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File: Calculus Pdf 169292 | 45302ef9b328a6c32869077580cd685d Mit18 02sc Supprobsol6
6 vector integral calculus in space 6a vector fields in space 6a 1 a the vectors are all unit vectors pointing radially outward b the vector at p has its ...

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                                                        6.  Vector Integral Calculus in Space 
                                                                   6A.  Vector Fields in Space 
                                6A-1  a)  the  vectors  are  all  unit  vectors,  pointing  radially  outward. 
                                       b)  the  vector  at  P  has  its  head  on  the  y-axis,  and  is  perpendicular  to  it 
                                         1 
                                6A-2  2(−xi −yj −z k ) 
                                6A-3  ω(−z j + yk ) 
                                6A-4  A  vector  field  F =  M  i +  N  j +  P  k  is  parallel  to  the  plane  3x  − 4y +  z  = 2 if it is 
                                perpendicular  to  the  normal  vector  to  the  plane,  3i − 4j +  k :  the  condition  on  M;N;P 
                                therefore is 3M  − 4N  +  P  = 0,  or  P  = 4N  − 3M. 
                                   The most general  such  field is therefore  F =  M  i +N  j +(4N  −3M)k ,  where  M  and  N 
                                are  functions  of  x;y;z. 
                                                                6B.  Surface Integrals and Flux 
                                6B-1      Wehave  n =  xi + yj + z k ;  therefore  F· n =  a. 
                                                                     a 
                                                          �  �                                        3 
                                   Flux through  S  =         S  F ·  n dS  =  a(area  of S) = 4π a  :
                                6B-2      Since    k  is  parallel  to  the  surface,  the  field  is  everywhere  tangent  to  the  cylinder, 
                                hence  the  flux  is  0.                                                                                               1 
                                           i +  j +  k                                                             1                                          n 
                                6B-3           √          is  a  normal  vector  to  the  plane,  so  F ·  n =  √ .                                2 
                                                  3                                                                 3                                     S 
                                                                                                              √ √ √                                               1 
                                                                                    1                       1         3 
                                                              area  of  region      2(base)(height)         2( 2)(  2     2)     1              1 
                                   Therefore,       flux  =          √           =          √            =         √           =  2 .
                                                                       3                     3                      3
                                                xi +  yj +  z  k                 y2 
                                6B-4      n =           a          ;   F·  n =  a  :     Calculating  in  spherical  coordinates, 
                                flux  =  � �     y2 dS  =  1  �  π  �  π  a 4 sin3 φ sin2 θ dφdθ  =  a 3 �  π  �  π  sin3 φsin2 θ dφdθ. 
                                             S  a          a   0    0                                   0    0 
                                   Inner  integral:    sin2 θ(−cosφ+  1 cos3 φ)�π  =  4 sin2 θ;
                                                                           3           0       3 
                                                        4  3 1       1         �π       2   3 
                                   Outer integral:      3a (2θ − 4 sin2θ) 0  =  3πa .
                                                                                        1 
                                                                               2                                                                                                               E.  18.02 EXERCISES 
                                                                                                                          i +  j +  k                                                              z 
                                                                               6B-5                      n =                         √3                     ;         F ·  n =  √3 . 
                                                                                                                � �                z         dxdy                              1       � �                                               dxdy                        �  1 �  1−y 
                                                                                        flux  =                                  √ |n· k |  = √                                                       (1 −x −y)                                  √ =                                               (1 −x −y)dxdy. 
                                                                                                                          S           3                                           3              S                                       1= 3                            0          0 
                                                                                                                                                                1  2                        �1−y                     1                        2                                                                                                                   1 
                                                                                        Inner  integral:                                  =  x  − 2x −xy  0                                                 =  2(1 −y) :                                                                                                                                                                     n 
                                                                                                                                                    �  1  1                                                     1               1                                  �1               1 
                                                                                        Outer  integral:                                    =                        (1 −y)2dy  =                                     · −             ·  (1 − y)3                           = :                                                                                                 S 
                                                                                                                                                        0 2                                                     2               3                                      0            6 
                                                                                                                                                                                                                                                                                                                                                                                                       1 
                                                                                                                                                                                                                                                                                                                                                 1                        x+y=1 
                                                                               6B-6                      z  =  f(x;y) =  x2 +  y2  (a paraboloid).                                                                                       By (13)  in Notes V9, 
                                                                                                                                                                             dS = (−2xi −2yj +  k )dxdy. 
                                                                               (This points generally “up”, since the  k component is positive.)  Since  F =  xi +yj +z k , 
                                                                                                                                                              �  � S F ·  dS = �  � R (−2x 2 − 2y 2 +  z)dxdy                                                                                                                                                                 ,
                                                                               where  R  is  the  interior  of  the  unit  circle  in  the  xy-plane,  i.e.,  the  projection  of  S  onto  the 
                                                                                                                                                         2               2 
                                                                               xy-plane).  Since  z  =  x +  y ,  the  above  integral 
                                                                                        =  − � �  (x 2 +  y 2)dxdy  =  − �  2π  �  1 r 2 ·  r dr dθ  =  −2π ·  1  =  − π  : 
                                                                                                                R                                                                      0              0                                                                    4                    2 
                                                                               The  answer  is  negative  since  the  positive  direction  for  flux  is  that  of  n,  which  here  points 
                                                                               into  the  inside  of  the  paraboloidal  cup,  whereas  the  flow  xi +  y j +  z  k  is generally from 
                                                                               the  inside  toward  the  outside  of  the  cup,  i.e.,  in  the  opposite  direction. 
                                                                                                                                                                                                                 xi +  yj                                                       y2 
                                                                               6B-8                      On  the  cylindrical  surface,  n =                                                                                a               ;          F·  n =  a  : 
                                                                               In  cylindrical  coordinates,  since  y  =  asinθ,  this  gives  us  F · dS =  F· n dS  =  a2 sin2 θ dz dθ.
                                                                               Flux  =  �  π=2  �  k  a 2 sin2 θ dz dθ  =  a 2h �  π=2  sin2 θ dθ  =  a 2h� θ  −  sin2θ�π=2                                                                                                                                                             = π a2h  : 
                                                                                                              −π=2 0                                                                                          −π=2                                                                2                    4               −π=2                      2 
                                                                               6B-12                          Since the distance from  a point (x;y;0)  up  to  the  hemispherical  surface  is  z, 
                                                                                                                                                                                                                                                   �� S  z dS 
                                                                                                                                                                                average  distance  =                                                 �� S  dS  : 
                                                                               In  spherical  coordinates,  � �  z dS  =  �  2π  �  π=2 acosφ ·  a 2 sinφdφdθ. 
                                                                                                                                                                           S                               0               0 
                                                                                                                         3 �  π=2                                                                    3 sin2 φ �π=2                                     a3                                                         a3 �  2π                                         3 
                                                                                        Inner:  =  a                                            sinφcosφdφ  =  a  (                                                2                          =  2  :                            Outer:  =  2                                             dθ  =  πa : 
                                                                                                                                 0                                                                                                0                                                                                            0
                                                                               Finally,  �  �                              dS  =  area  of  hemisphere                                                           =  2πa2,  so  average  distance  =  πa3  =  a : 
                                                                                                                                                                                                                                                                                                                         2πa2                      2
                                                                                                                     S 
                                                                          6.   VECTOR INTEGRAL CALCULUS IN SPACE                                                                3 
                                                                                   6C.  Divergence Theorem 
                                      6C-1a          div  F =  Mx  +  Ny  +  Pz  = 2xy  +  x  +  x  = 2x(y + 1): 
                                      6C-2         Using  the  product  and  chain  rules  for  the  first,  symmetry  for  the  others, 
                                                 n               n−1 x            n         n               n−1 y            n         n              n−1 z            n
                                              (ρ x)x  =  nρ            ρ x  +  ρ ;       (ρ y)y  =  nρ            ρ y +  ρ ;        (ρ z)z  =  nρ            ρ  z  +  ρ ;
                                                                                                          x2 +  y2 +  z2 
                                                                                                    n−1                                 n         n
                                      adding  these  three,  we  get               div  F =  nρ                    ρ           + 3ρ =  ρ (n +3): 
                                           Therefore,  div  F = 0  ⇔  n  =  −3. 
                                      6C-3  Evaluating  the  triple  integral  first,  we  have  div  F = 3,  therefore 
                                                                       � � �                                                2     3           3 
                                                                                 div  F dV  = 3(vol.of  D) = 3  3πa = 2πa : 
                                                                              D 
                                      To  evaluate  the  double  integral  over  the  closed  surface  S1 +  S2,  the  normal  vectors  are: 
                                                          n =  xi + yj + z k                 (hemisphere S );                 n =  −k  (disc S ); 
                                                            1                a                                    1             2                         2
                                      using  these,  the  surface  integral  for  the  flux  through  S  is 
                                                           � �     F ·  dS =  � �         x2 +  y2 +  z2 dS  +  � �            −zdS  =  � �          adS; 
                                                                S                    S1           a                        S2                    S1 
                                                 2      2      2       2       2 
                                      since  x +y +z =  ρ =  a on  S1,  and  z  = 0  on  S2.  So  the  value  of  the  surface  integral  is 
                                                                                                                    2             3 
                                                                                    a(area  of S1)= a(2πa ) = 2πa , 
                                      which  agrees  with  the  triple  integral  above.                                                                                1
                                      6C-5         The  divergence  theorem  says                   �  � S F ·  dS =  � � � D  div  F dV:                                              1 
                                           Here div  F = 1,  so that the  right-hand integral is just the  volume  of  the 
                                      tetrahedron,  which  is  1(base)(height)=  1(1)(1) =  1.                                                                   1
                                                                        3                           3  2            6 
                                      6C-6         The  divergence  theorem  says                   �  � S F ·  dS =  � � � D  div  F dV: 
                                           Here div  F =  1,  so  the  right-hand  integral  is  the  volume  of  the  solid  cone,  which  has 
                                      height  1  and  base  radius  1;  its  volume  is  1(base)(height)= π=3. 
                                                                                                      3 
                                      6C-7a  Evaluating  the  triple  integral  first,  over  the  cylindrical  solid  D,  we  have 
                                                                           div  F = 2x  +  x  = 3x;                � � � D  3xdV  = 0, 
                                      since  the  solid  is  symmetric  with  respect  to  the  yz-plane.  (Physically,  assuming the  density 
                                      is  1,  the  integral  has  the  value  x¯(mass  of  D),  where  x ¯ is  the  x-coordinate  of  the  center  of 
                                      mass;  this  must  be  in  the  yz  plane  since  the  solid  is  symmetric  with  respect  to  this  plane.) 
                                           To  evaluate  the  double  integral,  note  that  F has  no  k -component,  so  there  is  no  flux 
                                      across  the  two  disc-like  ends  of  the  solid.  To  find  the  flux  across  the  cylindrical  side, 
                                                                n =  xi +  yj ;             F·  n =  x3 +  xy2 =  x3 +  x(1 − x2) =  x; 
                                      4                                                    E.  18.02 EXERCISES 
                                      since  the  cylinder  has  radius  1  and  equation  x2 +  y2 = 1.  Thus 
                                                                   � �     xdS  =  �  2π  �  1 cosθ dz dθ  =  �  2π  cosθ dθ  = 0: 
                                                                        S               0      0                        0 
                                      6C-8        a)   Reorient  the  lower  hemisphere  S2  by  reversing  its  normal  vector;  call  the  reori-
                                      ented  surface  S′ .  Then  S  =  S1 +  S′  is  a  closed  surface,  with  the  normal  vector  pointing 
                                                             2                              2 
                                      outward  everywhere,  so  by  the  divergence  theorem, 
                                                          �  �                 �  �                  �  �                  � � �                                              S 
                                                                  F ·  dS =             F ·  dS +            F ·  dS =              div  F dV  = 0;                            1 
                                                               S                    S1                   S′                      D 
                                                                                                           2 
                                      since by  hypothesis div  F = 0.  The  above  shows 
                                                                        �  �                     �  �                  �  �                                                  S 
                                                                                                                                                                              2 
                                                                             S F ·dS =  −             S′  F · dS =          S F ·  dS;
                                                                               1                        2                     2 
                                      since  reversing  the  orientation  of  a  surface  changes  the  sign  of  the  flux  through  it. 
                                          b)  The  same  statement  holds  if  S1  and  S2  are  two  oriented  surfaces  having  the  same 
                                      boundary  curve,  but  not  intersecting  anywhere  else,  and  oriented  so  that  S1 and  S′  (i.e., S2 
                                                                                                                                                                2 
                                      with  its  orientation  reversed)  together  make  up  a  closed  surface  S  with  outward-pointing 
                                      normal. 
                                      6C-10         If div  F = 0,  then  for  any  closed  surface  S,  we  have  by  the  divergence  theorem 
                                                                                �  � S F ·  dS =  � � � D  div  F dV  = 0. 
                                          Conversely:  �  � S  F · dS =  0  for  every  closed  surface  S                   ⇒      div  F = 0. 
                                      For  suppose  there  were  a  point  P0  at  which  (div  F)0  6=  0  —  say  (div  F)0  >  0.                                  Then 
                                      by  continuity,  div  F >  0  in  a  very  small  spherical  ball  D  surrounding  P0,  so  that  by  the 
                                      divergence theorem (S  is  the  surface  of  the  ball  D), 
                                                                              �  � S F ·  dS =  � � � D  div  F dV           >     0. 
                                      But  this  contradicts  our  hypothesis  that  �  � S  F ·  dS = 0  for  every  closed  surface  S.
                                      6C-11         flux  of  F =  �  � S F ·  dn =  � � � D  div  F dV  = � � � D  3dV  = 3(vol.  of  D):
                                                                               6D.  Line Integrals in Space 
                                      6D-1        a)    C  :    x  =  t;  dx  =  dt;     y  =  t2;  dy  = 2tdt;        z  =  t3;  dz  = 3t2 dt; 
                                              �                                     �  1  2            3                   2 
                                                C  y dx +  z dy  − xdz  =             0  (t )dt +  t (2tdt) − t(3t dt) 
                                                                           �  1                                                       �1 
                                                                                   2       4       3            t3      2t5      3t4            1     2      3            1 
                                                                      =      0 (t +2t −3t )dt  =  3 + 5  −  4                          0  =  3 + 5  − 4  =  −60 :
                                          b)   C  :    x  =  t;  y  =  t;  z  =  t;     � ydx+ zdy −xdz  =  �  1 tdt  =  1 : 
                                                                                          C                                     0               2
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...Vector integral calculus in space a fields the vectors are all unit pointing radially outward b at p has its head on y axis and is perpendicular to it xi yj z k j yk eld f m i n parallel plane x if normal condition therefore or most general such where functions of surface integrals flux wehave through s ds area since everywhere tangent cylinder hence ux so region base height calculating spherical coordinates sin d inner cos outer e exercises dxdy xy dy paraboloid by notes v this points generally up component positive r interior circle projection onto above dr...

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