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Information
for Session 1, 2004
- Lecturer:
Prof. Paul Curmi
- Lecture
times: Tues 2-3, Thurs 1-2
- Consultation
time: Fri 4-5
Brief
Syllabus:
Coordinate
systems; Newton's Laws; Lagrange's equations; Harmonic oscillator,
damped and forced motion, resonance; Central forces, inverse
square law orbits; Many particle systems; Hamilton's equations;
Coupled oscillators.
Assumed
Knowledge:
The
course assumes familiarity with first year physics, e.g. PHYS1002
or PHYS1221 or PHYS1231; and first year mathematics, e.g.
MATH1231 or MATH1241. Corequisites: 2nd year mathematics,
MATH 2011 or MATH2110 or MATH2100.
Course
Goals:
Mechanics
is the most basic and fundamental branch of physics, and has
been of central importance since the days of Galileo and Newton.
This course aims to provide students with further insight
into the principles and behaviour of mechanical systems, plus
an introduction into new mathematical formalisms which have
become the basis of much of modern physics, e.g in quantum
field theory, or the treatment of nonlinear systems. Specific
topics include:
- A
brief discussion of various coordinate systems which may
be useful in different problems;
- The
integration of Newton's law of motion for some standard
cases;
- An
advanced discussion of the harmonic oscillator, treating
the effects of a damping force and a harmonic driving force,
and the phenomenon of "resonance", which appears
in virtually every field of physics;
- A
general discussion of motion in a central field of force,
including the fundamental conservation laws. We cover the
special case of an inverse square force law, and the appearance
of elliptic orbits, providing some of the basic tools for
an understanding of astronomy;
- A
review of the general properties of many-particle systems;
- A
first discussion of the Lagrangian formulation of mechanics,
and Hamilton's principle, leading to the Lagrange equations
of motion. This formalism is a basic tool used in later
years in discussing advanced mechanics, and relativistic
quantum mechanics and field theory;
- A
first introduction to the alternative Hamiltonian formulation
of mechanics, and Hamilton's equations of motion;
- A
brief discussion of two coupled oscillators, providing a
first example of a system with non-trivial interactions
between different degrees of freedom.
Learning
Objectives
- Students
will gain a physical understanding of the important phenomena
of resonance in oscillating systems, of the motion of planets
and central force motion in general, and of coupled oscillators.
- Students
will learn to formulate and to solve differential equations
describing physical systems
- Students
will learn to understand and apply the sophisticated formalisms
of Lagrange and Hamilton, which are basic to advanced theoretical
physics.
Why
is mechanics important?
A
knowledge of mechanics is clearly vital in understanding the
world around us. The principles of mechanics are used in everything
from designing Moon rockets or building bridges, right down
to playing a game of billiards. Furthermore, the mathematical
techniques and formalisms learnt in mechanics are used as
basic tools in all other areas of physics. It is vital to
understand the 'classical' material in this course, before
one can understand or appreciate the principles and techniques
used in 'modern' physics.
The
course is strongly recommended as groundwork for a number
of 3rd year courses, e.g. PHYS3020 Statistical
Physics, PHYS3230 Electromagnetism, PHYS3410 Biophysics and
PHYS3510 Advanced Mechanics, Fields and Chaos, as well as
the 4th year Honours course in Quantum Field Theory.
The
material covered is not by any means new. Inverse square law
orbits were already understood by Isaac Newton; and the discussions
of Lagrange and Hamilton date back to the 1800s. But despite
its antiquity, mechanics remains a living and thriving field
of research. In third year PHYS3510, Advanced Mechanics, Fields
and Chaos, students will get a first glimpse of some fascinating
topics at the frontiers, such as:
- Nonlinear
systems, and 'solitary waves';
- The
road to chaos;
- Etc.
|
Space
Rocket changing from a circular orbit to an elliptical
one |
How
to succeed - Strategies for Learning
Some
students find this subject confusing, and have difficulty
telling the wood from the trees. It is important to keep an
eye on the basic principles that emerge, particularly old
favourites like the conservation of energy and momentum. Like
most subjects, the key to success is hard work. Rather than
waiting for it all to be presented on a plate, it is vital
that students sit down and work out most of the tutorial
problems, by themselves or with a group. Only in this
way can they get the practice and experience necessary to
understand the physical phenomena and mathematical techniques
presented here. Practice, practice, practice! Approximately
one in four of the class periods will be devoted to tutorials,
where solutions to selected problems will be discussed.
It
is also very useful, as in any course, for each student to
prepare a concise summary of the material presented
in lectures, to fix the main ideas in his/her memory.
Assessment
- 2
hour written examination 60%
- Two
assignments 20%
- Mid
session test 20%
For rules regarding conduct of examinations, special consideration, academic
honesty, etc, see the School website at http://www.phys.unsw.edu.au/2nd_and_3rd_syllabi/assessment_policy.html
Resources
Textbook
The
material presented in this subject is covered by many good
textbooks. Students are recommended to obtain one of two
texts, depending on their needs.
For
a more elementary treatment, one could use:
G.R.
Fowles and G.L. Cassaday, Analytical Mechanics, 5th
or 6th edition; or
G.R. Fowles, Analytical Mechanics, 3rd or 4th
edition.
Students
with a stronger theoretical background or students intending
to pursue future studies in advanced mechanics could use:
H. Goldstein, C. Poole & J. Safko, Classical Mechanics,
3rd edition; or
H. Goldstein, Classical Mechanics, 1st or 2nd edition.
Note:
Goldstein is the recommended text for PHYS3510 Advanced
Mechanics, Fields and Chaos.
Additional
References
- L.
D. Landau and E. M. Lifshitz, Mechanics (Pergamon Press)
- LN
Hand & JD Finch, Analytical Mechanics (Cambridge University
Press)
- F.
Scheck, Mechanics (Springer-Verlag)
-
JV Jose & EJ Saletan, Classical Dynamics A Contemporary
Approach (Cambridge University Press)
-
C. Lanczos, The Variational Principles of Mechanics (Dover)
M.R. Spiegel, Theoretical Mrechanics
(Schaum outline);
- B.P.
Cowan, Classical mechanics
- K.
Rossberg, A First Course in Analytical Mechanics
- K.R.
Symon, Mechanics
- A.P.
Arya, Introduction to Classical Mechanics
Those
students having difficulties should consult the lecturer for
help. Further information on student support services may
be found on the School website at http://www.phys.unsw.edu.au/2nd_and_3rd_syllabi/2nd_year_intro.html
Detailed
Syllabus
| TOPIC |
TEXT
REFERENCE
4th
Edition |
TEXT
REFERENCE
6th
Edition |
| Vectors:
coordinate systems, derivatives of vectors. Kinematics:
velocity and acceleration, angular velocity, relative
motion. |
Chapter
1 |
Chapter
1 |
| Mechanics:
Newton’s laws, consequences |
4.1,4.2 |
Chapter
2 |
| Conservative
forces, solution methods |
3.1-3.5 |
2.3,4.1 |
| Oscillatory
Motion |
|
|
| Harmonic
oscillator, damped and forced oscillations |
3.1-3.5 |
3.1-3.4 |
| Resonance,
power supplied, harmonic motion in 2 and 3 dimensions |
4.4 |
3.6,4.4 |
| Central
Forces |
|
|
| Conserved
quantities, equation of motion, energy equation, Kepler’s
laws, gravitational fields and forces, inverse square
law orbits and energies, stability and symmetry. |
Chapter
6 |
Chapter
6 |
| Many
Particle Systems |
|
|
| Internal
forces and torques, conservation laws, CM coordinates,
two-body problem, collisions, rotational inertia,
laminar motion of a rigid body. |
7.1-7.4
8.2-8.6 |
7.1-7.3,7.5
8.1-8.3,8.5-8.6 |
| Lagrange’s
Equations |
|
|
| Constraints,
generalized coordinates and forces, kinetic energy,
Lagrangian, generalized momenta. |
10.1-10.5 |
10.1-10.5 |
| Hamilton’s
equations, symmetries and conservation laws, examples. |
10.7 |
10.9 |
| Potential
function, equations of motion, normal frequencies
and modes, general solution, weighted and continuous
strings. |
Chapter
11 |
Chapter
11 |
For more
information about PHYS2010 contact:
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