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Potential due to a System of Charges

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Estimated time: 12 minutes
CBSE: Class 12

Definition: Electrostatic Potential

The electrostatic potential V at a point in an electric field is defined as the work done by an external force in bringing a unit positive charge (without acceleration) from infinity to that point.

CBSE: Class 12

Formula: Electrostatic Potential

V = \[\frac{W_{\infty\to P}}{q_{0}}\] (Work done per unit positive charge)

SI Unit: Volt (V) = Joule/Coulomb (J/C);
Dimensional Formula: [M1L2T−3A−1]

CBSE: Class 12

Potential Due to a System of Point Charges

When multiple point charges are present, the total potential at any point equals the algebraic sum of potentials due to each individual charge. This follows directly from the superposition principle. Since potential is a scalar, we simply add numbers — no vector components or angles required.

Derivation (Step-by-Step)

Setup: Consider nn point charges q1,q2,…,qn​ at distances r1P,r2P,…,rnP from a point P.

Step 1: Potential at P due to charge q1​ alone:

V1 = \[\frac{1}{4\pi\varepsilon_0}\cdot\frac{q_1}{r_{1P}}\]

Step 2: Similarly, for each charge qi​:

Vi = \[\frac{1}{4\pi\varepsilon_0}\cdot\frac{q_i}{r_{iP}}\]

Step 3: By the superposition principle, the total potential at P:

V = V1 + V2 + ⋯ + Vn   ...(2.17)
V = \[{\frac{1}{4\pi\varepsilon_{0}}\left(\frac{q_{1}}{r_{1P}}+\frac{q_{2}}{r_{2P}}+\cdots+\frac{q_{n}}{r_{nP}}\right)=\frac{1}{4\pi\varepsilon_{0}}\sum_{i=1}^{n}\frac{q_{i}}{r_{iP}}}\]   ...(2.18)
CBSE: Class 12

Potential Due to a Continuous Charge Distribution

For a continuous charge distribution with volume charge density ρ(r):

  • Divide the distribution into infinitesimal volume elements, each of size Δv carrying charge ρ⋅Δv
  • Find potential due to each element
  • Integrate over the entire distribution
    V(r) = \[\frac{1}{4\pi\varepsilon_0}\int\frac{\rho(\mathbf{r}^{\prime})}{|\mathbf{r}-\mathbf{r}^{\prime}|}dv^{\prime}\]
CBSE: Class 12

Potential of a Uniformly Charged Spherical Shell

4.1 Three Cases

Region Condition Electric Field ((E)) Potential ((V))
Outside the shell (r > R) \[\displaystyle E=\frac{1}{4\pi\varepsilon_0}\frac{q}{r^2}) (radially outward\] \[\displaystyle V=\frac{1}{4\pi\varepsilon_0}\frac{q}{r}\]
On the surface (r = R) \[\displaystyle E=\frac{1}{4\pi\varepsilon_0}\frac{q}{R^2}\] \[\displaystyle V=\frac{1}{4\pi\varepsilon_0}\frac{q}{R}\]
Inside the shell (r < R) \[\displaystyle E=0) (everywhere\] \[\displaystyle V=\frac{1}{4\pi\varepsilon_0}\frac{q}{R}=\text{constant}\]
 
 

4.2 Key Equations

Outside (r ≥ R):

V = \[{\frac{1}{4\pi\varepsilon_0}\cdot\frac{q}{r}}\]   ...[2.19(a)]

Inside (r < R):

V = \[{\frac{1}{4\pi\varepsilon_0}\cdot\frac{q}{R}}\] = constant   ...[2.19(b)]
 

Example 1

Example 2

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