Work-Energy Principle for Particles

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dynamics work energy kinetic energy potential energy conservation

Core Idea

The work-energy principle states that net work done on a particle equals its change in kinetic energy: U₁₋₂ = T₂ − T₁, where T = ½mv². Work by a force along a path is U = ∫F·dr. Conservative forces (gravity, springs) have associated potential energy: V_g = mgh, V_e = ½kx². For conservative systems, total mechanical energy is conserved: T₁ + V₁ = T₂ + V₂. When non-conservative forces (friction, applied forces) act, the work they do modifies the energy balance: T₁ + V₁ + U₁₋₂(nc) = T₂ + V₂.

How It's Best Learned

Classify every force as conservative or non-conservative. For conservative systems, apply energy conservation directly between two states without integrating equations of motion. For problems with friction or variable applied forces, compute work integrals explicitly.

Common Misconceptions

Explainer

Newton's second law and the work-energy principle are two ways to analyze the same motion, but they are not equally convenient for every problem. Newton's law requires tracking acceleration at each instant; work-energy connects two states — a start and an end — using scalar energy quantities, avoiding vectors and integration of force over time. Whenever you care only about how fast a particle is moving at one point given its speed at another, work-energy is usually faster.

The central equation is U₁₋₂ = T₂ − T₁, where U₁₋₂ = ∫F·dr is the net work done on the particle between states 1 and 2, and T = ½mv² is kinetic energy. Work is a dot product: only the component of force along the displacement contributes. This is why a normal force — always perpendicular to motion along a surface — does zero work. Gravity does work equal to mg times the vertical drop, regardless of the path taken; this path-independence is the hallmark of a conservative force.

For conservative forces (gravity and ideal springs), we define potential energy so that work can be expressed as a change in stored energy: U_gravity = −ΔV_g = −mgΔh, U_spring = −ΔV_e = −Δ(½kx²). When only conservative forces act, T + V = constant, which is the conservation of mechanical energy. This is a powerful shortcut: pick any two points on the path, write the energy balance, and solve — no need to integrate equations of motion.

When non-conservative forces act — friction, air drag, applied motors — they add or remove mechanical energy. The modified equation is T₁ + V₁ + U₁₋₂(nc) = T₂ + V₂. Friction always contributes a negative U(nc) equal to the friction force times the distance slid. The key habit is first classifying every force: conservative (gets a potential energy term) or non-conservative (its work must be computed explicitly and added to the equation). Missing a friction term, or including the normal force as a contributor, are the two most common sources of wrong answers.

Spring problems carry an additional trap: the deformation x in ½kx² must be measured from the spring's natural (unstretched) length, not from an arbitrary reference position. If the spring is pre-compressed by x₀ and then further compressed to x₁, the change in spring potential energy is ½k(x₁² − x₀²), not ½k(x₁ − x₀)². Computing ½k(Δx)² instead of Δ(½kx²) is a systematic error that gives wrong answers whenever the spring has any initial deformation.

Practice Questions 3 questions

Prerequisite Chain

Counting to 10Counting to 20Understanding ZeroThe Number ZeroCounting to FiveOne-to-One CorrespondenceCombining Small Groups Within 5Addition Within 10Addition Within 20Two-Digit Addition Without RegroupingTwo-Digit Addition with RegroupingAddition Within 100Repeated Addition as MultiplicationMultiplication Facts Within 100Division as Equal SharingDivision as Grouping (Measurement Division)Division: Grouping (Repeated Subtraction) ModelDivision: Fair Sharing ModelDivision as Equal SharingDivision as GroupingBasic Division FactsDivision Facts Within 100Two-Digit by One-Digit DivisionDivision with RemaindersRemainders and Quotients in DivisionDivision Word ProblemsIntroduction to Long DivisionFactors and MultiplesPrime and Composite NumbersEquivalent FractionsRelating Fractions and DecimalsDecimal Place ValueReading and Writing DecimalsComparing and Ordering DecimalsAdding and Subtracting DecimalsMultiplying DecimalsDividing DecimalsDividing FractionsMixed Number ArithmeticOrder of OperationsInteger Order of OperationsVariable ExpressionsCombining Like TermsOne-Step EquationsTwo-Step EquationsSolving Multi-Step EquationsEquations with Variables on Both SidesAngle Pairs: Complementary, Supplementary, and VerticalParallel Lines and TransversalsCorresponding AnglesAlternate Interior AnglesTriangle Angle Sum TheoremExterior Angle TheoremTriangle Inequality TheoremSimilar Triangles: AA SimilaritySimilar Triangles: SSS and SAS SimilarityProportions in Similar TrianglesRight Triangle Trigonometry IntroductionTrigonometric Ratios ReviewRadian MeasureConverting Between Degrees and RadiansThe Unit CircleGraphing Sine and CosineGraphing Tangent and Reciprocal Trigonometric FunctionsDerivatives of Trigonometric FunctionsAntiderivativesIterated Integrals and Fubini's TheoremDouble Integrals in Cartesian CoordinatesDouble Integrals over Rectangular RegionsDouble Integrals in Polar CoordinatesDouble Integrals: Definition and SetupIterated Integrals and Fubini's TheoremDouble Integrals over Rectangular RegionsDouble Integrals over General RegionsApplications of Double Integrals: Area, Mass, and MomentsCenter of MassConservation of Linear MomentumElastic CollisionsInelastic CollisionsCoefficient of RestitutionCollision Analysis and Real-World ApplicationsTwo-Body Collisions in the Center-of-Mass FrameReduced Mass and Two-Body ProblemsKinematics in Two DimensionsProjectile MotionCircular Motion: KinematicsRotational KinematicsTorqueMoment of InertiaRotational Kinetic EnergyThe Work-Energy TheoremConservation of Mechanical EnergyWork-Energy Principle for Particles

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