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Current and Resistance

Current and Resistance

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Board Coverage AQA Paper 1 | Edexcel CP2 | OCR (A) Paper 2 | CIE P2

Resistance in a Wire

Explore the simulation above to develop intuition for this topic.

1. Electric Current

Definition. Electric current is the rate of flow of charge:

I=dQdt\boxed{I = \frac{dQ}{dt}}

For constant current: I=QtI = \frac{Q}{t}. The SI unit is the ampere (A), where 1 A = 1 C s1^{-1}.

Conventional current flows from positive to negative (historical convention). In metals, the actual charge carriers are electrons, which flow from negative to positive.

Current as Charge per Unit Time

If NN charge carriers, each with charge qq, pass a point in time tt:

I=NqtI = \frac{Nq}{t}

Derivation of I=nAevdI = nAev_d

Consider a conductor of cross-sectional area AA with nn free charge carriers per unit volume, each carrying charge qq and moving with drift velocity vdv_d.

In time Δt\Delta t, each carrier moves a distance vdΔtv_d \Delta t. The volume swept is AvdΔtAv_d \Delta t, containing nAvdΔtnAv_d \Delta t carriers. The total charge passing is:

ΔQ=nAvdΔtq\Delta Q = nAv_d \Delta t \cdot q

I=LBΔQRB◆◆LBΔtRB=nAqvd\boxed{I = \frac◆LB◆\Delta Q◆RB◆◆LB◆\Delta t◆RB◆ = nAqv_d}

For metals, q=e=1.60×1019q = e = 1.60 \times 10^{-19} C:

I=nAevdI = nAev_d

Definition. Drift velocity vdv_d is the average net velocity of charge carriers in a conductor in the direction of the applied electric field, resulting from the superposition of rapid random thermal motion and a slow directional drift due to the field.

Intuition. The drift velocity is surprisingly small — typically 104\sim 10^{-4} m s1^{-1} for copper. This is because electrons undergo frequent collisions with the lattice ions, scattering randomly. The net motion is a slow drift superimposed on rapid random thermal motion (106\sim 10^6 m s1^{-1}).

Details

Example: Drift Velocity in Copper A copper wire of cross-sectional area 1.0×1061.0 \times 10^{-6} m2^2 carries a current of 2.0 A. The number density of free electrons in copper is 8.5×10288.5 \times 10^{28} m3^{-3}. Calculate the drift velocity.

Answer. vd=InAe=LB2.0RB◆◆LB8.5×1028×1.0×106×1.60×1019RB=LB2.0RB◆◆LB1.36×104RB=1.47×104v_d = \frac{I}{nAe} = \frac◆LB◆2.0◆RB◆◆LB◆8.5 \times 10^{28} \times 1.0 \times 10^{-6} \times 1.60 \times 10^{-19}◆RB◆ = \frac◆LB◆2.0◆RB◆◆LB◆1.36 \times 10^4◆RB◆ = 1.47 \times 10^{-4} m s1^{-1}.

2. Potential Difference and Electromotive Force

Definition. Potential difference (p.d.) VV between two points in a circuit is the energy transferred per unit charge when charge moves between those points: V=W/QV = W/Q. The SI unit is the volt (V), where 1 V = 1 J C1^{-1}.

Potential difference (p.d.) VV between two points is the energy transferred per unit charge:

V=WQV = \frac{W}{Q}

Definition. Electromotive force (e.m.f.) E\mathcal{E} is the total energy transferred per unit charge by a source when charge passes through it, including both energy delivered to the external circuit and energy dissipated internally: E=W/Q\mathcal{E} = W/Q.

Electromotive force (e.m.f.) E\mathcal{E} is the energy transferred per unit charge when charge passes through a source (e.g., a cell):

E=WQ\mathcal{E} = \frac{W}{Q}

The distinction: p.d. refers to energy dissipated in a component; e.m.f. refers to energy gained from a source.

3. Ohm's Law

Definition. Ohm's law states that the current through an ohmic conductor is directly proportional to the potential difference across it, provided the physical conditions (especially temperature) remain constant: V=IRV = IR.

Ohm's Law. The current through a metallic conductor is directly proportional to the potential difference across it, provided the temperature remains constant:

V=IRV = IR

where RR is the resistance.

Definition. Resistance RR is a measure of the opposition to current flow in a conductor, defined as the ratio of potential difference to current: R=V/IR = V/I. The SI unit is the ohm (Ω\Omega).

An ohmic conductor obeys Ohm's law — its II-VV graph is a straight line through the origin.

Microscopic origin. In a metal, conduction electrons accelerate in the electric field but collide with lattice ions, losing energy. The average time between collisions is the relaxation time τ\tau. The drift velocity is vd=LBeEτRB◆◆LBmeRBv_d = \frac◆LB◆eE\tau◆RB◆◆LB◆m_e◆RB◆, so IEVI \propto E \propto V, giving V=IRV = IR.

Derivation of Ohm's Law from the Microscopic Model

  1. In a conductor of length LL with p.d. VV, the electric field is E=V/LE = V/L.
  2. A conduction electron of charge ee and mass mem_e experiences force F=eEF = eE.
  3. Between collisions (mean relaxation time τ\tau), the electron accelerates to drift velocity: vd=aτ=(eE/me)τv_d = a\tau = (eE/m_e)\tau.
  4. Current density: J=nevd=neLBeEτRB◆◆LBmeRB=LBne2τRB◆◆LBmeRBEJ = nev_d = ne \cdot \frac◆LB◆eE\tau◆RB◆◆LB◆m_e◆RB◆ = \frac◆LB◆ne^2\tau◆RB◆◆LB◆m_e◆RB◆E.
  5. Since JEJ \propto E, the material is ohmic. Integrating: I=JA=LBne2τARB◆◆LBmeRBVLI = JA = \frac◆LB◆ne^2\tau A◆RB◆◆LB◆m_e◆RB◆ \cdot \frac{V}{L}.
  6. Rearranging: V=LBmLRB◆◆LBne2τARBI=RIV = \frac◆LB◆mL◆RB◆◆LB◆ne^2\tau A◆RB◆ \cdot I = RI.

V=IR\boxed{V = IR}

\square

4. Resistivity

Definition. Resistivity ρ\rho is an intrinsic property of a material that quantifies how strongly it resists electric current flow, defined by R=ρL/AR = \rho L / A. The SI unit is the ohm-metre (Ω\Omega m).

The resistance of a uniform conductor depends on its geometry and material:

R=LBρLRB◆◆LBARB\boxed{R = \frac◆LB◆\rho L◆RB◆◆LB◆A◆RB◆}

where ρ\rho is the resistivity (a property of the material, not the geometry), LL is the length, and AA is the cross-sectional area.

Derivation of the Resistivity Formula

Derivation. Consider a conductor of length LL, cross-sectional area AA, with electric field E=V/LE = V/L.

I=nAevd=nAeLBeEτRB◆◆LBmeRB=LBne2τRB◆◆LBmeRBAE=LBne2τRB◆◆LBmeRBAVLI = nAev_d = nAe \cdot \frac◆LB◆eE\tau◆RB◆◆LB◆m_e◆RB◆ = \frac◆LB◆ne^2\tau◆RB◆◆LB◆m_e◆RB◆ \cdot AE = \frac◆LB◆ne^2\tau◆RB◆◆LB◆m_e◆RB◆ \cdot A \cdot \frac{V}{L}

R=VI=LBmLRB◆◆LBne2τARBR = \frac{V}{I} = \frac◆LB◆mL◆RB◆◆LB◆ne^2\tau A◆RB◆

Comparing with R=ρL/AR = \rho L/A:

ρ=LBmRB◆◆LBne2τRB\boxed{\rho = \frac◆LB◆m◆RB◆◆LB◆ne^2\tau◆RB◆}

\square

This shows that resistivity depends on the material's charge carrier density nn and relaxation time τ\tau, but not on its geometry.

Intuition. Longer conductors have more resistance (more collisions). Thicker conductors have less resistance (more parallel paths). A higher resistivity means the material is intrinsically more resistant to current flow.

MaterialResistivity (Ω\Omega m)
Copper1.7×1081.7 \times 10^{-8}
Aluminium2.7×1082.7 \times 10^{-8}
Constantan4.9×1074.9 \times 10^{-7}
Nichrome1.1×1061.1 \times 10^{-6}
Silicon6.4×1026.4 \times 10^{2}
Glass1012\sim 10^{12}
warning

warning particular component. A long thin copper wire has high resistance but copper still has low resistivity.

5. I-V Characteristics

Metallic Conductor (Ohmic)

Straight line through origin. Resistance is constant. Temperature rises with current, slightly increasing resistance (positive temperature coefficient).

Filament Lamp

Current increases rapidly at low p.d., then curves over. At higher currents, the filament heats up, increasing the lattice ion vibrations and hence the resistance. The II-VV graph is a curve that flattens at high VV.

Semiconductor Diode

  • Forward bias: very little current until the threshold voltage (0.6\sim 0.6 V for silicon) is reached, then current rises sharply.
  • Reverse bias: almost zero current until breakdown voltage.

Thermistor (NTC)

Negative temperature coefficient. As temperature increases, resistance decreases (more charge carriers are released from the lattice).

6. Electrical Energy and Power

Energy transferred when charge QQ moves through p.d. VV:

W=QV=VItW = QV = VIt

Power (rate of energy transfer):

P=IVP = IV

Using V=IRV = IR:

P=I2R=V2RP = I^2R = \frac{V^2}{R}

Derivation of P=I2RP = I^2R. Substituting V=IRV = IR into P=IVP = IV:

P=IIR=I2RP = I \cdot IR = I^2R

Derivation of P=V2/RP = V^2/R. Substituting I=V/RI = V/R into P=IVP = IV:

P=VRV=V2RP = \frac{V}{R} \cdot V = \frac{V^2}{R}

Choosing the right formula:

Known quantitiesFormula to use
II and VVP=IVP = IV
II and RRP=I2RP = I^2R
VV and RRP=V2/RP = V^2/R

Energy:

E=Pt=VIt=I2Rt=V2tRE = Pt = VIt = I^2Rt = \frac{V^2t}{R}

The SI unit of energy is the joule (J). For domestic billing, the kilowatt-hour (kWh) is used:

1kWh=1000W×3600s=3.6×106J1 \mathrm{ kWh} = 1000 \mathrm{ W} \times 3600 \mathrm{ s} = 3.6 \times 10^6 \mathrm{ J}

tip

Exam Technique When calculating energy for resistors in series, use P=I2RP = I^2R (same current). For resistors in parallel, use P=V2/RP = V^2/R (same voltage).

7. Temperature Dependence of Resistance

Microscopic Derivation: Why Metallic Resistance Increases with Temperature

From Section 4, the resistivity of a metal is:

ρ=LBmeRB◆◆LBne2τRB\rho = \frac◆LB◆m_e◆RB◆◆LB◆ne^2\tau◆RB◆

In a metal, the number density of free electrons nn is essentially fixed (every atom contributes roughly one conduction electron, and the total number of atoms does not change with temperature). The electron mass mem_e and charge ee are constants. Therefore, the only temperature-dependent quantity is the relaxation time τ\tau.

Proof that τ\tau decreases with temperature. At temperature TT, the lattice ions vibrate with mean square amplitude u2T\langle u^2 \rangle \propto T (from the equipartition theorem: 12ku2=12kBT\frac{1}{2}k\langle u^2 \rangle = \frac{1}{2}k_BT per degree of freedom). The probability that an electron scatters off a lattice ion is proportional to the amplitude of the ion's displacement from its equilibrium position. Therefore the scattering rate 1/τ1/\tau is proportional to TT, and the relaxation time decreases:

τ1T\tau \propto \frac{1}{T}

Consequently:

ρ=LBmeRB◆◆LBne2τRBT\rho = \frac◆LB◆m_e◆RB◆◆LB◆ne^2\tau◆RB◆ \propto T

R(T)=R0[1+α(TT0)]\boxed{R(T) = R_0\left[1 + \alpha(T - T_0)\right]}

where R0R_0 is the resistance at reference temperature T0T_0 and α\alpha is the temperature coefficient of resistance. For copper, α3.9×103\alpha \approx 3.9 \times 10^{-3} C1^\circ\mathrm{C}^{-1}; for tungsten, α4.5×103\alpha \approx 4.5 \times 10^{-3} C1^\circ\mathrm{C}^{-1}.

This is a linear approximation valid over moderate temperature ranges. The full relationship is not perfectly linear, but for A-level purposes the linear model suffices.

NTC Thermistors: Why Resistance Decreases with Temperature

A negative temperature coefficient (NTC) thermistor is a semiconductor device whose resistance decreases as temperature increases. This is the opposite of what happens in metals.

Physical mechanism. In a semiconductor, not all electrons are free to conduct. Electrons must be promoted from the valence band across the band gap EgE_g into the conduction band. The number of charge carriers is strongly temperature-dependent:

n(T)T3/2exp(Eg2kBT)n(T) \propto T^{3/2} \exp\left(-\frac{E_g}{2k_BT}\right)

As TT increases, the exponential factor dominates and the carrier density increases dramatically. Since ρ=m/(ne2τ)\rho = m/(ne^2\tau) and nn grows exponentially, the resistivity drops. This overwhelms any decrease in τ\tau due to increased lattice vibrations.

For a typical NTC thermistor, the resistance approximately follows:

R=R0exp(BTBT0)R = R_0 \exp\left(\frac{B}{T} - \frac{B}{T_0}\right)

where BB is a material constant (typically 3000--5000 K).

Example: Resistance of Copper at Elevated Temperature

A copper wire has resistance 10.0 Ω\Omega at 20C^\circ\mathrm{C}. Calculate its resistance at 80C^\circ\mathrm{C}. (α=3.9×103\alpha = 3.9 \times 10^{-3} C1^\circ\mathrm{C}^{-1}.)

Answer.

R=R0[1+α(TT0)]=10.0×[1+3.9×103×(8020)]R = R_0[1 + \alpha(T - T_0)] = 10.0 \times [1 + 3.9 \times 10^{-3} \times (80 - 20)]

=10.0×[1+0.234]=10.0×1.234=12.3= 10.0 \times [1 + 0.234] = 10.0 \times 1.234 = 12.3 Ω\Omega.

The resistance increased by 23.4%. This is why components can overheat in circuits --- increased resistance leads to more power dissipation (P=I2RP = I^2R), which raises the temperature further, a positive feedback loop.

If you get this wrong, revise: Temperature Dependence of Resistance

warning

Common Pitfall Do not confuse the behaviour of metals and semiconductors. Metals have a positive temperature coefficient (RR increases with TT). Semiconductors (thermistors) have a negative temperature coefficient (RR decreases with TT). The physical mechanism is entirely different: in metals, τ\tau changes; in semiconductors, nn changes.

8. Superconductivity

Definition. A superconductor is a material that exhibits zero electrical resistance below a critical temperature TcT_c.

Key Properties

When a material enters the superconducting state (by being cooled below TcT_c), three remarkable properties emerge:

  1. Zero DC resistance. A current induced in a superconducting loop persists indefinitely with no decay. This has been experimentally verified: currents have been observed to flow for years with no measurable decrease.

  2. Meissner effect. A superconductor expels all magnetic flux from its interior. If a superconductor is cooled below TcT_c in an external magnetic field, the field lines are pushed out. This is not a consequence of zero resistance --- it is a distinct thermodynamic property. The magnetic field penetrates only a thin surface layer of depth λ\lambda (the London penetration depth, typically 20--200 nm).

  3. Critical parameters. Superconductivity is destroyed if any of three critical values are exceeded:

    • Critical temperature TcT_c: above this, normal resistivity returns.
    • Critical magnetic field BcB_c: above this field, superconductivity is destroyed.
    • Critical current density JcJ_c: above this current density, the magnetic field generated by the current itself destroys superconductivity.

These three parameters are related. In the simplest model (Type I), Bc(T)Bc(0)[1(T/Tc)2]B_c(T) \approx B_c(0)\left[1 - (T/T_c)^2\right].

Type I vs Type II Superconductors

Type I superconductors (e.g., lead, mercury, aluminium) exhibit a sharp transition: below BcB_c they are fully superconducting, above BcB_c they revert to normal. Their critical fields are low (typically <\lt{} 0.1 T).

Type II superconductors (e.g., niobium-titanium, YBCO) have two critical fields Bc1B_{c1} and Bc2B_{c2}:

  • Below Bc1B_{c1}: full Meissner effect (Meissner state).
  • Between Bc1B_{c1} and Bc2B_{c2}: mixed state (vortex state) where magnetic flux penetrates in quantised vortices. The material still carries supercurrent but with some flux penetration.
  • Above Bc2B_{c2}: normal state.

Type II superconductors typically have much higher Bc2B_{c2} values (tens of tesla), making them practically useful.

BCS Theory (Conceptual Overview)

The Bardeen-Cooper-Schrieffer (BCS) theory (1957) explains superconductivity as follows:

At low temperatures, electrons with opposite momenta and spins form Cooper pairs via an indirect attraction mediated by lattice vibrations (phonons). An electron distorts the positive ion lattice as it passes; this distortion attracts a second electron. The net effect is an attractive interaction between two electrons, despite their Coulomb repulsion.

Cooper pairs are bosons (integer spin) and can all occupy the same quantum ground state --- a Bose-Einstein condensate. The Cooper pairs move coherently through the lattice without scattering (there is no individual state to scatter into, since the ground state is already full). This is the origin of zero resistance.

The energy gap Δ\Delta (the minimum energy to break a Cooper pair) is typically 10310^{-3}--10210^{-2} eV, which is why thermal energy at TcT_c (where kBTcΔk_BT_c \approx \Delta) destroys superconductivity.

Applications

  • MRI scanners: superconducting coils generate the strong, uniform magnetic fields (1.5--7 T) required for imaging.
  • Particle accelerators: the LHC uses superconducting magnets to steer proton beams at 7 TeV.
  • Maglev trains: superconducting magnets provide levitation via the Meissner effect.
  • SQUIDs (Superconducting Quantum Interference Devices): extremely sensitive magnetometers capable of detecting fields as small as 101510^{-15} T.
  • Power transmission: lossless power lines (currently limited by the cost of cooling).

9. Semiconductors

Intrinsic Semiconductors

Pure silicon and germanium are intrinsic semiconductors. At absolute zero, their valence band is completely full and their conduction band is completely empty --- they are insulators. As temperature increases, thermal energy promotes some electrons across the band gap EgE_g into the conduction band, leaving behind holes in the valence band. Both electrons and holes act as charge carriers.

For silicon, Eg=1.1E_g = 1.1 eV. For germanium, Eg=0.67E_g = 0.67 eV.

Derivation of carrier concentration. The intrinsic carrier concentration is given by:

ni=CT3/2exp(Eg2kBT)\boxed{n_i = C \cdot T^{3/2} \exp\left(-\frac{E_g}{2k_BT}\right)}

where CC is a material constant and kB=1.38×1023k_B = 1.38 \times 10^{-23} J K1^{-1} is the Boltzmann constant. The factor of 2 in the denominator arises because creating one electron-hole pair requires energy EgE_g, so each carrier's average energy cost is Eg/2E_g/2.

At room temperature (300 K), silicon has ni1.5×1016n_i \approx 1.5 \times 10^{16} m3^{-3}, compared with copper's n8.5×1028n \approx 8.5 \times 10^{28} m3^{-3} --- a difference of 12 orders of magnitude.

Extrinsic Semiconductors: Doping

The carrier concentration of an intrinsic semiconductor is far too low for practical electronics. Doping introduces impurity atoms that dramatically increase carrier concentration.

n-type semiconductor. A group V element (e.g., phosphorus) is substituted for a silicon atom. Phosphorus has 5 valence electrons; four bond with neighbouring silicon atoms, and the fifth is weakly bound (ionisation energy 0.05\approx 0.05 eV, far less than the band gap). At room temperature, virtually all donor atoms are ionised, contributing free electrons. The majority carriers are electrons.

p-type semiconductor. A group III element (e.g., boron) is substituted for a silicon atom. Boron has 3 valence electrons; it accepts an electron from a neighbouring silicon atom to complete its bonds, creating a hole. At room temperature, virtually all acceptor atoms are ionised, contributing holes. The majority carriers are holes.

Typical doping concentrations are 102110^{21}--102310^{23} m3^{-3}, compared with ni1016n_i \approx 10^{16} m3^{-3} for intrinsic silicon. Doping increases conductivity by 5--7 orders of magnitude.

Charge neutrality. In n-type material: n=ND+pNDn = N_D + p \approx N_D (since npn \gg p). In p-type material: p=NA+nNAp = N_A + n \approx N_A (since pnp \gg n). Here NDN_D is the donor concentration and NAN_A is the acceptor concentration.

The Hall Effect

When a current-carrying conductor is placed in a magnetic field, a transverse voltage is developed perpendicular to both the current and the field. This is the Hall effect.

Derivation. Consider a slab of thickness dd carrying current II in the xx-direction, with magnetic field BB in the zz-direction. Charge carriers of charge qq and drift velocity vdv_d experience a magnetic force:

FB=qvdBF_B = qv_dB

This deflects carriers to one face, building up charge until the electric field EHE_H creates a force that balances the magnetic force:

qEH=qvdBqE_H = qv_dB

EH=vdBE_H = v_dB

The Hall voltage across the thickness dd is:

VH=EHd=vdBdV_H = E_H \cdot d = v_dBd

Substituting vd=I/(nqA)=I/(nqwd)v_d = I/(nqA) = I/(nq \cdot wd) where ww is the width:

VH=BInqd\boxed{V_H = \frac{BI}{nqd}}

Determining carrier type. The sign of VHV_H reveals the sign of the charge carriers. In n-type material, VHV_H is negative on one face (electrons accumulate). In p-type material, VHV_H is positive on that same face (holes accumulate).

Determining carrier density. Rearranging:

n=BIqVHdn = \frac{BI}{qV_Hd}

Measurement of VHV_H, BB, II, and dd gives nn directly.

Example: Hall Voltage Calculation

A copper strip of thickness 0.50 mm carries a current of 10 A in a magnetic field of 1.5 T perpendicular to the strip. Calculate the Hall voltage. (Take n=8.5×1028n = 8.5 \times 10^{28} m3^{-3}.)

Answer.

VH=BInqd=LB1.5×10RB◆◆LB8.5×1028×1.60×1019×0.50×103RBV_H = \frac{BI}{nqd} = \frac◆LB◆1.5 \times 10◆RB◆◆LB◆8.5 \times 10^{28} \times 1.60 \times 10^{-19} \times 0.50 \times 10^{-3}◆RB◆

=LB15RB◆◆LB8.5×1028×8.0×1023RB=LB15RB◆◆LB6.8×106RB=2.2×106= \frac◆LB◆15◆RB◆◆LB◆8.5 \times 10^{28} \times 8.0 \times 10^{-23}◆RB◆ = \frac◆LB◆15◆RB◆◆LB◆6.8 \times 10^{6}◆RB◆ = 2.2 \times 10^{-6} V =2.2= 2.2 μ\muV.

Note the very small Hall voltage in metals, due to the enormous carrier density. In semiconductors, where nn is much smaller, VHV_H is much larger and easier to measure.

If you get this wrong, revise: The Hall Effect

warning

warning direction of the magnetic field, not the width of the conductor perpendicular to the current. Sketch the geometry carefully.

tip

tip Hall effect, focus on the sign of the Hall voltage. Electrons (negative charge) deflect to one side, holes (positive charge) deflect to the opposite side.

10. Power Transmission

Why AC is Used for Long-Distance Transmission

The fundamental reason AC is used for power transmission is that transformers allow voltage to be stepped up at the generating station and stepped down near the consumer. This is only possible with AC (or with complex DC-DC conversion technology, which was not available historically and is still more expensive).

Derivation of Transmission Losses

Consider transmitting power PP over a distance LL through cables of resistance RR at voltage VV.

The current in the transmission line is:

I=PVI = \frac{P}{V}

The power dissipated as heat in the cables is:

Ploss=I2R=(PV)2RP_{\mathrm{loss}} = I^2R = \left(\frac{P}{V}\right)^2 R

Proof that doubling the voltage quarters the loss. If V2VV \to 2V:

Ploss=(P2V)2R=14P2V2R=LBPlossRB◆◆LB4RBP_{\mathrm{loss}}' = \left(\frac{P}{2V}\right)^2 R = \frac{1}{4} \cdot \frac{P^2}{V^2}R = \frac◆LB◆P_{\mathrm{loss}}◆RB◆◆LB◆4◆RB◆

\square

This is the central result: power loss scales as 1/V21/V^2. This is why the National Grid transmits at very high voltages (typically 275 kV or 400 kV in the UK).

The National Grid

The National Grid (or equivalent in other countries) is the network of cables and transformers that distributes electricity from power stations to consumers:

  1. Step-up transformer at the power station: generator output (typically 15--25 kV) is stepped up to 275 or 400 kV for transmission.
  2. High-voltage transmission lines: carry power at high voltage to minimise I2RI^2R losses.
  3. Step-down transformers: near towns, voltage is reduced in stages (e.g., 132 kV \to 33 kV \to 11 kV \to 230 V) for distribution to consumers.
Example: Comparing Transmission Losses at Different Voltages

Transmit 100 MW of power over 50 km of aluminium cable (resistivity 2.7×1082.7 \times 10^{-8} Ω\Omega m, cross-sectional area 5.0×1045.0 \times 10^{-4} m2^2). Compare losses at 10 kV and 400 kV.

Answer.

Resistance of the cable (there and back):

R=LBρ×2LRB◆◆LBARB=LB2.7×108×2×50000RB◆◆LB5.0×104RB=LB2.7×103RB◆◆LB5.0×104RB=5.4R = \frac◆LB◆\rho \times 2L◆RB◆◆LB◆A◆RB◆ = \frac◆LB◆2.7 \times 10^{-8} \times 2 \times 50\,000◆RB◆◆LB◆5.0 \times 10^{-4}◆RB◆ = \frac◆LB◆2.7 \times 10^{-3}◆RB◆◆LB◆5.0 \times 10^{-4}◆RB◆ = 5.4 Ω\Omega.

At 10 kV: I=P/V=100×106/(10×103)=10000I = P/V = 100 \times 10^6 / (10 \times 10^3) = 10\,000 A.

Ploss=I2R=(10000)2×5.4=5.4×108P_{\mathrm{loss}} = I^2R = (10\,000)^2 \times 5.4 = 5.4 \times 10^8 W =540= 540 MW.

This exceeds the total power being transmitted! Clearly 10 kV is impractical.

At 400 kV: I=100×106/(400×103)=250I = 100 \times 10^6 / (400 \times 10^3) = 250 A.

Ploss=(250)2×5.4=3.375×105P_{\mathrm{loss}} = (250)^2 \times 5.4 = 3.375 \times 10^5 W =338= 338 kW.

Percentage loss =338000/100000000=0.34%= 338\,000 / 100\,000\,000 = 0.34\%.

Stepping up from 10 kV to 400 kV reduced losses from 540% (impossible!) to 0.34%. This demonstrates why high-voltage transmission is essential.

If you get this wrong, revise: Power Transmission

tip

Exam Technique When calculating transmission losses, remember to include both the outward and return cables (total length =2L= 2L). Also remember that the voltage in P=IVP = IV is the transmission voltage, not the voltage drop across the line resistance.

Problem Set

Details

Problem 1 A copper wire has length 2.0 m, cross-sectional area 1.5×1061.5 \times 10^{-6} m2^2, and resistivity 1.7×1081.7 \times 10^{-8} Ω\Omega m. Calculate its resistance.

Answer. R=LBρLRB◆◆LBARB=LB1.7×108×2.0RB◆◆LB1.5×106RB=LB3.4×108RB◆◆LB1.5×106RB=0.0227R = \frac◆LB◆\rho L◆RB◆◆LB◆A◆RB◆ = \frac◆LB◆1.7 \times 10^{-8} \times 2.0◆RB◆◆LB◆1.5 \times 10^{-6}◆RB◆ = \frac◆LB◆3.4 \times 10^{-8}◆RB◆◆LB◆1.5 \times 10^{-6}◆RB◆ = 0.0227 Ω=0.023\Omega = 0.023 Ω\Omega.

If you get this wrong, revise: Resistivity

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Problem 2 A wire carries a current of 3.0 A. How much charge flows past a point in 2 minutes?

Answer. Q=It=3.0×120=360Q = It = 3.0 \times 120 = 360 C.

If you get this wrong, revise: Electric Current

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Problem 3 Calculate the drift velocity of electrons in a silver wire of diameter 1.0 mm carrying a current of 5.0 A. The number density of free electrons in silver is 5.9×10285.9 \times 10^{28} m3^{-3}.

Answer. A=π(0.5×103)2=7.85×107A = \pi(0.5 \times 10^{-3})^2 = 7.85 \times 10^{-7} m2^2.

vd=InAe=LB5.0RB◆◆LB5.9×1028×7.85×107×1.60×1019RB=LB5.0RB◆◆LB7.42×103RB=6.74×104v_d = \frac{I}{nAe} = \frac◆LB◆5.0◆RB◆◆LB◆5.9 \times 10^{28} \times 7.85 \times 10^{-7} \times 1.60 \times 10^{-19}◆RB◆ = \frac◆LB◆5.0◆RB◆◆LB◆7.42 \times 10^3◆RB◆ = 6.74 \times 10^{-4} m s1^{-1}.

If you get this wrong, revise: Derivation of I=nAevdI = nAev_d

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Problem 4 A 12 V battery delivers a current of 2.5 A to a resistor. Calculate: (a) the resistance, (b) the power dissipated, (c) the energy transferred in 10 minutes.

Answer. (a) R=V/I=12/2.5=4.8R = V/I = 12/2.5 = 4.8 Ω\Omega.

(b) P=IV=2.5×12=30P = IV = 2.5 \times 12 = 30 W.

(c) E=Pt=30×600=18000E = Pt = 30 \times 600 = 18\,000 J = 18 kJ.

If you get this wrong, revise: Electrical Energy and Power

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Problem 5 A nichrome wire has resistance 8.0 Ω\Omega at 20C20^\circ\mathrm{C}. The wire is stretched to twice its original length. What is its new resistance? (Assume the volume remains constant.)

Answer. If L2LL \to 2L and volume AL=constAL = \mathrm{const}, then AA/2A \to A/2.

R=LBρ(2L)RB◆◆LBA/2RB=LB4ρLRB◆◆LBARB=4R=32R' = \frac◆LB◆\rho(2L)◆RB◆◆LB◆A/2◆RB◆ = \frac◆LB◆4\rho L◆RB◆◆LB◆A◆RB◆ = 4R = 32 Ω\Omega.

If you get this wrong, revise: Resistivity

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Problem 6 A 2.5 kW heater operates on a 230 V mains supply. Calculate the current it draws and its resistance.

Answer. P=IVP = IV, so I=P/V=2500/230=10.9I = P/V = 2500/230 = 10.9 A.

R=V/I=230/10.9=21.2R = V/I = 230/10.9 = 21.2 Ω\Omega.

If you get this wrong, revise: Electrical Energy and Power

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Problem 7 Explain why the resistance of a filament lamp increases as the current through it increases.

Answer. As the current increases, more energy is dissipated per second (P=I2RP = I^2R), heating the filament. The increased temperature causes the metal lattice ions to vibrate more vigorously, increasing the frequency of collisions between the conduction electrons and the lattice. This reduces the mean relaxation time τ\tau, and since ρ=m/(ne2τ)\rho = m/(ne^2\tau), the resistivity increases. Since R=ρL/AR = \rho L/A, the resistance increases.

If you get this wrong, revise: Resistivity and I-V Characteristics

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Problem 8 A student measures the resistance of a wire at different lengths. The results are: 10 cm → 0.50 Ω\Omega, 20 cm → 1.05 Ω\Omega, 30 cm → 1.45 Ω\Omega, 40 cm → 2.00 Ω\Omega. Plotting RR against LL gives a gradient of 5.0 Ω\Omega m1^{-1}. If the wire diameter is 0.40 mm, calculate the resistivity.

Answer. A=π(0.20×103)2=1.26×107A = \pi(0.20 \times 10^{-3})^2 = 1.26 \times 10^{-7} m2^2. From R=ρL/AR = \rho L/A: gradient =ρ/A=5.0= \rho/A = 5.0. ρ=5.0×1.26×107=6.3×107\rho = 5.0 \times 1.26 \times 10^{-7} = 6.3 \times 10^{-7} Ω\Omega m.

If you get this wrong, revise: Resistivity

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Problem 9 Two resistors of 6 Ω\Omega and 3 Ω\Omega are connected in series across a 9 V battery. Calculate the current and the power dissipated in each resistor.

Answer. Total resistance Rtotal=6+3=9R_{\mathrm{total}} = 6 + 3 = 9 Ω\Omega. Current I=V/R=9/9=1.0I = V/R = 9/9 = 1.0 A.

Power in 6 Ω\Omega: P=I2R=12×6=6P = I^2R = 1^2 \times 6 = 6 W.

Power in 3 Ω\Omega: P=12×3=3P = 1^2 \times 3 = 3 W.

If you get this wrong, revise: Electrical Energy and Power

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Problem 10 A thermistor has resistance 2000 Ω\Omega at 20C20^\circ\mathrm{C} and 400 Ω\Omega at 80C80^\circ\mathrm{C}. It is connected in series with a 500 Ω\Omega fixed resistor and a 6.0 V battery. Calculate the p.d. across the thermistor at each temperature.

Answer. At 20C20^\circ\mathrm{C}: Rtotal=2000+500=2500R_{\mathrm{total}} = 2000 + 500 = 2500 Ω\Omega. VT=20002500×6.0=4.80V_T = \frac{2000}{2500} \times 6.0 = 4.80 V.

At 80C80^\circ\mathrm{C}: Rtotal=400+500=900R_{\mathrm{total}} = 400 + 500 = 900 Ω\Omega. VT=400900×6.0=2.67V_T = \frac{400}{900} \times 6.0 = 2.67 V.

If you get this wrong, revise: I-V Characteristics

Problem 11

A copper wire has resistance 5.00 Ω\Omega at 20C^\circ\mathrm{C}. The temperature coefficient of resistance for copper is α=3.9×103\alpha = 3.9 \times 10^{-3} C1^\circ\mathrm{C}^{-1}. Calculate: (a) the resistance at 100C^\circ\mathrm{C}, (b) the temperature at which the resistance doubles, (c) the resistance at 40C-40^\circ\mathrm{C}.

Answer. (a) R=5.00×[1+3.9×103×(10020)]=5.00×[1+0.312]=5.00×1.312=6.56R = 5.00 \times [1 + 3.9 \times 10^{-3} \times (100 - 20)] = 5.00 \times [1 + 0.312] = 5.00 \times 1.312 = 6.56 Ω\Omega.

(b) 2R0=R0[1+α(TT0)]2R_0 = R_0[1 + \alpha(T - T_0)], so 2=1+α(T20)2 = 1 + \alpha(T - 20), giving α(T20)=1\alpha(T - 20) = 1, so T20=1/(3.9×103)=256T - 20 = 1/(3.9 \times 10^{-3}) = 256, so T=276T = 276^\circC.

(c) R=5.00×[1+3.9×103×(4020)]=5.00×[10.234]=5.00×0.766=3.83R = 5.00 \times [1 + 3.9 \times 10^{-3} \times (-40 - 20)] = 5.00 \times [1 - 0.234] = 5.00 \times 0.766 = 3.83 Ω\Omega.

If you get this wrong, revise: Temperature Dependence of Resistance

Problem 12

A semiconductor sample has thickness d=1.0d = 1.0 mm and width w=5.0w = 5.0 mm. A current of 15 mA flows through it. When a magnetic field of 0.80 T is applied perpendicular to the flat face, a Hall voltage of 12 mV is measured across the width. (a) Calculate the carrier density. (b) Determine whether the material is n-type or p-type if the Hall voltage is positive on the face closest to the north pole of the magnet (conventional current flows left to right, magnetic field points into the page).

Answer. (a) n=BIqVHd=LB0.80×15×103RB◆◆LB1.60×1019×12×103×1.0×103RBn = \frac{BI}{qV_Hd} = \frac◆LB◆0.80 \times 15 \times 10^{-3}◆RB◆◆LB◆1.60 \times 10^{-19} \times 12 \times 10^{-3} \times 1.0 \times 10^{-3}◆RB◆

=LB0.012RB◆◆LB1.60×1019×1.2×105RB=LB0.012RB◆◆LB1.92×1024RB=6.25×1021= \frac◆LB◆0.012◆RB◆◆LB◆1.60 \times 10^{-19} \times 1.2 \times 10^{-5}◆RB◆ = \frac◆LB◆0.012◆RB◆◆LB◆1.92 \times 10^{-24}◆RB◆ = 6.25 \times 10^{21} m3^{-3}.

(b) By the right-hand rule (or Fleming's left-hand rule), positive carriers moving left-to-right in a field into the page experience an upward force. Since VHV_H is positive on the top face, the carriers accumulating there are positive --- the material is p-type.

If you get this wrong, revise: The Hall Effect

Problem 13

A power station generates 500 MW and transmits it over 80 km of cable with total resistance 4.0 Ω\Omega. Calculate the power loss and efficiency when transmitting at: (a) 25 kV, (b) 132 kV, (c) 400 kV.

Answer. (a) I=500×106/(25×103)=20000I = 500 \times 10^6 / (25 \times 10^3) = 20\,000 A. Ploss=(20000)2×4.0=1.6×109P_{\mathrm{loss}} = (20\,000)^2 \times 4.0 = 1.6 \times 10^9 W =1600= 1600 MW. Efficiency =500/(500+1600)=23.8%= 500/(500 + 1600) = 23.8\%.

(b) I=500×106/(132×103)=3788I = 500 \times 10^6 / (132 \times 10^3) = 3788 A. Ploss=(3788)2×4.0=5.74×107P_{\mathrm{loss}} = (3788)^2 \times 4.0 = 5.74 \times 10^7 W =57.4= 57.4 MW. Efficiency =500/557.4=89.7%= 500/557.4 = 89.7\%.

(c) I=500×106/(400×103)=1250I = 500 \times 10^6 / (400 \times 10^3) = 1250 A. Ploss=(1250)2×4.0=6.25×106P_{\mathrm{loss}} = (1250)^2 \times 4.0 = 6.25 \times 10^6 W =6.25= 6.25 MW. Efficiency =500/506.25=98.8%= 500/506.25 = 98.8\%.

If you get this wrong, revise: Power Transmission

Problem 14

A Type I superconducting lead wire has a critical field of Bc=0.080B_c = 0.080 T at T=0T = 0 K and a critical temperature of Tc=7.2T_c = 7.2 K. The wire has radius 1.0 mm. Calculate the maximum current the wire can carry at (a) 0 K, (b) 4.0 K. Use the approximation Bc(T)=Bc(0)[1(T/Tc)2]B_c(T) = B_c(0)[1 - (T/T_c)^2].

Answer. The critical field at the surface of the wire due to current II in a wire of radius rr is B=μ0I/(2πr)B = \mu_0 I / (2\pi r). Superconductivity is destroyed when this field reaches Bc(T)B_c(T).

(a) At T=0T = 0: Bc(0)=0.080B_c(0) = 0.080 T. Imax=LB2πrBcRB◆◆LBμ0RB=LB2π×1.0×103×0.080RB◆◆LB4π×107RB=LB5.03×104RB◆◆LB1.257×106RB=400I_{\max} = \frac◆LB◆2\pi r B_c◆RB◆◆LB◆\mu_0◆RB◆ = \frac◆LB◆2\pi \times 1.0 \times 10^{-3} \times 0.080◆RB◆◆LB◆4\pi \times 10^{-7}◆RB◆ = \frac◆LB◆5.03 \times 10^{-4}◆RB◆◆LB◆1.257 \times 10^{-6}◆RB◆ = 400 A.

(b) At T=4.0T = 4.0 K: Bc(4.0)=0.080×[1(4.0/7.2)2]=0.080×[10.309]=0.080×0.691=0.0553B_c(4.0) = 0.080 \times [1 - (4.0/7.2)^2] = 0.080 \times [1 - 0.309] = 0.080 \times 0.691 = 0.0553 T.

Imax=LB2π×1.0×103×0.0553RB◆◆LB4π×107RB=277I_{\max} = \frac◆LB◆2\pi \times 1.0 \times 10^{-3} \times 0.0553◆RB◆◆LB◆4\pi \times 10^{-7}◆RB◆ = 277 A.

If you get this wrong, revise: Superconductivity

Problem 15

Silicon has a band gap of 1.1 eV and an intrinsic carrier concentration of ni=1.5×1016n_i = 1.5 \times 10^{16} m3^{-3} at 300 K. (a) Estimate nin_i at 350 K. (b) A sample of silicon is doped with phosphorus at a concentration of ND=5.0×1021N_D = 5.0 \times 10^{21} m3^{-3}. Calculate the ratio of conductivities: σdoped/σintrinsic\sigma_{\mathrm{doped}} / \sigma_{\mathrm{intrinsic}} at 300 K. (Assume mobility is the same for both.)

Answer. (a) ni(350)ni(300)=(350300)3/2exp[Eg2kB(13501300)]\frac{n_i(350)}{n_i(300)} = \left(\frac{350}{300}\right)^{3/2} \exp\left[-\frac{E_g}{2k_B}\left(\frac{1}{350} - \frac{1}{300}\right)\right].

Eg2kB=LB1.1×1.60×1019RB◆◆LB2×1.38×1023RB=LB1.76×1019RB◆◆LB2.76×1023RB=6377\frac{E_g}{2k_B} = \frac◆LB◆1.1 \times 1.60 \times 10^{-19}◆RB◆◆LB◆2 \times 1.38 \times 10^{-23}◆RB◆ = \frac◆LB◆1.76 \times 10^{-19}◆RB◆◆LB◆2.76 \times 10^{-23}◆RB◆ = 6377 K.

13501300=0.0028570.003333=4.76×104\frac{1}{350} - \frac{1}{300} = 0.002857 - 0.003333 = -4.76 \times 10^{-4} K1^{-1}.

ni(350)=1.5×1016×(1.167)3/2×exp(6377×4.76×104)n_i(350) = 1.5 \times 10^{16} \times (1.167)^{3/2} \times \exp(6377 \times 4.76 \times 10^{-4})

=1.5×1016×1.260×exp(3.035)=1.5×1016×1.260×20.8=3.93×1017= 1.5 \times 10^{16} \times 1.260 \times \exp(3.035) = 1.5 \times 10^{16} \times 1.260 \times 20.8 = 3.93 \times 10^{17} m3^{-3}.

(b) Since σ=nqμ\sigma = nq\mu and mobility μ\mu is the same: σdoped/σintrinsic=ND/ni=5.0×1021/1.5×1016=3.3×105\sigma_{\mathrm{doped}}/\sigma_{\mathrm{intrinsic}} = N_D/n_i = 5.0 \times 10^{21} / 1.5 \times 10^{16} = 3.3 \times 10^{5}.

Doping increased conductivity by over 5 orders of magnitude.

If you get this wrong, revise: Semiconductors

Problem 16

A copper wire of length 1.00 m and diameter 0.50 mm has resistance R0R_0 at 20C20^\circ\mathrm{C}. It is uniformly stretched to 1.50 times its original length. (a) Calculate the ratio R/R0R'/R_0 of the new resistance to the original resistance. (b) If the original resistance was 0.087 Ω\Omega, what is the new resistance? (c) The wire is now at a temperature of 60C60^\circ\mathrm{C}. What is its resistance? (α=3.9×103\alpha = 3.9 \times 10^{-3} C1^\circ\mathrm{C}^{-1}.)

Answer. (a) Volume conservation: A0L0=ALA_0 L_0 = A' L', so A=A0L0/L=A0/1.50A' = A_0 L_0/L' = A_0/1.50.

R/R0=(ρL/A)/(ρL0/A0)=(L/L0)×(A0/A)=1.50×1.50=2.25R'/R_0 = (\rho L'/A') / (\rho L_0/A_0) = (L'/L_0) \times (A_0/A') = 1.50 \times 1.50 = 2.25.

(b) R=2.25×0.087=0.196R' = 2.25 \times 0.087 = 0.196 Ω\Omega.

(c) R=R[1+α(6020)]=0.196×[1+3.9×103×40]=0.196×1.156=0.227R'' = R'[1 + \alpha(60 - 20)] = 0.196 \times [1 + 3.9 \times 10^{-3} \times 40] = 0.196 \times 1.156 = 0.227 Ω\Omega.

If you get this wrong, revise: Resistivity and Temperature Dependence of Resistance

Problem 17

An NTC thermistor with B=3900B = 3900 K has resistance R0=5000R_0 = 5000 Ω\Omega at T0=298T_0 = 298 K (25C^\circ\mathrm{C}). It is connected in a potential divider circuit with a 1000010\,000 Ω\Omega fixed resistor and a 9.0 V supply. (a) Calculate the thermistor resistance at 50C50^\circ\mathrm{C} (323 K). (b) Calculate the output voltage across the thermistor at 25C25^\circ\mathrm{C} and at 50C50^\circ\mathrm{C}. (c) Calculate the output voltage across the fixed resistor at each temperature.

Answer. (a) R=R0exp[B(1/T1/T0)]=5000×exp[3900×(1/3231/298)]R = R_0 \exp[B(1/T - 1/T_0)] = 5000 \times \exp[3900 \times (1/323 - 1/298)]

=5000×exp[3900×(3.096×1033.356×103)]= 5000 \times \exp[3900 \times (3.096 \times 10^{-3} - 3.356 \times 10^{-3})]

=5000×exp[3900×(2.60×104)]= 5000 \times \exp[3900 \times (-2.60 \times 10^{-4})]

=5000×exp(1.014)=5000×0.363=1813= 5000 \times \exp(-1.014) = 5000 \times 0.363 = 1813 Ω\Omega.

(b) At 25C25^\circ\mathrm{C}: Rtotal=5000+10000=15000R_{\mathrm{total}} = 5000 + 10\,000 = 15\,000 Ω\Omega. VT=500015000×9.0=3.00V_T = \frac{5000}{15\,000} \times 9.0 = 3.00 V.

At 50C50^\circ\mathrm{C}: Rtotal=1813+10000=11813R_{\mathrm{total}} = 1813 + 10\,000 = 11\,813 Ω\Omega. VT=181311813×9.0=1.38V_T = \frac{1813}{11\,813} \times 9.0 = 1.38 V.

(c) At 25C25^\circ\mathrm{C}: VR=9.03.00=6.00V_R = 9.0 - 3.00 = 6.00 V. (Or VR=1000015000×9.0=6.00V_R = \frac{10\,000}{15\,000} \times 9.0 = 6.00 V.)

At 50C50^\circ\mathrm{C}: VR=9.01.38=7.62V_R = 9.0 - 1.38 = 7.62 V. (Or VR=1000011813×9.0=7.62V_R = \frac{10\,000}{11\,813} \times 9.0 = 7.62 V.)

If you get this wrong, revise: Temperature Dependence of Resistance

Problem 18

A battery with e.m.f. E=12.0\mathcal{E} = 12.0 V and internal resistance r0=0.50r_0 = 0.50 Ω\Omega at 20C20^\circ\mathrm{C} is connected to an external load of RL=5.0R_L = 5.0 Ω\Omega. The internal resistance has a positive temperature coefficient of αr=4.0×103\alpha_r = 4.0 \times 10^{-3} C1^\circ\mathrm{C}^{-1}. (a) Calculate the current and power delivered to the load at 20C20^\circ\mathrm{C}. (b) If the battery warms up to 60C60^\circ\mathrm{C} during operation, calculate the new current and power delivered to the load. (c) Calculate the power dissipated within the battery at each temperature.

Answer. (a) At 20C20^\circ\mathrm{C}: r=0.50r = 0.50 Ω\Omega. Total resistance =0.50+5.0=5.50= 0.50 + 5.0 = 5.50 Ω\Omega.

I=E/Rtotal=12.0/5.50=2.18I = \mathcal{E}/R_{\mathrm{total}} = 12.0/5.50 = 2.18 A. PL=I2RL=(2.18)2×5.0=23.8P_L = I^2 R_L = (2.18)^2 \times 5.0 = 23.8 W.

(b) At 60C60^\circ\mathrm{C}: r=0.50×[1+4.0×103×(6020)]=0.50×1.16=0.580r = 0.50 \times [1 + 4.0 \times 10^{-3} \times (60 - 20)] = 0.50 \times 1.16 = 0.580 Ω\Omega.

Total resistance =0.580+5.0=5.580= 0.580 + 5.0 = 5.580 Ω\Omega. I=12.0/5.580=2.151I = 12.0/5.580 = 2.151 A.

PL=(2.151)2×5.0=23.1P_L = (2.151)^2 \times 5.0 = 23.1 W.

(c) At 20C20^\circ\mathrm{C}: Pint=I2r=(2.18)2×0.50=2.38P_{\mathrm{int}} = I^2 r = (2.18)^2 \times 0.50 = 2.38 W.

At 60C60^\circ\mathrm{C}: Pint=(2.151)2×0.580=2.68P_{\mathrm{int}} = (2.151)^2 \times 0.580 = 2.68 W.

Note: even though the internal resistance only increased by 16%, the internal power dissipation increased by 12.6%, while the useful power to the load decreased. This illustrates why battery heating is a serious engineering concern.

If you get this wrong, revise: Temperature Dependence of Resistance and Electrical Energy and Power


tip

Diagnostic Test Ready to test your understanding of Current and Resistance? The diagnostic test contains the hardest questions within the A-Level specification for this topic, each with a full worked solution.

Unit tests probe edge cases and common misconceptions. Integration tests combine Current and Resistance with other physics topics to test synthesis under exam conditions.

See Diagnostic Guide for instructions on self-marking and building a personal test matrix.

danger

Common Pitfalls

  • Confusing conventional current with electron flow: Conventional current flows from positive to negative (historical convention). Electrons actually flow from negative to positive. In circuit diagrams and exam questions, always assume conventional current direction unless specifically asked about electron flow.

  • Forgetting to convert units in I = nAev_d calculations: The drift velocity v_d is typically very small (around 0.1 mm/s), but students often forget to convert to metres per second before substituting. Similarly, cross-sectional area A must be in m squared, not cm squared or mm squared.

  • Misunderstanding what resistance depends on: Resistance depends on the material (resistivity), length, and cross-sectional area (R = rho * L / A), but NOT on the current or voltage applied. Resistance is a property of the component itself, not the circuit it is connected to.

  • Confusing resistivity with resistance: Resistivity (rho) is an intrinsic property of the material that does not depend on the dimensions of the wire. Resistance depends on both the material AND the dimensions. A thicker wire of the same material has lower resistance but the same resistivity.