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    1. For velocity-dependent force, we can use the integral equation

      displaymath171

      Here tex2html_wrap_inline173 and F(v') = -bv' so the integral gives

      displaymath177

      which we invert to obtain

      displaymath179

      Integrating and applying the initial condition x(0) = 0 gives

      displaymath183

      We can solve for tex2html_wrap_inline185 in terms of x,

      displaymath189

      to give v(x):

      displaymath193

    2. As in review problem 2b, we can rearrange Newton's second law to directly relate v and x, by using the chain rule for the assumed solution v(x):

      displaymath201

      This gives for Newton's second law, for velocity-dependent force,

      displaymath203

      or

      displaymath205

      (Note that the integrand really should be written in terms of dummy variables x', v', as position and velocity are varying up to the final values x and v.) Plugging in F = -bv gives

      displaymath215

      since tex2html_wrap_inline217 . This confirms our result in (a),

      displaymath193

    3. Note that tex2html_wrap_inline221 comes to rest in the finite distance tex2html_wrap_inline223 . Once it comes to rest, the force -bv vanishes, so that the particle remains stopped.
  1. We use the same coordinate system as in section 1.4; that is, x=0 at the earth's surface and increases upward, so that the skydiver feels force

    displaymath229

    (gravity downward, air resistance up).

    The skydiver starts at t=0 at altitude x = h and velocity tex2html_wrap_inline235 and falls, reaching altitude x and velocity v at time t. Thus at time t he has fallen through distance h-x, and we're asked to find velocity as a function of this distance fallen h-x.

    To do this we relate the integrand dx to a v-dependent integrand and integrate. As in problem 1, Newton's second law is rewritten in terms of v, x to give

    displaymath203

    or

    displaymath205

    With the limits above, and tex2html_wrap_inline259 , we have

    displaymath261

    or

    eqnarray63

    Let's call the distance fallen d, so d = h-x; we're asked to invert this relation to find v(d). Multiplying both sides by 2c/m then exponentiating gives

    displaymath271

    Further rearranging to solve for v gives

    displaymath275

    or

    displaymath277

    noting the terminal velocity tex2html_wrap_inline279 .

    This gives the general relation between velocity v and distance fallen d. Specifically, tex2html_wrap_inline285 when

    displaymath287

    Taking tex2html_wrap_inline289 of both sides and rearranging,

    displaymath291

    Note tex2html_wrap_inline293 which here gives, since tex2html_wrap_inline295 and tex2html_wrap_inline297 , m/c = 297.6 m. Thus

    displaymath301

    1. Note that the table's normal force opposes the force of gravity for the length l-x of cable which remains on the table. Gravity acts unopposed on the hanging length x. This portion has mass mx/l, so the total force pulling the cable over the table edge is F = mgx/l (acting to increase the hanging length x). Newton II thus gives

      displaymath313

    2. The requested methods again use tex2html_wrap_inline315 to rewrite Newton II as an equation relating v and x-dependent integrands:

      displaymath317

      We integrate both sides for our motion, with F(x) = mgx/l and initial tex2html_wrap_inline321 , v = 0. This gives (after cancelling factors of m)

      eqnarray100

    3. We know that dx/dt = v(x), so dt = dx/v(x), an equation between integrands each depending only on one variable, which we may integrate between the endpoints of our motion:

      displaymath331

      Doing the integrals gives

      eqnarray124

      This is a rather ugly relationship, one not easily inverted to find x(t). It could be made a little bit nicer,

      displaymath335

      but remains a bit baffling.

    4. We can confirm that tex2html_wrap_inline337 , a solution found easily by other methods, obeys the initial conditions and our result of part c. First, initial conditions:

      displaymath339

      do have tex2html_wrap_inline341 as needed. Note that

      eqnarray145

      using the exponential definitions of cosh and sinh,

      displaymath343

      This confirms our result of part c. Thus these closed integral methods remain consistent with ODE approaches, even when they're not very helpful.




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Next: About this document

Katherine Benson
Tue Jan 29 02:42:00 EST 2002