The lecture begins with the application of Newton's three laws, with the warning that they are not valid for objects that move at speeds comparable to the speed of light or objects that are incredibly small and of the atomic scale. Friction and static friction are discussed. The dreaded inclined plane is dealt with head on. Finally, Professor Shankar explains the motion of objects using Newton's laws in specific problems related to objects in circular motion, such as roller coasters and a planet orbiting the Sun.

1. Course Introduction and Newtonian Mechanics
2. Vectors in Multiple Dimensions
3. Newton's Laws of Motion
4. Newton's Laws (cont.) and Inclined Planes
5. Work-Energy Theorem and Law of Conservation of Energy
6. Law of Conservation of Energy in Higher Dimensions
7. Kepler's Laws
8. Dynamics of a Multiple-Body System and Law of Conservation of Momentum
9. Rotations, Part I: Dynamics of Rigid Bodies
10. Rotations, Part II: Parallel Axis Theorem
11. Torque
12. Introduction to Relativity
13. Lorentz Transformation
14. Introduction to the Four-Vector
15. Four-Vector in Relativity
16. The Taylor Series and Other Mathematical Concepts
17. Simple Harmonic Motion
18. Simple Harmonic Motion (cont.) and Introduction to Waves
19. Waves
20. Fluid Dynamics and Statics and Bernoulli's Equation
21. Thermodynamics
22. The Boltzmann Constant and First Law of Thermodynamics
23. The Second Law of Thermodynamics and Carnot's Engine
24. The Second Law of Thermodynamics (cont.) and Entropy

This course provides a thorough introduction to the principles and methods of physics for students who have good preparation in physics and mathematics. Emphasis is placed on problem solving and quantitative reasoning. This course covers Newtonian mechanics, special relativity, gravitation, thermodynamics, and waves.