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Class 12 Physics β€’ Class Notes
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Class 12 Physics: Electrostatic Potential & Capacitance

2.1 Electrostatic Potential and Potential Difference

Conservative Nature of the Electrostatic Force

Core Definitions
Figure 2.1 β€” Work done in moving a charge between two points in an electric field
Figure 2.1 β€” Work done in moving a charge between two points in an electric field

Derivation: Potential due to a Single Point Charge

Let a source charge $+q$ be at origin O. We find the potential at point P, at a distance $r$ from O. We bring a test charge $+q_0$ from infinity to P very slowly (in equilibrium, no kinetic energy gained) along any path (say, radial).

At an intermediate distance $x$ from origin, the electrostatic (repulsive) force on the test charge is: $$\vec{F}_{elec} = \frac{1}{4\pi\epsilon_0} \frac{q \cdot q_0}{x^2} \hat{x} \quad \text{(directed away from O, i.e., outward)}$$

The external force required to move it without acceleration: $\vec{F}_{ext} = -\vec{F}_{elec}$ (directed inward).

Work done by external force from $\infty$ to $r$: $$W = \int_\infty^r \vec{F}_{ext} \cdot d\vec{x} = \int_\infty^r \left(-\frac{1}{4\pi\epsilon_0} \frac{q q_0}{x^2}\right)(-dx)$$ $$W = \frac{q q_0}{4\pi\epsilon_0} \int_\infty^r \frac{dx}{x^2}$$ $$= \frac{q q_0}{4\pi\epsilon_0}\left[-\frac{1}{x}\right]_\infty^r$$ $$= \frac{q q_0}{4\pi\epsilon_0}\left(-\frac{1}{r} + \frac{1}{\infty}\right) = \frac{q q_0}{4\pi\epsilon_0 r}$$

Since $V = \frac{W}{q_0}$, we get:

Formula: Potential due to Point Charge $$\boxed{V = \frac{1}{4\pi\epsilon_0} \frac{q}{r} = \frac{kq}{r}}$$

Superposition Principle for Potential

Since potential is a scalar quantity, the net potential at a point due to a system of $n$ charges is simply the algebraic sum of the individual potentials. No vector addition needed!

$$V_{net} = V_1 + V_2 + \cdots + V_n = \frac{1}{4\pi\epsilon_0}\sum_{i=1}^{n}\frac{q_i}{r_i}$$

where $r_i$ is the distance of the $i$-th charge from the point in question, and $q_i$ carries its sign.

2.1 (Continued) β€” Potential due to an Electric Dipole

A dipole consists of two equal and opposite charges $+q$ and $-q$ separated by a small distance $2a$, with dipole moment $\vec{p} = q \times 2a$ directed from $-q$ to $+q$.

Derivation: General Formula for Dipole Potential at Point P($r$, $\theta$)

Let point P be at distance $r$ from the centre O of the dipole. Let OP make angle $\theta$ with the dipole axis (direction of $\vec{p}$). Let $r_1$ = distance from $+q$ to P, and $r_2$ = distance from $-q$ to P.

For a short dipole ($r \gg a$), using the perpendicular dropped from $+q$ and $-q$ to line OP:

Net potential at P: $$V = \frac{1}{4\pi\epsilon_0}\left[\frac{q}{r_1} + \frac{(-q)}{r_2}\right]$$ $$= \frac{q}{4\pi\epsilon_0}\left[\frac{1}{r-a\cos\theta} - \frac{1}{r+a\cos\theta}\right]$$ $$V = \frac{q}{4\pi\epsilon_0}\cdot\frac{(r+a\cos\theta)-(r-a\cos\theta)}{r^2-a^2\cos^2\theta}$$ $$= \frac{q}{4\pi\epsilon_0}\cdot\frac{2a\cos\theta}{r^2-a^2\cos^2\theta}$$

Since $r \gg a$, we have $r^2 \gg a^2\cos^2\theta$, so we drop $a^2\cos^2\theta$. Also $q \times 2a = p$:

Formula: Dipole Potential at General Point $$\boxed{V = \frac{1}{4\pi\epsilon_0}\frac{p\cos\theta}{r^2}}$$

Special Cases of Dipole Potential

Figure 2.2 β€” Electric Dipole: Geometry for Potential Derivation
Figure 2.2 β€” Electric Dipole: Geometry for Potential Derivation

2.2 Equipotential Surfaces

Definition: A surface (real or imaginary) on which the electric potential has the same value at every point is called an equipotential surface. Moving a charge along such a surface requires zero work since $\Delta V = 0$.

Properties of Equipotential Surfaces β€” High Yield for Boards/NEET/JEE
  1. No work is done in moving a charge along an equipotential surface.
    Since $\Delta V = 0$ for any two points on the surface, $W = q \Delta V = 0$. Therefore the electrostatic force does zero work along the surface.
  2. Electric field lines are always perpendicular (normal) to an equipotential surface.
    Proof: If $\vec{E}$ had a component $E_{\parallel}$ parallel to the surface, work done moving charge $q$ by displacement $ds$ along the surface would be $W = qE_{\parallel}ds \neq 0$. This contradicts property 1. Hence $\vec{E} \perp$ equipotential surface at every point.
  3. Two equipotential surfaces can never intersect each other.
    If they intersected at a point, that point would have two different potential values β€” which is physically impossible (potential is a single-valued function of position).
  4. Equipotential surfaces are closer together where the electric field is stronger.
    Since $E = -\frac{dV}{dr}$, a large $E$ means a large change in $V$ over a small distance β€” so the surfaces are crowded (closer spacing). The field is strong near a positive charge, so surfaces are closer near it.
  5. The surface of a conductor in equilibrium is always an equipotential surface.
    Since $E = 0$ inside a conductor, $-\frac{dV}{dr} = 0 \Rightarrow V =$ constant inside and on the surface.
  6. Relation: $E = -\frac{dV}{dr}$ β€” Electric field is negative gradient of potential. Field points in the direction of decreasing potential (from high $V$ to low $V$).

Shapes of Equipotential Surfaces for Different Charge Configurations

Charge ConfigurationShape of Equipotential SurfacesShape of Field Lines
Isolated Positive Point ChargeConcentric spheres centred on the charge (closer near charge, farther away)Radial straight lines pointing outward from the charge
Isolated Negative Point ChargeConcentric spheres centred on the chargeRadial straight lines pointing inward towards the charge
Uniform Electric Field (e.g., between large plates)Flat planes perpendicular to the field direction (equally spaced)Parallel straight lines (equally spaced)
Electric DipoleComplex 3D surfaces β€” near each charge they look like spheres, but in between they form saddle-shaped surfacesFrom $+q$ to $-q$, curving around; like loops of a bar magnet
Surface of a ConductorThe surface itself is equipotential; entire interior volume is also equipotentialLines emerge perpendicular to the conductor surface
Figure 2.3 β€” Equipotential Surfaces for Different Charge Configurations
Figure 2.3 β€” Equipotential Surfaces for Different Charge Configurations

Relation Between Electric Field and Potential Gradient

Consider moving a unit positive charge through a small displacement $dr$ in the direction of field $\vec{E}$. The work done by the field: $dW = E\,dr$. By definition $dW = -dV$. Therefore:

$$\boxed{E = -\frac{dV}{dr}}$$

The quantity $\frac{dV}{dr}$ is called the potential gradient. SI unit: V/m (same as N/C for electric field).

2.3 Potential Energy of a System of Charges

A. Potential Energy of Two Point Charges

Formula: PE of Two Point Charges $$\boxed{U = \frac{1}{4\pi\epsilon_0}\frac{q_1 q_2}{r_{12}}}$$

B. Potential Energy of a System of Three or More Charges

For $n$ charges, calculate the potential energy for every distinct pair and add algebraically. For $n$ charges, there are $\dfrac{n(n-1)}{2}$ pairs.

For three charges $q_1, q_2, q_3$ at mutual separations $r_{12}, r_{23}, r_{13}$:

$$\boxed{\begin{aligned} U &= \frac{1}{4\pi\epsilon_0} \Big[ \frac{q_1 q_2}{r_{12}} \\ & \quad + \frac{q_2 q_3}{r_{23}} + \frac{q_1 q_3}{r_{13}} \Big] \end{aligned}}$$

2.4 Potential Energy in an External Field

A. Single Charge $q$ at Position $\vec{r}$ in External Field

If the external field creates a potential $V(\vec{r})$ at the position of charge $q$:

$$\boxed{U = qV(\vec{r})}$$

Example: A charge $+Q$ placed at a point where external potential is $V_0$ has PE = $QV_0$. If $V_0 > 0$ and $Q > 0$, then $U > 0$ (energy was stored).

B. System of Two Charges in an External Field

Consider two charges $q_1$ at $\vec{r_1}$ and $q_2$ at $\vec{r_2}$ in an external field that produces potentials $V(\vec{r_1})$ and $V(\vec{r_2})$ at their positions. The total PE has three contributions:

$$\boxed{U = q_1 V(\vec{r}_1) + q_2 V(\vec{r}_2) + \frac{1}{4\pi\epsilon_0}\frac{q_1 q_2}{r_{12}}}$$

C. Potential Energy of a Dipole in a Uniform External Field β€” Derivation

A dipole $\vec{p}$ placed in a uniform external field $\vec{E}$ at angle $\theta$ with the field experiences a torque that tends to align it. The torque magnitude: $\tau = pE\sin\theta$.

Work done by external torque to rotate dipole from angle $\theta_1$ to $\theta_2$: $$W = \int_{\theta_1}^{\theta_2}\tau\,d\theta = pE\int_{\theta_1}^{\theta_2}\sin\theta\,d\theta = pE[-\cos\theta]_{\theta_1}^{\theta_2} = pE(\cos\theta_1 - \cos\theta_2)$$

Taking $\theta_1 = 90Β°$ as the reference position ($U = 0$) and $\theta_2 = \theta$: $$W = pE(\cos90Β° - \cos\theta) = pE(0 - \cos\theta) = -pE\cos\theta$$ This work equals the potential energy stored:

Formula: PE of Dipole in Uniform Field $$\boxed{U = -\vec{p}\cdot\vec{E} = -pE\cos\theta}$$
Orientation (ΞΈ)PE (U)StabilityTorque
$0^\circ$ (aligned with field)$-pE$ (minimum)Stable equilibrium$0$ (no tendency to rotate)
$90^\circ$ (perpendicular)$0$ (reference)Neither stable nor unstable$pE$ (maximum)
$180^\circ$ (anti-parallel)$+pE$ (maximum)Unstable equilibrium$0$ (but any small displacement rotates it)
Figure 2.4 β€” Dipole in Uniform External Electric Field: PE and Torque
Figure 2.4 β€” Dipole in Uniform External Electric Field: PE and Torque

2.5 Electrostatics of Conductors

5 Golden Properties of Conductors in Electrostatic Equilibrium
  1. Net electric field inside a conductor is ZERO ($\vec{E}_{inside} = 0$).
    Reason: In electrostatic equilibrium, free electrons are stationary. If $E \neq 0$ inside, electrons would experience force $F = eE$, move, constitute a current β€” contradicting equilibrium. So $E = 0$ at all interior points.
  2. All excess charge resides ONLY on the outer surface.
    Reason (by Gauss's Law): Draw any closed surface inside the conductor material. Since $E = 0$ inside, flux through this Gaussian surface $= 0 \Rightarrow q_{enclosed} = 0$. Hence no net charge at any interior point. All charge is on the surface.
  3. Electric potential is constant throughout the volume AND surface of a conductor.
    Reason: Since $E = 0$ inside, $-\frac{dV}{dr} = 0 \Rightarrow V$ = constant. The conductor (interior + surface) is an equipotential region.
  4. Electric field just outside the surface is perpendicular to the surface and has magnitude $\dfrac{\sigma}{\epsilon_0}$.
    Where $\sigma$ is the local surface charge density. If $E$ had a tangential (parallel) component, it would drive surface currents β€” violating electrostatics.
  5. Charge density is non-uniform on an irregular conductor: highest at regions of greatest curvature (sharp tips).
    Since $E = \sigma/\epsilon_0$, the electric field is also strongest near sharp points. This is the principle behind lightning rods (corona discharge / point discharge).

Electrostatic Shielding

The interior cavity of a hollow conductor is completely shielded from external electric fields.

Applications:

Figure 2.5 β€” Electrostatic Shielding: Hollow Conductor in External Field
Figure 2.5 β€” Electrostatic Shielding: Hollow Conductor in External Field

2.6 Dielectrics and Polarisation

Types of Dielectric Molecules

PropertyNon-polar MoleculesPolar Molecules
Centre of positive chargeCoincides with centre of negative chargeDoes NOT coincide with centre of negative charge
Net dipole moment (without field)ZeroNon-zero (permanent dipole moment)
ExamplesHβ‚‚, Oβ‚‚, Nβ‚‚, COβ‚‚, CHβ‚„, C₆H₆Hβ‚‚O, HCl, NH₃, SOβ‚‚, HF
Behaviour in external fieldField induces a dipole moment (stretches the electron cloud)Field partially aligns the permanent dipoles
Figure 2.6 β€” Polarisation of Non-polar and Polar Dielectrics in an External Field
Figure 2.6 β€” Polarisation of Non-polar and Polar Dielectrics in an External Field

Polarisation of a Dielectric in an External Field

When a dielectric is placed in an external electric field $\vec{E}_0$:

In both cases, the net effect is: the dielectric develops a macroscopic dipole moment per unit volume, called the Polarisation Vector $\vec{P}$.

Key Concepts: Polarisation, Susceptibility, Dielectric Constant
MaterialDielectric Constant (K)Electric Susceptibility ($\chi_e = K - 1$)
Vacuum1 (definition)0
Air (dry)β‰ˆ 1.0006β‰ˆ 0.0006
Paraffin2.21.2
Paper3.52.5
Mica5–74–6
Glass5–104–9
Water (liquid)8079
Titanate ceramics~10,000~9,999

2.7 Capacitors and Capacitance

When charge $+Q$ is given to one plate, it induces charge $-Q$ on the other plate (connected to ground or being a conductor). This creates a potential difference $V$ between the plates.

Definition: Capacitance $$\boxed{C = \frac{Q}{V}}$$

Derivation: Capacitance of a Parallel Plate Capacitor (Board Exam Favourite β€” 5 marks)

A parallel plate capacitor consists of two large, flat, parallel conducting plates each of area $A$, separated by distance $d$, with $d \ll \sqrt{A}$ (edge effects negligible). Plate 1 carries $+Q$ (surface charge density $\sigma = Q/A$), Plate 2 carries $-Q$.

Figure 2.7 β€” Parallel Plate Capacitor: Derivation Diagram
Figure 2.7 β€” Parallel Plate Capacitor: Derivation Diagram

Step 1: Find Electric Field between the plates.
Each plate acts as an infinite plane of charge. Using Gauss's Law (pillbox Gaussian surface): $$E_{each\,plate} = \frac{\sigma}{2\epsilon_0}$$ Between the plates, fields from both plates add up (same direction): $$\boxed{E = \frac{\sigma}{\epsilon_0} = \frac{Q}{\epsilon_0 A}} \quad \text{(uniform, from + to βˆ’ plate)}$$ Outside the capacitor, fields from both plates cancel: $E_{outside} = 0$.

Step 2: Find Potential Difference $V$ between the plates.
In a uniform field, potential difference = field Γ— distance: $$V = E \times d = \frac{Qd}{\epsilon_0 A}$$

Step 3: Calculate Capacitance. $$C = \frac{Q}{V} = \frac{Q}{\dfrac{Qd}{\epsilon_0 A}}$$

Key Formula: Parallel Plate Capacitor $$\boxed{C_0 = \frac{\epsilon_0 A}{d}}$$

Energy Stored in a Capacitor β€” Derivation

When a capacitor is charged from $q=0$ to $q=Q$, at an intermediate stage when charge is $q$ and potential is $v = q/C$, the work done in adding a further small charge $dq$: $$dW = v\,dq = \frac{q}{C}\,dq$$ Total work done (= energy stored) in charging from 0 to $Q$: $$U = \int_0^Q \frac{q}{C}\,dq = \frac{1}{C}\cdot\frac{q^2}{2}\bigg|_0^Q = \frac{Q^2}{2C}$$

Energy Stored in a Capacitor β€” All 3 Forms $$\boxed{U = \frac{Q^2}{2C} = \frac{1}{2}CV^2 = \frac{1}{2}QV}$$

All three forms are equivalent (use $Q = CV$ to convert between them). Choose the most convenient form depending on what is given.

Energy Density (Energy per unit volume of field): $$\boxed{u = \frac{U}{\text{Volume}} = \frac{\frac{1}{2}CV^2}{Ad} = \frac{\frac{1}{2}\cdot\frac{\epsilon_0 A}{d}\cdot(Ed)^2}{Ad} = \frac{1}{2}\epsilon_0 E^2}$$ This is a universal formula β€” energy density of any electric field is $\dfrac{1}{2}\epsilon_0 E^2$.

2.8 Effect of Dielectric on Capacitance

A. Capacitor Completely Filled with Dielectric (Dielectric Constant $K$)

When the full space between the plates is filled with a dielectric of constant $K$:

$$\boxed{C_{dielectric} = KC_0 = K\frac{\epsilon_0 A}{d} = \frac{K\epsilon_0 A}{d} = \frac{\epsilon_0 \epsilon_r A}{d}}$$

where $\epsilon_r = K$ is the relative permittivity and $\epsilon = K\epsilon_0$ is the absolute permittivity of the dielectric.

B. Partial Dielectric Slab β€” Derivation (Important Board Question β€” 5 marks)

A dielectric slab of thickness $t$ (where $t < d$) and dielectric constant $K$ is inserted between the plates. The remaining gap $(d - t)$ is vacuum.

Figure 2.8 β€” Parallel Plate Capacitor with Partial Dielectric Slab of Thickness t
Figure 2.8 β€” Parallel Plate Capacitor with Partial Dielectric Slab of Thickness t

Step 1: Electric field in each region.
The surface charge density $\sigma = Q/A$ is unchanged. Using boundary conditions (normal D-field is continuous): $$E_0 = \frac{Q}{\epsilon_0 A} \quad \text{(vacuum region of thickness } d-t\text{)}$$ $$E = \frac{Q}{K\epsilon_0 A} = \frac{E_0}{K} \quad \text{(inside dielectric of thickness } t\text{)}$$

Step 2: Total potential difference $V$. $$V = E_0(d-t) + E \cdot t$$ $$= \frac{Q}{\epsilon_0 A}(d-t) + \frac{Q}{K\epsilon_0 A}\cdot t$$ $$= \frac{Q}{\epsilon_0 A}\left[(d-t) + \frac{t}{K}\right]$$

Step 3: Capacitance $C = Q/V$.

Formula: Capacitor with Partial Dielectric Slab $$\boxed{C = \frac{\epsilon_0 A}{d - t + \dfrac{t}{K}}}$$

Special Cases:
β€’ If $K \to \infty$ (conducting slab, not a dielectric but useful limit): $C = \dfrac{\epsilon_0 A}{d - t}$ β€” equivalent to reducing plate separation by $t$.
β€’ If $K = 1$ (vacuum/air slab): $C = \dfrac{\epsilon_0 A}{d}$ β€” original capacitance (as expected).
β€’ If $t = d$ (full dielectric): $C = \dfrac{K\epsilon_0 A}{d}$ β€” full dielectric formula.

C. Battery Connected vs. Battery Disconnected β€” Comparison Table

When a dielectric slab (constant $K$) is inserted into a charged parallel plate capacitor, the outcome depends on whether the battery is connected:

Quantity Battery DISCONNECTED (Q = constant) Battery CONNECTED (V = constant)
Capacitance $C$Increases: $C' = KC_0$Increases: $C' = KC_0$
Charge $Q$Constant: $Q' = Q_0$Increases: $Q' = KQ_0$ (battery supplies more charge)
Voltage $V$Decreases: $V' = V_0/K$Constant: $V' = V_0$ (maintained by battery)
Electric Field $E$Decreases: $E' = E_0/K$Constant: $E' = E_0$ (same since $V, d$ unchanged)
Energy $U$Decreases: $U' = U_0/K$ (dielectric is pulled in β€” does work)Increases: $U' = KU_0$ (battery does extra work; energy stored increases)

2.9 Combination of Capacitors

A. Capacitors in Series β€” Derivation

When capacitors are connected end-to-end (in a single chain), they are in series.

Key property of series: Same charge $Q$ appears on every capacitor (charge cannot accumulate between the capacitors in the chain). The total voltage splits.

For $n$ capacitors $C_1, C_2, \ldots, C_n$ in series with total voltage $V$: $$V = V_1 + V_2 + \cdots + V_n = \frac{Q}{C_1} + \frac{Q}{C_2} + \cdots + \frac{Q}{C_n} = Q\left(\frac{1}{C_1} + \frac{1}{C_2} + \cdots + \frac{1}{C_n}\right)$$ Since $V = Q/C_{eq}$, dividing both sides by $Q$:

Series Combination Formula $$\boxed{\frac{1}{C_{eq}} = \frac{1}{C_1} + \frac{1}{C_2} + \cdots + \frac{1}{C_n}}$$

For two capacitors in series: $C_{eq} = \dfrac{C_1 C_2}{C_1 + C_2}$ (product over sum).

B. Capacitors in Parallel β€” Derivation

Key property of parallel: Same voltage $V$ appears across every capacitor. The total charge splits.

For $n$ capacitors $C_1, C_2, \ldots, C_n$ in parallel with voltage $V$: $$Q = Q_1 + Q_2 + \cdots + Q_n = C_1V + C_2V + \cdots + C_nV = V(C_1 + C_2 + \cdots + C_n)$$ Since $Q = C_{eq}V$, dividing by $V$:

Parallel Combination Formula $$\boxed{C_{eq} = C_1 + C_2 + \cdots + C_n}$$
Figure 2.9 β€” Series and Parallel Combination of Capacitors
Figure 2.9 β€” Series and Parallel Combination of Capacitors

2.10 Energy Loss in Sharing Charges Between Capacitors

Derivation of Common Potential

Let capacitor $C_1$ have initial charge $Q_1$ (at potential $V_1 = Q_1/C_1$), and capacitor $C_2$ have initial charge $Q_2$ (at potential $V_2 = Q_2/C_2$). They are connected positive plate to positive plate and negative plate to negative plate.

Principle of Conservation of Charge: Total charge is conserved (no charge is created or destroyed).

Total charge: $Q_{total} = Q_1 + Q_2$. After connection, both capacitors reach common potential $V_{common}$. New charges: $Q_1' = C_1 V$ and $Q_2' = C_2 V$. By conservation:

$$Q_1' + Q_2' = Q_1 + Q_2 \Rightarrow (C_1 + C_2)V = Q_1 + Q_2$$
Common Potential Formula $$\boxed{V = \frac{Q_1 + Q_2}{C_1 + C_2} = \frac{C_1 V_1 + C_2 V_2}{C_1 + C_2}}$$ (using $Q_1 = C_1 V_1$ and $Q_2 = C_2 V_2$)

Derivation of Energy Loss

Initial total energy (before connection): $$U_i = \frac{1}{2}C_1 V_1^2 + \frac{1}{2}C_2 V_2^2$$

Final total energy (after connection, both at common potential $V$):
$$U_f = \frac{1}{2}(C_1 + C_2)V^2$$ $$= \frac{1}{2}(C_1+C_2)\left(\frac{C_1V_1+C_2V_2}{C_1+C_2}\right)^2$$ $$= \frac{(C_1V_1+C_2V_2)^2}{2(C_1+C_2)}$$

Energy lost:
$$\Delta U = U_i - U_f$$ $$= \frac{1}{2}C_1V_1^2 + \frac{1}{2}C_2V_2^2 - \frac{(C_1V_1+C_2V_2)^2}{2(C_1+C_2)}$$

After algebraic simplification (multiplying and expanding):
$$\Delta U = \frac{1}{2(C_1+C_2)}\Big[C_1(C_1+C_2)V_1^2$$ $$+ C_2(C_1+C_2)V_2^2 - (C_1V_1+C_2V_2)^2\Big]$$ $$\begin{aligned} &= \frac{1}{2(C_1+C_2)}\Big[C_1C_2V_1^2 \\ & \quad + C_1C_2V_2^2 - 2C_1C_2V_1V_2\Big] \end{aligned}$$

Energy Loss Formula (Always Positive) $$\boxed{\Delta U = U_i - U_f = \frac{C_1 C_2}{2(C_1 + C_2)}(V_1 - V_2)^2}$$
Figure 2.10 β€” Energy Loss When Two Charged Capacitors are Connected
Figure 2.10 β€” Energy Loss When Two Charged Capacitors are Connected