.
Physics 271: Advanced Honors Physics I
Recitations
Fall 2017
Week-by-week summary of recitation activities
Week 1: df/dx=f and other separable differential equations,
1D constant acceleration review and practice (including diagnosis of
need to review unit conversions and/or sig figs), diagrammatic
derivation of transformation of coordinates between two coordinate
systems with different origins. The sheet
of practice problems and answers/comments.
Week 1 to do: finish the in-class problems (answers will be posted
Friday after the last recitation). If you discovered that you are
rusty on (or never properly learned) unit conversions and/or sig
figs, study the links in the Week 1 Useful Resources. Do homework 1
to hand in at Monday lecture (start working on it right away if you
have not already done so).
Week 2: review projectile motion, uniform circular motion,
relative motion in 1D, normal force, string tension force,
constraints in problems with pulleys. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #1
#2
#3
#4
#5.
If you have difficulties, review on your own or come to office hours
before this week's recitation. In recitation, we reviewed the
conical pendulum, talked about choosing reference frames (examples
in 1D), rolling without slipping, force exerted by a string on a
pulley, and practiced identifying constraints in dynamics problems.
Week 2 to do: if you have not seen it before (or even if you have),
watch the short film "Frames of Reference" (links in the Useful
Resources section) This post-Sputnik (1960) geeky classic is
arguably the most perfect physics film ever made. To me, it's like
Casablanca -- it gets better every time I watch it.
Week 3: review static and kinetic friction, drag force,
simple harmonic motion, gravitational shell theorem and
gravitational orbits. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #1
#2
#3
#4
#5.
If you have difficulties, review on your own or come to office
hours before this week's recitation. In recitation, we reviewed
drawing force diagrams in systems with static or kinetic friction,
two objects of similar mass circularly orbiting around each other,
and the motion of a string with mass on a frictionless pulley.
Week 3 to do: students in the Thursday 12:15 recitation should
check out the rule for deciding which direction to draw the
friction force which can be found in the problem solving toolbox
below. Go over your notes for the motion of a string with mass on
a frictionless pulley and fill in the remaining steps to find the
magnitude of the acceleration of the string. If you need to
refresh your memory or learn Taylor series (as used in the
recitation discussion of the rope on the pulley), study Notes 1.2
and 1.3 on pp. 37-38 of KK. For a mathematical review, see the
link in Useful Resources to the relevant pages (Sec 10.7 in 2nd
ed) from the calculus text by Rogawski which is often used in Math
151/152/251.
Week 4: review Chapters 1-3 for in-class exam Monday
October 2. An important reminder: take some time to prepare your
two-sided note sheet -- this will help you study and may come in
handy during the exam. We listed some of the topics that are "fair
game" for the exam: reference frames (see Problem 1 of HW2), polar
coordinates (you can be sure that you will need to know
acceleration vector in polar coordinates!), Newton's law problems
(define coordinates, constraints, drawing force diagrams (real
physical forces only!), Newton's 2nd law, solving the equations,
making sure they are reasonable, checking that the solution is
reasonable), knowing when the friction is static and when it is
kinetic (eg. "just about to slip"), remember that the static
friction force is not always mu N, how to figure out the direction
of the friction force when you are drawing the force diagram, know
how to approach max-min problems, solve separable differential
equations and determine the coefficients in the solution from
initial conditions. The full list of problems that we discussed in
at least one of the recitations: KK 2.15 "disk with a catch" (to
review motion and acceleration in polar coordinates), KK
2.8 solution "two masses and two pulleys" (to review how
to write constraint equations), KK 2.12 "painter on scaffold" (to
review force diagrams and Newton's THIRD Law), and KK 3.17
"turning car" (circular motion and friction). Scanned solutions
for these 4 problems coming...
Week 5: review center of mass, momentum, conservation of
momentum, impulse, rocket motion. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #5
#11
#25
#39
#77
#79.
We discussed Problem 4.5 (acrobat and monkey), rederived the
rocket equation keeping open the possibility of various M(t) and
external forces on the rocket, derived a similar general equation
for freight cars and sand and applied it to various
freight-car-and-sand problems. YOU ARE READY AND STRONGLY
ENCOURAGED TO DO THE FOLLOWING 7 PROBLEMS FROM HW4 FOR THIS MONDAY
(10/9): 4.1, 4.4, 4.7, 4.9, 4.10, 4.15, 4.16. A few helpful
comments and pointers, most of which we discussed in recitation,
are as follows:
KK 4.4. Treat the rocket as a projectile that's launched at a
particular speed and angle from the launch point.
KK 4.7 Divide the motion into two time intervals and solve in each
time interval separately using an appropriate approach.
KK 4.7 You will need to understand the motion of the center of
mass
(though
in fact not the motions of the individual masses, though it is
good more generally for you to understand those too) in the
Push-Me-Pull-You in Example 4.7. A link to a video demo of the Push-Me-Pull-You
is in the Useful Resources below.
KK 4.9 Take the sled's initial mass as M_0 (a notation that will
reduce confusion with the function M(t))
KK 4.16 I suggest you solve this problem using the techniques from
Chapter 3 (that is, don't try to use momentum, as the external
forces exerted by the corner of the table on the string are not
obvious).
Week 6: review flow of momentum, work done by various
forces in 1D, 2D and 3D, work-kinetic energy theorem. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #29
#8
#17
#27
#37
#39.
Week 7: review power, small oscillations about
equilibrium and elastic and inelastic collisions in 1D and 2D. DO
THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #45
#11
#83
#50
#61
#71.
IMPORTANT: in inelastic collisions, momentum is conserved but
mechanical energy is NOT! The force exerted on object A by object
B is equal and opposite to the force exerted on object B by object
A (Newton's 3rd law) but the work done by object B on object A is
not necessarily equal and opposite to the work done by object A on
object B for nonconservative forces such as friction.
Week 8: review of moments of inertia, rotational
kinetic energy, torque, work done by torque, conservation of
angular momentum. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #35
#45
#59
#47
#53
#7.
The geometry of the bug and ring problem in the HW is that the ring
is lying flat on the table (x-y coordinate system). It has a hole
drilled for the pivot and rotates around the pivot point: define the
angle of the ring's position to be the angle made with the x axis by
the vector from the pivot to the center of the ring.
Tip: for the falling stick problem in 7.14, the force applied at A
is only to establish the initial condition for the falling stick --
that it is horizontal and not moving at t=0.
Tip: for the small oscillation problems 7.16 and 7.17, you can
either compute the restoring torque for a small displacement OR
expand the potential energy to quadratic order in the small
displacement amplitude. For the small oscillation problem 7.9, you
have no choice because of the friction forces -- you have to compute
the restoring force for a small displacement.
In Problem 7.9, treat the bar as being infinitesimally thin.
Week 9: review of rolling without slipping,
conservation of energy in rolling problems, the yo-yo. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #2
#3 #11
#18
#51
#83.
*Most of the HW problems are best tackled by the extended Newton's
law approach. First draw a diagram and identify the forces. Write
the constraints (eg the rolling without slipping condition),
Newton's 2nd law for the center of mass motion, and the torque
equation, and solve. The problems involving collisions need to be
solved using conservation laws (momentum, angular momentum, and
mechanical energy -- it's up to you to recognize which quantities
are conserved in each problem) -- the forces acting during the
collision are too complicated, which rules out the Newton's law
approach. For conservation law problems, draw detailed before and
after diagrams.
*7.34 is another small oscillation problem (see the tip for
week 8). All small oscillations (of which we have already done many
and will do many more) should be approached the same way. Draw a
diagram of the equilibrium state and identify the "small
displacement" quantity (it might be an angle). Then, if the forces
in the problem are conservative, you have a choice: you can either
compute the restoring force (or torque if the small displacement is
an angle) and put it into a form proportional to the small
displacement quantity (this might involve a linear approximation to
a function of the quantity) OR you can write the kinetic and
potential energies, and expand the potential energy to QUADRATIC
order in the small displacement quantity). In the force/torque case,
then look at your Newton's law/torque equation and map the
quantities to the spring equation m x.. = - k x to get the frequency
f = root (k/m)/(2 pi). In the energy case, look at the mechanical
energy and map the quantities to the spring mechanical energy (1/2)
m x.^2 + (1/2) k x^2 to get the frequency f = root (k/m)/(2 pi).
NOTE that if there are nonconservative forces (eg kinetic friction)
in the problem then you HAVE TO compute the restoring force or
torque (example is the bar and rollers problem from HW 7).
*Specifically for 7.34: you are given that b<<R. This means
that you are allowed to replace R - b by R and that you are allowed
to use the flat surface rolling without slipping condition for the
curved surface of the dish, which makes the problem quite easy. In
fact, with a little more care, you can solve the problem without
using approximations based on b<<R and still get a simple
answer which is not the same but becomes the same in the limit b/R
-> 0. If you want to try this, let me know and I'll give you any
help you need.
*The optional falling plank problem is not as difficult as the book
scares you into thinking. You should have no difficulty writing the
equations with the extended Newton's law approach. It is true that
to solve the equations, you need a small "trick" to get there
quickly. If you are having trouble solving your equations, come to
office hours or email them to me (ok to email a photo from your
phone). I will check them and if correct, tell you the trick so you
can finish the problem easily.
*The optional two rubber wheels problem is a rolling with slipping
problem like 7.30 and 7.31. The angular momentum of the two-wheel
system is NOT conserved -- can you see why?
Week 10: Exam review. List of topics covered on the exam
here.
We discussed strategies for recognizing and getting started with
the different types of problems that might appear on the exam, and
how to prepare your formula sheet to help with this. The specific
types of problems we discussed were drawn from the practice exam:
collision problems (#9), conservation of energy problems (#9) and
rocket problems (#11). Many times the problems will be
combinations of types, for example collision with fixed axis
rotation (#12).
Week 11: Rigid body motion. First, a general strategy for
solving the problems:
Step 1: find fixed point (need not be in the body). Write vector
omega using the description of the motion given in the problem.
Step 2: Find vector L. For most of the problems, I recommend
finding L with respect to the center of mass (the vector omega is
the same). Decompose vector omega into pieces for which the
angular momentum is parallel to the angular velocity, Here's
a big time-saver - in most of the problems, the next step will be
to differentiate L with respect to t to get the torque, so you
only need to find the component of L that depends on time -- don't
waste effort working out the time-independent component.
Step 3: Compute vector dL/dt.
Step 4: Draw a force diagram showing all forces and points of
application. Find the torque around the reference point you chose in
step 2. Set this equal to dL/dt from step 3. Solve the equation for
the unknown quantity,
Now, some comments on the specifics of the problems:
8.2. In the exact solution, the rotation of the disk by the
turntable contributes a time-dependent angular momentum when the
disk is tilted. Here, the statement that Capital Omega <<
omega_0 means that you are allowed to neglect this. So, the only
time-dependent angular momentum that you need to consider comes from
the omega_0 spin of the disk.
8.4. In order for us to compute the forces and torques on the
system, since we haven't discussed the torque when the contact is
not a point, we need to redraw the mechanism shown. Neglect w and
imagine that the axle is rigidly attached to the wheel and connected
to the shaft by a ball and socket arrangement that allows free
rotation around the axis defined by the axle and is fixed in the
other directions (stays perpendicular to the shaft and rotates with
it). Then you can identify the force exerted by the shaft on the
rigid body consisting of the wheel and axle.
8.6. (1) NOTE: the picture has many errors -- the labelling of b and
R and the direction of omega_s, in particular, so draw your own.
(2) The coin cannot roll in a circle without static friction between
the coin and the floor. Look at the motion of the cm and use
Newton's 2nd law to help you find the direction and magnitude of the
friction force.
(3) Assume b<<R. This allows you to make the approximation in
the parentheses, and also to neglect the contribution to the angular
momentum of the rotation of the coin around its diameter as it rolls
(this makes it a lot easier to solve the final equation).
Week 12: Fictitious forces. Here's a alternative
derivation of the expression for the fictitious force in a
rotating frame (this is what we discussed in the Thursday office
hour) here.
In the Friday recitation, we considered what the motion of an object
that is stationary in the inertial frame looks like in the
noninertial frame, and related that motion to the ficitious force we
computed for the noninertial frame. I'll add a writeup here if
anyone asks for it.
The general strategy for solving the problems:
Step 1: Identify the noninertial frame you are working and compute
the fictitious force.
Step 2: Identify the real forces acting.
Step 3. Solve the problem (usually using Newton's 2nd law) including
both real and fictitious forces.
Now, some comments on the specifics of the problems:
9.1. At equilibrium, this rod is balanced on the pivot. The
equilibrium is UNSTABLE (like a ball at the top of a hill) -- if the
rod is displaced by a small angle or given a small angular velocity
at the equilbrium position, it will not return to equilibrium -- it
will fall. Note that the differential equation describing the motion
is the same type as that which describes the motion of the bead on
the wire.
9.7, 9.9, 9.11. You will need to be careful to draw vector omega and
vector r correctly in the reference frame fixed to the surface of
the earth. Vector r is always pointing up for an observer standing
on the surface of the earth. The direction of vector omega depends
on your latitude. For example, if you are at the North Pole then
vector omega points up.
9.12 First find the equilibrium angle at which the pendulum hangs.
Then use Taylor expansion to expand the torque as a function of the
small angle that the pendulum is displaced away from equilibrium (it
might be helpful to re-read the small oscillation problem tips from
week 9 above).
Week 13: Central forces. DO THE WARM
UP PROBLEMS BEFORE RECITATION. Check your answers here: #45
#49 #51
#63.
ellipse
facts
short
excerpt from HRW10 on Kepler's laws
(see fig 13-12 for quick basic ellipse facts)
NEW: Information about summer research
opportunities
Aresty
Summer Science Research Program: an intensive, full-time,
on-campus research experience for Rutgers-New Brunswick rising
sophomores only
Useful resources
Office hours
- Sundays 6:00 PM - 7:15 PM, Scott Hall 101
- Mondays 1:05 PM - 1:55 PM, lobby of Physics Lecture Hall
- Wednesdays 1:05 PM - 1:55 PM, lobby of Physics Lecture Hall
- Thursdays 1:10 PM - 1:55 PM, ARC 206
- Fridays 1:20 PM - 1:55 PM, SEC 212
Referring back to your previous physics textbook
In the first recitation, I suggested that you could use the
textbook from your previous physics course as a reference to
refresh your memory on basics you have learned before which we
expect you to know. I did not take into account the fact that in
most high school courses, you give the textbook back to the school
at the end of the course. There are of course lots of resources on
the internet where you can find the materials you need. However,
if you would find it helpful to have a standard university-level
calculus-based textbook (maybe even the same one you used) on hand
for reference, I can lend you one for the duration of the course
-- send me an email (kmrabe@physics.rutgers.edu) to let me know if
you are interested. Depending on how many people ask, I should be
able to get one to you without much difficulty.
If you have questions about the course or about the homework
problems, email me at kmrabe@physics.rutgers.edu
This page is maintained by Karin
Rabe.