PH 314 Homework Fall 2003


Set 1 Due Monday September 8, 2003
 

Set 2 Due Friday September 12, 2003 Set 3 Due Thursday September 18, 2003 Set 4 Due Friday September 26, 2003 Set 5 Due Friday October 3, 2003 Set 6 Due Tuesday October 14 2003
 
1. Turn in the dimensions of your homemade coupled pendulum setup. Sketch the setup. Say what you used for masses. Report the pendulum frequency and how it compares to theory. Report the time for energy exchange between masses and report how it compares to theory.

2. Work out the tabletop problem with a string length of 2.5 m, and a hanging 2.0-kg mass and a 1.0-kg mass on the tabletop. Let the initial angle be zero, the initial rdot = +0.6 m/s, initial r = 1.0 m, and initial thetadot = 0.5 rad/sec. Calculate the max and min r values theoretically, solving a numerical equation for r.

3. Do an RK2 simulation of this problem, and obtain numerical values of rmax and rmin. Email me the spreadsheet.
 

Set 7 Due Tuesday October 21, 2003
1.Turn in your analysis of the coupled oscillation problem. M1 = 0.2178 kg, M2 = 0.2839 kg,  freq with m2 and spring: 0.52 Hz. Find the oscillation frequencies of the two modes, and determine the amplitude ratios for each mode.
2. Show that the total energy E in an elliptical orbit is -k/(2a), where k is the gravitational coefficient, and a is the semi-major axis of the ellipse. [Hint: look at r_max and r_min.]
3. Then show that the semi-minor axis is given by b = L/sqrt(2 mu |E|). [For this, you may use the result of #2. The numerator of this expression is the angular momentum, L, not 1.]
Set 8 Due Thursday October 30, 2003
1,2.  Create a spreadsheet for the inverted driven pendulum. Let the pendulum be a rod of length 0.30 m, driven at one end. Launch it a 0.1 radians and find a; driving frequency and amplitude for it to be stable inverted. Measure the period of the stable motion. Calculate the period from the formula, and compare to your simulation.
3.Create a spreadsheet for a Foucault pendulum of length 20.0 m.  In order to see anything in a few swings, you will have to greatly increase the Earth's rotational rate. Your graph should show rotation of the plane of oscillation. Calculate the rotation rate, and measure it from your simulation.
Set 9 Due Thursday November 6, 2003

1. Model a water molecule having a mass 16 u at the origin, a mass u a distance L along the x-axis, and a mass u at a distance L from the
origin at an angle of 110° fromthe x-axis.
a) Calculate the CM of this system.
b) Calculate the inertia tensor for the water molecule in a coordinate system centered on the molecule's CM, with axes parallel to the x and y
axes.
2. Perform a similarity transformation on the inertia tensor by going to a coordinate system rotated by 55°. This should result in a diagonal tensor,
giving the principal moments of the water molecule. (The principal axes are supposed to lie along the symmetry directions of the body.)
3. The fractional difference in the Earth's moments of inertia is about 1/300, the Earth being slightly flattened at the poles. Use this
information to calculate the rate at which the Earth's angular velocity vector precesses (wobbles) about the direction of the Earth's
rotational angular momentum (you could say this is the rotational North pole)
4. Consider a uniform rectangular plate of sides a and b, which is forced to rotate about an axis through a diagonal of the plate with an
angular velocity W.
a) Show that the principal moments of inertia of this plate are (M/12) a^2, (M/12)b^2, and (M/12)(a^2+b^2).
b) Identify the direction of torque needed to rotate the plate. (Give this in relation to the plane of the plate.)
c) Find the magnitude of the torque, in terms of M, a, b, and W.
5. Calculate the landing point for a projectile launched (ignore air resistance) from the N pole 1500 km due South at an angle of 45 degrees. Use the coriolis correction to find its displacement, to first order in the angular velocity of the Earth.. (You can also independently check this.)

Friday November 14, 2003 (optional)

1. Start with the lagrangian function for the two-body problem 8.20, and obtain the Hamiltonian, and the two hamiltonian equations of motion.
2. For the football pictures, write out the relations for the moments about 1 and 3 axes, use theta = 22 degrees, use 'measured' phidot, and psidot, and obtain a numerical estimate of  I_12 / I_3.