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Electric Fields

Electric Fields

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Board Coverage AQA Paper 2 | Edexcel CP3 | OCR (A) Paper 2 | CIE P4

1. Coulomb's Law

Coulomb's Law. The electrostatic force between two point charges q1q_1 and q2q_2 separated by distance rr in vacuum is:

F=LBq1q2RB◆◆LB4πε0r2RB\boxed{F = \frac◆LB◆q_1 q_2◆RB◆◆LB◆4\pi\varepsilon_0 r^2◆RB◆}

where ε0=8.85×1012\varepsilon_0 = 8.85 \times 10^{-12} F m1^{-1} is the permittivity of free space and k=1/(4πε0)=8.99×109k = 1/(4\pi\varepsilon_0) = 8.99 \times 10^9 N m2^2 C2^{-2} is Coulomb's constant.

The force is repulsive for like charges and attractive for opposite charges, directed along the line joining them.

Superposition Principle

The net force on a charge due to multiple other charges is the vector sum of the individual Coulomb forces:

Fnet=iLBqqiRB◆◆LB4πε0ri2RBr^i\mathbf{F}_{\mathrm{net}} = \sum_i \frac◆LB◆q\,q_i◆RB◆◆LB◆4\pi\varepsilon_0 r_i^2◆RB◆\,\hat{\mathbf{r}}_i

This linearity is fundamental: each pair of charges interacts independently of all others.

Comparison with Gravitational Force

PropertyGravitationalElectrostatic
LawF=Gm1m2/r2F = Gm_1m_2/r^2F=kq1q2/r2F = kq_1q_2/r^2
ConstantG=6.67×1011G = 6.67 \times 10^{-11}k=8.99×109k = 8.99 \times 10^9
NatureAlways attractiveAttractive or repulsive
Acts onMassCharge
Relative strengthVery weakVery strong

The electrostatic force is approximately 103610^{36} times stronger than gravity for proton--proton interactions. This enormous ratio explains why atomic and molecular structure is governed entirely by electromagnetic forces.

2. Electric Field Strength

Definition. The electric field strength E\mathbf{E} at a point is the force per unit positive charge:

E=LBFRB◆◆LBqRB\boxed{\mathbf{E} = \frac◆LB◆\mathbf{F}◆RB◆◆LB◆q◆RB◆}

SI units: N C1^{-1}, equivalent to V m1^{-1}.

Field of a Point Charge

E=LBQRB◆◆LB4πε0r2RB\boxed{E = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0 r^2◆RB◆}

Proof. Place test charge qq at distance rr from QQ. By Coulomb's law: F=Qq/(4πε0r2)F = Qq/(4\pi\varepsilon_0 r^2). Therefore E=F/q=Q/(4πε0r2)E = F/q = Q/(4\pi\varepsilon_0 r^2). \square

The field points radially outward from a positive charge and radially inward toward a negative charge.

Uniform Electric Field Between Parallel Plates

E=Vd\boxed{E = \frac{V}{d}}

where VV is the potential difference and dd is the plate separation.

Proof. A charge qq between the plates experiences force F=qEF = qE. Work done moving from one plate to the other: W=Fd=qEdW = Fd = qEd. But also W=qVW = qV. Therefore qEd=qVqEd = qV, giving E=V/dE = V/d. \square

The field is uniform (constant magnitude and direction) between the plates, with fringe effects at the edges.

Electric Field Lines

Field lines provide a visual representation of the electric field:

  • The direction of the line at any point gives the direction of E\mathbf{E}.
  • The density of lines is proportional to the field strength.
  • Lines begin on positive charges and end on negative charges.
  • Lines never cross (the field has a unique direction at every point).
  • Lines are perpendicular to conducting surfaces at equilibrium.

3. Electric Potential

Definition. The electric potential VV at a point is the work done per unit positive charge in bringing a small test charge from infinity to that point:

V=LBQRB◆◆LB4πε0rRB\boxed{V = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0 r◆RB◆}

SI units: volts (V), where 1 V = 1 J C1^{-1}.

Derivation from Coulomb's Law

V=Wq=1qrLBQqRB◆◆LB4πε0r2RBdr=LBQRB◆◆LB4πε0RB[1r]r=LBQRB◆◆LB4πε0rRBV = \frac{W}{q} = \frac{1}{q}\int_{\infty}^{r}\frac◆LB◆Qq◆RB◆◆LB◆4\pi\varepsilon_0 r'^2◆RB◆\,dr' = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0◆RB◆\left[-\frac{1}{r'}\right]_{\infty}^{r} = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0 r◆RB◆

\square

Sign convention. Potential is positive near a positive charge (work must be done against repulsion) and negative near a negative charge (the field does work). Potential decreases with distance, approaching zero at infinity.

Field--Potential Relationship

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

Proof. Consider a test charge qq moved by drdr in the direction of the field. Work done by the field: dW=qEdrdW = qE\,dr. This equals the loss in potential energy: dW=qdVdW = -q\,dV. Therefore qEdr=qdVqE\,dr = -q\,dV, giving E=dV/drE = -dV/dr. \square

The minus sign means the field points in the direction of decreasing potential.

Verification for a point charge. V=Q/(4πε0r)V = Q/(4\pi\varepsilon_0 r).

dVdr=LBQRB◆◆LB4πε0RB(1r2)=LBQRB◆◆LB4πε0r2RB=E-\frac{dV}{dr} = -\frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0◆RB◆\left(-\frac{1}{r^2}\right) = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0 r^2◆RB◆ = E\quad\checkmark

Electric Potential Energy

U=LBq1q2RB◆◆LB4πε0rRB\boxed{U = \frac◆LB◆q_1 q_2◆RB◆◆LB◆4\pi\varepsilon_0 r◆RB◆}

This is the work required to bring two charges from infinite separation to distance rr.

4. Equipotential Surfaces

Definition. An equipotential surface is a surface on which every point has the same electric potential.

Properties

  1. No work is done moving a charge along an equipotential surface (since ΔV=0\Delta V = 0).
  2. The electric field is always perpendicular to equipotential surfaces (since E=dV/drE = -dV/dr and dV=0dV = 0 along the surface).
  3. Equipotential surfaces never cross (each point has a unique potential).
  4. For a point charge, equipotentials are concentric spheres.
  5. For a uniform field, equipotentials are parallel planes perpendicular to the field.
  6. Equipotentials are closer together where the field is stronger (steeper potential gradient).

Mapping Equipotentials Experimentally

A practical method uses conducting paper with electrodes painted on:

  1. Connect electrodes to a power supply, establishing a potential difference.
  2. Use a voltmeter probe to locate points of equal potential.
  3. Plot the equipotential lines by joining points of equal voltage.
  4. Draw field lines perpendicular to the equipotentials.
warning

warning the field is zero on an equipotential. The field is non-zero and perpendicular; only the component tangent to the surface is zero.

5. Motion of Charged Particles in Uniform Fields

Parabolic Trajectory

A particle of charge qq and mass mm enters a uniform electric field EE with initial velocity vv perpendicular to the field, between plates of length LL.

Horizontal (perpendicular to field): uniform motion.

x=vt,t=Lvx = vt, \qquad t = \frac{L}{v}

Vertical (parallel to field): uniformly accelerated.

F=qE,a=qEmF = qE, \qquad a = \frac{qE}{m}

y=12at2=qEL22mv2y = \frac{1}{2}at^2 = \frac{qEL^2}{2mv^2}

Eliminating tt: y=qE2mv2x2y = \frac{qE}{2mv^2}\,x^2. This is a parabola.

Vertical velocity at exit: vy=at=qELmvv_y = at = \frac{qEL}{mv}.

Deflection angle: tanθ=vyv=qELmv2\tan\theta = \frac{v_y}{v} = \frac{qEL}{mv^2}.

Energy Method

An alternative approach uses energy conservation. The kinetic energy gained by the particle equals the work done by the field:

ΔEk=qV=qEd\Delta E_k = qV = qEd

where dd is the vertical displacement. This is often quicker than the kinematic approach.

Details

Worked Example: Electron Deflection An electron enters a uniform field of E=5000E = 5000 V m1^{-1} between plates of length 5.0 cm with speed 3.0×1073.0 \times 10^7 m s1^{-1}. Calculate the vertical deflection and deflection angle.

Answer. a=eEme=LB1.60×1019×5000RB◆◆LB9.11×1031RB=8.78×1014a = \frac{eE}{m_e} = \frac◆LB◆1.60 \times 10^{-19} \times 5000◆RB◆◆LB◆9.11 \times 10^{-31}◆RB◆ = 8.78 \times 10^{14} m s2^{-2}.

t=L/v=0.050/(3.0×107)=1.67×109t = L/v = 0.050 / (3.0 \times 10^7) = 1.67 \times 10^{-9} s.

y=12at2=12×8.78×1014×(1.67×109)2=1.22×103y = \frac{1}{2}at^2 = \frac{1}{2} \times 8.78 \times 10^{14} \times (1.67 \times 10^{-9})^2 = 1.22 \times 10^{-3} m =1.22= 1.22 mm.

vy=at=8.78×1014×1.67×109=1.47×106v_y = at = 8.78 \times 10^{14} \times 1.67 \times 10^{-9} = 1.47 \times 10^6 m s1^{-1}.

tanθ=vy/v=1.47×106/(3.0×107)=0.0489\tan\theta = v_y/v = 1.47 \times 10^6 / (3.0 \times 10^7) = 0.0489. θ=2.80\theta = 2.80^\circ.

6. Deflection of Electrons

Cathode Ray Tube (CRT)

A CRT uses electric fields to control and deflect a beam of electrons:

  1. Electron gun: A heated cathode emits electrons by thermionic emission. A high potential difference VaccV_{\mathrm{acc}} accelerates them through a potential difference, giving kinetic energy 12mev2=eVacc\frac{1}{2}m_e v^2 = eV_{\mathrm{acc}}.
  2. Deflection system: Two pairs of parallel plates (X and Y) apply transverse electric fields, deflecting the beam horizontally and vertically.
  3. Fluorescent screen: Electrons strike a phosphor coating, producing visible light.

Acceleration Voltage and Beam Speed

From energy conservation:

12mev2=eVacc\frac{1}{2}m_e v^2 = eV_{\mathrm{acc}}

v=LBLB2eVaccRB◆◆LBmeRB◆◆RB\boxed{v = \sqrt◆LB◆\frac◆LB◆2eV_{\mathrm{acc}}◆RB◆◆LB◆m_e◆RB◆◆RB◆}

For Vacc=2000V_{\mathrm{acc}} = 2000 V: v=LB2×1.60×1019×2000/9.11×1031RB=2.65×107v = \sqrt◆LB◆2 \times 1.60 \times 10^{-19} \times 2000 / 9.11 \times 10^{-31}◆RB◆ = 2.65 \times 10^7 m s1^{-1}.

Sensitivity of a CRT

The deflection sensitivity SS is the deflection per unit deflection voltage:

S=yVd=eL22mev2d=LBL2RB◆◆LB4VaccdRBS = \frac{y}{V_d} = \frac{eL^2}{2m_e v^2 d} = \frac◆LB◆L^2◆RB◆◆LB◆4V_{\mathrm{acc}}\,d◆RB◆

where LL is the plate length and dd is the plate separation. Higher sensitivity requires longer plates, closer spacing, and lower acceleration voltage.

warning

Common Pitfall A common error is to confuse the acceleration voltage VaccV_{\mathrm{acc}} (which determines beam speed) with the deflection voltage VdV_d (which determines deflection). The deflection is proportional to VdV_d and inversely proportional to VaccV_{\mathrm{acc}}.

7. Electric Fields of Extended Charge Distributions

Field on the Axis of a Charged Ring

A ring of radius aa carrying total charge QQ. The field at distance xx from the centre along the axis:

E=LBQxRB◆◆LB4πε0(x2+a2)3/2RB\boxed{E = \frac◆LB◆Qx◆RB◆◆LB◆4\pi\varepsilon_0(x^2 + a^2)^{3/2}◆RB◆}

Proof. By symmetry, the transverse components cancel. Each element dqdq contributes dE=dq/(4πε0(x2+a2))dE = dq/(4\pi\varepsilon_0(x^2 + a^2)). The axial component is dEx=dEx/x2+a2dE_x = dE \cdot x/\sqrt{x^2 + a^2}. Integrating over the ring:

Ex=LBQRB◆◆LB4πε0RBx(x2+a2)3/2E_x = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0◆RB◆\cdot\frac{x}{(x^2 + a^2)^{3/2}}

\square

Checks. At x=0x = 0: E=0E = 0 (by symmetry). For xax \gg a: EQ/(4πε0x2)E \approx Q/(4\pi\varepsilon_0 x^2) (point charge limit). \checkmark

Field of an Infinite Line of Charge

For a line of charge with linear charge density λ\lambda (C m1^{-1}):

E=LBλRB◆◆LB2πε0rRB\boxed{E = \frac◆LB◆\lambda◆RB◆◆LB◆2\pi\varepsilon_0 r◆RB◆}

where rr is the perpendicular distance from the line. Note: the field falls off as 1/r1/r, not 1/r21/r^2, because a line charge is an extended source in one dimension.

8. Potential Gradient and the Millikan Experiment

Millikan's Oil Drop Experiment

Millikan (1909--1913) measured the elementary charge ee by observing electrically charged oil drops in a uniform electric field.

Method: An oil drop of mass mm carries charge qq. In a uniform upward field EE, the drop is suspended when the electric force balances gravity:

qE=mgqE = mg

q=mgE\boxed{q = \frac{mg}{E}}

The mass is found from the terminal velocity (using Stokes' law for the drag force in air). Millikan found that all measured charges were integer multiples of e=1.60×1019e = 1.60 \times 10^{-19} C.

Significance. This experiment proved that charge is quantised — it comes in discrete packets of size ee.

9. Capacitance and Stored Energy

For a parallel-plate capacitor with plate area AA and separation dd:

C=LBε0ARB◆◆LBdRBC = \frac◆LB◆\varepsilon_0 A◆RB◆◆LB◆d◆RB◆

The energy stored when the capacitor carries charge QQ at potential difference VV:

U=12QV=12CV2=Q22C\boxed{U = \frac{1}{2}QV = \frac{1}{2}CV^2 = \frac{Q^2}{2C}}

Proof. During charging, the p.d. at any instant is v=q/Cv = q/C. Work to transfer charge dqdq: dW=vdq=qdq/CdW = v\,dq = q\,dq/C.

W=0QqCdq=Q22CW = \int_0^Q \frac{q}{C}\,dq = \frac{Q^2}{2C}

\square

The energy is stored in the electric field between the plates. The energy density is:

u=12ε0E2u = \frac{1}{2}\varepsilon_0 E^2

Problem Set

Details

Problem 1 Two point charges, q1=+3.0μq_1 = +3.0\,\muC and q2=5.0μq_2 = -5.0\,\muC, are separated by 0.20 m. Calculate the force between them.

Answer. F=LBkq1q2RB◆◆LBr2RB=LB8.99×109×3.0×106×5.0×106RB◆◆LB0.040RB=3.37F = \frac◆LB◆k|q_1||q_2|◆RB◆◆LB◆r^2◆RB◆ = \frac◆LB◆8.99 \times 10^9 \times 3.0 \times 10^{-6} \times 5.0 \times 10^{-6}◆RB◆◆LB◆0.040◆RB◆ = 3.37 N (attractive).

Details

Problem 2 Calculate the electric field strength at 0.10 m from a point charge of +8.0μ+8.0\,\muC.

Answer. E=kQr2=LB8.99×109×8.0×106RB◆◆LB0.010RB=7.19×106E = \frac{kQ}{r^2} = \frac◆LB◆8.99 \times 10^9 \times 8.0 \times 10^{-6}◆RB◆◆LB◆0.010◆RB◆ = 7.19 \times 10^6 N C1^{-1}.

Details

Problem 3 Two parallel plates are separated by 2.0 cm with p.d. 500 V. Calculate the field strength and the force on a proton between the plates.

Answer. E=V/d=500/0.020=2.5×104E = V/d = 500/0.020 = 2.5 \times 10^4 V m1^{-1}. F=qE=1.60×1019×2.5×104=4.0×1015F = qE = 1.60 \times 10^{-19} \times 2.5 \times 10^4 = 4.0 \times 10^{-15} N.

Details

Problem 4 Calculate the electric potential at 5.0 cm from a +2.0μ+2.0\,\muC point charge. A second charge of 1.0μ-1.0\,\muC is placed at this point. Calculate the potential energy of the system.

Answer. V=kQr=LB8.99×109×2.0×106RB◆◆LB0.050RB=3.60×105V = \frac{kQ}{r} = \frac◆LB◆8.99 \times 10^9 \times 2.0 \times 10^{-6}◆RB◆◆LB◆0.050◆RB◆ = 3.60 \times 10^5 V.

U=q2V=(1.0×106)(3.60×105)=0.360U = q_2 V = (-1.0 \times 10^{-6})(3.60 \times 10^5) = -0.360 J.

Details

Problem 5 Starting from E=dV/drE = -dV/dr, derive the field of a point charge from its potential.

Answer. V=Q/(4πε0r)V = Q/(4\pi\varepsilon_0 r). E=dVdr=LBQRB◆◆LB4πε0RBddr(r1)=LBQRB◆◆LB4πε0RB(r2)=LBQRB◆◆LB4πε0r2RBE = -\frac{dV}{dr} = -\frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0◆RB◆\cdot\frac{d}{dr}(r^{-1}) = -\frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0◆RB◆(-r^{-2}) = \frac◆LB◆Q◆RB◆◆LB◆4\pi\varepsilon_0 r^2◆RB◆. \square

Details

Problem 6 An electron is accelerated through 3000 V in a CRT. Calculate its final speed and kinetic energy.

Answer. Ek=eV=1.60×1019×3000=4.80×1016E_k = eV = 1.60 \times 10^{-19} \times 3000 = 4.80 \times 10^{-16} J.

v=2Ek/me=LB2×4.80×1016/9.11×1031RB=3.25×107v = \sqrt{2E_k/m_e} = \sqrt◆LB◆2 \times 4.80 \times 10^{-16}/9.11 \times 10^{-31}◆RB◆ = 3.25 \times 10^7 m s1^{-1}.

Details

Problem 7 In a Millikan-type experiment, an oil drop of mass 1.2×10141.2 \times 10^{-14} kg is suspended between parallel plates with field E=4.8×104E = 4.8 \times 10^4 V m1^{-1}. Calculate the charge on the drop and determine how many elementary charges it carries.

Answer. q=mg/E=1.2×1014×9.81/(4.8×104)=2.45×1018q = mg/E = 1.2 \times 10^{-14} \times 9.81 / (4.8 \times 10^4) = 2.45 \times 10^{-18} C.

n=q/e=2.45×1018/1.60×1019=15.3n = q/e = 2.45 \times 10^{-18} / 1.60 \times 10^{-19} = 15.3.

Since nn must be an integer, the drop carries 15 elementary charges (the discrepancy is within experimental uncertainty).

Details

Problem 8 Sketch the equipotential lines and field lines for two equal positive charges separated by distance dd. Explain why the field is zero at the midpoint.

Answer. The equipotential lines form peanut-shaped closed curves around each charge, with a zero-potential surface at infinity. The field lines radiate outward from each charge, curving away from each other.

At the midpoint, the fields due to each charge are equal in magnitude (kq/(d/2)2kq/(d/2)^2) and opposite in direction (each points away from its own charge). By symmetry, E1+E2=0\mathbf{E}_1 + \mathbf{E}_2 = 0. This is an unstable equilibrium point.

Details

Problem 9 A proton is released from rest in a uniform electric field of 3.0×1043.0 \times 10^4 V m1^{-1}. Calculate its acceleration and the kinetic energy gained after moving 5.0 cm.

Answer. a=qE/mp=1.60×1019×3.0×104/1.67×1027=2.88×1012a = qE/m_p = 1.60 \times 10^{-19} \times 3.0 \times 10^4 / 1.67 \times 10^{-27} = 2.88 \times 10^{12} m s2^{-2}.

Ek=qEd=1.60×1019×3.0×104×0.050=2.4×1016E_k = qEd = 1.60 \times 10^{-19} \times 3.0 \times 10^4 \times 0.050 = 2.4 \times 10^{-16} J.

Details

Problem 10 A charged sphere of mass 0.50 g is suspended by a thread in a horizontal uniform field of 5.0×1035.0 \times 10^3 V m1^{-1}. The thread makes 1515^\circ with the vertical. Calculate the charge.

Answer. Resolving: qE=Tsin15qE = T\sin 15^\circ, mg=Tcos15mg = T\cos 15^\circ.

tan15=qE/(mg)\tan 15^\circ = qE/(mg). q=mgtan15/E=0.50×103×9.81×0.268/5000=2.63×107q = mg\tan 15^\circ / E = 0.50 \times 10^{-3} \times 9.81 \times 0.268 / 5000 = 2.63 \times 10^{-7} C =263= 263 nC.