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Class 12 · Physics · Part 1

Chapter 1: Electric Charges and Fields

Revision notes, practice numericals, a question bank, assertion and reason questions and answers to the NCERT questions. Tap a group to open it; opening one closes the others.

1.1Electric chargeCharging by rubbing, two kinds of charge, the electroscope

Charging by rubbing

When a glass rod is rubbed with silk, or a plastic comb is rubbed with dry hair, the objects begin to attract small bits of paper. They are said to be electrified or charged. The word comes from the Greek elektron for amber, which shows this effect when rubbed.

Two kinds of charge

  • There are only two kinds of charge. Benjamin Franklin named them positive and negative.
  • Like charges repel and unlike charges attract each other.
  • A glass rod rubbed with silk becomes positive and the silk becomes negative. A plastic rod rubbed with fur becomes negative.
  • Electrification by rubbing happens because electrons are transferred from one body to the other. The body that loses electrons becomes positive and the body that gains them becomes negative.
  • A body with equal positive and negative charge is neutral. Neutral does not mean there is no charge in it; it means the total is zero.
++Like charges repelFF−−Like charges repelFF+−Unlike charges attractFF
Like charges repel each other and unlike charges attract each other. The arrows show the force on each body.

Gold-leaf electroscope

An electroscope detects charge. When a charged object touches the knob, the charge spreads to the metal rod and the two gold leaves. The leaves carry like charge, so they repel and spread apart. The more charge, the wider the leaves open.

charged rodmetal knobmetal rodgold leavesThe leaves carry like charge, repel each other and diverge.
Gold-leaf electroscope. When a charged object touches the knob, charge flows to the leaves and they diverge; a bigger spread means more charge.

Unit of charge

  • The SI unit of charge is the coulomb (C).
  • One coulomb is the charge that flows in one second through a wire carrying a current of one ampere: 1 C = 1 A × 1 s.
  • Common smaller units: 1 mC = 10⁻³ C, 1 μC = 10⁻⁶ C, 1 nC = 10⁻⁹ C.
1.2Conductors and insulatorsHow charge moves, earthing and charging by induction

Conductors and insulators

  • Conductors such as metals, the human body and the earth allow charge to move through them easily, because some electrons are free to move.
  • Insulators such as glass, plastic, rubber and dry wood do not allow charge to flow easily. Charge placed on them stays where it is.
  • When a charged body is connected to the earth by a conductor, its extra charge flows into the earth. This is called earthing (grounding).

Charging by conduction

When a charged conducting body touches an uncharged one, charge is shared between them. Both end up with charge of the same sign. Two identical spheres share the total charge equally.

Charging by induction

  • Bring a charged rod near (but not touching) a neutral metal sphere on an insulating stand. The free electrons of the sphere shift: the near side gets the opposite charge and the far side gets the same charge as the rod.
  • Touch the far side with a finger (earth it). The same-sign charge flows to the earth.
  • Remove the finger first and then the rod. The sphere is left with charge opposite to that of the rod.
  • Here the rod loses no charge, and the sphere acquires charge of the opposite sign.

Why charged bodies attract paper

A charged comb induces opposite charge on the near side of a bit of paper. The attraction to the near, opposite charge is stronger than the repulsion from the far, same charge, so the paper is pulled towards the comb.

1.3Basic properties of electric chargeAdditivity, conservation and quantisation

Additivity of charge

Charge is a scalar. The total charge of a system is the algebraic sum of the charges in it, with their signs. For example, +5 μC and −3 μC together make +2 μC.

Conservation of charge

  • The total charge of an isolated system never changes. Charge can be transferred from one body to another but it is neither created nor destroyed.
  • In rubbing, the charge gained by one body equals the charge lost by the other.
  • Even in processes such as the creation of an electron–positron pair, the total charge stays the same.

Quantisation of charge

  • Charge always comes in whole-number multiples of a basic unit, the charge of an electron: q = ± n e, where n = 1, 2, 3, ….
  • The elementary charge is e = 1.6 × 10⁻¹⁹ C. An electron has charge −e and a proton has charge +e.
  • Charge was first measured by Millikan in his oil-drop experiment.
  • In everyday situations we deal with charges of millions of e, so the steps are too small to notice and charge appears to change smoothly. At the microscopic level the quantisation is important.
  • To find how many electrons make a charge: n = q / e.
1.4Coulomb's lawThe force between two point charges

Statement

  • Coulomb's law: the force between two point charges is directly proportional to the product of the charges and inversely proportional to the square of the distance between them. It acts along the line joining the charges.
  • In magnitude: F = k q₁ q₂ / r²
  • The constant is k = 1 / (4π ε₀) = 9 × 10⁹ N m² C⁻², where ε₀ = 8.85 × 10⁻¹² C² N⁻¹ m⁻² is the permittivity of free space.
  • A point charge is a charged body whose size is very small compared with the distance to other bodies.
++F₁₂F₂₁rq₁q₂q₁q₂ > 0: repulsion+−F₁₂F₂₁rq₁q₂q₁q₂ < 0: attraction
Coulomb force between two point charges. The two forces are equal in magnitude and opposite in direction, along the line joining the charges.

Direction and vector form

  • If q₁q₂ > 0 (same sign) the force is repulsive; if q₁q₂ < 0 (opposite sign) it is attractive.
  • The forces on the two charges are equal and opposite (Newton's third law): F₁₂ = −F₂₁.
  • In vector form, the force on charge 2 due to charge 1 is F₂₁ = k q₁q₂ r̂₂₁ / r², where r̂₂₁ is the unit vector from 1 to 2.

Coulomb force and gravity

  • Both forces follow an inverse-square law and act along the line joining the bodies.
  • Gravity is always attractive, but the electric force can attract or repel.
  • The electric force is far stronger. For an electron and a proton, F_electric / F_gravity ≈ 2.4 × 10³⁹.
  • Charge does not depend on speed, and the electric force between charges does not depend on whether other charges are nearby (see superposition).
1.5Forces between multiple chargesThe principle of superposition

Principle of superposition

  • The force on a charge due to several other charges is the vector sum of the forces due to each of them, found as if the others were absent.
  • For a charge q₁ with other charges q₂, q₃, …: F₁ = F₁₂ + F₁₃ + …
  • Each force is found with Coulomb's law. The forces must be added as vectors, using components.
+++q₁q₂q₃F₁₂F₁₃F₁ = F₁₂ + F₁₃
Principle of superposition: the force on q₁ is the vector sum of F₁₂ and F₁₃, each found as if the other charge were absent.

How to solve

  • Draw the charges and show the direction of each force (away for like charges, towards for unlike charges).
  • Find each magnitude with F = k q₁q₂ / r².
  • Resolve into x and y components, add them, and then find the resultant: F = √(Fₓ² + F_y²).
  • On a straight line, simply add the forces with a sign for direction.
1.6Electric fieldField of a point charge and of a system

Definition

  • A charge Q changes the space around it. The charge sets up an electric field, and any other charge in the region feels a force because of it.
  • The electric field at a point is the force per unit positive test charge: E = F / q₀, taking a very small q₀ so that it does not disturb the source charges.
  • SI unit: newton per coulomb (N C⁻¹). It is a vector quantity.
  • A charge q placed in a field E feels the force F = qE. The force is along E for a positive charge and opposite to E for a negative charge.

Field of a point charge

  • At distance r from a point charge Q: E = k Q / r² = Q / (4π ε₀ r²).
  • The direction is radially outward for a positive charge and radially inward for a negative charge.
  • The field depends only on the distance, so it is the same size at all points of a sphere around the charge.
+−Field of +Q: radially outwardField of −Q: radially inward
The electric field of a point charge is radial. The lines spread out as we go away from the charge, so the field becomes weaker.

Field due to a system of charges

  • By superposition, the field at a point is the vector sum of the fields due to the individual charges: E = E₁ + E₂ + E₃ + …
  • The field of a point charge is a vector field: it has a size and a direction at every point of space.
  • The field exists whether or not a test charge is placed there.
1.7Electric field linesPicturing the field

What field lines show

  • A field line is a curve whose tangent at any point gives the direction of the field at that point.
  • The closeness of lines shows the strength of the field: crowded lines mean a strong field, widely spaced lines mean a weak field.
  • Field lines are a way to picture the field; they are imaginary, not real threads.
+−Field lines of an electric dipole: from +q to −q
Field lines of two equal and opposite charges (a dipole). Lines start on +q and end on −q and never cross.

Properties of field lines

  • Field lines start on a positive charge and end on a negative charge (or go to infinity). They do not start or stop in the middle of empty space.
  • Two field lines never cross: if they did, the field would have two directions at the crossing point.
  • The lines of a static electric field do not form closed loops, unlike magnetic field lines.
  • The lines are continuous curves without breaks.
  • The tangent to a line at a point gives the direction of the force on a positive charge placed there.
  • Where the lines are closer the field is stronger. Around a point charge the lines spread out, so the field gets weaker with distance.
1.8Electric fluxHow much field passes through a surface

Definition

  • For a small flat area ΔS in a field E, the electric flux is Δφ = E ΔS cos θ, where θ is the angle between E and the normal to the surface.
  • Flux is a scalar. Its SI unit is N m² C⁻¹ (or V m).
  • It is largest when the surface faces the field (θ = 0°) and zero when the field lies along the surface (θ = 90°).
  • For a closed surface the normal is taken to point outward. Field lines going out give positive flux; lines coming in give negative flux.
  • The total flux through a closed surface is the sum of the flux through all its small parts.
θn̂ΔSEFlux through ΔS = E ΔS cos θ
The flux through a tilted area element depends on the angle θ between E and the normal n̂. It is largest at θ = 0 and zero at θ = 90°.

Flux through a closed surface

If as many field lines enter a closed surface as leave it, the net flux is zero. This is the case when the surface contains no net charge. If more lines leave than enter, the surface encloses a net positive charge.

1.9Electric dipoleDipole moment, its field and the torque on it

Dipole and dipole moment

  • An electric dipole is a pair of equal and opposite charges +q and −q separated by a small distance 2a.
  • The dipole moment is p = q × 2a. It is a vector directed from −q to +q. Its SI unit is the coulomb metre (C m).
  • The total charge of a dipole is zero, but its field is not zero.
  • Many molecules are dipoles. Polar molecules such as H₂O and HCl have a permanent dipole moment; non-polar molecules such as O₂ and CO₂ do not.

Field of a dipole

  • On the axis (the line through both charges) at a distance r from the centre, for r ≫ a: E = 2 k p / r³, in the direction of p.
  • On the equatorial line (the perpendicular bisector) at distance r, for r ≫ a: E = k p / r³, in the direction opposite to p.
  • So the axial field is twice the equatorial field at the same distance.
  • A dipole field falls as 1/r³, faster than the 1/r² of a single charge, because the fields of the two charges partly cancel.
−+pO−q+qPErQrEaxis
Dipole field at large distance: along the axis E points the same way as p (E = 2p / 4πε₀r³); on the equatorial line E points opposite to p (E = p / 4πε₀r³ in magnitude).

Dipole in a uniform field

  • The forces +qE and −qE on the two charges are equal and opposite, so the net force is zero.
  • They act at different points, so they form a couple. The torque is τ = p × E, with magnitude τ = p E sin θ.
  • The torque turns the dipole so that p lines up with E. It is greatest at θ = 90° (τ = pE) and zero at θ = 0° or 180°.
  • In a non-uniform field there is also a net force on the dipole.
EE+−qE−qEθpTorque τ = p × E, magnitude p E sin θ
In a uniform field the two forces are equal and opposite, so the net force is zero, but they act at different points and produce a torque that turns p towards E.
1.10Continuous charge distributionLine, surface and volume charge densities

Charge densities

  • When charge is spread over a body, we describe it by a density.
  • Linear charge density λ = Δq / Δl (unit C m⁻¹), for charge on a wire.
  • Surface charge density σ = Δq / ΔS (unit C m⁻²), for charge on a surface.
  • Volume charge density ρ = Δq / ΔV (unit C m⁻³), for charge in a volume.

Field of a continuous distribution

Divide the body into small elements of charge Δq, treat each as a point charge, and add their fields as vectors. When the elements are made very small, the sum becomes an integral. For a uniformly charged body, q = λ l, q = σ A or q = ρ V.

1.11Gauss's lawFlux and enclosed charge

Statement

  • Gauss's law: the total electric flux through a closed surface equals 1/ε₀ times the net charge enclosed by it: φ = q_enclosed / ε₀.
  • The closed surface used is called a Gaussian surface. It is an imaginary surface chosen for convenience.
  • Only the charge inside contributes to the flux. A charge outside sends as many lines in as out, so its net flux is zero. But E at a point on the surface is due to all charges, inside and outside.
  • The flux does not depend on the shape or the size of the Gaussian surface, only on the enclosed charge.
+qrΔSE ∥ ΔS everywhereTotal flux = E × 4πr² = q / ε₀
A sphere of radius r around a point charge. The field is the same size at every point of the sphere and is along the outward normal, so the flux is simply E × 4πr².

Gauss's law and Coulomb's law

For a point charge q at the centre of a sphere of radius r, E is the same everywhere on the sphere and is along the outward normal. So E × 4π r² = q / ε₀, which gives E = q / (4π ε₀ r²), exactly Coulomb's law.

Choosing a Gaussian surface

Gauss's law is easy to use when the charge distribution is symmetric. Choose a surface on which E has a constant magnitude and is perpendicular to the surface (or parallel, where it gives no flux).

1.12Applications of Gauss's lawWire, sheet and spherical shell

Infinitely long straight charged wire

  • Take a coaxial cylinder of radius r and length l. The field is radial, so the flux goes only through the curved surface of area 2π r l.
  • E × 2π r l = λ l / ε₀, so E = λ / (2π ε₀ r), directed away from the wire if λ > 0.
  • The field falls as 1/r.
lrline charge λE is radial and the same size all over the curved surface
Gaussian cylinder around an infinitely long charged wire. Only the curved surface (area 2πrl) contributes to the flux; the two ends do not.

Infinite thin plane sheet

  • Take a small box straddling the sheet. The flux passes through the two faces parallel to the sheet, each of area A.
  • 2 E A = σ A / ε₀, so E = σ / (2 ε₀), directed away from a positively charged sheet.
  • The field is uniform: it does not depend on the distance from the sheet.
face 1face 2Flux = 2EA, charge enclosed = σAsheet, σarea Aarea A
Gaussian box through an infinite charged sheet. Only the two faces parallel to the sheet carry flux, so 2EA = σA / ε₀ and E = σ / 2ε₀.

Uniformly charged thin spherical shell

  • Outside (r > R): the shell acts as if all its charge q were at the centre: E = q / (4π ε₀ r²).
  • On the surface (r = R): E = q / (4π ε₀ R²).
  • Inside (r < R): a Gaussian sphere encloses no charge, so E = 0.
  • The surface charge density is σ = q / (4π R²).
POrR(a) P outside: r > RPOrR(b) P inside: r < R, E = 0
Solid circle: the charged shell of radius R. Dashed circle: the Gaussian sphere through P. Outside, the enclosed charge is q; inside it is zero.
Quick referenceFormulas at a glanceRevise before the exam

Key results

  • Quantisation: q = n e, e = 1.6 × 10⁻¹⁹ C
  • Coulomb's law: F = k q₁q₂ / r², k = 9 × 10⁹ N m² C⁻²
  • Field of a point charge: E = k Q / r²; force F = qE
  • Flux: φ = E S cos θ; Gauss's law: φ = q / ε₀
  • Dipole moment: p = 2 a q; axial E = 2kp / r³; equatorial E = kp / r³
  • Torque on a dipole: τ = p E sin θ
  • Infinite wire: E = λ / (2π ε₀ r); infinite sheet: E = σ / (2 ε₀)
  • Thin shell: E = kq / r² outside, 0 inside

Common mistakes

  • Adding forces or fields as numbers instead of as vectors.
  • Using the distance in cm in k q₁q₂ / r²: always convert to metres.
  • Forgetting that Gauss's law counts only the enclosed charge for flux.
  • Writing the dipole field direction wrongly: along p on the axis and opposite to p on the equator.