V V A r 2 A   2 r r r Integrating again gives A V  B r 159
  • 160. SOLUTION TO EXAMPLE 16 (Cont’d) To obtain the value of constant A and B, use boundary conditions, where: A When, r  b, V  0  0    B b A B  b Thus, 1 1 V  A   b r  160
  • 161. SOLUTION TO EXAMPLE 16 (Cont’d) When, r  a, V  V0 : 1 1  V  V0  A   b r  1 1  V0  A   b a  V0 A 1 1  b a 161
  • 162. SOLUTION TO EXAMPLE 16 (Cont’d) Therefore, the potential difference V 1 1    V  V0 b r  1 1    b a 162
  • 163. SOLUTION TO EXAMPLE 16 (Cont’d) Apply the gradient to obtain E: V A E  V   ar   2 ar r r So, the electric field intensity E   1  V0  E 2  a r r 1  1  b a  163
  • 164. SOLUTION TO EXAMPLE 16 (Cont’d) The total charges Q is: Q   D  dS   E  dS   2   0 rV0  1  2    2  1 1 r sin dd  0  0 r    b a  164
  • 165. SOLUTION TO EXAMPLE 16 (Cont’d) This yields to: 2    0 rV0 Q  d  sin d 1 1  0  0  b a  4 0 rV0  1 1  b a 165
  • 166. SOLUTION TO EXAMPLE 16 (Cont’d) Thus, substituting the values of a, b and V0 to get the total charges, Q Q   4 8.854  10 2.5100 12  1 1  0.3 0.1  4.1723 nC 166
  • 167. SOLUTION TO EXAMPLE 16 (Cont’d) And for the potential difference V = V0. So, the capacitance, C Q 4.1723 nC C   41.723 pF V 100 V 167
  • 169. PRACTICAL APPLICATION  Laser Printer  Electret Microphone  Electrolytic Capacitors 169
  • 171. LASER PRINTER (Cont’d) • OPC drum : Organic Photoconductive Cartridge – has a special coating will hold electrostatic charge. • The surface is photoconductive – will discharge if surface hit by light. i. A portion of drum passes under a negative charged wire large negative charges induces a positive charge on the drum. ii. Image to be printed is delivered to this charged region by laser and spinning mirror combination. iii. Wherever the laser light strikes the drum, the photoconductive material is discharged. 171
  • 172. LASER PRINTER (Cont’d) iv. The drum rolls past a toner The toner is black powder and positive charge drawn to those portions of the charge that have been discharged by the laser. v. Paper is fed through same speed as drum it passes over positively charged wire that gives the paper a strong negative charge. vi. The positively charged toner drum is transferred to the stronger negative charged on the paper then it passes near a negatively charged wire that removes the negative charge from the paper, prevents it from statically clinging to the drum 172
  • 173. LASER PRINTER (Cont’d) vii.The paper and loose toner powder passed through heated fuser rollers powder melts into the paper fiber the warm paper exits the printer. • The drum continues rolling, passing through high intensity light discharges all the photoconductors to erase the image from the drum, and ready for application of positive charge again from corona wire. 173
  • 174. SUMMARY (1) •The force exerted on a charge Q1 on charge Q2 in a medium of permittivity ε is given by Coulomb’s Law: Q1Q 2 F12  a 12 4  R 12 2 Where R12  R12a12 is a vector from charge Q1 to Q2 •Electric field intensity E1 is related to force F12 by: F12 E1  Q2 174
  • 175. SUMMARY (2) The Coulomb’s Law can be rewritten as: Q E aR 4  0 R 2 For a continuous charge distribution: dQ E  4  0 R a 2 R •For a point charge at origin: Q E ar 4  0 r 2 175
  • 176. SUMMARY (3) •For an infinite length line charge ρL on the z axis L E a 2  •For an infinite extent sheet of charge ρS S E aN 2 •Electric flux density related to field intensity by: D   r 0E Where εr is the relative permittivity in a linear, isotropic and homogeneous material. 176
  • 177. SUMMARY (4) • Electric flux passing through a surface is given by:    D  dS • Gauss’s Law states that the net electric flux through any closed surface is equal to the total charge enclosed by that surface:  D  dS  Qenc Point form of Gauss’s Law is   D  V 177
  • 178. SUMMARY (5) • The electric potential difference Vab between a pair of points a and b in an electric field is given by: b Vba    E  dL  Vb  Va a Where Va and Vb are the electrostatics potentials at a and b respectively. For a distribution of charge in the vicinity of the origin, where a zero reference voltage is taken at infinite radius: dQ V  4r 178
  • 179. SUMMARY (6) • E is related to V by the gradient equation: E  V Which for Cartesian coordinates is: V V V V  ax  ay  az x y z • The conditions for the fields at the boundary between a pair of dielectrics is given by: ET 1  ET 2 and a 21  D1  D2    S 179
  • 180. SUMMARY (7) Where ET1 and ET2 are the electric field components tangential to the boundary, a21 is a unit vector from medium 2 to 1 and ρS is the surface charge at the boundary. If no surface charge is present, the components of D normal to the boundary are equal: D N1  D N 2 At the boundary between a conductor and a dielectric, the conditions are: ET  0 and DN  S 180
  • 181. SUMMARY (8) • Poisson’s equation is: V  V  2  Where the Laplacian of V in Cartesian coordinates is given by: V V V 2 2 2 V 2  2  2 2 x y z In a charge free medium, Poisson’s equation reduces to Laplace’s equation  V 0 2 181
  • 182. SUMMARY (9) • Capacitance is a measure of charge storage capability and is given by: Q C V For coaxial cable: L 2L Vab  ln b a  So, C 2 ln b a  For two concentric spheres: Q 1 1 4 Vab     So, C 4  a b  1 a 1 b 182