
This course emphasizes a systematic approach to the mathematical
formulation of mechanics problems and to the physical interpretation of
the mathematical solutions. Topics covered include: Newton's laws of motion,
kinematics and dynamics of a single particle, vector analysis, motion
of particles, and gravitation. Recommended background: PH 1110, PH 1120, PH 1130, PH 1140,
MA 1021, MA 1022, MA 1023, MA 1024 and concurrent registration in or completion
of MA 2051. (The more important courses are in bold.)
The concepts of PH 1110 serve you very well for PH 2201. The
problems
in this course are more challenging, however, and emphasis is placed on
your problem-solving skills and effective communication of your
solutions. PH 2201 problems tend to be very practically oriented. If
you continue on to PH 2202, you will learn new, more theoretical
physics.
The text is "Classical Mechanics", by J.R. Taylor,
available in the bookstore. The
supplementary text is "An Introduction to Mechanics", by Kleppner and
Kolenkow. There will be a few copies of K&K on reserve in the
Gordon Library, and as many copies as I can gather together in the
Physics Library, in the care of Mrs. Malone. Give your WPI ID to her and
ask to borrow one during business hours. PH 1111 students will also
have copies.
We meet in OH 223 on MTThF at 9:00. Instructor: Professor NA Burnham, nab@wpi.edu.
| % |
Activity |
| 60% | Exams. 10% penalty for make-ups. |
| 40% | Email, reading summaries, computer work, and homework. No late work
accepted. Full credit for 200 out of the 230 possible points. |
| Points | For each problem (out of five possible points): |
| -5 | No symbolic solution. |
| -5 |
Symbolic solution has wrong dimensions. |
| -1 to -5 | Write-up hard to read or understand. |
| -1 | Vectors confused with scalars or vice versa. |
| -1 | No evaluation. |
| -1 | No box around symbolic or numerical answer. |
| In general, for any given problem: | |
| 5 = | Very good -- write-up clear and correct. |
| 4 = | Good -- write-up clear and nearly correct, or understandable and correct. |
| 3 = | Acceptable -- write-up understandable and nearly correct. |
| For the reading summaries (out of five possible points): |
|
| -5 |
Equations or symbols in summary. |
| -1 to -5 |
Not enough detail. |
| -1 to -5 |
If handwritten, penalty for hard-to-read writing. |
| -1 |
Shorter or longer than specified length, in increments of 50 words. |
| -1 |
No word count. |
| And for an entire assignment: | |
| -1 | No staple. |
| -1 | No name. |
| -1 | Ragged edges. |
1. What do you hope to learn from this course?Feel free to add anything else you would like me to know.
2. What do you hope to do with this new knowledge?
3. What are your previous math and physics courses?
4. What is your goal for this course?
5. Did you have any problems printing from myWPI?
Reading summaries
Reading summaries provide you with a chance to preview upcoming material. Because the quality of hand writing varies so much, please use a word processor to typeset them. Each reading summary should be 300 to 600 words in length, with the word count listed at the end. Use no equations or symbols. Here is an example summary of Taylor Sections 1.1 to 1.5.
Mechanics is the study of motion. Its history dates from Galileo and Newton and was developed further by Lagrange and Hamilton. About a hundred years ago, scientists started to develop relativistic mechanics and quantum mechanics, and to distinguish among them, the traditional form of mechanics has become known as "Classical Mechanics".The list of reading summaries can be found at myWPI, under Assignments.
Newton's famed three laws of motion are based upon ideas that concern space, time, mass, and force. Space can be described by coordinate systems, the simplest one being the cartesian coordinate system, which has three orthogonal axes. The position of an object can be determined by a position vector, and the next few pages of the text reviews vector algebra. After further reminders of time, reference frames, mass, and force, Newton's laws are introduced.
The First Law says that a particle moves with a constant velocity unless acted upon by an external force. The Second Law states the relationship between mass, a scalar, and acceleration, a vector. Their product equals the vector sum of all the forces acting on a particle. Since acceleration is the second derivative of position with respect to time, the Second Law is a differential equation. Newton's Laws hold in what are called inertial reference frames. They do not always hold for relativistic or quantum systems. Nonetheless, they are valid over a wide range of scales in size and speed and are thus worthy of study.
The Third Law states the relationship between "action" forces and "reaction" forces. They are equal in magnitude and opposite in direction, but act on two different bodies. From the Third Law, which considers only one particle, one can construct a theory for many particles. Internal forces in a multiparticle system have no influence on the total momentum. In other words, if the external forces are constant, then momentum is conserved. Taylor gives an example where, apparently, the Third Law is violated, but then explains that mechanical momentum is not the only form of momentum. It can, for example, be electromagnetic. However, Taylor assures us that for the rest of his text, we will consider situations only in which the Third Law holds.
353 words
Computer work
Based on freshman mechanics, the computer work is a means for you to review introductory mechanics. If you get a significant number of the questions wrong, that is a warning! It means that you are missing fundamental concepts from Physics I. It is unlikely you will do well in this course if you are still learning last year's material. Take the time to review your freshman mechanics book, if needed. There are plenty of them in the physics library, OH 118, a good place to study. The doors of Olin Hall remain open until 21:00 during the week.
Download the computer work assignments from myWPI, under Documents. Please print a copy of each assignment to help you prepare to submit your responses at myWPI. There are ten multiple-choice questions for each of the seven assignments (ten possible points per assignment). You should bring the paper copies of the assignments to class, where we will go over the more difficult problems. You must submit your answers by 8:00 a.m. on the due date. If you have network problems, you may bring the answers to class on a piece of paper and submit them at the beginning of class. (Email answers not accepted.)
Homework assignments
There are eight homework sets of three problems each (fifteen possible points per assignment), none of which will be accepted late. If you can not or choose not to attend class, I expect to see your work in my mailbox (near the Physics Department office) at 9:00 the day that it is due. If you are not able to perform your homework on time, I still recommend that you do it, as exam problems will be similar. Far fewer problems are assigned than should be, due to limitations on grading time. The homework assignments are available under the Assignment section of PH 2201 at myWPI. I will give the grader the grading scheme above. You are encouraged to collaborate on the homework problems, but you must each write up your own solutions.
Summary for assignments (due dates given on calendar below):
Activity Submission # Pts each Total points
1
5
5
RS
paper
7
5
35
CW myWPI 7 10 70 HW paper 8 15 120 Total 230
| Week of | Monday | Tuesday | Wednesday | Thursday | Friday |
| 22. August 2004 | What's
due Today's material Sections | -- Intro, Vectors T 1.1-1.2 | Email Newton's Laws T 1.3-1.6 | ||
| 29. August | HW1 Polar coordinates T 1.7 | RS1 v, a in polar coord T 1.7 | CW1 Free-body diagrams KK 2.4 | HW2 Problem solving KK 2.4 | |
| 5. September | Labor Day | RS2 Constraints KK 2.5 | Exam 1 | CW2 Gravity and Kepler KK 2.5, 9.7 | |
| 12. September | HW3 Tension KK 2.5 | RS3 Linear air resistance T 2.1-2.2 | CW3 Quadratic air resistance T 2.3-2.4 | HW4 Momentum T 3.1 | |
| 19. September | RS4 Rockets T 3.2, KK 3.4 | Exam 2 | CW4 Momentum transport KK 3.5 | HW5 Center of mass T 3.3 | |
| 26. September | RS5 Angular momentum T 3.4 | CW5 Moment of inertia T 3.5 | HW6 Work-energy T 4.1 | Exam 3 | |
| 3. October | RS6 Potentials T 4.2 | CW6 Energy diagrams T 4.6 | HW7 Energy conservation T 4.7 | RS7 Effective potentials T 8.4 | |
| 10. October | CW7 Kepler orbits T 8.5-8.7 | HW8 Review -- | Exam 4 |
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