Page 190 - Schaum's Outline of Theory and Problems of Advanced Calculus
P. 190

CHAP. 7]                             VECTORS                                    181

                                                  dT       dB        dN
                                                     ¼  N;    ¼  N;     ¼  B    T
                                                   ds       ds        ds
                           These are called the Frenet-Serret formulas and are of fundamental importance in differential geometry.In
                           these formulas   is called the curvature,   is called the torsion; and the reciprocals of these,   ¼ 1=  and
                             ¼ 1= ,are called the radius of curvature and radius of torsion, respectively.

                     7.96.  (a)Prove that the radius of curvature at any point of the plane curve y ¼ f ðxÞ; z ¼ 0 where f ðxÞ is differ-
                           entiable, is given by

                                                                   02 3=2
                                                                ð1 þ y Þ
                                                             ¼
                                                                  y  00

                           (b)Find the radius of curvature at the point ð =2; 1; 0Þ of the curve y ¼ sin x; z ¼ 0.
                                    ffiffiffi
                                   p
                           Ans.  (b)2 2
                     7.97.  Prove that the acceleration of a particle along a space curve is given respectively in  (a)cylindrical,
                           (b)spherical coordinates by
                                                     ð €       _   Þe   þð  €   þ 2 _   _  z
                                                           2




                                                                       Þe   þ € ze z
                                             2
                                      2
                                                             2
                                          2



                                                                          r


                                                        r



                                  r

                                  ð€ r   r _     r _   sin  Þe r þðr €   þ 2_ r _   r _   sin   cos  Þe   þð2_ r _ sin   þ 2r _   _ cos   þ r €   sin  Þe
                           where dots denote time derivatives and e   ; e   ; e z ; e r ; e   ; e   are unit vectors in the directions of increasing
                            ;  ; z; r; ; , respectively.
                     7.98.  Let E and H be two vectors assumed to have continuous partial derivatives (of second order at least) with
                           respect to position and time.  Suppose further that E and H satisfy the equations
                                                                       1 @H           1 @E
                                         r  E ¼ 0;  r  H ¼ 0;              ;
                                                                       c @t    r  H ¼  c @t           ð1Þ
                                                               r  E ¼
                           prove that E and H satisfy the equation
                                                                    2
                                                                  1 @
                                                             2
                                                            r   ¼  2  2                               ð2Þ
                                                                 c @t
                           where   is a generic meaning, and in particular can represent any component of E or H.
                           [The vectors E and H are called electric and magnetic field vectors in electromagnetic theory. Equations (1)
                           are a special case of Maxwell’s equations.  The result (2) led Maxwell to the conclusion that light was an
                           electromagnetic phenomena.  The constant c is the velocity of light.]
                     7.99.  Use the relations in Problem 7.98 to show that
                                                     @    2   2
                                                       1
                                                      f ðE þ H Þg þ cr  ðE   HÞ¼ 0
                                                     @t  2
                     7.100. Let A 1 ; A 2 ; A 3 be the components of vector A in an xyz rectangular coordinate system with unit vectors
                           i 1 ; i 2 ; i 3 (the usual i; j; k vectors), and A 1 ; A 2 ; A 3 the components of A in an x y z rectangular coordinate
                                                          0
                                                                                   0 0 0
                                                       0
                                                             0
                           system which has the same origin as the xyz system but is rotated with respect to it and has the unit vectors
                           i 1 ; i 2 ; i 3 .  Prove that the following relations (often called invariance relations) must hold:
                             0
                           0
                               0
                                                          0    0     0   n ¼ 1; 2; 3
                                                  A n ¼ l 1n A 1 þ l 2n A 2 þ l 3n A 3
                           where i m   i n ¼ l mn .
                                0
                     7.101. If A is the vector of Problem 7.100, prove that the divergence of A, i.e., r  A,isaninvariant (often called a
                           scalar invariant), i.e., prove that
                                                      0    0   0
                                                    @A 1  @A 2  @A 3  @A 1  @A 2  @A 3
                                                    @x  0  þ  @y  0  þ  @z  0  ¼  @x  þ  @y  þ  @z
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