The second course in the General
Physics sequence. This course extends the ideas of Newton's laws and
energy concepts to oscillations and waves, including sound; to heat and
temperature, the thermal properties of materials and the principles of
thermodynamics; and to light, geometrical optics,
and interference and diffraction. (It is almost like three short
courses, rather than the continuous thread of related topics that was
encountered in Phys 131.)
If the first course in the
sequence dealt with the motion of objects - either single particles or
collections of particles that can be treated as
single objects (like balls or blocks), this course can be thought of as
dealing with the collective motion of systems of particles. Liquids and
gases are interacting systems of huge numbers of particles - but can be
understood as systems without knowing how individual particles behave.
Wave motion is a further extension of the ideas with the description of
the motion of "disturbances" being the interest. All thermodynamic
processes are ultimately related to the microscopic motions of the
atoms
that make up the objects or systems being described. And finally, the
ideas of wave motion will be applied to light - with analogies to the
discussion of sound being made where appropriate.
This course is a special section
of the Physics 132 course for students enrolled in the Cal Poly Honors
Program - and for Physics majors. The course will be offered with an
integrated lecture/laboratory/workshop format. The course is
cross-listed with the honors program course HNRS132.
[NOTE: To be enrolled in Sect. 70 you must also be enrolled in
either Sect. 73 (Tues. 8-11) or Sect. 72 (Tues. 12-3) of Phys 132
Laboratory.]
Instructor: Dr.
Ron
Brown - Physics
Department Office Hours: Mon 11-12 and 2-3; Wed 11-12 and 2-3;
Thurs 10-11; Fri 11-12
Textbook: PHYSICS for Scientists and
Engineers
by Randall D. Knight
(Addison-Wesley, 2004)
Reference: Brown, Physics 132 SUPPLEMENTAL NOTES
AND PROBLEMS, El Corral
NOTES FOR PHYS 132 Honors - SPRING 2004
- Look here for information for PHYS 132-70/HNRS132
Course
Syllabus
Calendar
Physics
132 Assignment Sheet
Physics 132
Homepage - Homework hints and solutions.
Great Ideas
that Have Changed Our Worldview - An essay
Physics Central - A
great link!
Resources
Physics 132 Topics and Notes
Chapter 14 - Oscillations
Chapter 20 - Traveling Waves - Waves
on Strings, Sound, Light
Chapter 21 - Superposition - Standing
Waves and Interference
Chapter 22 - Wave Optics - Light and
Optics, Interference and Diffraction
Chapter 23 - Ray Optics -
Reflection, Refraction, Image Formation, Lenses and Lens Systems
Chapter 15 - Pressure
Chapter 16 - A Macroscopic Description
of Matter - Solids, Liquids, Gases; Temperature and Phase Changes
Chapter 17 - Work, Heat, and the First
Law of
Thermodynamics
Chapter 18 - The Micro/Macro
Connection - Pressure and Temperature, Entropy and the Second
Law of Thermo
Chapter 19 - Heat Engines and
Refrigerators - Thermodynamic Efficiency
This Week's Laboratory - Look here each week
for information about that week's laboratory experiment.
RESOURCES:
Textbook: PHYSICS for Scientists and Engineers
by Randall D. Knight
(Addison-Wesley, 2004)
Required: Physics 132 SUPPLEMENTAL NOTES AND
PROBLEMS by Ronald
Brown (El Corral)
The
supplement is intended to be used along with the text to help you
relate the
important ideas of the course.
It is available in El Corral
with the physics textbooks.
This supplemental set of notes (about 60 pages) summarizes the
important concepts
of this course. The notes treat the material differently than the text
-
the focus is on the concepts, the underlying ideas,
rather than on how to apply the ideas to problems. You should look at
the Supplement and decide whether it would be helpful for you.
Included are questions and problems to test your thinking.
Office Hours - Make good use of the access you have to
your
faculty in all courses. Don't wait until you are in trouble in a class
to seek help. When you don't understand something, ask! If you just
want to discuss the ideas or look for reassurance on your line of
reasoning, make use of office hours. If you cannot get to office hours
for some reason, contact your instructor after class or by email to set
up a time to meet - or just stop by the office.
Private Tutoring - Individual arrangements can be made
with
Physics majors available for tutoring in Sci. Bldg. room E-25 (known
affectionately as "h-bar" - a physics in-joke)
Drop-In Help - Those same tutors will also usually help
for
free if you just stop by "h-bar" or go to the Learning Center.
Mathematics and Science Learning Center - The Learning
Center will be open starting the second week of classes. - Faculty and
student tutors from Physics department hold office hours in the
Learning Center - Sci. Bldg. C-20. It is a good place to go
to work HW (with help immediately available) or to ask questions of
whoever is "on call".
Learning Center Hours: Mon. 9 am - noon;
Tues., Wed. 9 am - 2 pm; Thurs. noon - pm; Fri. 9 am - noon.
NOTE: Hours may change when Center
opens the second week of
classes.
Useful Links: The following are links to three very helpful
discussions on how to approach studying physics and the necessary
problem
solving that goes with studying physics, written by Dr. Dan Styer,
Physics
Dept., Oberlin College.
Tips
for Studying Physics
The
Whys and Hows of Physics Problems
Solving
Problems in Physics
HOMEWORK: The questions, exercises, and problems on
the
assignment sheet are to help you understand the material. You should do
the problems systematically and carefully in a HW notebook - and ask
questions about problems you have difficulty with. Solutions will be
posted on the web: Problem
Solutions
Posted Solutions and Hints - Selected problem hints
and/or
solutions will be posted on the bulletin board just outside room E-47
in the Science Bldg (Bldg.52).
[Look here for comments related to the Honors
Section of Physics 132.]
This class is scheduled to meet three times per week for lecture and
once for a lab. To be in the Honors section, you must be enrolled in
one of the honors labs - either 8 -11 or 12 - 3 on Tuesdays. The
format will include some lecture and some discussion each day - with
occasional problem solving workshops in both the lecture and lab
meetings.
It will be expected that you will come to the class having read the
related material in the text and the supplemental notes and that you
will have attempted some of the problems - so that the work done in
class is not your first exposure to that material. There will be
laboratory reports - either individual or group reports for each of the
lab experiments. Quizzing and testing may be done in the more
relaxed laboratory environment to leave more class time for discussion
of the material.
Week
No. 2
HW Prob. Set No. 1 due Monday
We will continue the discussion of harmonic oscillators - and
especially deal with the energy of oscillating systems. That will lead
to the discussion of damping and the effect of non-conservative forces
acting on a harmonic oscillator. Although we will not deal with the
details of the solution of the damped oscillator problem, we will
interpret the effect of the damping on the motion. Either in lab on
Tuesday - or in class on Wed., we will talk about resonance - the
effect of a sinusioidal driving force on a system which has a natural
frequency of oscillation.
We may have a short quiz in lab - just to see where you are with
the ideas of simple harmonic motion at this point.
This important chapter is the basis
for understanding many natural phenomena involving oscillatory behavior
- from atoms in crystals to Cepheid variable stars. The ideas follow
directly from Newton's laws and must be understood well in order to
understand the descriptions of mechanical wave motion - the material
that follows in the next chapter. Harmonic motion is ultimately a
consequence of the
natural tendancy of things to seek their lowest potential energy,
"overshoot", and then oscillate around their equilibrium positions. The
discussion will lead to the idea of resonance - a phenonomenon which
occurs throughout nature.
The general discussion of wave motion is
important because the ideas of wave propagation are ubiquitous. In
nearly all areas of science (and therefore real life) energy is
transferred via the vibrations that make up waves. Examples of wave
motion include waves on strings, water waves, earthquakes, sound, all
electromagnetic radiation including light, heat, x-rays, etc. There are
many common elements to all the various types of wave motion that can
be described - and these will be pointed out. There are also some
differences - especially between the mechanical waves such as waves on
strings and sound and all electromagnetic waves - which will be
important in some discussions. What is common to all forms of wave
motion is the idea that a disturbance is being propagated from one
place to another without the necessity for the medium through which the
disturbance is being propagated to itself be transported.
After the general description of the motion of
harmonic
oscillators is understood, it is not difficult to extend the ideas to
allow for the description of waves propagating along a taut string.
That description will be mathematically identical to the very wide
variety of wave motions - including water waves, seismic waves, sound
waves, and even electromagnetic waves. A consequence
of the way waves propagate through a medium (string, air, water, it
doesn't matter), is that waves can also interfere. And wave
interference can be either constructive or destructive - with the
consequence of either enhancing or suppressing the wave amplitude - an
important idea.
The main ideas of this chapter are that
sound is a longitudinal
wave (as opposed to the transverse waves on a string).
The
speed of sound in air depends on the "bulk modulus" and mass density of
the air - and can ultimately be expressed in terms of the absolute
temperature (ie, T in kelvins). The apparent loudness of a sound can be
expressed in terms of the intensity of sound in decibels -
which
is a logarithmic scale. The equations that describe sound waves are
essentially the same as those that describe waves on strings. You
should
look carefully at the sections that deal with interference from two
sources - as that can lead to constructive and destructive interference
-
and to the beat frequencies associated with two sources whose
frequencies
differ slightly. Standing wave resonance is as important in sound waves
as
it was in the waves-on-a-string discussion. But while the most common
problems with waves on a string had nodes at each end (as in lab), the
sound wave resonances discussion will commonly involve tubes with
either
one or both ends open - which means antinodes occur at the end - and
that
changes the relationship between tube length and wavelength. And
finally, you should look carefully at the Doppler effect - the apparent
shift in frequency of sound due to motion of either the source of
the sound or of the observer (listener).
Look here each week for a
brief description of the laboratory experiment.
Week 2: Exp. 10 - HARMONIC MOTION
This week's experiment deals with a
mass-spring system. The purpose is to verify the relationship between
the period and the mass. The experiment
has two parts: You will first suspend weight from a coiled spring to
determine the spring constant (by plotting the force required to
stretch the spring vs the extension - then taking the slope of the
graph). In
the second part of the experiment, you determine the period of the
mass-spring system as a function of the mass in order to experimentally
verify the equations used in describing simple harmonic motion.
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