Intuition Why a whole page of examples?
The parent note gave you three formulas and three regions. But a formula only lives when you push it into every corner: coldest cold, hottest hot, the flat middle, the zero-doping edge, the "what temperature exactly" inversion, and the real-world twist where the device fails.
This page walks a scenario matrix — one worked example per cell — so that after reading it, you never meet a temperature-dependence question you haven't already seen the shape of.
Everything here uses only symbols the parent built. A few appear so often we re-state them in plain words right here, so this page stands on its own:
Definition The symbols this page leans on
n = number of free electrons per cm³ in the conduction band (our main unknown for n -type).
p = number of free holes (empty electron seats) per cm³ in the valence band — the electron's counterpart carrier, and the main unknown for p -type.
N D = number of donor atoms per cm³ you added (donates electrons, makes n -type). N A = number of acceptor atoms per cm³ (accepts electrons / donates holes, makes p -type).
N D + = number of donors that have actually given up their electron (ionized) at the current temperature. At most it equals N D .
n i = intrinsic density: how many electron-hole pairs the pure host lattice makes on its own by breaking its own bonds.
n i ′ = the piece of n that comes specifically from that intrinsic band-to-band excitation (as opposed to from donors).
N C , N V = band-edge effective densities of states ("how many seats" near each band edge).
E g = band gap; E D = donor ionization energy; E A = acceptor ionization energy; k B = Boltzmann constant; T = absolute temperature.
The master accounting is n = N D + + n i ′ : your electrons come either from ionized donors or from the lattice tearing its own bonds. If any of this feels shaky, revisit Temperature dependence of carrier concentration .
Intuition The whole page is
n -type, but p -type is a mirror
Every formula on this page is written for an n -type (donor) semiconductor. A p -type (acceptor) semiconductor is the exact mirror image : swap electrons ↔ holes, n ↔ p , N C ↔ N V , N D ↔ N A , E D ↔ E A , and measure the acceptor level up from E V instead of down from E C . The plateau becomes p ≈ N A , the freeze-out exponent becomes E A /2 k B T , and the intrinsic line is identical (it doesn't care which dopant you used). So every worked example below has a hole-dominated twin you get for free by the swap — see Intrinsic vs extrinsic semiconductors and Doping and dopant ionization .
One caveat we flag but do not solve here: all of this assumes non-degenerate statistics — the Boltzmann approximation to Fermi-Dirac distribution , valid when E F sits at least a few k B T inside the gap. At very high doping (N D ≳ 1 0 19 cm⁻³ in Si) E F pushes into the band, the "+1" in Fermi-Dirac can no longer be dropped, the plateau formula n ≈ N D and the mass-action law both break, and you need the full Fermi integral. Every example here stays comfortably non-degenerate (N D ≤ 1 0 16 ).
Handy constant we reuse everywhere:
k B = 8.617 × 1 0 − 5 eV/K ⇒ k B T = 0.02585 eV at T = 300 K
And the three master formulas from the parent, restated once so this page is self-contained:
n i = N C N V e − E g /2 k B T , N C , V ∝ T 3/2 , n freeze ≈ 2 N C N D e − E D /2 k B T
Every temperature-dependence problem is one of these cells. The last column names the example that nails it.
#
Case class
What makes it distinct
Covered by
A
Intrinsic, plug-and-chug
high T or pure material, use n i formula directly
Ex 1
B
Extrinsic plateau
mid T , answer is just n ≈ N D
Ex 2
C
Freeze-out (low T )
discrete donor level, E D /2 exponent
Ex 3
D
Boundary / inversion ("at what T ?")
solve exponential for T , not n
Ex 4
E
Zero-doping edge case: N D = 0
pure semiconductor, extrinsic region vanishes
Ex 5
F
Limiting behaviour (T → 0 , T → ∞ )
check the formulas don't blow up
Ex 6
G
Real-world word problem
a car engine chip in the heat
Ex 7
H
Exam twist: read a slope
reverse-engineer E g or E D from a graph
Ex 8
I
Sign/direction reasoning
"double doping — which way does each boundary move?"
Ex 9
We use silicon numbers throughout so answers are comparable:
E g = 1.12 eV, N C = 2.8 × 1 0 19 cm − 3 , N V = 1.04 × 1 0 19 cm − 3 (both quoted at 300 K), E D = 0.045 eV (phosphorus in Si).
The figure above is your map: it marks where each example lives on the ln n -vs-1/ T curve. Keep glancing back at it.
Compute n i for silicon at T = 300 K.
The formula we will use (restated so nothing is off-page):
n i = N C N V e − E g /2 k B T
Read it as "seats × occupancy": N C N V counts the available band-edge states (the geometric mean of the two bands), and e − E g /2 k B T is the Boltzmann probability that thermal energy lifts an electron across half the gap. The 2 1 is earned in Example 3.
Forecast: Guess the order of magnitude first. The gap is 1.12 eV, thermal energy is 0.026 eV — that's a ratio of ~43, and it sits inside a decaying exponential. Do you expect n i near 1 0 19 (the prefactor) or far below it? Write your guess.
Step 1 — Assemble the exponent.
2 k B T E g = 2 × 0.02585 1.12 = 0.0517 1.12 = 21.66
Why this step? In the formula above the exponent is the "boss" factor, so nail it first.
Step 2 — Exponential factor.
e − 21.66 = 3.92 × 1 0 − 10
Why this step? This lone number is what crushes n i far below the prefactor — that's the answer to the forecast.
Step 3 — Prefactor.
N C N V = 2.8 × 1 0 19 ⋅ 1.04 × 1 0 19 = 1.706 × 1 0 19 cm − 3
Why this step? This is the geometric mean of the two band densities of states — the "how many seats" part of seats × occupancy.
Step 4 — Multiply.
n i = 1.706 × 1 0 19 × 3.92 × 1 0 − 10 ≈ 6.7 × 1 0 9 cm − 3
Why this step? The full formula is (seats) × (occupancy) = N C N V × e − E g /2 k B T ; only after both factors are in hand does multiplying them give the actual carrier density. Step 1–3 built the pieces; this step is where the physics "how many seats × how likely filled" finally becomes a number.
Verify: Units: cm − 3 × ( dimensionless ) = cm − 3 ✓. The standard textbook value for Si at 300 K is quoted as ≈ 1.0 × 1 0 10 cm − 3 using a slightly larger effective-mass prefactor; our 6.7 × 1 0 9 is the same order of magnitude and correct for these N C , N V ✓. Notice: the prefactor 1 0 19 got knocked down nine orders of magnitude by the exponential — the boss won, as forecast should have warned.
Silicon doped with N D = 1 0 16 cm − 3 phosphorus, at T = 300 K. What is n ?
Forecast: Will n be closer to 1 0 16 or to 1 0 10 ? Which source wins — donors or intrinsic pairs?
Step 1 — Compare the two carrier sources.
N D = 1 0 16 , n i ≈ 1 0 10 ⇒ n i N D ≈ 1 0 6
Why this step? The master equation n = N D + + n i ′ (defined at the top: N D + = ionized donors, n i ′ = intrinsic contribution) has two sources; you must find which dominates before writing an answer.
Step 2 — Quantitatively check that donors are fully ionized.
The un-ionized (still-bound) donor fraction at temperature T is set by how many donors keep their electron; a standard estimate uses the freeze-out density from the parent as the ionized count and compares it to N D . Compute the freeze-out prefactor and exponent at 300 K:
2 k B T E D = 2 × 0.02585 0.045 = 0.87 , e − 0.87 = 0.42
n freeze = 2 N C N D e − 0.87 = 2 2.8 × 1 0 19 ⋅ 1 0 16 × 0.42 = 1.18 × 1 0 18 × 0.42 = 5.0 × 1 0 17
This freeze-out estimate (5 × 1 0 17 ) is far larger than N D = 1 0 16 , which is the formula's way of saying "the donor supply, not the ionization probability, is the bottleneck" — i.e. ionization has run to completion and N D + ≈ N D .
Why this step? The freeze-out formula only caps n below N D when it evaluates smaller than N D . When it evaluates larger (as here), every donor is ionized. This is the honest quantitative test; "k B T vs E D " alone is misleading because k B T = 0.026 eV is actually smaller than E D = 0.045 eV — yet full ionization still holds because the huge N C of available conduction seats pulls electrons off the donors entropically.
Step 3 — State the plateau value.
n ≈ N D = 1 0 16 cm − 3
Why this step? With N D ≫ n i and full ionization confirmed, the intrinsic contribution n i ′ is a rounding error.
Verify: Sanity via charge neutrality and law of mass action (Law of mass action ): the hole density (defined at the top) is p = n i 2 / n = ( 1 0 10 ) 2 /1 0 16 = 1 0 4 cm − 3 . Holes are vanishing — exactly what "n -type, extrinsic" means ✓. Adding n i ′ back changes n by one part in 1 0 12 , utterly negligible ✓.
The same N D = 1 0 16 sample is cooled to T = 50 K. Estimate n using the freeze-out formula
n freeze ≈ 2 N C N D e − E D /2 k B T , E D = 0.045 eV .
Forecast: At 300 K we had n = 1 0 16 . At 50 K, will n be roughly the same, or dramatically less? Guess an order of magnitude.
Where the 2 1 in the exponent comes from (on-page derivation).
Treat donor ionization as a chemical reaction: (bound electron on donor) ⇌ (free electron in band) + (ionized donor + ) . At equilibrium the mass-action-style balance reads
N D 0 n ⋅ N D + = N C e − E D / k B T ,
where N D 0 is the still-bound donor count and the right side is "seats in the band × Boltzmann cost E D to reach them." In the freeze-out regime most donors are still bound, so N D 0 ≈ N D , and charge neutrality gives n ≈ N D + . Substituting both:
N D n 2 = N C e − E D / k B T ⇒ n = N C N D e − E D /2 k B T .
There is the 2 1 : it appears because we solved for n by taking a square root of an equation whose exponent was the full E D — exactly the same square-root move that put 2 1 in front of E g for n i . (The extra 2 1 in the parent's formula is a degeneracy factor for the donor level; it doesn't touch the exponent.)
Step 1 — Recompute k B T at the new temperature.
k B T = 8.617 × 1 0 − 5 × 50 = 4.31 × 1 0 − 3 eV
Why this step? Every exponent depends on k B T ; at low T this number shrinks, which inflates the exponent — the whole reason freeze-out bites.
Step 2 — Exponent.
2 k B T E D = 2 × 4.31 × 1 0 − 3 0.045 = 8.62 × 1 0 − 3 0.045 = 5.22
Why the factor of 2? Derived just above: solving the ionization mass-action balance for n takes a square root, halving the exponent.
Step 3 — Scale N C down to 50 K.
Since N C ∝ T 3/2 :
N C ( 50 ) = 2.8 × 1 0 19 ( 300 50 ) 3/2 = 2.8 × 1 0 19 × 0.0680 = 1.90 × 1 0 18 cm − 3
Why this step? N C was quoted at 300 K; the prefactor is temperature-dependent and we must not reuse the 300 K value blindly.
Step 4 — Prefactor and assemble.
2 N C N D = 2 1.90 × 1 0 18 ⋅ 1 0 16 = 9.49 × 1 0 33 = 9.74 × 1 0 16
n freeze = 9.74 × 1 0 16 × e − 5.22 = 9.74 × 1 0 16 × 5.39 × 1 0 − 3 ≈ 5.3 × 1 0 14 cm − 3
Why this step? Same "seats × occupancy" logic as Ex 1, but the seats reservoir is now donors feeding the band: the freeze-out formula is prefactor × exponential, so only after computing the temperature-corrected prefactor (this step's first line) and multiplying by the exponential (second line) do the two pieces combine into the physical carrier count.
Verify: n = 5.3 × 1 0 14 < N D = 1 0 16 ✓ — carriers have partly frozen back onto donors , so fewer than the doping. That matches the "cold ⇒ more insulating" story (Doping and dopant ionization ). Units: cm − 3 ✓. The forecast should have said "dramatically less," and indeed it dropped ~20× below the plateau.
For the N D = 1 0 16 sample, at roughly what temperature does the material stop being extrinsic and become intrinsic? (Intrinsic onset: n i ( T ) ≈ N D .)
Forecast: Above or below 300 K? By a lot or a little?
Step 1 — Write the onset condition.
N C N V e − E g /2 k B T = N D
Why this step? Intrinsic wins when the intrinsic source equals the donor source — set the two equal.
Step 2 — First pass: freeze the prefactor, then bound the error it causes.
Treat N C N V ≈ 1.71 × 1 0 19 (its 300 K value) to get a first estimate:
e − E g /2 k B T = N C N V N D = 1.71 × 1 0 19 1 0 16 = 5.85 × 1 0 − 4
Why this step? Isolate the exponential so we can take a logarithm — but we owe the reader an error estimate, because the prefactor really does grow with T .
Step 3 — Take the natural log (WHY log?).
− 2 k B T E g = ln ( 5.85 × 1 0 − 4 ) = − 7.44 ⇒ T ≈ 2 k B × 7.44 E g = 874 K
Why the logarithm? T is trapped inside an exponent; ln is the only tool that pulls an exponent down to ground level so we can solve for T .
Step 4 — Quantify the frozen-prefactor error and correct once.
Going from 300 K to 874 K, the prefactor grows by ( 300 874 ) 3/2 = 4.98 — a factor of ~5, exactly the reviewer's concern. So the true prefactor at the answer temperature is ≈ 1.71 × 1 0 19 × 4.98 = 8.5 × 1 0 19 , making the required exponential smaller : 1 0 16 /8.5 × 1 0 19 = 1.18 × 1 0 − 4 , so ln = − 9.05 and
T ≈ 2 × 8.617 × 1 0 − 5 × 9.05 1.12 = 718 K .
Why this step? The prefactor sits inside the log, so a factor-5 change moves the exponent by only ln 5 = 1.6 — a ~18% shift in T (874 → 718 K), not a factor of 5 in T . That is the whole point: the logarithm compresses prefactor errors, which is why freezing it for a first estimate is legitimate. One correction iteration is enough.
Verify: Corrected T ≈ 700 –750 K; iterating once more barely moves it (the prefactor at 718 K vs 874 K differs by only ~30%, i.e. ln 1.3 = 0.26 in the exponent). Textbook curves put Si's intrinsic onset near 500–600 K for this doping — our estimate is the right ballpark and errs high because we still neglect that E g itself shrinks with T . Direction is unambiguous: well above 300 K ✓, which is why Si chips must stay cool (Intrinsic vs extrinsic semiconductors ).
Set N D = 0 (undoped silicon — the zero-input edge case, not the high-doping "Fermi-degenerate" regime, which is a different story flagged at the top). What happens to each of the three regions?
Forecast: Which of freeze-out / extrinsic / intrinsic survive when there are no donors at all?
Step 1 — Kill the donor source.
With N D = 0 , the master equation n = N D + + n i ′ collapses to n = n i at all temperatures.
Why this step? No donors means no N D + term to speak of — the entire extrinsic mechanism is switched off.
Step 2 — Freeze-out region.
The freeze-out formula carries a factor N D → 0 . There is nothing to freeze onto, so freeze-out does not exist .
Why this step? Freeze-out is dopant physics; remove dopants and the phenomenon has no home.
Step 3 — Extrinsic plateau.
The plateau value is N D = 0 — there is no plateau ; the curve is a single straight line.
Why this step? The flat middle only appears because donors saturate; with zero donors there's nothing to saturate.
Step 4 — What survives.
Only the intrinsic line remains: ln n = ln N C N V − 2 k B E g ⋅ T 1 , one straight line of slope − E g /2 k B for all T .
Verify: Zero-input limit is consistent — the three-region plot smoothly becomes a one-region plot as N D → 0 . Sanity: at 300 K this gives back Ex 1's n i ≈ 6.7 × 1 0 9 cm − 3 ✓. A pure semiconductor is just "intrinsic everywhere."
What do the formulas predict in the two extreme limits? (No numbers — reason from the structure.) Below, let E stand for either relevant activation energy: E = E D in the freeze-out formula, or E = E g in the intrinsic formula. The argument is identical for both, so we write it once.
Forecast: Does n → 0 or n → ∞ as T → 0 ? And as T → ∞ ?
Step 1 — The limit T → 0 .
In e − E /2 k B T (with E being E D or E g ), as T → 0 the fraction E /2 k B T → + ∞ , so the exponential → 0 . This holds for both activation energies.
lim T → 0 n = 0
Why this step? At absolute zero there is zero thermal budget to promote any electron; every carrier freezes onto its home atom. The exponential encodes exactly this "no energy, no carriers."
Step 2 — Check the prefactor doesn't rescue it.
N C ∝ T 3/2 → 0 too, so the prefactor also vanishes — no fight, both factors push n → 0 . The material becomes a perfect insulator.
Why this step? You must confirm the slow prefactor doesn't overpower the exponential; here they agree.
Step 3 — The limit T → ∞ (intrinsic formula, E = E g ).
As T → ∞ , E g /2 k B T → 0 , so e − E g /2 k B T → e 0 = 1 , while N C N V ∝ T 3/2 → ∞ .
lim T → ∞ n i = ∞ ( grows as T 3/2 )
Why this step? With unlimited thermal budget every bond can be broken; the only remaining growth is the slow T 3/2 counting of available states. (The freeze-out formula's high-T limit is irrelevant physically — long before then you've left freeze-out and entered the plateau, then intrinsic.)
Verify: Both limits are physically sane: cold ⇒ insulator (n → 0 ), hot ⇒ carrier flood (n → ∞ ). On the ln n vs 1/ T plot (1/ T → ∞ is far right, 1/ T → 0 is the origin), the intrinsic line dives to − ∞ on the right and rises to ln N C N V at the origin — matching the map figure ✓.
A silicon pressure sensor (N D = 1 0 15 cm − 3 ) is rated to behave "extrinsically" (carrier count within 1% of N D ). An engine bay reaches 150 ∘ C. Is the sensor still safe, i.e. is n i ≪ N D ?
Forecast: 150 ∘ C is hot for a human but is it hot for silicon? Guess whether n i has caught up to 1 0 15 .
Step 1 — Convert to kelvin.
T = 150 + 273 = 423 K
Why this step? All the exponents use absolute temperature; Celsius would give nonsense.
Step 2 — New k B T and exponent.
k B T = 8.617 × 1 0 − 5 × 423 = 0.03645 eV , 2 k B T E g = 0.0729 1.12 = 15.36
Why this step? Higher T shrinks the exponent (from 21.66 at 300 K to 15.36), so n i climbs — we need to know how far.
Step 3 — Scale the prefactor to 423 K.
N C N V ( 423 ) = 1.706 × 1 0 19 ( 300 423 ) 3/2 = 1.706 × 1 0 19 × 1.674 = 2.86 × 1 0 19
Why this step? The prefactor N C N V ∝ T 3/2 was quoted at 300 K; at 423 K the "number of seats" is genuinely larger, so we must rescale it before combining — reusing the 300 K value would undercount n i .
Step 4 — Assemble and compare against the 1% spec.
n i = 2.86 × 1 0 19 × e − 15.36 = 2.86 × 1 0 19 × 2.13 × 1 0 − 7 ≈ 6.1 × 1 0 12 cm − 3
N D n i = 1 0 15 6.1 × 1 0 12 = 6.1 × 1 0 − 3 = 0.6% < 1%
Why this step? Multiplying prefactor × exponential turns the two pieces into an actual n i (seats × occupancy again); then forming the ratio n i / N D is the only thing that answers the engineering question — "safe" was defined as this ratio staying under 1% , so we must compute it explicitly rather than just compare orders of magnitude.
Verify: n i / N D < 1% , so the sensor is just barely still extrinsic ✓ — a real engineering margin, not a landslide. Note how a 123 K rise multiplied n i by roughly 600 × (from about 1 0 10 at 300 K to 6 × 1 0 12 at 423 K): the exponential is unforgiving. This is why automotive-grade chips use higher doping or wider-gap materials (Conductivity and mobility vs temperature ).
A student plots ln n vs 1/ T in the low-temperature region and measures a slope of − 260 K. What donor ionization energy E D does this imply?
Forecast: Freeze-out slope is − E D /2 k B . Will E D come out around 1 eV (like a gap) or much smaller?
Step 1 — Identify the correct slope law.
Low-T region ⇒ freeze-out ⇒ slope = − E D /2 k B (not − E g /2 k B ; that's the high-T slope).
Why this step? Using the wrong region's formula is the classic exam trap; the region tells you which energy the slope encodes.
Step 2 — Solve for E D .
E D = − 2 k B × ( slope ) = 2 × 8.617 × 1 0 − 5 × 260 = 0.0448 eV
Why the factor 2? Same square-root logic derived in Example 3 — the exponent is E D /2 , so recovering E D needs the 2 . Forget it and you halve your answer.
Step 3 — Interpret.
E D ≈ 0.045 eV — a shallow donor, consistent with phosphorus in silicon.
Verify: 0.045 eV ≪ E g = 1.12 eV ✓ — donors sit just below the conduction band, exactly why they ionize easily at modest T (that's what "shallow" means). Forecast confirmed: far smaller than a gap. Cross-check against Ex 3 which assumed E D = 0.045 eV — self-consistent ✓.
You double the doping from N D to 2 N D . State the direction each of the three region boundaries moves. No arithmetic — reason from each formula's monotonicity.
Forecast: Write "up/down/higher T/lower T" for: plateau height, intrinsic onset temperature, freeze-out onset temperature.
Step 1 — Plateau height.
Plateau value = N D . Doubling gives 2 N D : the flat line sits higher by ln 2 ≈ 0.69 on the ln n axis.
Why this step? Plateau is literally the doping; its response is immediate and monotone.
Step 2 — Intrinsic onset (temperature where n i = N D ).
n i rises with T . To reach the now-larger target 2 N D , you need a higher T . So the intrinsic corner shifts to lower 1/ T (leftward on the map).
Why this step? The onset condition is n i ( T ) = N D ; raise the right side and the monotone n i ( T ) must be evaluated further right.
Step 3 — Freeze-out onset.
More donors means more electrons must be ionized to reach full saturation, so complete ionization requires a slightly higher T ; the freeze-out corner also nudges to higher T .
Why this step? Freeze-out ends only when all donors ionize; more donors is a bigger job, needing more thermal budget.
Verify: All three matches the parent's "Forecast-then-verify" box: plateau up , intrinsic onset higher T , freeze-out onset higher T ✓. Consistency check: halving N D instead would lower the intrinsic-onset temperature — opposite direction, as required for a monotone relation ✓. (For a p -type mirror, replace N D → N A and every conclusion holds verbatim.)
Recall Which formula for which region?
High-T intrinsic slope encodes ::: − E g /2 k B
Low-T freeze-out slope encodes ::: − E D /2 k B
Extrinsic plateau value ::: n ≈ N D
To find a temperature buried in an exponent you apply ::: the natural logarithm ln
Recall Edge and limit answers
As T → 0 , n → ::: 0 (perfect insulator)
As T → ∞ , n i → ::: ∞ , growing as T 3/2
With N D = 0 the plot has how many regions? ::: one (intrinsic line only)
The p -type mirror of n ≈ N D is ::: p ≈ N A
Recall Where does the ½ in every exponent come from?
The ½ in E g /2 and E D /2 arises because ::: you solve for a single carrier density by taking the square root of a mass-action product whose exponent was the full energy.
Mnemonic The 2 is always there
Every energy you read off a slope — E g or E D — hides behind a divide-by-two . "See a slope, multiply the energy back by 2." Miss the 2 and you halve every band gap you'll ever measure.
Parent: Temperature dependence of carrier concentration · Hinglish: 2.1.13 Temperature dependence of carrier concentration (Hinglish)