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Momentum Density in Electromagnetic Fields

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Electromagnetic Field Energy and ConservationPoynting Vector and Electromagnetic Energy Flow+1 more→→Angular Momentum Density in Electromagnetic FieldsMaxwell Stress Tensor and Field Forces
momentum-density radiation-pressure field-momentum

Core Idea

Electromagnetic fields carry momentum density g = S/c² = (ε₀/c²)(E × B), where S is the Poynting vector. This momentum transfers to matter in the form of radiation pressure, with magnitude equal to energy density divided by c².

Explainer

You've already established from the Poynting vector that electromagnetic fields carry energy, with energy flux S = (1/μ₀)(E × B) measured in watts per square meter. The deeper and perhaps more surprising result is that fields also carry momentum. This isn't obvious classically — momentum seems like a property of matter — but it follows inescapably from the requirement that momentum be conserved when light interacts with matter.

Here's the argument: when an electromagnetic wave hits an absorbing surface and the charges in the surface begin to move, the Lorentz force F = q(E + v×B) has two parts. The electric field accelerates the charges, and then the magnetic field exerts a force on those moving charges. This secondary magnetic force is directed along the propagation direction of the wave — it pushes the surface forward. Something must be carrying that momentum before the wave is absorbed, and that something is the field itself. The momentum density is g = S/c² = ε₀(E × B), pointing in the same direction as the energy flow, with magnitude equal to the energy density divided by c.

The transfer of field momentum to matter is called radiation pressure. For a plane wave with energy density u, the radiation pressure on a perfect absorber is P = u (in SI units of N/m²), and on a perfect reflector it's P = 2u (because the momentum reverses). These are tiny forces in everyday life — the radiation pressure of sunlight on Earth is about 5 μPa — but they become significant in astrophysics (stellar winds blow material away from stars), in optical trapping (laser tweezers grip microscopic beads), and in proposed solar sail spacecraft.

The relationship g = S/c² has a profound implication: energy and momentum in electromagnetic fields are not independent, but tied by g = u/c = energy/(c·volume). This is exactly the relationship for massless particles, and it foreshadows the photon picture in quantum mechanics — photons carry energy E = hf and momentum p = h/λ = E/c. The classical result for field momentum per unit volume matches the quantum mechanical count of photon momenta, confirming that even the classical field theory anticipates the quantum nature of light.

Practice Questions 5 questions

Prerequisite Chain

Understanding Zero → The Number Zero → Counting to Five → Counting to 10 → Counting to 20 → Counting a Set of Objects Up to 20 → Cardinality: The Last Number Counted → Matching Numerals to Quantities → Subitizing Small Quantities → Addition Within 10 → Number Bonds to 10 → Addition Within 20 → Doubles and Near Doubles → Doubles Facts Within 10 → Near Doubles Facts Within 20 → Mental Math Strategies for Addition → Mental Math: Adding and Subtracting Tens → Addition Within 100 → Repeated Addition as Multiplication → Multiplication as Equal Groups → Multiplication: Arrays → Basic Multiplication Facts (0s, 1s, 2s, 5s, 10s) → Multiplication Facts Within 100 → Division as Equal Sharing → Division as Grouping (Measurement Division) → Division: Grouping (Repeated Subtraction) Model → Division: Fair Sharing Model → Division as Equal Sharing → Division as Grouping → Basic Division Facts → Division Facts Within 100 → Multiplication and Division Fact Families → Relationship Between Multiplication and Division → Division Facts as Inverse of Multiplication → Remainders and Quotients in Division → Division Word Problems → Multi-Step Word Problems → Solving Multi-Step Word Problems → Multiplication Word Problems → Division Word Problems → Introduction to Long Division → Factors and Multiples → Prime and Composite Numbers → Equivalent Fractions → Relating Fractions and Decimals → Decimal Place Value → Integers and the Number Line → Comparing and Ordering Integers → Absolute Value → Adding Integers → Subtracting Integers → Multiplying Integers → Dividing Integers → Unit Rates → Proportions → Percent Concept → Converting Between Fractions, Decimals, and Percents → Operations with Rational Numbers → Two-Step Equations → Solving Multi-Step Equations → Equations with Variables on Both Sides → Angle Pairs: Complementary, Supplementary, and Vertical → Parallel Lines and Transversals → Corresponding Angles → Alternate Interior Angles → Triangle Angle Sum Theorem → Exterior Angle Theorem → Triangle Inequality Theorem → Similar Triangles: AA Similarity → Similar Triangles: SSS and SAS Similarity → Proportions in Similar Triangles → Right Triangle Trigonometry Introduction → Sine, Cosine, and Tangent Ratios → Trigonometric Ratios Review → Radian Measure → Converting Between Degrees and Radians → The Unit Circle → Graphing Sine and Cosine → Graphing Tangent and Reciprocal Trigonometric Functions → Derivatives of Trigonometric Functions → Antiderivatives → Indefinite Integrals → Basic Integration Rules → Riemann Sums → Definite Integral Definition → Double Integrals: Definition and Setup → Iterated Integrals and Fubini's Theorem → Double Integrals over Rectangular Regions → Double Integrals over General Regions → Applications of Double Integrals: Area, Mass, and Moments → Center of Mass → Conservation of Linear Momentum → Elastic Collisions → Inelastic Collisions → Coefficient of Restitution → Collision Analysis and Real-World Applications → Two-Body Collisions in the Center-of-Mass Frame → Reduced Mass and Two-Body Problems → Kinematics in Two Dimensions → Projectile Motion → Circular Motion: Kinematics → Circular Motion: Dynamics and Centripetal Force → Magnetic Dipole Moment from Current Loops → Force on Current-Carrying Conductors in Magnetic Fields → Biot-Savart Law → Ampère's Law → Magnetic Flux and Electromagnetic Induction → Faraday's Law of Electromagnetic Induction → Faraday's Law of Induction → Maxwell's Equations in Integral Form → Maxwell's Equations in Differential Form → Derivation of the Electromagnetic Wave Equation → Plane Electromagnetic Waves → Poynting Vector and Electromagnetic Energy Flow → Electromagnetic Angular Momentum → Momentum Density in Electromagnetic Fields

Longest path: 116 steps · 849 total prerequisite topics

Prerequisites (3)

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