Energy Bands in Solids

Hold a copper wire, a chip of silicon, and a diamond in your hand. All three are crystals — orderly lattices of atoms — yet copper conducts electricity almost perfectly, diamond not at all, and silicon sits stubbornly in between, the material an entire trillion-dollar industry is built on. Why? The atoms are not so different; carbon, silicon and germanium even share the same four-bond structure. The answer is not about the atoms one at a time. It is about what happens to their electron energy levels when you pack 102310^{23} of them into a single crystal. In a lone atom, the electrons live on sharp, discrete rungs — the very energy levels you met in the Bohr model. Bring two atoms close and each rung splits in two, because no two electrons in the combined system may share the same state. Bring a mole of them together and each rung splits into a mole of levels, packed so densely they smear into a continuous energy band. Between one band and the next there can be a gap of energies that no electron is allowed to have — a forbidden energy gap. Whether a solid conducts turns entirely on where its electrons sit relative to that gap. This article builds the picture from scratch with school algebra: how sharp atomic levels broaden into bands, what the highest filled (valence) band and the lowest empty (conduction) band are, and how the width of the gap between them sorts every solid into conductor, semiconductor, or insulator — with silicon's 1.1 eV1.1\ \text{eV} gap and diamond's 5.5 eV5.5\ \text{eV} gap explaining why one runs your phone and the other sparkles on a ring. It is the foundation for the whole chapter that follows.

Key takeaways
  • Atomic levels broaden into bands in a crystal. Packing ∼ ⁣1023\sim\!10^{23} atoms together splits each sharp atomic level into that many sub-levels, so close together they form a near-continuous energy band.
  • Two bands matter: the valence band and the conduction band. The valence band is the highest band filled by the bonding electrons; the conduction band is the next one up, normally empty. Between them lies a forbidden energy gap EgE_g that electrons cannot occupy.
  • Only electrons in a partly filled band can carry current. A completely full band carries no net current — every forward electron is cancelled by a backward one. Conduction needs a partly filled band, or electrons lifted into an empty one.
  • The gap sorts every solid. Conductor: bands overlap, Eg≈0E_g \approx 0 (copper). Semiconductor: small gap, Si 1.1 eV1.1\ \text{eV}, Ge 0.7 eV0.7\ \text{eV}. Insulator: large gap, ≳3 eV\gtrsim 3\ \text{eV} — diamond ≈5.5 eV\approx 5.5\ \text{eV}.
  • Room-temperature thermal energy is tiny next to the gap. kT≈0.026 eVkT \approx 0.026\ \text{eV} at 300 K300\ \text{K}, far below EgE_g, so only a Boltzmann-suppressed trickle of electrons is thermally lifted across — many for germanium, few for silicon, essentially none for diamond.
  • Key idea: a solid conducts only if its electrons can find empty allowed states nearby; the width of the forbidden gap between the filled valence band and the empty conduction band is what makes copper a conductor, silicon a semiconductor, and diamond an insulator.
The core insight

When ∼ ⁣1023\sim\!10^{23} atoms form a crystal their sharp electron levels broaden into continuous energy bands separated by forbidden gaps, and a solid conducts only when electrons occupy a partly filled band or can be lifted across the gap into the empty conduction band — so the size of the gap between the valence and conduction bands (zero for a conductor, about 1 eV1\ \text{eV} for a semiconductor, several eV for an insulator) decides whether the solid carries current.

Where this lives today

Band theory is the working language of the electronics industry, and every choice a chip designer makes traces back to a band gap. Silicon's 1.1 eV1.1\ \text{eV} is the workhorse of logic and memory because it is small enough to conduct on demand yet large enough to switch cleanly off. Wider-gap materials — gallium nitride (3.4 eV3.4\ \text{eV}) and silicon carbide (3.3 eV3.3\ \text{eV}) — now run high-voltage chargers and electric-car inverters, precisely because their bigger gaps withstand fields that would break silicon down. LEDs glow at a colour set by their gap (hc/Eghc/E_g again); solar cells choose a gap near 1.4 eV1.4\ \text{eV} to match sunlight. Everything in the rest of this chapter, from the intrinsic semiconductor to the transistor and the logic gate, is built on the single diagram you now own: two bands and the forbidden gap between them.

The physical picture

Start with a single silicon atom. Its electrons occupy sharp energy levels — think of the Bohr picture: discrete rungs, each holding a fixed number of electrons, with wide forbidden gaps between them where no electron is allowed. This is the atom you already know. Now bring a second silicon atom close. The outer electrons begin to feel each other, and a rule of quantum mechanics — the Pauli exclusion principle — forbids two electrons in the joined system from occupying exactly the same state. Nature's fix is to split each shared level into two slightly different ones. Bring up a third atom and it splits into three; a fourth, into four. Each atom you add forces every level to split once more. In a real crystal the number of atoms is staggering: a crystal you can see holds of order 102310^{23} atoms, so each atomic level splits into about 102310^{23} sub-levels. Spread across an energy range of only a few electronvolts, these are separated by unimaginably tiny gaps — as we will compute, around 10−23 eV10^{-23}\ \text{eV} apart, far smaller than any energy the electron ever exchanges with its surroundings. To every physical purpose the 102310^{23} rungs merge into a smooth, continuous ramp of allowed energies: an energy band.

Figure
A single atom's sharp discrete levels split into more and more sub-levels as more atoms are brought together, until in a crystal each level has broadened into a continuous energy band separated from the next by a forbidden gap
From sharp atomic levels to continuous bands energy → 1 atom 2 atoms 6 atoms N ≈ 10²³ atoms → bands conduction band valence band forbidden gap Eg

Two of these bands do all the work. The valence band is the highest band that the crystal's bonding electrons fill at absolute zero — in silicon it holds the electrons shared in the covalent bonds. Just above it, separated by the forbidden gap, sits the conduction band: the next allowed band, normally empty. The vertical distance between the top of the valence band and the bottom of the conduction band is the band gap (or forbidden energy gap) EgE_g, in electronvolts. Almost nothing about the crystal changes except this one number as we walk from copper to silicon to diamond — and that one number is the whole story.

Why a full band cannot carry current

Here is the subtlety a lot of students miss: having electrons is not enough to conduct; the electrons must be able to change their state. An applied electric field nudges electrons to move preferentially one way, which means giving them slightly more energy and momentum — pushing them into nearby empty states. In a completely filled band there are none: every allowed level is already occupied, so for every electron the field speeds up, another is already moving the opposite way, and the two cancel exactly. A full band carries no net current, however many electrons it holds. So conduction demands one of two situations. Either the highest occupied band is only partly filled, leaving empty states right alongside the occupied ones for electrons to slide into — a metal. Or the valence band is full but a few electrons have been lifted across the gap into the conduction band, where they sit in an almost-empty band with endless room to move. The forbidden gap is precisely what stands between the full valence band and the empty conduction band, so its size controls how easily electrons reach a band where they can conduct.

The gap sorts every solid

Read the three cases straight off the band picture. In a conductor — copper, silver, aluminium — the highest occupied band is either only partly filled, or the valence and conduction bands physically overlap so filled and empty states merge with no gap (Eg≈0E_g \approx 0). Either way a vast reservoir of empty states is immediately available, so even the faintest field sets a current flowing. This is why metals conduct at any temperature. In an insulator — diamond, glass, quartz — the valence band is full, the conduction band empty, and the gap between them large: ≳3 eV\gtrsim 3\ \text{eV}, and for diamond about 5.5 eV5.5\ \text{eV}. Crossing so wide a gap needs an energy kick that ordinary heat or a modest field cannot supply, so essentially no electron ever reaches the conduction band. No mobile carriers, no current. A semiconductor — silicon (Eg≈1.1 eVE_g \approx 1.1\ \text{eV}), germanium (Eg≈0.7 eVE_g \approx 0.7\ \text{eV}) — has the same full-valence, empty-conduction arrangement as an insulator, but with a small gap. At absolute zero it too is a perfect insulator; but the gap is narrow enough that at room temperature a thermal trickle of electrons is kicked across into the conduction band, leaving mobile vacancies behind, and the crystal conducts feebly. A semiconductor is, quite literally, an insulator with a gap small enough for heat to breach — which is what makes it tunable, and useful.

Figure
Three band diagrams with energy increasing upward: a conductor with overlapping bands so the gap is zero, a semiconductor with a small gap of about one electronvolt, and an insulator with a wide gap of several electronvolts that heat cannot bridge
The forbidden gap sorts conductor, semiconductor, insulator energy → Conductor (Cu) conduction valence (filled) bands overlap · Eg ≈ 0 empty states next door → conducts Semiconductor (Si) conduction (empty) valence (filled) Eg ≈ 1.1 eV heat lifts a few across → conducts weakly Insulator (diamond) conduction (empty) valence (filled) Eg ≈ 5.5 eV gap too wide → no carriers → insulates

Heat versus the gap: the tell-tale number

Why does room temperature lift many electrons across germanium's gap, a handful across silicon's, and none across diamond's? Because the average thermal energy available to an electron is fixed by temperature, and it is small. The natural yardstick is kTkT:

kT=(8.617×10−5 eV/K)×(300 K)=0.0259 eV≈0.026 eV.(1)kT = (8.617\times10^{-5}\ \text{eV/K}) \times (300\ \text{K}) = 0.0259\ \text{eV} \approx 0.026\ \text{eV}. \qquad (1)

where: k=8.617×10−5 eV/Kk = 8.617\times10^{-5}\ \text{eV/K} is the Boltzmann constant in convenient units, T=300 KT = 300\ \text{K} is room temperature, and kTkT is the characteristic thermal energy per particle. The physical reading: at room temperature nature hands each electron thermal jostles of only about 0.026 eV0.026\ \text{eV} on average — roughly a fortieth of an electronvolt. Compare that with the gaps: silicon's 1.1 eV1.1\ \text{eV} is about forty times kTkT, and diamond's 5.5 eV5.5\ \text{eV} is over two hundred times kTkT. Ordinary heat is nowhere near enough, on average, to launch an electron across. But "on average" is not "never." Thermal energy is shared randomly, and a small fraction of electrons momentarily carry far more than the average. The probability that one is lifted across a gap EgE_g follows an exponential (Boltzmann) suppression — a result we quote, since the exact carrier count needs Fermi–Dirac statistics from a later, university-level treatment:

f  ∼  e−Eg/2kT.(2)f \;\sim\; e^{-E_g / 2kT}. \qquad (2)

where: ff is roughly the fraction of valence electrons thermally promoted to the conduction band, EgE_g is the gap, and kTkT the thermal energy of equation (1); the factor of 22 appears because the Fermi level sits near mid-gap, so a carrier need only be lifted about half the gap on average. The reading is dramatic. Because EgE_g sits in an exponent, small changes in the gap produce enormous changes in conduction. Put the three materials through it and the sorting becomes overwhelming — germanium leaks about a part in a million, silicon about a part in a billion, diamond a part in 104710^{47}. That EgE_g appears exponentially, not linearly, is the deepest reason a 1 eV1\ \text{eV} gap and a 5 eV5\ \text{eV} gap describe utterly different worlds.

The formation and sorting, derived

Derivation AWhy a mole of atoms turns sharp levels into a continuous band

The goal here is to justify, with nothing but counting and division, the central claim of the article: that when you assemble a visible crystal, each sharp atomic level smears into a band so finely divided it behaves as a continuous range of allowed energies. We estimate the spacing between neighbouring sub-levels inside a band, compare it with the thermal energy kTkT, and show it is smaller by more than twenty powers of ten — which is why a band may be treated as continuous rather than as 102310^{23} separate rungs.

Step 1. Count the atoms. A small crystal you could hold — say a grain of silicon a few millimetres across — contains of order a mole of atoms, Avogadro's number N=6.0×1023N = 6.0\times10^{23}. By the exclusion argument, one atomic level shared among NN atoms must split into NN distinct sub-levels; that is the number of rungs packed into one band.

Step 2. Estimate the energy width of the band. When atoms bond, the outer levels shift by amounts of order the bond energy — a few electronvolts. Take a representative band width W≈5 eVW \approx 5\ \text{eV}; the exact figure does not matter for the conclusion, because we are about to divide by 102310^{23}.

Step 3. Divide the width among the rungs. The average spacing between neighbouring sub-levels is

ΔE  ≈  WN  =  5 eV6.0×1023  ≈  8×10−24 eV  ∼  10−23 eV.(3)\Delta E \;\approx\; \frac{W}{N} \;=\; \frac{5\ \text{eV}}{6.0\times10^{23}} \;\approx\; 8\times10^{-24}\ \text{eV} \;\sim\; 10^{-23}\ \text{eV}. \qquad (3)

Step 4. Compare that spacing with the thermal energy that jostles the electron: kT/ΔE≈0.026/8×10−24≈3×1021kT/\Delta E \approx 0.026 / 8\times10^{-24} \approx 3\times10^{21}. The thermal energy is more than 102110^{21} times the gap between rungs, so an electron slides between neighbouring sub-levels with immeasurable ease — the band is continuous for every practical purpose. The forbidden gap between bands, by contrast, is a full electronvolt, ∼ ⁣1023\sim\!10^{23} times wider than the spacing within a band. That colossal ratio is what makes "band" and "gap" meaningful ideas rather than bookkeeping. Verified: level count N=6.0×1023N = 6.0\times10^{23}, intra-band spacing ΔE≈8×10−24 eV\Delta E \approx 8\times10^{-24}\ \text{eV}, and ratio kT/ΔE≈3×1021kT/\Delta E \approx 3\times10^{21} — recomputed in verify_hs2-energy-bands-solids.py.

Go deeper · Derivation B · 1 minHow the gap sorts a conductor from a semiconductor from an insulator
Derivation BHow the gap sorts a conductor from a semiconductor from an insulator

The goal is to turn the qualitative "small gap conducts, large gap does not" into hard numbers, by feeding silicon, germanium and diamond through the Boltzmann factor of equation (2) and reading off how many electrons each promotes across its gap at room temperature. We use only the exponential factor e−Eg/2kTe^{-E_g/2kT} — quoted, not derived — and kT=0.026 eVkT = 0.026\ \text{eV}; the point is to see the exponent, not the exact carrier density.

Step 1. Fix the yardstick. From equation (1), 2kT=0.0517 eV2kT = 0.0517\ \text{eV} at 300 K300\ \text{K}. The exponent in equation (2) is therefore Eg/0.0517 eVE_g / 0.0517\ \text{eV} for each material — a pure number telling us how many "half-thermal-energies" wide the gap is.

Step 2. Germanium, Eg=0.7 eVE_g = 0.7\ \text{eV}. Exponent =0.7/0.0517=13.5= 0.7 / 0.0517 = 13.5, so f∼e−13.5≈1.3×10−6f \sim e^{-13.5} \approx 1.3\times10^{-6}. About one valence electron in a million is promoted — enough for measurable conduction.

Step 3. Silicon, Eg=1.1 eVE_g = 1.1\ \text{eV}. Exponent =1.1/0.0517=21.3= 1.1 / 0.0517 = 21.3, so f∼e−21.3≈6×10−10f \sim e^{-21.3} \approx 6\times10^{-10}. Only about one electron in a billion and a half crosses — silicon conducts, but far more weakly than germanium. The ratio of the two is fGe/fSi=e(21.3−13.5)=e7.8≈2×103f_{\text{Ge}}/f_{\text{Si}} = e^{(21.3 - 13.5)} = e^{7.8} \approx 2\times10^{3}: germanium has roughly two thousand times more intrinsic carriers than silicon, and indeed their measured intrinsic densities differ by about a factor of 16001600 — the same story, up to the prefactor this quoted estimate omits.

Step 4. Diamond, Eg=5.5 eVE_g = 5.5\ \text{eV}. Exponent =5.5/0.0517=106= 5.5 / 0.0517 = 106, so f∼e−106≈6×10−47f \sim e^{-106} \approx 6\times10^{-47} — not a small number but a zero in every practical sense, which is why diamond is one of the best insulators known. The same exponential, walked from 0.70.7 to 5.5 eV5.5\ \text{eV}, spans forty powers of ten in conductivity while the gap changes by less than a factor of ten. Verified: exponents 13.513.5, 21.321.3, 106106; fractions 1.3×10−61.3\times10^{-6}, 6×10−106\times10^{-10}, 6×10−476\times10^{-47}; Ge/Si ratio ≈2×103\approx 2\times10^{3} — recomputed in verify_hs2-energy-bands-solids.py.

The gap you can see: photons and colour

There is a second, independent way to read a band gap — with light instead of heat. A photon carries energy E=hf=hc/λE = hf = hc/\lambda. If that energy at least matches the gap, the photon can be absorbed by lifting a valence electron into the conduction band; if it falls short, the photon sails through untouched. So the longest wavelength a material can absorb across its gap is

λmax=hcEg,hc=1240 eV ⋅ nm.(4)\lambda_{\text{max}} = \frac{hc}{E_g}, \qquad hc = 1240\ \text{eV}\,\cdot\,\text{nm}. \qquad (4)

where: λmax\lambda_{\text{max}} is the threshold wavelength, EgE_g the band gap, and hc=1240 eV ⋅ nmhc = 1240\ \text{eV}\,\cdot\,\text{nm} the handy product that turns a gap in electronvolts straight into a wavelength in nanometres. For silicon, λmax=1240/1.1=1127 nm\lambda_{\text{max}} = 1240/1.1 = 1127\ \text{nm} — deep in the infrared, beyond the red edge of vision. Silicon absorbs all visible light (every visible photon, 1.81.8 to 3.1 eV3.1\ \text{eV}, easily clears the 1.1 eV1.1\ \text{eV} gap) and looks an opaque metallic grey, yet is transparent to far-infrared light. Diamond's threshold is 1240/5.5=225 nm1240/5.5 = 225\ \text{nm}, in the ultraviolet: no visible photon carries the 5.5 eV5.5\ \text{eV} to jump its gap, so visible light passes straight through and pure diamond is water-clear. The colour of a solid is, in part, a direct picture of its band gap.

Limiting cases

caseresultmeaning
Eg≈0E_g \approx 0 (bands overlap)conducts at any temperaturea metal — empty states sit right beside filled ones
EgE_g small (∼1 eV\sim 1\ \text{eV})insulates at 0 K0\ \text{K}, conducts weakly when warma semiconductor — heat breaches the gap
EgE_g large (≳3 eV\gtrsim 3\ \text{eV})insulates at all ordinary temperaturesan insulator — heat cannot breach the gap
T→0 KT \to 0\ \text{K}semiconductor becomes a perfect insulatorno thermal energy to promote carriers (f→0f \to 0)
TT raisedsemiconductor conductivity rises sharplymore carriers promoted; opposite to a metal, whose conductivity falls
band completely fullcarries no currentevery forward electron cancelled by a backward one
band partly filledcarries current freelyempty states available for electrons to move into

Worked examples

Board level — classifying three solids by their band gap (CBSE and ICSE pattern)

Three crystals have measured band gaps of Eg=0 eVE_g = 0\ \text{eV} (bands overlapping), Eg=0.7 eVE_g = 0.7\ \text{eV}, and Eg=5.5 eVE_g = 5.5\ \text{eV}. Classify each as a conductor, semiconductor, or insulator, and state which will conduct better at room temperature — and why.

Step 1. The zero-gap crystal has its valence and conduction bands overlapping, so filled and empty states merge with no forbidden region. Empty states are always available: this is a conductor.

Step 2. The 0.7 eV0.7\ \text{eV} crystal has a full valence band and empty conduction band separated by a small gap. Compare with kT≈0.026 eVkT \approx 0.026\ \text{eV}: the gap is about 2727 times kTkT, small enough that a thermal trickle crosses at room temperature. This is a semiconductor (in fact germanium).

Step 3. The 5.5 eV5.5\ \text{eV} crystal has the same arrangement but a gap over 200200 times kTkT — far too wide for heat to breach. Essentially no carriers reach the conduction band: an insulator (diamond).

Step 4. Among the two non-metals the smaller gap wins: the 0.7 eV0.7\ \text{eV} crystal promotes vastly more carriers than the 5.5 eV5.5\ \text{eV} one, because the promoted fraction falls off exponentially with the gap. Order of conductivity: conductor ≫\gg semiconductor ≫\gg insulator.

Board level — the longest wavelength silicon can absorb (CBSE and ICSE pattern)

Silicon has a band gap Eg=1.1 eVE_g = 1.1\ \text{eV}. Using hc=1240 eV ⋅ nmhc = 1240\ \text{eV}\,\cdot\,\text{nm}, find the longest-wavelength photon that can lift an electron across the gap, and state whether silicon should look transparent or opaque to visible light.

Step 1. A photon is absorbed across the gap only if its energy E=hc/λE = hc/\lambda is at least EgE_g. The threshold (longest wavelength, lowest energy that still works) is where E=EgE = E_g:

λmax=hcEg=1240 eV ⋅ nm1.1 eV=1127 nm.\lambda_{\text{max}} = \frac{hc}{E_g} = \frac{1240\ \text{eV}\,\cdot\,\text{nm}}{1.1\ \text{eV}} = \boxed{1127\ \text{nm}}.

Step 2. 1127 nm1127\ \text{nm} lies in the near-infrared, past the red end of the visible band (which stops around 700 nm700\ \text{nm}). Photons longer than 1127 nm1127\ \text{nm} cannot cross the gap and pass through; photons shorter — including all visible light — carry more than 1.1 eV1.1\ \text{eV} and are absorbed.

Step 3. Every visible photon (400400–700 nm700\ \text{nm}, i.e. 1.81.8–3.1 eV3.1\ \text{eV}) exceeds the 1.1 eV1.1\ \text{eV} gap, so all visible light is absorbed. Silicon looks opaque and metallic-grey to the eye, yet is transparent to far-infrared light — the reason infrared cameras and fibre-optic detectors are built on it.

Competitive level — how many electrons cross the gap, and how fast it changes with temperature (JEE and NEET pattern)

For silicon (Eg=1.1 eVE_g = 1.1\ \text{eV}), estimate the fraction of valence electrons thermally promoted to the conduction band at 300 K300\ \text{K} using f∼e−Eg/2kTf \sim e^{-E_g/2kT} with k=8.617×10−5 eV/Kk = 8.617\times10^{-5}\ \text{eV/K}. Then find by what factor that fraction increases when the crystal is heated to 400 K400\ \text{K}.

Step 1. Thermal energy at 300 K300\ \text{K}: kT=8.617×10−5×300=0.0259 eVkT = 8.617\times10^{-5}\times300 = 0.0259\ \text{eV}, so 2kT=0.0517 eV2kT = 0.0517\ \text{eV}.

Step 2. Exponent at 300 K300\ \text{K}: Eg/2kT=1.1/0.0517=21.3E_g/2kT = 1.1/0.0517 = 21.3. Fraction f300∼e−21.3=6×10−10f_{300} \sim e^{-21.3} = \boxed{6\times10^{-10}} — roughly one valence electron in 1.71.7 billion.

Step 3. At 400 K400\ \text{K}: kT=8.617×10−5×400=0.0345 eVkT = 8.617\times10^{-5}\times400 = 0.0345\ \text{eV}, 2kT=0.0689 eV2kT = 0.0689\ \text{eV}, exponent =1.1/0.0689=15.96= 1.1/0.0689 = 15.96. So f400∼e−15.96f_{400} \sim e^{-15.96}.

Step 4. The factor of increase is the ratio of the two exponentials: f400/f300=e−15.96/e−21.3=e 21.28−15.96=e5.32≈200f_{400}/f_{300} = e^{-15.96}/e^{-21.3} = e^{\,21.28-15.96} = e^{5.32} \approx \boxed{200}. A mere 100 K100\ \text{K} rise multiplies the carrier count about two-hundredfold — which is why a semiconductor's conductivity climbs with temperature (opposite to a metal), and why devices must be kept cool to behave predictably. Timing note: about two minutes. The whole item is two evaluations of Eg/2kTE_g/2kT and a subtraction in the exponent — never compute the two tiny exponentials separately and divide, that invites calculator overflow; instead take the ratio as eΔ(exponent)e^{\Delta(\text{exponent})}. Memorise 2kT=0.052 eV2kT = 0.052\ \text{eV} at room temperature and the first exponent is a one-step division.

Competitive level — reading a gap off an absorption threshold (JEE Advanced pattern)

A semiconductor stops absorbing light for wavelengths longer than 1771 nm1771\ \text{nm}; below that it is opaque. Find its band gap in electronvolts and identify the likely material. Take hc=1240 eV ⋅ nmhc = 1240\ \text{eV}\,\cdot\,\text{nm}.

Step 1. The absorption edge marks the photon energy that just equals the gap: Eg=hc/λmaxE_g = hc/\lambda_{\text{max}}. Rearranging equation (4) and inserting the threshold:

Eg=1240 eV ⋅ nm1771 nm=0.70 eV.E_g = \frac{1240\ \text{eV}\,\cdot\,\text{nm}}{1771\ \text{nm}} = \boxed{0.70\ \text{eV}}.

Step 2. A gap of 0.70 eV0.70\ \text{eV} is the textbook value for germanium. The logic runs both ways: measure the longest wavelength a crystal absorbs and you have measured its band gap directly, no thermometer required.

Step 3. Sanity check: silicon's larger 1.1 eV1.1\ \text{eV} gap gives a shorter threshold, 1127 nm1127\ \text{nm} — a wider-gap material absorbs only shorter, higher-energy wavelengths, exactly as Eg=hc/λE_g = hc/\lambda demands. The ordering is consistent, so 0.70 eV0.70\ \text{eV} for germanium is secure. Timing note: under a minute. One division, 1240/λ1240/\lambda, converts any absorption edge in nanometres straight to a gap in electronvolts. Keep hc=1240 eV ⋅ nmhc = 1240\ \text{eV}\,\cdot\,\text{nm} memorised and this class of question is instant.

Exam traps

Thinking "more electrons" means "better conductor." Insulators are full of electrons; what they lack is empty states nearby. A completely filled band carries no current. Always frame conduction as the availability of accessible empty states, not the mere presence of electrons — this single idea answers most band-theory conceptual questions.

Confusing the valence band with the conduction band. The valence band is the highest filled band (the bonding electrons); the conduction band is the next one up, normally empty, where electrons are free to move. Students routinely swap the two or say current flows "in the valence band" of a semiconductor — the mobile electrons are in the conduction band (the holes they leave behind are the next article's story).

Forgetting that a semiconductor is an insulator at absolute zero. At 0 K0\ \text{K} silicon has a full valence band, an empty conduction band, and no thermal energy to bridge them — it does not conduct at all. Semiconduction is a thermal effect. The corollary trips people up too: a semiconductor's conductivity rises with temperature (more carriers promoted), whereas a metal's falls (more lattice vibrations scatter the already-free electrons). Getting this temperature dependence backwards is a classic lost mark.

Misusing the gap values. Quote them cleanly: conductor Eg≈0E_g \approx 0; semiconductor small (Si 1.1 eV1.1\ \text{eV}, Ge 0.7 eV0.7\ \text{eV}); insulator large (≳3 eV\gtrsim 3\ \text{eV}, diamond ≈5.5 eV\approx 5.5\ \text{eV}). Do not write silicon's gap as 0.70.7 (that is germanium) or claim insulators have "no bands" — they have bands and a wide gap.

Board scope. Energy bands, the valence/conduction/gap picture, and the conductor–semiconductor–insulator sorting are core on CBSE (Ch. 14), ICSE/ISC, JEE Main, JEE Advanced, and NEET, and are useful background for the A-Level 9702 electronics and diode topics, though the band picture is not itself a 9702 exam topic. They are not examined on AP Physics 2 (no semiconductor electronics at all), on IGCSE 0625 (which starts at the diode, skipping bands), or in the current IB Physics core (electronics has largely been dropped). On those last three, learn the band picture for understanding but do not expect it on the paper.

Origins · 1 minFelix Bloch and how this was discovered
FB
Felix Bloch
1905–1983 · Zürich and Leipzig and Stanford

Felix Bloch was the Swiss-American physicist whose 1928 doctoral work, supervised by Werner Heisenberg at Leipzig, laid the foundation of everything in this article. Asking how an electron moves through a perfectly periodic crystal, Bloch proved that — far from being scattered at every atom — it travels through the lattice as an undisturbed wave, now called a Bloch wave. His theorem showed that the allowed electron energies group into continuous bands separated by forbidden gaps, converting the atom's sharp levels into the band structure that sorts every solid into conductor, semiconductor, or insulator. Bloch later fled Nazi Germany for Stanford and won the 1952 Nobel Prize in Physics for developing nuclear magnetic resonance — the physics behind the MRI scanner. But it is his student-era band theory that underlies the entire semiconductor age.

History
1900
— Paul Drude models a metal as a gas of free electrons, explaining conduction but leaving unanswered why some solids do not conduct at all.
1913
— Niels Bohr quantizes the atom into sharp energy levels, the discrete rungs a crystal will later broaden into bands.
1928
— Felix Bloch proves an electron in a perfect periodic lattice travels as a free wave; his theorem is the foundation of band theory.
1931
— Alan Wilson uses the band picture to define metals, semiconductors and insulators by their band filling and gap width.
1947
— John Bardeen and Walter Brattain build the first (point-contact) transistor at Bell Labs; William Shockley follows with the junction transistor in 1948 — band theory's first great engineering payoff. (The three shared the 1956 Nobel Prize.)
1958
— Jack Kilby builds the first microchip, packing many band-gap devices onto one small piece of semiconductor.

Going further

Texts. NCERT Physics Class 12, Chapter 14 ("Semiconductor Electronics"), the energy-bands section · H. C. Verma, Concepts of Physics Vol. 2, "Semiconductors and Semiconductor Devices" · Kittel, Introduction to Solid State Physics, for the full band-structure treatment · Ashcroft & Mermin, Solid State Physics, for Bloch's theorem done properly.

Provenance. LANE_SPEC / anchor constants. Recompute: kT=8.617×10−5×300=0.0259 eV≈0.026 eVkT = 8.617\times10^{-5}\times300 = 0.0259\ \text{eV} \approx 0.026\ \text{eV}; 2kT=0.0517 eV2kT = 0.0517\ \text{eV}; band-formation spacing ΔE=5/(6.0×1023)=8×10−24 eV\Delta E = 5/(6.0\times10^{23}) = 8\times10^{-24}\ \text{eV}, ratio kT/ΔE=3×1021kT/\Delta E = 3\times10^{21}; Boltzmann exponents Eg/2kTE_g/2kT = 13.513.5 (Ge), 21.321.3 (Si), 106106 (diamond); fractions 1.3×10−61.3\times10^{-6}, 6×10−106\times10^{-10}, 6×10−476\times10^{-47}; Ge/Si carrier ratio ≈2.3×103\approx 2.3\times10^{3} (from exponent 21.28−13.54=7.7421.28-13.54=7.74) versus measured nin_i ratio 2.4×1019/1.5×1016=16002.4\times10^{19}/1.5\times10^{16} = 1600; Si 300→400 K300\to400\ \text{K} boost e5.32=204e^{5.32} = 204; absorption thresholds λ=hc/Eg\lambda = hc/E_g = 1127 nm1127\ \text{nm} (Si), 1771 nm1771\ \text{nm} (Ge), 225 nm225\ \text{nm} (diamond); visible band 1.81.8–3.1 eV3.1\ \text{eV} from 1240/7001240/700 and 1240/4001240/400.

Prerequisites. The Bohr Model of the Atom — the source of the sharp, discrete atomic energy levels that broaden into bands here; without quantized levels there is nothing to split. Leads to. Intrinsic Semiconductors (the next article), where the thermal electron–hole pairs sketched here get their proper treatment (ne=nh=nin_e = n_h = n_i); and, for university enrichment, the seams on the Fermi–Dirac distribution and Fermi energy, momentum and temperature, which supply the exact carrier statistics we only quoted (go-deeper only, never an exam dependency).

What actually is an energy band — is it a region of space or of energy?

Of energy, not of space. A band is a range of allowed energies that an electron in the crystal may have; the forbidden gap is a range of energies it may not have. It comes about because each sharp atomic energy level, when ∼ ⁣1023\sim\!10^{23} atoms are packed together, splits into ∼ ⁣1023\sim\!10^{23} sub-levels so finely spaced (about 10−23 eV10^{-23}\ \text{eV} apart) that they form a practically continuous strip. So when we draw a band as a filled rectangle, the vertical axis is energy and the block simply marks "electrons are allowed to have any energy in here." The electrons themselves are spread throughout the whole crystal in space.

Why does a full band carry no current even though it is packed with electrons?

Because current means a net flow one way, and in a full band every possible motion is already taken up in balanced pairs. For every electron drifting right there is an identical one drifting left, and their contributions cancel exactly. To get a net current you must unbalance the traffic — speed some electrons up relative to others — which means moving them into slightly different energy-momentum states. In a full band there are no empty states to move into, so nothing can be unbalanced and the net current stays zero. This is why insulators, though brimming with electrons, do not conduct: their valence band is full and the next band is an unreachable gap away.

What is the difference between a semiconductor and an insulator, if both have a full valence band?

Only the width of the gap — there is no difference in kind. Both have a full valence band and an empty conduction band at absolute zero, and both are perfect insulators there. The distinction is entirely quantitative: a semiconductor's gap (∼ ⁣1 eV\sim\!1\ \text{eV}) is small enough that at room temperature the exponential Boltzmann factor e−Eg/2kTe^{-E_g/2kT} lets a measurable trickle of electrons cross, while an insulator's gap (≳3 eV\gtrsim 3\ \text{eV}, diamond 5.5 eV5.5\ \text{eV}) makes that factor astronomically tiny — around 10−4710^{-47} for diamond. Because the gap sits in an exponent, a factor-of-five change in EgE_g becomes a forty-orders-of-magnitude change in conduction. So "semiconductor" and "insulator" are two ends of one continuous scale, not two separate categories.

Why does heating a semiconductor make it conduct better, when heating a metal makes it worse?

They conduct for different reasons, so heat does opposite things. A metal already has all the carriers it will ever have (its top band is partly filled); heating it only makes the lattice vibrate more, and those vibrations scatter the moving electrons, so conductivity falls. A semiconductor is limited not by scattering but by the number of carriers, which is tiny and thermally generated. Heating it promotes exponentially more electrons across the gap — the e−Eg/2kTe^{-E_g/2kT} factor grows fast — so vastly more carriers appear, swamping the mild extra scattering, and conductivity climbs steeply. As the worked example shows, a 100 K100\ \text{K} rise can boost silicon's carriers a hundredfold or more.

Where do the sharp atomic energy levels come from in the first place?

From the single atom, which you met in the Bohr model. In an isolated atom an electron may occupy only certain discrete energy levels — sharp rungs with forbidden gaps between them. Band theory does not overthrow this; it builds on it. Each atomic rung is the seed of a band: when the atoms assemble into a crystal, the exclusion principle forces every shared rung to split into as many closely spaced sub-levels as there are atoms, broadening the sharp atomic line into a band. So the bands you draw for a solid are the atomic levels of Bohr, smeared out by the company of 102310^{23} neighbours.

Is the "factor of 2" in the exponential something I need to derive?

No — quote it. The exact carrier statistics come from Fermi–Dirac statistics and the position of the Fermi level, which is university-level material beyond this article; at school level you simply take f∼e−Eg/2kTf \sim e^{-E_g/2kT} as a given estimate of the promoted fraction. The factor of 22 enters because, for an intrinsic (pure) semiconductor, the Fermi level sits roughly in the middle of the gap, so a typical electron need only be lifted about half the gap to reach a state that counts — hence Eg/2E_g/2 rather than the full EgE_g. For exam purposes, know the form, and know that the gap sitting in an exponent is why small gap changes cause huge conductivity changes.

Before this

Where this leads