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Reading:

Read B & O Sections 2.4 -- 2.6; Griffiths Chapter 1 -- 1.4; KB 361 lecture notes 11 -- 15.
Problems for Review:
\

  1. Use B & O problem 2-15 for the definition of cylindrical and spherical coordinates (you may also wish to review Griffiths section 1.4).

    1. Calculate a particle's velocity and acceleration in cylindrical coordinates.
    2. Given the particle velocity

      displaymath147

      in spherical coordinates, derive the particle acceleration

      eqnarray27

  2. A natural use of cylindrical coordinates might be to describe motion on the surface of a cylinder, in the absence of gravity.
    1. What force must be applied to keep a particle's motion entirely on the cylinder (i. e. to keep tex2html_wrap_inline149 constant)?
    2. For constant tex2html_wrap_inline149 , with no forces applied in the z and tex2html_wrap_inline155 directions, what are the solutions for the particle's motion? Find their form in terms of t, and sketch them.
  3. Griffiths Example 1.3 (p 15).
    1. B & O 2-15.
    2. For a potential dependent only on tex2html_wrap_inline149 in cylindrical coordinates, sketch the equipotential surfaces, and the local gradient and force directions. Similarly, for a potential dependent only on r in spherical coordinates, sketch the equipotential surfaces, and the local gradient and force directions.
  4. Consider the potential energy tex2html_wrap_inline163 . Find
    1. The direction in which the potential energy is increasing most rapidly at tex2html_wrap_inline165 and the magnitude of the rate of increase. What then is the force at tex2html_wrap_inline165 ?
    2. The rate of change of potential energy with distance at tex2html_wrap_inline170 in the direction tex2html_wrap_inline172 . What is the component of force in this direction?
    3. The direction and magnitude of the force at tex2html_wrap_inline173 .
    4. The magnitude of the force at x = -1, any y.
  5. B & O 2-11.
    1. Griffiths Example 1.5 (p. 19).
    2. For tex2html_wrap_inline179 and tex2html_wrap_inline181 in Griffiths Example 1.5, find a closed curve C for which the line integral tex2html_wrap_inline185 is nonzero, and evaluate the line integral.
    1. Griffiths Example 1.6 (p. 25).
    2. For tex2html_wrap_inline187 in Griffiths Example 1.6, calculate tex2html_wrap_inline189 . How is this consistent with your answer to (a)?

Problems to Solve:
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  1. Recall that in spherical coordinates, the position vector has the following Cartesian components:

    displaymath191

    where we have used the spherical coordinate unit vectors in Cartesian components

    eqnarray70

    1. By differentiating, show that the particle velocity is

      displaymath193

      Identify velocity components tex2html_wrap_inline195 in the tex2html_wrap_inline197 directions respectively.

    2. Show that your expression for (a) is consistent with the infinitesimal displacement vector

      displaymath199

      derived geometrically in Griffiths equation (1.68).

    1. Consider a potential energy tex2html_wrap_inline201 , where V is in joules and x,y are in meters. Sketch an equipotential map, showing the contours V = 32, 24, 16, 8, 0 J.
    2. Sketch in the local gradient field on your equipotential map.
    3. If you start at the point (3,2) and proceed in the direction tex2html_wrap_inline211 , is the potential increasing or decreasing, and at what rate? What is the component of force in this direction?
  2. Griffiths Problem 1.27.
  3. Treating the vector functions in Griffiths problem 1.15 as forces tex2html_wrap_inline213 for each
    1. Calculate the curl.
    2. If the force is conservative, derive a potential V giving the force; if the force is not conservative, find a closed curve C for which the work integral tex2html_wrap_inline219 is nonzero, and evaluate the work integral.
  4. For the force tex2html_wrap_inline221 ,
    1. Evaluate tex2html_wrap_inline223 .
    2. Evaluate tex2html_wrap_inline219 , for the curve C shown in Griffiths Figure 1.34 (p. 36).



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Next: About this document

Katherine Benson
Mon Feb 25 10:16:53 EST 2002