Electric Field from Continuous Charge Distributions - Quick Notes

Continuous Charge Distributions: Quick Reference

  • Key idea: Electric field from a continuous distribution obtained by superposition of many infinitesimal charges dq.

    • At P, dE = dE=k dqr2 r^\displaystyle d\mathbf{E} = \frac{k\,dq}{r^{2}}\ \hat{\mathbf{r}} where k=14πε0k = \frac{1}{4\pi\varepsilon_{0}} and r^\hat{\mathbf{r}} points from dq to P.
    • Total field: E=∫dE=∫k dqr2 r^.\displaystyle \mathbf{E} = \int d\mathbf{E} = \int \frac{k\,dq}{r^{2}}\ \hat{\mathbf{r}}.
  • Differential charge elements and densities

    • Linear: dq=λ dl .dq = \lambda\,dl\,.
    • Surface: dq=σ dA .dq = \sigma\,dA\,.
    • Volume: dq=ρ dV .dq = \rho\,dV\,.
  • General procedure (continuous distributions)

    • Divide the charge into small elements dq.
    • Compute the field dE due to one element at P.
    • Sum (integrate) contributions from all elements: $\mathbf{E} = \int d\mathbf{E}.
  • Symmetry and direction of E

    • For symmetric objects, E points along the symmetry axis or perpendicular to symmetry planes.
    • Use components: sum along directions that survive symmetry; cancel others.
  • Common densities

    • Linear density: λ=dqdl\lambda = \dfrac{dq}{dl}
    • Surface density: σ=dqdA\sigma = \dfrac{dq}{dA}
    • Volume density: ρ=dqdV\rho = \dfrac{dq}{dV}
  • Key geometries and axis-field formulas (along symmetry axis)

    • Long straight wire (line charge density λ\lambda):
    • Magnitude: E=λ2πε0 r\displaystyle E = \frac{\lambda}{2\pi\varepsilon_{0}\,r}
    • Direction: radial outward from wire (if λ>0\lambda>0).
    • Ring of radius a
      with total charge QQ, field on axis at distance xx:
    • E(x)=kQx(x2+a2)3/2\displaystyle E(x) = \frac{k Q x}{(x^{2} + a^{2})^{3/2}}
    • Charged disk (radius RR), uniform surface density σ\sigma, axis distance zz:
    • E(z)=σ2ε0(1−zz2+R2)\displaystyle E(z) = \frac{\sigma}{2\varepsilon_{0}}\left(1 - \frac{z}{\sqrt{z^{2} + R^{2}}}\right)
    • Infinite plane with surface charge density σ\sigma:
    • Magnitude: E=σ2ε0\displaystyle E = \frac{\sigma}{2\varepsilon_{0}}
    • Direction: perpendicular to the plane, away from plane if σ>0\sigma>0.
  • Spherical and cylindrical cases

    • Solid sphere of radius RR with uniform density ρ\rho:
    • Outside (r > R): E(r)=14πε0Qr2,Q=43πR3ρ.\displaystyle E(r) = \frac{1}{4\pi\varepsilon_{0}}\frac{Q}{r^{2}}, \quad Q = \tfrac{4}{3}\pi R^{3}\rho.
    • Inside (r < R): E(r)=ρ r3ε<em>0=14πε</em>0QrR3.\displaystyle E(r) = \frac{\rho\,r}{3\varepsilon<em>{0}} = \frac{1}{4\pi\varepsilon</em>{0}}\frac{Q r}{R^{3}}.
    • Hollow spherical shell with inner radius R<em>1R<em>{1} and outer radius R</em>2R</em>{2}, density ρ=ρ06r\rho = \rho_{0}\frac{6}{r} (spherical symmetry):
    • Total charge: Q<em>shell=∫</em>R<em>1R</em>2ρ dV=12πρ<em>0 (R</em>22−R12).\displaystyle Q<em>{\text{shell}}= \int</em>{R<em>{1}}^{R</em>{2}} \rho \ dV = 12\pi\rho<em>{0}\,(R</em>{2}^{2}-R_{1}^{2}).
    • For r > R2: E(r)=14πε<em>0Q</em>shellr2.\displaystyle E(r) = \frac{1}{4\pi\varepsilon<em>{0}}\frac{Q</em>{\text{shell}}}{r^{2}}.
    • For r < R1: E(r)=0.\displaystyle E(r) = 0.
  • Nonuniform and composite shapes (examples)

    • Cylindrical shell with density ρ=ρ0 r\rho = \rho_{0}\,r for a<r<ba<r<b and height hh:
    • Total charge: Q=Q<em>shell=∫</em>abρ dV=2πhρ<em>0∫</em>abr2 dr=2πhρ03 (b3−a3).\displaystyle Q = Q<em>{shell} = \int</em>{a}^{b} \rho\,dV = 2\pi h \rho<em>{0} \int</em>{a}^{b} r^{2}\,dr = \frac{2\pi h\rho_{0}}{3}\,(b^{3}-a^{3}).
    • If h = 2b, then Q=4πbρ03 (b3−a3).Q = \frac{4\pi b\rho_{0}}{3}\,(b^{3}-a^{3}).
  • Point charge (reference)

    • For a point charge QQ at the origin, field at position r\mathbf{r}:
    • E(r)=14πε0Q∣r∣3 r=kQr2r^.\displaystyle \mathbf{E}(\mathbf{r}) = \frac{1}{4\pi\varepsilon_{0}}\frac{Q}{|\mathbf{r}|^{3}}\,\mathbf{r} = \frac{kQ}{r^{2}}\hat{\mathbf{r}}.
  • Quick example reference

    • If a single charge of Q=100 CQ=100\,\text{C} is at the origin and you evaluate at P=(3,4) mP=(3,4)\,\text{m}, the distance is r=32+42=5 mr = \sqrt{3^{2}+4^{2}} = 5\,\text{m} and the field magnitude is E=k∣Q∣r2=(8.988×109)×10025=3.5952×1010 N/CE = \dfrac{k|Q|}{r^{2}} = \dfrac{(8.988\times10^{9})\times100}{25} = 3.5952\times10^{10}\ \text{N/C} toward/away from the origin depending on the sign of Q.
  • Notes on applying to exam problems

    • Identify symmetry to pick the direction of E.
    • Choose appropriate dq, express dq in terms of the natural density for the geometry, then integrate over the region of interest.
    • Remember to include vector directions when adding contributions (use components if necessary).