Why Resistivity Values Differ Across Materials

We have already derived that the resistivity of a material is ρ=mne2τ,\rho = \frac{m}{n e^2 \tau}, where nn is the density of free charge carriers (per m3^3) and τ\tau is the mean free time between collisions. Two materials can have very different resistivities for two reasons:

  1. Different carrier densities (nn) — Metals have roughly n1028n \sim 10^{28} electrons/m3^3, semiconductors have n1016n \sim 10^{16} to 101910^{19} at room temperature, and insulators have almost no free carriers.
  2. Different relaxation times (τ\tau) — Even for two metals with similar nn, scattering from impurities, lattice defects, and thermal vibrations can make τ\tau very different.

That is why the resistivity of materials spans an astonishing 26 orders of magnitude, from superconductors (ρ=0\rho = 0) to fused quartz (ρ1016Ωm\rho \approx 10^{16}\,\Omega\cdot\text{m}).

Classification of materials by resistivity

[Memory hook] Remember the three classes:

  • Conductors: ρ108\rho \approx 10^{-8} to 106Ωm10^{-6}\,\Omega\cdot\text{m} (Ag, Cu, Al, Fe)
  • Semiconductors: ρ105\rho \approx 10^{-5} to 106Ωm10^{6}\,\Omega\cdot\text{m} (Ge, Si, C in graphite form)
  • Insulators: ρ1010\rho \approx 10^{10} to 1016Ωm10^{16}\,\Omega\cdot\text{m} (glass, rubber, fused quartz)

Key Point: The large gap between conductors and insulators is dominated mainly by the huge difference in carrier density nn.

Temperature Dependence — The Big Picture

Experiments show that for almost every material, resistivity changes with temperature. But how it changes depends on the material class:

Material class Sign of dρ/dTd\rho/dT Reason
Metals (conductors) Positive (ρ\rho rises with TT) Lattice vibrations increase → smaller τ\tau; nn barely changes
Alloys (Nichrome, Manganin, Constantan) Slightly positive, very small Disordered lattice already produces strong scattering; extra thermal scattering adds little
Semiconductors Negative (ρ\rho falls with TT) Thermal energy sets free many more carriers; rise in nn dominates over fall in τ\tau
Insulators Negative (similar to semiconductors) Carrier density is so low that any thermal generation has a huge fractional effect
Superconductors (below TcT_c) ρ\rho = 0 Cooper pairs move without scattering

Resistivity vs temperature for different materials

The equation ρ=m/(ne2τ)\rho = m/(n e^2 \tau) helps explain these trends:

  • In a metal, nn is fixed and τ\tau drops as TT rises, so ρ\rho increases.
  • In a semiconductor, as TT rises nn increases exponentially while τ\tau only falls slowly, so ρ\rho decreases.

Quantifying the Temperature Dependence in Metals

For metals in a limited range of temperatures, resistivity varies approximately linearly with temperature:

ρT=ρ0[1+α(TT0)]\boxed{\rho_T = \rho_0 \big[1 + \alpha (T - T_0)\big]}

where:

  • ρ0\rho_0 is the resistivity at a reference temperature T0T_0 (usually 00^\circC or 2020^\circC)
  • ρT\rho_T is the resistivity at temperature TT
  • α\alpha is the temperature coefficient of resistivity, with SI unit K1^{-1} (or ^\circC1^{-1})

Since the dimensions of a conductor change only slightly with temperature, the same form also holds for resistance:

RT=R0[1+α(TT0)]R_T = R_0 \big[1 + \alpha (T - T_0)\big]

Typical values of α\alpha at 2020^\circC

Material α\alpha (K1^{-1})
Silver (Ag) +4.1×103+4.1 \times 10^{-3}
Copper (Cu) +4.0×103+4.0 \times 10^{-3}
Aluminium (Al) +4.3×103+4.3 \times 10^{-3}
Iron (Fe) +6.5×103+6.5 \times 10^{-3}
Tungsten (W) +4.5×103+4.5 \times 10^{-3}
Manganin (alloy) +0.002×103+0.002 \times 10^{-3}
Nichrome (alloy) +0.4×103+0.4 \times 10^{-3}
Carbon (graphite) 0.5×103-0.5 \times 10^{-3}
Silicon (semiconductor) 70×103-70 \times 10^{-3}

Two things jump out:

  1. Pure metals all have similar α\alpha (4×103\sim 4 \times 10^{-3} K1^{-1}) — about 0.4% change per kelvin.
  2. Alloys have α\alpha hundreds of times smaller — that is exactly why Manganin and Constantan are used to make standard resistors and resistance boxes.

Alloy vs pure metal: temperature dependence

[JEE Tip] Over wide temperature ranges the relation ρT=ρ0[1+α(TT0)]\rho_T = \rho_0[1+\alpha(T-T_0)] breaks down. For a clean metal at very low TT, ρ\rho approaches a non-zero residual resistivity due to impurity scattering — it does not go to zero.

Why Do Semiconductors Have Negative α\alpha?

In a semiconductor the number of free carriers depends strongly on temperature. The density of carriers obeys (approximately):

n(T)T3/2eEg/(2kBT),n(T) \propto T^{3/2}\, e^{-E_g / (2 k_B T)},

where EgE_g is the energy band gap and kBk_B is Boltzmann's constant.

As TT increases:

  • The exponential factor grows very rapidly — many more electrons can jump across the band gap.
  • Hence nn rises much faster than τ\tau falls.
  • From ρ=m/(ne2τ)\rho = m/(n e^2 \tau), the rise in nn dominates and ρ\rho decreases with TT.

This explains why:

  • A thermistor (semiconductor resistor) is used in circuits to compensate for temperature drift — its resistance falls as it heats up.
  • Semiconductor thermometers exploit this strong TT-dependence to measure small temperature changes.
  • A semiconductor at very low temperatures can behave almost like an insulator — not enough thermal energy to lift electrons into the conduction band.

[Common trap] Students sometimes say "semiconductors have negative α\alpha because electrons collide less at high TT." This is wrong — τ\tau still decreases at higher TT. The real reason is the huge rise in nn.

Superconductivity — When Resistivity Becomes Exactly Zero

At very low temperatures, certain metals, alloys, and ceramic oxides lose all resistance — a phenomenon discovered by Kamerlingh Onnes in 1911 while cooling mercury below 4.24.2 K. Below a material-specific critical temperature TcT_c, the resistivity drops sharply to exactly zero.

Superconductor transition

Key features:

  • Below TcT_c, electrons form correlated pairs (Cooper pairs) that glide through the lattice without scattering.
  • A current set up in a superconducting loop can persist for years with no measurable decay — a test of ρ=0\rho = 0 to incredible precision.
  • Superconductors expel magnetic fields from their interior (Meissner effect) — this is why they can levitate magnets.

Some important TcT_c values

Material TcT_c (K)
Mercury (Hg) 4.2
Lead (Pb) 7.2
Niobium (Nb) 9.3
YBa2_2Cu3_3O7_7 (YBCO) 92
HgBa2_2Ca2_2Cu3_3O8_8 134

Materials with Tc>77T_c > 77 K (the boiling point of liquid nitrogen) are called high-temperature superconductors. Their discovery in 1986 was a huge leap — you no longer need expensive liquid helium to cool them.

Applications

  • Superconducting magnets (MRI, particle accelerators, fusion reactors).
  • SQUIDs — extremely sensitive magnetometers used in biomedical imaging.
  • Maglev trains — frictionless magnetic levitation.
  • Efficient power transmission (zero I2RI^2 R losses).

Key Point: A superconductor does not merely have low resistance — it has exactly zero resistance, and hence zero voltage drop for any finite current below TcT_c.

Solved Examples

Example 1: Resistance of Copper Wire at a High Temperature

The resistance of a copper coil at 2020^\circC is 2.5Ω2.5\,\Omega. Find its resistance at 100100^\circC. (αCu=4.0×103\alpha_\text{Cu} = 4.0 \times 10^{-3} K1^{-1})

Solution: Using RT=R0[1+α(TT0)],R_T = R_0[1 + \alpha(T - T_0)], we get R=2.5[1+4.0×103(10020)]=2.5(1+0.32)=2.5×1.32=3.30ΩR = 2.5[1 + 4.0 \times 10^{-3}(100 - 20)] = 2.5(1 + 0.32) = 2.5 \times 1.32 = 3.30\,\Omega

Final Answer: 3.30Ω3.30\,\Omega

Example 2: Finding the Temperature Coefficient

A platinum resistance thermometer reads 5.0Ω5.0\,\Omega at 00^\circC and 5.2Ω5.2\,\Omega at 5050^\circC. Find α\alpha for platinum.

Solution: Using RT=R0[1+α(TT0)],R_T = R_0[1 + \alpha(T - T_0)], we get 5.2=5.0[1+50α]5.2 = 5.0[1 + 50\alpha] 1.04=1+50α1.04 = 1 + 50\alpha 50α=0.0450\alpha = 0.04 α=8.0×104K1\alpha = 8.0 \times 10^{-4}\,\text{K}^{-1}

Final Answer: 8.0×104K18.0 \times 10^{-4}\,\text{K}^{-1}

Example 3: Temperature from a Measured Resistance

A tungsten filament has R0=100ΩR_0 = 100\,\Omega at 2020^\circC. When the bulb is lit, its resistance is 1100Ω1100\,\Omega. Estimate the operating temperature. (αW=4.5×103\alpha_\text{W} = 4.5 \times 10^{-3} K1^{-1})

Solution: 1100=100[1+4.5×103(T20)]1100 = 100[1 + 4.5 \times 10^{-3}(T - 20)] 11=1+4.5×103(T20)11 = 1 + 4.5 \times 10^{-3}(T - 20) 4.5×103(T20)=104.5 \times 10^{-3}(T - 20) = 10 T20=104.5×1032222T - 20 = \frac{10}{4.5 \times 10^{-3}} \approx 2222 T2242CT \approx 2242^\circ\text{C}

Final Answer: 2242C\approx 2242^\circ\text{C}

Example 4: Two Resistors in Series — Effective α\alpha

A 40Ω40\,\Omega wire of copper (α1=4.0×103\alpha_1 = 4.0 \times 10^{-3} K1^{-1}) is joined in series with a 60Ω60\,\Omega wire of iron (α2=5.0×103\alpha_2 = 5.0 \times 10^{-3} K1^{-1}). Find the effective temperature coefficient of the combination.

Solution: For small temperature change, αeff=R1α1+R2α2R1+R2\alpha_\text{eff} = \frac{R_1\alpha_1 + R_2\alpha_2}{R_1 + R_2} So, αeff=40(4.0×103)+60(5.0×103)100\alpha_\text{eff} = \frac{40(4.0 \times 10^{-3}) + 60(5.0 \times 10^{-3})}{100} =0.16+0.30100=4.6×103K1= \frac{0.16 + 0.30}{100} = 4.6 \times 10^{-3}\,\text{K}^{-1}

Final Answer: 4.6×103K14.6 \times 10^{-3}\,\text{K}^{-1}

Example 5: Designing a Temperature-Stable Resistor

You want a series combination of a carbon resistor (αC=5×104\alpha_C = -5 \times 10^{-4} K1^{-1}) and a copper wire (αCu=+4.0×103\alpha_\text{Cu} = +4.0 \times 10^{-3} K1^{-1}) so that the total resistance is nearly temperature-independent. If the copper wire has resistance RCu=10ΩR_\text{Cu} = 10\,\Omega at 2020^\circC, how large should the carbon resistance be?

Solution: For zero net temperature coefficient, RCαC+RCuαCu=0R_C\alpha_C + R_\text{Cu}\alpha_\text{Cu} = 0 RC=RCuαCuαC=10×4.0×1035×104=80ΩR_C = -\frac{R_\text{Cu}\alpha_\text{Cu}}{\alpha_C} = -\frac{10 \times 4.0 \times 10^{-3}}{-5 \times 10^{-4}} = 80\,\Omega

Final Answer: 80Ω80\,\Omega

Example 6: Silver Wire Near a Flame

A silver wire has resistivity ρ0=1.62×108Ωm\rho_0 = 1.62 \times 10^{-8}\,\Omega\cdot\text{m} at 27.527.5^\circC. Find its resistivity at 100100^\circC. (αAg=4.1×103\alpha_\text{Ag} = 4.1 \times 10^{-3} K1^{-1})

Solution: Using ρT=ρ0[1+α(TT0)],\rho_T = \rho_0[1 + \alpha(T - T_0)], we get ρ=1.62×108[1+4.1×103(10027.5)]\rho = 1.62 \times 10^{-8}[1 + 4.1 \times 10^{-3}(100 - 27.5)] =1.62×108[1+0.29725]= 1.62 \times 10^{-8}[1 + 0.29725] =1.62×108×1.297252.10×108Ωm= 1.62 \times 10^{-8} \times 1.29725 \approx 2.10 \times 10^{-8}\,\Omega\cdot\text{m}

Final Answer: 2.10×108Ωm2.10 \times 10^{-8}\,\Omega\cdot\text{m}

Example 7: Negative α\alpha — A Thermistor

A thermistor has resistance R0=2000ΩR_0 = 2000\,\Omega at 2020^\circC. Its temperature coefficient in this range is α=0.045\alpha = -0.045 K1^{-1}. Find its resistance at 4040^\circC.

Solution: R=2000[1+(0.045)(4020)]=2000(10.9)=200ΩR = 2000[1 + (-0.045)(40 - 20)] = 2000(1 - 0.9) = 200\,\Omega

Final Answer: 200Ω200\,\Omega

Note: This uses the linear approximation over a small range.

Example 8: A Heating Coil's Hot Resistance

A nichrome heating coil has resistance 50Ω50\,\Omega at 3030^\circC. In operation, it reaches 830830^\circC. If αNichrome=4.0×104\alpha_\text{Nichrome} = 4.0 \times 10^{-4} K1^{-1}, find its hot resistance.

Solution: R=50[1+4.0×104(83030)]=50[1+0.32]=50×1.32=66ΩR = 50[1 + 4.0 \times 10^{-4}(830 - 30)] = 50[1 + 0.32] = 50 \times 1.32 = 66\,\Omega

Final Answer: 66Ω66\,\Omega

Example 9: Solving for the Temperature Coefficient from Two Measurements

A wire has R1=2.0ΩR_1 = 2.0\,\Omega at T1=25T_1 = 25^\circC and R2=2.5ΩR_2 = 2.5\,\Omega at T2=150T_2 = 150^\circC. Find the temperature coefficient of the wire's material, taking T1T_1 as reference.

Solution: Using R2=R1[1+α(T2T1)],R_2 = R_1[1 + \alpha(T_2 - T_1)], we get α=R2R1R1(T2T1)=2.52.02.0(15025)=0.5250=2.0×103K1\alpha = \frac{R_2 - R_1}{R_1(T_2 - T_1)} = \frac{2.5 - 2.0}{2.0(150 - 25)} = \frac{0.5}{250} = 2.0 \times 10^{-3}\,\text{K}^{-1}

Final Answer: 2.0×103K12.0 \times 10^{-3}\,\text{K}^{-1}

Example 10: Resistance Doubles at What Temperature?

A copper conductor has R0=5ΩR_0 = 5\,\Omega at 2020^\circC. At what temperature will its resistance be twice its value at 2020^\circC? (αCu=4.0×103\alpha_\text{Cu} = 4.0 \times 10^{-3} K1^{-1})

Solution: For doubling, 2R0=R0[1+α(T20)]2R_0 = R_0[1 + \alpha(T - 20)] 2=1+α(T20)2 = 1 + \alpha(T - 20) 1=α(T20)1 = \alpha(T - 20) T20=14.0×103=250T - 20 = \frac{1}{4.0 \times 10^{-3}} = 250 T=270CT = 270^\circ\text{C}

Final Answer: 270C270^\circ\text{C}

Example 11: Why α\alpha Depends on Reference Temperature

In a data table, the temperature coefficient of copper is listed as α0=4.3×103\alpha_0 = 4.3 \times 10^{-3} K1^{-1} at 00^\circC and α20=4.0×103\alpha_{20} = 4.0 \times 10^{-3} K1^{-1} at 2020^\circC. Why are they different?

Solution: The coefficient α\alpha is defined relative to a reference temperature T0T_0: α=1ρ0dρdTT=T0\alpha = \frac{1}{\rho_0}\frac{d\rho}{dT}\Bigg|_{T=T_0} Since ρ0\rho_0 depends on the reference temperature, the quoted value of α\alpha changes slightly when the reference temperature changes.

Final Answer: α\alpha depends on the chosen reference temperature, so α0\alpha_0 and α20\alpha_{20} need not be exactly equal.

Example 12: Manganin — Why It Is Special

Standard resistance coils are made of Manganin, whose temperature coefficient is about 2×1052 \times 10^{-5} K1^{-1}. Compare the fractional change in resistance over ΔT=50\Delta T = 50^\circC for Manganin and pure copper.

Solution: For Manganin: ΔRR=αΔT=2×105×50=103=0.1%\frac{\Delta R}{R} = \alpha \Delta T = 2 \times 10^{-5} \times 50 = 10^{-3} = 0.1\%

For copper: ΔRR=4.0×103×50=0.20=20%\frac{\Delta R}{R} = 4.0 \times 10^{-3} \times 50 = 0.20 = 20\%

Thus copper changes 200 times more for the same temperature rise.

Final Answer:

  • Manganin: 0.1%0.1\%
  • Copper: 20%20\%
  • Copper changes 200 times more