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NCERT Exemplar · Q1

Q.The conductivity of a semiconductor increases with increase in temperature because

(a) number density of free current carriers increases.
(b) relaxation time increases.
(c) both number density of carriers and relaxation time increase.
(d) number density of current carriers increases, relaxation time decreases but effect of decrease in relaxation time is much less than increase in number density.
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Concept understanding — Intrinsic Carrier Concentration

Intrinsic carrier concentration is a foundational idea in semiconductor physics — let’s build it from the ground up, with no prior knowledge of semiconductors needed.


1. Intuition: What does "intrinsic" mean?

Imagine a pure, perfect crystal of silicon — no impurities, no defects. At absolute zero temperature (0 K0 \text{ K}), all electrons are tightly bound in the crystal lattice. No current flows.

Now, heat it up. Thermal energy shakes the atoms. Some electrons gain enough energy to break free from their bonds. When an electron leaves, it leaves behind a hole — a missing electron that behaves like a positive charge.

In this pure crystal, every free electron comes from a broken bond, and every broken bond creates one hole. So:

Number of free electrons = Number of holes

This balance is the hallmark of an intrinsic semiconductor.


2. The precise definition

Intrinsic carrier concentration (nin_i) is the number of free electrons (or holes) per unit volume in a pure, undoped semiconductor at thermal equilibrium.

It is denoted by nin_i and has units of cm−3\text{cm}^{-3} or m−3\text{m}^{-3}.

Key points:

  • It depends only on the material and temperature — not on doping.
  • For silicon at room temperature (300 K300 \text{ K}):

ni≈1.5×1010 cm−3n_i \approx 1.5 \times 10^{10} \text{ cm}^{-3}

  • For germanium: ni≈2.5×1013 cm−3n_i \approx 2.5 \times 10^{13} \text{ cm}^{-3}
  • For gallium arsenide: ni≈1.8×106 cm−3n_i \approx 1.8 \times 10^{6} \text{ cm}^{-3}

3. The formula (for exams)

The precise expression is:

ni=NcNv⋅e−Eg/(2kT)n_i = \sqrt{N_c N_v} \cdot e^{-E_g / (2kT)}

Where:

  • NcN_c = effective density of states in the conduction band
  • NvN_v = effective density of states in the valence band
  • EgE_g = bandgap energy (eV)
  • kk = Boltzmann constant (8.617×10−5 eV/K8.617 \times 10^{-5} \text{ eV/K})
  • TT = absolute temperature (K)

Important: The exponential term e−Eg/(2kT)e^{-E_g/(2kT)} dominates — a small change in EgE_g or TT causes a huge change in nin_i.


4. Why does it matter?

  • It sets the baseline for all semiconductor devices. Doping increases one carrier type, but the product n⋅p=ni2n \cdot p = n_i^2 always holds at equilibrium.
  • Temperature sensitivity: nin_i roughly doubles for every 10∘C10^\circ\text{C} rise in silicon. This is why circuits fail in heat.
  • Device limits: In a p-n junction, leakage current depends on ni2n_i^2.

5. Quick check for understanding

Question: If you heat a pure silicon crystal from 300 K300\text{ K} to 400 K400\text{ K}, what happens to nin_i?

Answer: It increases dramatically — the exponential term e−Eg/(2kT)e^{-E_g/(2kT)} becomes much larger because TT is in the denominator of the exponent. For silicon, nin_i rises from ≈1.5×1010\approx 1.5\times10^{10} to roughly ≈5×1012 cm−3\approx 5\times10^{12}\ \text{cm}^{-3} (about 2-3 orders of magnitude, not 4).


Bottom line: Intrinsic carrier concentration is the natural electron-hole population in a pure semiconductor — a fundamental property that governs all semiconductor behaviour.

"Intrinsic carrier concentration formula semiconductor" and "semiconductor electronics class 12 physics ncert" are commonly searched phrases, both anchored in the Semiconductor Electronics chapter of the NCERT/CBSE Class 12 Physics curriculum. This baseline electron-hole concentration also underlies several JEE Main and NEET p-n junction questions.

Why this formula?

Why Intrinsic Carrier Concentration Has That Formula

The intrinsic carrier concentration nin_i is the number of electrons (or holes) per unit volume in a pure, undoped semiconductor at thermal equilibrium. The formula you see in every textbook is:

ni=NcNv e−Eg/2kTn_i = \sqrt{N_c N_v} \, e^{-E_g / 2kT}

where NcN_c and NvN_v are the effective density of states in the conduction and valence bands, EgE_g is the bandgap energy, kk is Boltzmann's constant, and TT is absolute temperature.

This isn't pulled from thin air. It comes from a simple physical balance: in an intrinsic semiconductor, every electron in the conduction band leaves behind a hole in the valence band. So the electron concentration nn must equal the hole concentration pp, and both equal nin_i.

Step 1: The electron and hole concentrations individually

Electrons in the conduction band follow Fermi-Dirac statistics. For non-degenerate semiconductors (which intrinsic ones are, since the Fermi level lies near midgap), the distribution approximates the Maxwell-Boltzmann tail:

n=Nc e−(Ec−EF)/kTn = N_c \, e^{-(E_c - E_F)/kT}

Similarly, holes in the valence band:

p=Nv e−(EF−Ev)/kTp = N_v \, e^{-(E_F - E_v)/kT}

Here EcE_c is the conduction band edge, EvE_v is the valence band edge, and EFE_F is the Fermi level. The effective densities NcN_c and NvN_v come from integrating the density of states times the Boltzmann factor — they depend on the effective masses of electrons and holes and on temperature.

Step 2: The intrinsic condition

In an intrinsic semiconductor, there are no dopants. Every electron that jumps to the conduction band creates exactly one hole. So:

n=pn = p

Set the two expressions equal:

Nc e−(Ec−EF)/kT=Nv e−(EF−Ev)/kTN_c \, e^{-(E_c - E_F)/kT} = N_v \, e^{-(E_F - E_v)/kT}

Take natural logs and solve for EFE_F:

−(Ec−EF)+ln⁡Nc=−(EF−Ev)+ln⁡Nv-(E_c - E_F) + \ln N_c = -(E_F - E_v) + \ln N_v

EF=Ec+Ev2+kT2ln⁡NvNcE_F = \frac{E_c + E_v}{2} + \frac{kT}{2} \ln\frac{N_v}{N_c}

The Fermi level in an intrinsic semiconductor sits very close to the middle of the bandgap, shifted slightly by the ratio Nv/NcN_v/N_c. For most practical purposes, it's at midgap.

Step 3: Multiply to eliminate EFE_F

Now here's the clever part. Instead of solving for EFE_F directly, multiply nn and pp:

np=NcNv e−(Ec−EF)/kT e−(EF−Ev)/kTn p = N_c N_v \, e^{-(E_c - E_F)/kT} \, e^{-(E_F - E_v)/kT}

The EFE_F terms cancel:

np=NcNv e−(Ec−Ev)/kT=NcNv e−Eg/kTn p = N_c N_v \, e^{-(E_c - E_v)/kT} = N_c N_v \, e^{-E_g/kT}

This product npnp is a constant for a given material at a given temperature — it does not depend on the Fermi level. This is the law of mass action for semiconductors.

Step 4: Apply the intrinsic condition

Since n=p=nin = p = n_i in an intrinsic semiconductor:

ni2=NcNv e−Eg/kTn_i^2 = N_c N_v \, e^{-E_g/kT}

Take the square root:

ni=NcNv e−Eg/2kTn_i = \sqrt{N_c N_v} \, e^{-E_g/2kT}

Important

The factor of 1/21/2 in the exponent comes directly from the square root — it's not an arbitrary fudge. Physically, it reflects that creating an electron-hole pair requires energy EgE_g, but the probability of that event involves both an electron being excited and a hole being left behind, each contributing half the Boltzmann factor.

Why this formula makes physical sense

  • Bandgap EgE_g: A larger gap means fewer electrons can be thermally excited across it — nin_i drops exponentially.
  • Temperature TT: Higher temperature gives more thermal energy, so nin_i rises sharply (the exponential dominates).
  • Effective masses (through NcN_c and NvN_v): Materials with heavier carriers have more states near the band edges, so nin_i is larger.
Watch out

A common mistake is to think nin_i depends on doping. It does not — nin_i is a material property at a given temperature. Doping changes nn and pp individually, but their product npnp always equals ni2n_i^2 at equilibrium.

The temperature dependence in practice

For silicon at 300 K, ni≈1.5×1010 cm−3n_i \approx 1.5 \times 10^{10} \text{ cm}^{-3}. For germanium, it's about 2.4×1013 cm−32.4 \times 10^{13} \text{ cm}^{-3} — the smaller bandgap (0.67 eV vs 1.12 eV) makes a huge difference. For gallium arsenide (1.43 eV), nin_i is only about 2×106 cm−32 \times 10^6 \text{ cm}^{-3}.

The formula ni=NcNv e−Eg/2kTn_i = \sqrt{N_c N_v} \, e^{-E_g/2kT} is the foundation for understanding pn junctions, transistors, and essentially all semiconductor device physics. It's not just a memorised equation — it's the direct consequence of thermal equilibrium and the requirement that charge neutrality holds in a pure crystal.

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