Phy 300
Classical Mechanics
Sir Issac Newton 
Instructor: Dr. Jose' D'Arruda
Office: Sci 320 Phone 910 521 6247
E-mail Jose@nat.uncp.edu
Text: Marion,Thornton, Classical Dynamics, 4th edition, Harcourt Brace College Publishers
General Description: Mechanics of particles and system of particles. Solution of problems in Newtonian Mechanics, one dimensional motion, linear, damped and driven oscillations; two particle collisions, introduction to Lagrangian and Hamiltonian Dynamics. Central force motion.
Specific Competencies: Upon completion of the course, the student should acquire the following competencies:
1. Know how to work with vectors and vector calculus . Be able to solve first order linear differential equations. Know how to solve second order linear equations . Know how to applied initial conditions to the solutions of these equation. Know how to make series expansions of a function, and be able to consistently ignore terms of higher order.
2. Have a thorough knowledge of measurement including knowledge of the SI system of units
3. Understanding of Newton Laws of motion and Newton's law of gravitation.
4. Have a general knowledge of inertial frames of reference.
5. Understand Simple Harmonic Oscillators in one and two dimensions, understand phase diagrams, damped oscillations, driven oscillation and other physical systems which show oscillatory motion.
6. Understand the methods of Calculus of variations and Euler's equation.
7. Be able to solve Lagrangian equations and compare these solutions to the solution obtained using the concept of the force and the Newtonian method.
8. Be able to solve the Hamiltonian and see how this formulation leads one to Quantum Mechanic formulation.
9. Understand central force motion and the dynamics of a system of particles.
Topical Outline: 1. Vectors
2. Coordinate Transformations
3. Gradient Operations
4. Newton's Laws
5. Frames of Reference
6. Conservation Theorems
7. Simple Harmonic Oscillators
8. Damped Oscillators
9. Phase Diagrams
10. Sinusoidal Driving Forces
11. Physical System Oscillations
12. Gravitational Potential
13. Lines of Forces and Equipotential Surfaces
14. Euler's Equation
15. Functions with several Dependent Variables
16. Hamilton's Principle
17. Generalized Coordinates
18. Lagrange's Equations of Motions
19. Equivalence of Lagrange's and Newton's Equations
20. Canonical Equations of Motion
21. Hamiltonian Dynamics
22. Reduced Mass
23. Orbits in a Central Field
24. Orbital Dynamics
25. Center of Mass
26. System of particles and Conservation Laws
Methods of Teaching: The Class will be consist of lecture and demonstrations.
Evaluation/Grading: There will be three test and one final. This will account for 80% of the students grade. Homework and class participation will account for 20% of the student grade.