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🧲Electromagnetism I

Current Density Formulas

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Why This Matters

Current density is where the rubber meets the road in electromagnetism—it's how we describe where current actually flows and how much passes through any given cross-section of material. You're being tested on your ability to connect microscopic charge motion to macroscopic current, relate electric fields to current flow through material properties, and understand how changing fields create effective currents even in empty space. These formulas appear throughout circuit analysis, magnetostatics, and Maxwell's equations.

Don't just memorize these equations—know what physical principle each one captures. Whether it's charge conservation, Ohm's law at the microscopic level, or the magnetic effects of currents, each formula represents a distinct concept that exam questions will probe. Master the "why" behind each relationship, and you'll be ready for anything from quick calculations to multi-part FRQs asking you to connect current density to fields and forces.


Microscopic Origins of Current

Current density fundamentally describes charge carriers in motion. The drift of electrons (or other carriers) through a material creates the macroscopic current we measure in circuits.

Current Density Vector

  • J=nqv\vec{J} = nq\vec{v} connects microscopic particle motion to macroscopic current—nn is number density, qq is charge per carrier, v\vec{v} is drift velocity
  • Drift velocity is typically very small (mm/s in metals), but huge carrier densities make currents substantial
  • Direction of J\vec{J} follows positive charge flow convention—opposite to electron drift in conductors

Relationship Between Current and Current Density

  • I=JdAI = \iint \vec{J} \cdot d\vec{A} defines total current as the flux of current density through a surface
  • Geometry matters—the same J\vec{J} produces different currents depending on cross-sectional area and orientation
  • Dot product means only the component of J\vec{J} perpendicular to the surface contributes to current flow

Compare: J=nqv\vec{J} = nq\vec{v} vs. I=JdAI = \iint \vec{J} \cdot d\vec{A}—both describe current, but the first is local (at a point) while the second is global (through a surface). FRQs often ask you to start with J\vec{J} and integrate to find II.


Material Response to Electric Fields

How a material responds to an applied electric field determines whether it conducts, resists, or blocks current flow. Conductivity is the bridge between fields and currents.

Ohm's Law (Microscopic Form)

  • J=σE\vec{J} = \sigma \vec{E} is the local version of Ohm's law—current density is proportional to electric field
  • Conductivity σ\sigma measures how easily charge flows; high σ\sigma means good conductor, low σ\sigma means insulator
  • Resistivity ρ=1/σ\rho = 1/\sigma is the inverse—useful for calculating resistance in specific geometries

Compare: J=σE\vec{J} = \sigma \vec{E} vs. V=IRV = IR—the first applies at every point in a material, while the second describes entire circuit elements. If asked to derive resistance from first principles, start with J=σE\vec{J} = \sigma \vec{E}.


Conservation and Continuity

Charge doesn't appear or disappear—it's conserved. The continuity equation is the mathematical statement of charge conservation applied to current flow.

Continuity Equation

  • J+ρt=0\nabla \cdot \vec{J} + \frac{\partial \rho}{\partial t} = 0 states that charge is neither created nor destroyed
  • Divergence of J\vec{J} measures net current leaving a point—if positive, charge density must decrease there
  • Steady-state condition (ρ/t=0\partial \rho / \partial t = 0) gives J=0\nabla \cdot \vec{J} = 0, meaning current has no sources or sinks

Magnetic Effects of Currents

Currents create magnetic fields, and current density tells us exactly how. Ampère's law connects the curl of B\vec{B} to the current density producing it.

Ampère's Law (Differential Form)

  • ×B=μ0J\nabla \times \vec{B} = \mu_0 \vec{J} relates magnetic field curl to current density in magnetostatics
  • μ0\mu_0 is the permeability of free space—it sets the strength of magnetic effects from currents
  • Curl operation means B\vec{B} circulates around regions of nonzero J\vec{J}—the basis for solenoid and wire problems

Magnetization Current Density

  • Jm=×M\vec{J}_m = \nabla \times \vec{M} describes effective currents from aligned magnetic dipoles in materials
  • Magnetization M\vec{M} is magnetic dipole moment per unit volume—its curl acts like a real current
  • Bound currents from magnetization contribute to B\vec{B} inside magnetic materials like iron

Compare: ×B=μ0J\nabla \times \vec{B} = \mu_0 \vec{J} vs. Jm=×M\vec{J}_m = \nabla \times \vec{M}—the first gives B\vec{B} from free currents, the second gives effective currents from magnetization. In magnetic materials, you need both to find the total field.


Time-Varying Fields and Displacement Current

When fields change in time, new types of "current" appear—even in vacuum. Displacement and polarization currents complete Maxwell's equations.

Displacement Current Density

  • Jd=ε0Et\vec{J}_d = \varepsilon_0 \frac{\partial \vec{E}}{\partial t} is the current density from a changing electric field
  • No actual charges move—this is an effective current that produces magnetic fields just like real current
  • Capacitor gaps are the classic example—Jd\vec{J}_d between plates ensures Ampère's law works everywhere

Polarization Current Density

  • Jp=Pt\vec{J}_p = \frac{\partial \vec{P}}{\partial t} arises when polarization in a dielectric changes with time
  • Polarization P\vec{P} is electric dipole moment per unit volume—bound charges shift as P\vec{P} changes
  • Dielectric response to AC fields creates oscillating Jp\vec{J}_p, contributing to energy dissipation

Compare: Jd=ε0Et\vec{J}_d = \varepsilon_0 \frac{\partial \vec{E}}{\partial t} vs. Jp=Pt\vec{J}_p = \frac{\partial \vec{P}}{\partial t}—both involve time-varying fields, but Jd\vec{J}_d exists even in vacuum while Jp\vec{J}_p requires a polarizable material. Together with free current, they give the full Ampère-Maxwell law.


Coordinate System Representations

Complex geometries require expressing J\vec{J} in appropriate coordinates. Matching your coordinate system to the problem's symmetry simplifies calculations dramatically.

Current Density in Cylindrical Coordinates

  • J=Jrr^+Jϕϕ^+Jzz^\vec{J} = J_r \hat{r} + J_\phi \hat{\phi} + J_z \hat{z} decomposes current density into radial, azimuthal, and axial components
  • Cylindrical symmetry (wires, coaxial cables, solenoids) makes JϕJ_\phi and JrJ_r often zero, leaving only JzJ_z
  • Integration for total current becomes I=0RJz(r)2πrdrI = \int_0^R J_z(r) \cdot 2\pi r \, dr for axially symmetric flow

Current Density in Spherical Coordinates

  • J=Jrr^+Jθθ^+Jϕϕ^\vec{J} = J_r \hat{r} + J_\theta \hat{\theta} + J_\phi \hat{\phi} handles radial, polar, and azimuthal components
  • Spherical symmetry (point sources, spherical shells) typically has only Jr0J_r \neq 0
  • Surface integrals use I=Jrr2sinθdθdϕI = \oint J_r \cdot r^2 \sin\theta \, d\theta \, d\phi for current through spherical surfaces

Compare: Cylindrical vs. spherical coordinates—choose cylindrical for wires, tubes, and anything with an axis of symmetry; choose spherical for point-like sources or shells. Mismatched coordinates make integrals unnecessarily painful.


Quick Reference Table

ConceptKey Formulas
Microscopic current originJ=nqv\vec{J} = nq\vec{v}
Current from current densityI=JdAI = \iint \vec{J} \cdot d\vec{A}
Ohm's law (local form)J=σE\vec{J} = \sigma \vec{E}
Charge conservationJ+ρt=0\nabla \cdot \vec{J} + \frac{\partial \rho}{\partial t} = 0
Magnetic field from current×B=μ0J\nabla \times \vec{B} = \mu_0 \vec{J}
Displacement currentJd=ε0Et\vec{J}_d = \varepsilon_0 \frac{\partial \vec{E}}{\partial t}
Magnetization currentJm=×M\vec{J}_m = \nabla \times \vec{M}
Polarization currentJp=Pt\vec{J}_p = \frac{\partial \vec{P}}{\partial t}

Self-Check Questions

  1. What physical principle does the continuity equation J+ρt=0\nabla \cdot \vec{J} + \frac{\partial \rho}{\partial t} = 0 express, and what does it simplify to in steady-state conditions?

  2. Compare J=σE\vec{J} = \sigma \vec{E} and V=IRV = IR: which is more fundamental, and how would you derive the macroscopic form from the microscopic one?

  3. Both Jd\vec{J}_d and Jp\vec{J}_p involve time derivatives—what's the key physical difference between displacement current in vacuum and polarization current in a dielectric?

  4. If you're calculating the magnetic field around a long straight wire, which coordinate system should you use for J\vec{J}, and which component of J\vec{J} will be nonzero?

  5. An FRQ gives you J(r)=J0er/az^\vec{J}(r) = J_0 e^{-r/a} \hat{z} for a cylindrical wire of radius RR. Set up (but don't solve) the integral for total current II, and explain why the exponential form means current concentrates near the wire's axis.