Applying Newton’s Laws – Force & Motion Explained | Chapter 5 of University Physics
Applying Newton’s Laws – Force & Motion Explained | Chapter 5 of University Physics
Chapter 5 applies Newton’s laws to real-world scenarios, guiding you through equilibrium, dynamics, friction, circular motion, and the fundamental forces that govern interactions. Using free-body diagrams and vector components, you’ll learn systematic strategies to solve both static and accelerated systems.
Watch the full video summary here for step-by-step problem-solving examples.

Equilibrium of Particles
Under Newton’s First Law, systems in equilibrium have zero net force and zero acceleration. To solve equilibrium problems—such as hanging masses, objects on inclined planes, or ropes under tension—follow these steps:
- Draw a free-body diagram isolating the particle.
- Identify and label all forces (weight, tension, normal).
- Resolve forces into components and set ΣFx = 0, ΣFy = 0.
- Solve algebraically for the unknown forces.
Dynamics: Non-Equilibrium Systems
When forces don’t balance, Newton’s Second Law F = ma governs motion. Break forces into components and apply Fx = m ax, Fy = m ay. Analyze connected systems—like masses on pulleys—by writing separate F = ma equations for each mass and relating their accelerations.
Friction Forces
Friction opposes motion between surfaces:
- Kinetic friction: fk = μk n
- Static friction: fs ≤ μs n
- Rolling friction: use μr for rolling resistance.
Examples—such as dragging crates or sleds—show how friction affects the net force and must be included in free-body diagrams.
Dynamics of Circular Motion
Objects in uniform circular motion at speed v require centripetal acceleration toward the center:
arad = v²/R, giving Frad = m v²/R. In nonuniform motion, tangential acceleration alters speed in addition to the radial component. Avoid invoking “centrifugal force” in inertial frames.
The Fundamental Forces of Nature
All macroscopic forces—weight, normal, tension, friction—stem from four fundamental interactions:
- Gravitational
- Electromagnetic
- Strong nuclear
- Weak nuclear
Recognizing these origins deepens your understanding of how forces behave.
Conclusion
By mastering free-body diagrams and applying Newton’s laws across equilibrium, dynamics, friction, and circular motion, you gain essential tools for analyzing any mechanical system. Continue practicing these strategies to solve complex problems with confidence.
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