Coulomb force and electric field
From the force between stationary point charges to the vector field of an arbitrary charge distribution: source/observation coordinates, superposition, dimensional checks, symmetry, the infinite-line integral, point-source singularities, and the difference between the model of a static source and physical measurements with moving probes.
- State Coulomb's law as a vector force with a consistent source-to-observer displacement and SI dimensions.
- Separate the force on a test charge from the electric field produced by the other charges; state the ideal-test-charge limit.
- Derive point-source and finite-discrete-source fields and show superposition component by component.
- Convert discrete sums to charge-density integrals and correctly include the differential charge element dq.
- Compute a finite dipole's on-axis field and identify its far-field scaling without substituting the far-field formula near the charges.
- Derive the field of an ideal infinite uniformly charged line by a convergent integral and state its idealization.
- Use parity/symmetry to cancel components before integrating; distinguish true cancellation from omitted vector directions.
- Describe electric-field lines without confusing a drawing convention with a dynamical particle trajectory.
- Identify singular/self-field limitations and the scope of electrostatics in vacuum.
- Solve numerical and symbolic exercises with SI units, sign checks and a limiting-case validation.
How can a charge act on a distant charge without putting a fictitious force arrow at every point in space? We define a source-generated vector field, then compute that field at any observation point. This chapter assumes stationary charge distributions in vacuum and treats point charges as idealized sources with a singular location.
01.1Charges, SI units, and the model boundary
Electric charge q is signed and measured in coulombs (C). In a vacuum, the SI permittivity ε₀ relates charge to the electrostatic field; write k=1/(4π ε₀). In engineering estimates, k≈8.99×10⁹ N·m²/C². Coulomb's force law models the interaction of stationary point charges separated by a nonzero distance, not a self-force at the source location.
The field produced by prescribed static sources is not altered in this ideal model by an infinitesimal test charge. A finite probe can perturb a source distribution; real current-carrying or moving systems require a broader electromagnetic description.
The displacement is R=r−r′, FROM source TO observation. For the displayed q>0, E(r)=qR̂/(4πε0R2) points right. F=q0E is right only for q0>0; reversing the test-charge sign reverses F without reversing E. The drawing is not a field-line diagram.
01.2Derive a vector law rather than guessing a direction
Place a source charge q₁ at position r₁ and a second stationary charge q₂ at r₂. The displacement from the source to the observation point is R=r₂−r₁, with R=|R| and unit vector R̂=R/R. The force ON charge 2 BY charge 1 is
If q₁q₂ is positive, force on 2 points from source 1 toward observation 2 (repulsion); if negative it points toward the source (attraction). Interchanging source and observation gives R→−R and F₁←₂=−F₂←₁. The vector formula stores the sign; do not attach a second ad hoc sign to R̂.
01.3Define E independently of the test-charge magnitude
Choose a test charge qₜ at observation point r. Let Fₜ,ext be the electrostatic force exerted on it by OTHER charges. Formally the field at r is the small-test-charge limit of force divided by charge, with prescribed sources held fixed:
The limit is operational: it removes probe-induced disturbance. A negative qₜ experiences force opposite E; the field direction itself is defined by the force on a positive test charge. At the location of an ideal point source its own field formula diverges, so never evaluate that source's self-field by substituting r=r₁.
01.4Point-charge field and the superposition principle
Insert the vector force of §01.2 into the definition of E and cancel qₜ. For a point source qᵢ located at rᵢ, and observation r distinct from every source position,
Superposition is vector addition. In Cartesian coordinates calculate Ex, Ey and Ez separately; adding field magnitudes generally fails. The formula assumes a fixed linear vacuum model. In a material, polarization can change the total source distribution and must be modeled explicitly.
01.5One numerical vector check
Let q=+3.00 nC be at the origin and observe at r=(0.200 m,0,0). Here R=0.200 m and R̂=+x̂, so
For a −2.00 nC test charge at the same point, F=qₜE≈−1.35×10⁻⁶ x̂ N. The negative force sign follows solely from qₜ; the field did not reverse. The result scales as 1/R² and is undefined at R=0 in the point-source idealization.
01.6From discrete charges to continuous source densities
Partition a finite distribution into small elements dq. A fixed observation r sees each source element at r′. Taking the continuum limit replaces the sum by an integral. Do not substitute a one-dimensional density into a volume element:
λ has C/m, σ has C/m², and ρ has C/m³; the primed coordinates label the SOURCE and the unprimed coordinates label the fixed observation point. The integral excludes or treats carefully singular source–observation coincidences; an ideal zero-thickness charged surface can have different one-sided limiting fields.
01.7Symmetry is an algebraic cancellation, not a picture
For a uniformly charged infinite line along the z axis, inspect the point (s,0,0), s>0. Source elements at +z′ and −z′ have equal x components and opposite z components. Hence Ez cancels and E points radially away from the line if λ>0 (toward it if λ<0). This cancellation follows by pairing integrand values; it is valid before integrating.
This method fails if the charge density is not symmetric: if λ(z′) differs from λ(−z′), the paired z components do not cancel. The full integral must then be retained.
01.8Integrate the uniformly charged infinite line
After the odd component has vanished, perform the remaining convergent integral. For s>0,
The 1/s falloff differs from the point source's 1/R² because an infinite line contains arbitrarily remote contributing charges. The idealization fails near the finite wire's ends and at distances comparable to its finite radius; at s=0 the ideal infinitely thin line is singular.
01.9Finite dipole and a controlled far-field limit
Take +q at z=+a and −q at z=−a (q>0). On the positive z axis at z>a, the positive charge pushes toward +z while the negative charge pulls toward −z. Therefore
The exact expression is valid only on this axis segment and excludes z=a; the 1/z³ expression is the leading far-field term. Approaching a charge with the dipole approximation is invalid. The dipole vector p points from −q to +q; the full angular field will be derived later from the potential.
01.10Field lines, physical limitations, and mastery exercises
Field lines are tangent to E where E is nonzero; their arrow direction is the force direction for a POSITIVE test charge. Their drawn density is a visualization convention, not an additional equation or charge trajectory. A particle trajectory depends on inertia, initial velocity and any magnetic field. Never assume field lines can replace vector components or boundary conditions.
- Prove F₁←₂=−F₂←₁ by exchanging r₁ and r₂ in the vector formula.
- Compute E at r=(0.200 m,0,0) for q=−3.00 nC at the origin. What is the force on a positive +2.00 nC probe?
- Two equal +1.00 nC charges sit at (−0.030 m,0) and (+0.030 m,0). Find the field at (0,+0.040 m); justify the vanished component.
- For λ=+1.00 nC/m and s=0.020 m, compute the ideal-line field and check its units.
- For +q at +a and −q at −a, derive the exact axial dipole expression by combining denominators and identify the condition for the far-field formula.
- Give two reasons an electrostatic field line is generally not the trajectory of a released charged particle.
Worked solutions and validity checks
1. Exchange indices: R′=r₁−r₂=−R, while q₁q₂ is unchanged; hence the force reverses.
2. E=−6.74×10² x̂ N/C. A +2.00 nC probe feels F=−1.35×10⁻⁶ x̂ N. Field and force share direction only for a positive probe.
3. Each source is at distance 0.050 m. Horizontal components are equal and opposite. Vertical component from one is k(1.00×10⁻⁹)(0.040)/(0.050)³≈2.876×10³ N/C, so E≈+5.75×10³ ŷ N/C.
4. E=2kλ/s≈2(8.99×10⁹)(1.00×10⁻⁹)/(0.020)=8.99×10² N/C, outward. kλ/s has units (N·m²/C²)(C/m)/m=N/C.
5. [(z+a)²−(z−a)²]/(z²−a²)²=4az/(z²−a²)². For z≫a, (z²−a²)²≈z⁴, giving 4kqa/z³=2kp/z³.
6. Nonzero mass and initial velocity make the trajectory a solution of Newton's equation, not a static tangent curve; a negative probe accelerates opposite E, and magnetic forces can further bend its path.
Next: Chapter 02 builds electric potential from the work done by this static field, and fixes the sign of the potential difference before introducing Gauss's law.