Average and Instantaneous Rate of Motion - Chapter 4.

Motion at Constant Acceleration - Chapter 5. Vectors are introduced and discussed in multiple dimensions. Vector magnitude and direction are also explained. Null vectors, minus vectors, unit and velocity vectors are discussed along with their properties. Finally, several specific problems are solved to demonstrate how vectors can be added, and problems of projectile motion are expounded. Review of Motion at Constant Acceleration - Chapter 2.

The First Law on inertia states that every object will remain in a state of rest or uniform motion in a straight line unless acted upon by an external force. Several different forces are discussed in the context of this law. The lecture ends with the Third Law which states that action and reaction are equal and opposite. Review of Vectors - Chapter 2. Second Law and Measurements as conventions - Chapter 4. Newton's Third Law - Chapter 6. Fundamentals of Physics PHYS 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. Continuation of Types of External Forces - Chapter 2. Kinetic and Static Friction - Chapter 3. Inclined Planes - Chapter 4. Pulleys - Chapter 5. Professor Shankar then reviews basic terminology in relation to work, kinetic energy and potential energy.

He then goes on to define the Work-Energy Theorem. Finally, the Law of Conservation of Energy is discussed and demonstrated with specific examples. Work-Energy Theorem and Power - Chapter 3. The notion of a function with two variables is reviewed. Conservative forces are explained and students are taught how to recognize and manufacture them. Conservative and Non-conservative Forces - Chapter 4. Application to Gravitational Potential Energy Complete course materials are available at the Yale Online website: online.

The three laws of Kepler are stated and explained. Planetary motion is discussed in general, and how this motion applies to the planets moving around the Sun in particular. Review of Conservative and Non-conservative Forces - Chapter 2. Kepler's 3 Laws - Chapter 3. Deriving the Nature of Gravitational Force - Chapter 4. Through a variety of examples, the professor demonstrates how to locate the center of mass and how to evaluate it for a number of objects.

Finally, the Law of Conservation of Momentum is introduced and discussed. The lecture ends with problems of collision in one dimension focusing on the totally elastic and totally inelastic cases. The Center of Mass - Chapter 3. The Rocket Equation - Chapter 5.

Elastic and Inelastic Collisions Complete course materials are available at the Yale Online website: online. The lecture begins with examining rotation of rigid bodies in two dimensions. The concepts of "rotation" and "translation" are explained. The use of radians is introduced. Angular velocity, angular momentum, angular acceleration, torque and inertia are also discussed. Finally, the Parallel Axis Theorem is expounded. Torque and Work Energy Theorem - Chapter 6.

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Complete cours. The lecture begins with an explanation of the Parallel Axis Theorem and how it is applied in problems concerning rotation of rigid bodies. The moment of inertia of a disk is discussed as a demonstration of the theorem. Angular momentum and angular velocity are examined in a variety of problems.

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Example Problem: Torque on a Disk - Chapter 6. While previous problems examined situations in which?

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If there is no torque,? The lecture starts with a simple example of a seesaw and moves on to discuss a collection of objects that are somehow subject to a variety of forces but remain in static equilibrium. The Seesaw Example - Chapter 3. The Case of the Leaning Ladder - Cha. The lecture begins with a historical overview and goes into problems that aim to describe a single event as seen by two independent observers.

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## Full text of "Fundamentals Of Physics Mechanics Relativity And Thermodynamics"

Maxwell's theory, as well as the Galilean and Lorentz transformations are also discussed. The Meaning of Relativity - Chapter 2. The Galilean Transformation and its Consequences - Chapter 3. The Medium of Light - Chapter 4. The Two Postulates of Relativity - Chapter 5. Length Contraction and Time Dilation - Chapter 6. Deriving the Lorentz Transformation Complete course materials are available at the Yale Online website: online. Fundamentals of Physics PHYS This lecture offers detailed analysis of the Lorentz transformations which relate the coordinates of an event in two frames in relative motion.

It is shown how length, time and simultaneity are relative. Describing an Event with Two Observers - Chapter 2. The Relativity of Simultaneity - Chapter 3. Time Dilation - Chapter 4. The algebra is, of course, very trivial here. I want to know what happens.

## Fundamentals of Physics : Mechanics, Relativity, and Thermodynamics (Open Yale Courses) [Paperback]

One way is just to use your common sense and realize that these two blocks are going to move together. What about gravity? What about the force due to the table on which the masses are moving? Imagine that this occurs in outer space where there is no gravity and no need for a table. My 10 N is certainly acting on it.

What other force is acting? Bottom: The free-body diagram for the two blocks showing all the forces on each block. Notice the third law is being invoked.

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Next consider the 2-kg mass. Here is the mistake some people make: they add to that the 10 Newtons. They feel that the 2 kg will surely feel it since that is what is behind all the acceleration. That will be a mistake. If it accelerated less than the first, the first would have plowed into the second.