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Classical Mechanics
Foundations & Vectors
01SI Units and the Constants That Define Them02Defining the Second and the Meter03Redefining the Kilogram via Planck's Constant04Defining SI Units from Fixed Constants05Radians, Steradians & Small Angles06Dimensional Analysis: M, L, and T07Deriving Laws from Dimensions08Fermi EstimationProblem set0/10Problem set 20/10Practice∞
01Vector Addition and Scalar Multiplication02Cartesian and Cylindrical Coordinates03Vector Components in Cartesian Coordinates04Solving Vector Problems with Components05Vector Components Under Coordinate Rotation06The Cross Product07The Cross Product FormulaProblem set0/10Problem set 20/10Practice∞
Kinematics
01Position, Time Intervals, and Displacement02Instantaneous Velocity and the Derivative03Acceleration as the Second Derivative04Kinematic Equations from Graph Areas05Integration and the Fundamental Theorem06Polynomial and Piecewise AccelerationProblem set0/10Problem set 20/10MIT problem set0/4Practice∞
01Independent Motion Along x and y Axes02Setting Up a Projectile Motion Problem03Time of Flight and Maximum Height04Eliminating Time to Find the Parabola05Aim Straight at the Falling BucketProblem set0/10Problem set 20/10MIT problem set0/1Practice∞
01Centripetal Acceleration and Central Motion02Polar Unit Vectors and the Velocity of Circular Motion03Deriving v = rω from Chord Length and Small Angles04Radial and Tangential Acceleration in Polar Coordinates05Uniform Circular Motion: Period, Frequency, and v²/R06Angular Velocity and Acceleration as Vectors07Variable Radius: Radial Velocity and the Coriolis TermProblem set0/10Problem set 20/10Practice∞
Dynamics
01Defining Force: Mass, Acceleration, and Force as a Vector02Newton's First Law: Inertia and Inertial Reference Frames03Newton's Second and Third Laws: Force as the Rate of Change of MomentumProblem set0/10Problem set 20/10Practice∞
Force Laws
01Force Laws and Hooke's Law: Measuring the Spring Force02Universal Gravitation and the Principle of Equivalence03Electric Charge, Coulomb's Law, and Newton's Third LawProblem set0/10Problem set 20/10MIT problem set0/1Practice∞
Constraint Forces
01The Normal Force: Why It Isn't Your Weight02Static and Kinetic Friction and the f = μN Laws03Free-Body Diagrams and Building a Physical Model04Tension in a Rope: Massless vs. Massive05Tension in a Hanging Rope: Two MethodsProblem set0/10Problem set 20/10MIT problem set0/4Practice∞
Applying Newton's Laws
01The Staircase Problem: Friction, Launch, and Landing02Cart, Pulley, and Hanging Block: Finding the Tension03Inextensible Strings: Constraints in a Pulley System04A Block on an Accelerating Frictionless Wedge05The Capstan Equation: Rope Friction Around a Post06Terminal Velocity and the Hyperbolic-Tangent LawProblem set0/10Problem set 20/10MIT problem set0/4Practice∞
Fluid Resistance
01The Drag Force: Two Regimes of Fluid Resistance02Stokes' Law: Terminal Velocity of a Falling Sphere03Quadratic Drag: The Reciprocal Velocity DecayProblem set0/10Problem set 20/10MIT problem set0/2Practice∞
Circular Motion & Gravitation
01Newton's Second Law for Circular Motion02Universal Gravitation: Deriving the Moon's Period03Geostationary Satellites and Binary Star Orbits04Tension in Circular Motion: From Masses to a Rope05Circular Motion on a Cone and a Turntable06The Shell Theorem: Gravity Acts From the CenterProblem set0/10Problem set 20/10MIT problem set0/6Practice∞
Momentum & Center of Mass
01Impulse and Momentum: Newton's Second Law as an Integral02Drawing the System Boundary: Why Only External Forces Count03Center of Mass: From Two Particles to a Continuous Rod04Center-of-Mass Motion and Conservation of Momentum05Setting Up Any Momentum Problem: System, Axes, Diagrams06The Exploding Projectile: Where the Larger Fragment Lands07Inelastic Collision Then Friction: The Plane and the SandbagProblem set0/10Problem set 20/10MIT problem set0/5Practice∞
Relative Motion & Variable Mass
01Reference Frames and the Galilean Transformation02Relative Velocity Worked Examples: Circle and Cart03Feynman, Challenger, and the Limits of a Curve Fit04Momentum with Flowing Mass: The Four Categories05Leaking Sand vs. Blown-In Grain: Two Freight Cars06The Boat and the Fire Hose: Mass In, Momentum In07Deriving the Rocket Equation: Where Thrust Comes From08Rocket Speed, Mass Ratio, and Why Rockets StageProblem set0/10Problem set 20/10MIT problem set0/5Practice∞
Energy & Work
01Conservation of Energy: System, Boundary, and Surroundings02Kinetic Energy: From Speed Squared to Force Times Distance03Work Done by a Constant Force: Positive, Negative, or Zero04Work as Area Under the Curve and the Work-Energy Theorem05Power: Average, Instantaneous, and Force Times VelocityProblem set0/10Problem set 20/10MIT problem set0/2Practice∞
Work in Three Dimensions
01The Scalar Product: Work as Force Dot Displacement02Work as a Line Integral Along Any Curved Path03Inverse-Square Forces, 3D Work-Energy, and Power04Reduced Mass and the Work Inside a Two-Body SystemProblem set0/10Problem set 20/10MIT problem set0/1Practice∞
Conservative Forces & Potential Energy
01Conservative Forces: Why Gravity's Work Ignores the Path02The Closed-Loop Theorem: Why Conservative Forces Give Energy Back03Defining Potential Energy from Newton's Third Law04Three Potential Energies from One Recipe, and Where the Zero GoesProblem set0/10Problem set 20/10MIT problem set0/1Practice∞
Conservation of Mechanical Energy
01Conservation of Mechanical Energy: Closed Systems, Conservative Forces02The Spring Energy Diagram: Turning Points and Forbidden Regions03Stable vs Unstable Equilibrium on a Cubic Energy Diagram04Non-Conservative Forces: When Mechanical Energy Is Not Conserved05Dissipation and the System Boundary: Where Friction's Energy GoesProblem set0/10Problem set 20/10MIT problem set0/2Practice∞
Energy Methods in Practice
01Escape Velocity: Zero Total Energy on Asteroid Toro02Loop-the-Loop: Pairing Energy with Newton's Second Law03Friction That Grows With Distance: The Energy Integral04Maximum Spring Compression on a Frictional Incline05Sliding Off a Sphere: The Angle Where Contact BreaksProblem set0/10Problem set 20/10MIT problem set0/2Practice∞
Collision Theory
01Relative Velocity, Reduced Mass, and the Center-of-Mass Frame02Coefficient of Restitution and the One-Dimensional Elastic Collision03Elastic Collisions Reverse in the Center-of-Mass Frame04Stacked Superballs: Why the Small Ball Rises Nine Times Higher05Two-Dimensional Elastic Collisions in the Laboratory Frame06The Right-Angle Rule for Equal Masses, via the Dot Product07From Center-of-Mass Angle to Laboratory Angle in ScatteringProblem set0/10Problem set 20/10MIT problem set0/6Practice∞
Fixed-Axis Rotation
01Rigid Bodies and Fixed-Axis Rotation02Angular Signs: Speeding Up or Slowing Down03Rotational Kinetic Energy and Moment of Inertia04The Uniform Disc and the Parallel Axis Theorem05Energy Conservation with a Massive Pulley06The Rod-and-Disc Pendulum: Speed at the Bottom07Proving the Parallel Axis TheoremProblem set0/10Problem set 20/10MIT problem set0/3Practice∞
Rotational Dynamics
01Torque About a Point: Moment Arm and Sign Conventions02Torque by Components: A Tilted Lever and the Ankle on Tiptoe03Deriving τ = Iα: Newton's Second Law for Rotation04Center of Gravity and Unequal Tensions on a Massive Pulley05Measuring a Rotor's Moment of Inertia from Two RunsProblem set0/10Problem set 20/10MIT problem set0/1Practice∞
Rotational Work & Static Equilibrium
01Torque Through an Angle: Rotational Work and Power02Static Equilibrium and the Lever Law03The Generalized Lever Law: Forces at an Angle04The Hinged Rod and the Person on a Hill05The Knee Joint and Torque About Any PointProblem set0/10Problem set 20/10MIT problem set0/2Practice∞

Coefficient of Restitution and the One-Dimensional Elastic Collision

Why does dividing the energy equation by the momentum equation make the masses vanish and simply reverse the relative velocity?


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Your summary note

    1. 1

      Coefficient of restitution eee and the four collision types

      Define eee as the final relative speed over the initial one, and tabulate e=1e = 1e=1 with ΔK=0\Delta K = 0ΔK=0, e<1e < 1e<1, e=0e = 0e=0 with ΔK=−12μvA2\Delta K = -\frac{1}{2}\mu v_A^2ΔK=−21​μvA2​, and e>1e > 1e>1.

    2. 2

      The one-dimensional energy-momentum principle

      Factor the energy equation as a difference of squares, divide it by the momentum equation, and reach v1x,i−v2x,i=v2x,f−v1x,fv_{1x,i} - v_{2x,i} = v_{2x,f} - v_{1x,f}v1x,i​−v2x,i​=v2x,f​−v1x,f​, a relation carrying no masses.

    3. 3

      Closed-form final velocity components

      Substitute the reversed relative velocity into momentum conservation and solve for v1x,f=m1−m2m1+m2v1x,i+2m2m1+m2v2x,iv_{1x,f} = \frac{m_1-m_2}{m_1+m_2}v_{1x,i} + \frac{2m_2}{m_1+m_2}v_{2x,i}v1x,f​=m1​+m2​m1​−m2​​v1x,i​+m1​+m2​2m2​​v2x,i​ together with the mirror-image expression for v2x,fv_{2x,f}v2x,f​.

    4. 4

      Limits m1≫m2m_1 \gg m_2m1​≫m2​ and m1=m2m_1 = m_2m1​=m2​

      Expand the results for a heavy incident object, recording that the light one rebounds at the initial relative speed while equal masses simply exchange their velocity components.

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