Semiconductor Physics
Semiconductor physics is the foundation of modern electronics. The remarkable properties of semiconductor materials, which conduct electricity better than insulators but not as well as metals, enable the transistors, diodes, and integrated circuits that power our digital world. Understanding semiconductor physics reveals why these materials behave as they do and how their properties can be controlled to create useful electronic devices.
This field bridges quantum mechanics, solid-state physics, and electrical engineering. The concepts introduced here explain how electrons move through crystalline materials, how adding impurities dramatically changes electrical properties, and how junctions between different semiconductor regions create the fundamental building blocks of electronic devices.
Crystal Structure and Atomic Bonding
Semiconductor behavior begins with atomic structure. Silicon, the most common semiconductor, has four valence electrons that form covalent bonds with neighboring atoms. In a pure silicon crystal, each atom shares its four valence electrons with four neighboring atoms, creating a tetrahedral crystal structure known as the diamond cubic lattice. The cubic unit cell measures about 5.43 angstroms on a side and contains eight atoms, giving a density of roughly 5 x 1022 atoms per cubic centimeter.
This crystalline arrangement is crucial for semiconductor properties. The regular periodic structure creates an environment where electron behavior can be described using quantum mechanical band theory. Because the lattice is periodic, electron wavefunctions take the form of Bloch waves, and their allowed energies organize into bands indexed by crystal momentum. Defects in the crystal structure, whether intentional or unintentional, significantly affect electrical properties. Point defects, dislocations, and grain boundaries introduce energy states within the bandgap that trap carriers and accelerate recombination, which is why device-grade silicon is grown as a single crystal, typically by the Czochralski or float-zone method, and why semiconductor processing must achieve extraordinary levels of purity and crystalline perfection.
Crystal orientation also matters. Silicon wafers are commonly cut on the (100) plane for MOS devices, because that surface yields the lowest density of electrically active states at the interface with the gate oxide, while (111) material appears in some bipolar and mechanical applications. Amorphous and polycrystalline silicon, used in thin-film transistors and inexpensive solar cells, lack long-range order; their carrier mobilities are orders of magnitude lower, and their electronic behavior is dominated by localized states rather than clean bands.
Other semiconductor materials include germanium (also with four valence electrons), gallium arsenide (a compound semiconductor with the closely related zincblende structure), gallium nitride (usually wurtzite), and silicon carbide (which forms many stacking sequences, or polytypes, of which 4H is the one used for power devices). Each has a specific crystal structure and bonding arrangement that determines its electrical and thermal properties, making it suitable for different applications.
Energy Bands and the Bandgap
In isolated atoms, electrons occupy discrete energy levels. When atoms combine into a solid crystal, these discrete levels broaden into continuous bands of allowed energies. The two most important bands for understanding semiconductor behavior are the valence band and the conduction band.
The valence band contains electrons that participate in covalent bonding and are relatively localized near their parent atoms. The conduction band contains electrons that are free to move through the crystal and participate in electrical conduction. Between these bands lies the bandgap, a range of energies that electrons cannot occupy in a perfect crystal.
The bandgap is what distinguishes semiconductors from conductors and insulators. In conductors like metals, the valence and conduction bands overlap, so electrons can move freely. In insulators the bandgap is so large that essentially no electrons reach the conduction band at ordinary temperatures; silicon dioxide, the classic gate insulator, has a bandgap near 9 eV. Semiconductors occupy the middle ground, with bandgaps ranging from a few tenths of an electron volt to roughly 3.5 eV. Indium antimonide sits near 0.17 eV, germanium near 0.66 eV, silicon at 1.12 eV, gallium arsenide at 1.42 eV, 4H silicon carbide near 3.26 eV, and gallium nitride near 3.4 eV. The boundary between a wide-bandgap semiconductor and an insulator is a matter of convention rather than a sharp physical line.
Because carrier concentration depends exponentially on the ratio of bandgap to thermal energy, this modest spread in bandgap produces an enormous spread in behavior. A narrow-gap material conducts readily but leaks badly and cannot tolerate heat; a wide-gap material blocks high voltages and works at high temperature but demands more energy to turn on. Choosing a semiconductor is largely a matter of choosing where on that continuum a device should sit.
Silicon Bandgap Characteristics
Silicon has a bandgap of approximately 1.12 eV at room temperature. This value decreases slightly as temperature increases, which contributes to the sharp rise in thermally generated carriers, and therefore in junction leakage, that every silicon device shows when it runs hot. The temperature dependence follows the relationship:
Eg(T) = Eg(0) - (alpha * T2) / (T + beta)
Where Eg(0) is the bandgap at absolute zero, and alpha and beta are the Varshni parameters, which are material-specific. For silicon (alpha approximately 4.73 x 10-4 eV/K, beta approximately 636 K), the bandgap falls from about 1.17 eV at absolute zero to 1.12 eV at 300 K, shrinking by roughly 0.25 meV per kelvin near room temperature. The physical causes are lattice thermal expansion and, more importantly, the increasing interaction between electrons and lattice vibrations as temperature rises.
Heavy doping narrows the bandgap further. Above roughly 1018 dopant atoms per cubic centimeter, the impurity levels broaden into a band that merges with the nearest band edge, and carrier-carrier interactions shift the edges toward each other. This bandgap narrowing raises the effective intrinsic carrier concentration in heavily doped regions and is a first-order effect in bipolar transistor emitters, where it limits achievable current gain.
Direct and Indirect Bandgaps
Semiconductors are classified as having either direct or indirect bandgaps based on the relationship between electron energy and momentum in the crystal. In a direct bandgap material like gallium arsenide, the minimum energy state in the conduction band aligns with the maximum energy state in the valence band in momentum space. Electrons can transition between bands by absorbing or emitting photons without changing momentum.
Silicon has an indirect bandgap, meaning the conduction band minimum and valence band maximum occur at different momentum values. Transitions require both a photon and a phonon (lattice vibration) to conserve momentum. Because a three-body process is far less probable than a two-body one, silicon is inefficient at light emission, which is why LEDs and laser diodes typically use direct bandgap materials like gallium arsenide, indium gallium arsenide phosphide, or gallium nitride.
The same distinction governs absorption. A material absorbs photons whose energy exceeds its bandgap, so the long-wavelength cutoff follows from the bandgap directly: wavelength in nanometers is approximately 1240 divided by the bandgap in electron volts. Silicon therefore stops absorbing near 1100 nm, which is why silicon image sensors and solar cells are blind to the 1310 nm and 1550 nm wavelengths used in fiber optics, and why those links rely on indium gallium arsenide detectors instead. Indirect absorption is also weak near the band edge, so a silicon solar cell needs on the order of 100 micrometers of material to absorb red and near-infrared light, whereas a direct-gap gallium arsenide cell absorbs the same light within a few micrometers.
Charge Carriers: Electrons and Holes
Electrical conduction in semiconductors involves two types of charge carriers: electrons and holes. When an electron gains enough energy to move from the valence band to the conduction band, it leaves behind an empty state called a hole. This hole behaves as a positive charge carrier and can move through the crystal as neighboring electrons fill it, creating a new hole elsewhere.
In intrinsic (pure) semiconductors, electrons and holes are created in pairs and exist in equal concentrations. This intrinsic carrier concentration, denoted ni, depends strongly on temperature and the bandgap:
ni = sqrt(Nc * Nv) * exp(-Eg / 2kT)
Where Nc and Nv are the effective density of states in the conduction and valence bands, Eg is the bandgap, k is Boltzmann's constant, and T is absolute temperature. For silicon at 300 K both Nc and Nv are on the order of 1019 cm-3, and ni works out to approximately 1.0 x 1010 carriers per cubic centimeter. (Many older texts quote 1.45 x 1010, but careful measurement has shown that value to be too high; the accepted figure is closer to 1.0 x 1010.) This is a vanishingly small fraction of the roughly 5 x 1022 silicon atoms per cubic centimeter, which is why even trace doping dominates the carrier population: one dopant atom per billion silicon atoms already contributes five thousand times the intrinsic carrier density.
The exponential dependence on bandgap explains the practical ordering of materials. Germanium, with its 0.66 eV gap, has an intrinsic concentration near 2 x 1013 cm-3 at room temperature, roughly three orders of magnitude above silicon, which is why germanium junctions leak heavily and lose rectifying behavior at modest temperatures. Gallium arsenide and the wide-bandgap materials run many orders of magnitude below silicon, so their devices retain blocking capability at junction temperatures where silicon has long since gone intrinsic.
Effective Mass
Electrons and holes in a semiconductor crystal do not behave exactly like free particles. The periodic potential of the crystal lattice affects their motion, which is accounted for by assigning them an effective mass different from the free electron mass. This effective mass depends on the curvature of the energy bands and differs for electrons and holes, and even varies with direction in the crystal.
Silicon illustrates how much structure this single word conceals. Its conduction band has six equivalent minima along the crystal axes, and within each the electron mass is highly anisotropic: about 0.98 times the free electron mass along the valley axis and about 0.19 times the free electron mass transverse to it. Averaging these appropriately yields a conductivity effective mass near 0.26 free electron masses, the figure used in mobility calculations, and a somewhat larger density-of-states effective mass, close to the free electron mass, used to evaluate Nc. The valence band is more complicated still, consisting of overlapping heavy-hole and light-hole bands plus a third band split off by spin-orbit coupling; the resulting conductivity effective mass for holes is about 0.39 free electron masses.
The practical consequence is that holes in silicon are slower than electrons, so n-channel MOSFETs deliver roughly two to three times the current of p-channel devices of the same geometry. CMOS layouts compensate by making p-channel transistors wider. Gallium arsenide, by contrast, has a light electron effective mass near 0.067 free electron masses, which gives it electron mobility several times that of silicon and underpins its use in high-frequency circuits.
Doping and Extrinsic Semiconductors
The real power of semiconductors comes from the ability to precisely control their electrical properties through doping, the intentional introduction of impurity atoms. By adding atoms with different numbers of valence electrons, semiconductor conductivity can be increased by many orders of magnitude and made predominantly due to either electrons or holes.
N-Type Semiconductors
When silicon is doped with atoms having five valence electrons, such as phosphorus, arsenic, or antimony, the extra electron from each dopant atom is loosely bound and easily ionized into the conduction band. These dopants are called donors because they donate electrons. The resulting material is n-type, with electrons as the majority carriers and holes as minority carriers.
Donor atoms introduce energy levels just below the conduction band edge. In silicon the common donors lie roughly 40 to 55 meV below the edge, with antimony the shallowest, phosphorus in the middle, and arsenic the deepest of the three. Because thermal energy at room temperature is about 26 meV, these levels are shallow enough that virtually all donors are ionized, so the electron concentration approximately equals the donor concentration for typical doping levels. At cryogenic temperatures, ionization becomes incomplete and carriers "freeze out" onto their parent atoms, which is why ordinary silicon devices stop working far below room temperature.
Practical doping concentrations span an enormous range. Lightly doped drift regions in power devices may hold 1014 atoms per cubic centimeter, general-purpose logic wells fall between 1016 and 1018, and contact and source/drain regions are doped above 1019 to reduce resistance and enable ohmic metal contacts. Resistivity varies by about four orders of magnitude across that doping range, and undoped silicon is far more resistive still, on the order of 105 ohm-centimeters.
P-Type Semiconductors
Doping with atoms having three valence electrons, such as boron, aluminum, or gallium, creates acceptor sites that can capture electrons from the valence band, leaving behind holes. These materials are p-type, with holes as majority carriers. Acceptor levels lie just above the valence band edge; boron, the standard p-type dopant for silicon, sits about 45 meV above it, and like the shallow donors it is essentially fully ionized at room temperature. Boron is preferred in silicon technology because its small atomic size allows high solid solubility with little lattice strain, although that same small size makes it diffuse rapidly and therefore hard to confine in very shallow junctions.
The ability to create both n-type and p-type regions in the same crystal is fundamental to semiconductor device operation. Transistors, diodes, and integrated circuits all depend on controlled junctions between differently doped regions. In modern fabrication, dopants are introduced by ion implantation, which offers precise control of dose and depth, followed by a thermal anneal that repairs implantation damage and moves the dopant atoms onto lattice sites where they become electrically active.
Compensation and Carrier Concentration
When both donors and acceptors are present, they partially compensate each other. The net carrier type depends on which dopant has higher concentration. The carrier concentration is reduced by compensation, and the mobility may also be affected due to increased scattering from ionized impurities.
The relationship between carrier concentrations in thermal equilibrium is governed by the mass action law:
n * p = ni2
This relationship holds in thermal equilibrium regardless of doping, though it breaks down under illumination or current injection, where excess carriers push the product above ni2. If electrons are the majority carrier with concentration n = ND (the donor concentration), then the hole concentration is p = ni2 / ND, which can be many orders of magnitude smaller. Silicon doped with 1016 donors per cubic centimeter holds only about 104 holes per cubic centimeter, a ratio of a trillion to one. Minority carriers are scarce, yet they control the behavior of bipolar transistors, solar cells, and diode reverse leakage, because their relative changes are enormous even when their absolute numbers are tiny.
Compensation is exploited deliberately as well as tolerated. Every CMOS process builds n-type wells inside p-type substrates and p-type source/drain regions inside n-type wells by over-doping the existing background, so most working regions of a chip are compensated to some degree. Deliberate counter-doping also produces the high-resistivity, nearly intrinsic material used for radiation detectors and some power-device drift layers.
Carrier Transport Mechanisms
Charge carriers in semiconductors move through two primary mechanisms: drift under the influence of electric fields and diffusion due to concentration gradients. Understanding both is essential for analyzing device behavior.
Drift Current
When an electric field is applied to a semiconductor, charge carriers accelerate in response but are frequently scattered by lattice vibrations (phonons) and ionized impurities. This results in a constant average velocity called the drift velocity, proportional to the electric field:
vd = mu * E
Where mu is the carrier mobility and E is the electric field. Mobility has units of cm2/(V*s) and depends on temperature, doping concentration, and the semiconductor material. For lightly doped silicon at room temperature, electron mobility is roughly 1350 to 1450 cm2/(V*s) and hole mobility is roughly 450 to 500 cm2/(V*s).
Two scattering mechanisms dominate. Lattice or phonon scattering grows stronger as temperature rises and more vibrational modes are excited, so the mobility it permits falls with increasing temperature. Ionized impurity scattering, by contrast, weakens as temperature rises, because faster carriers spend less time deflected by each charged dopant ion, so the mobility it permits increases with temperature. The two combine approximately by Matthiessen's rule, in which the reciprocals of the individual mobilities add. In lightly doped silicon near room temperature, phonon scattering wins and mobility falls with heating; in heavily doped material at low temperature, impurity scattering dominates.
Doping therefore carries a penalty. Raising the donor concentration from 1015 to 1019 per cubic centimeter multiplies the carrier count ten-thousandfold but cuts electron mobility by roughly an order of magnitude, so conductivity rises by less than the doping ratio alone would suggest. A further reduction occurs at surfaces: carriers in a MOSFET inversion layer are pressed against the oxide interface by the gate field and scatter from interface roughness and charge, giving effective mobilities well below bulk values.
The drift current density is:
Jdrift = q * (n * mun + p * mup) * E = sigma * E
Where sigma is the conductivity. This is the semiconductor form of Ohm's law.
Diffusion Current
Carriers also move from regions of high concentration to low concentration through diffusion, even without an applied electric field. The diffusion current density for electrons is:
Jdiff,n = q * Dn * (dn/dx)
Where Dn is the electron diffusion coefficient. The corresponding hole term carries the opposite sign, Jdiff,p = -q * Dp * (dp/dx), because holes carry positive charge while both species flow down their own concentration gradient. The diffusion coefficient is related to mobility through the Einstein relation:
D = (kT/q) * mu
At 300 K, kT/q is about 25.9 mV, commonly rounded to 26 mV and called the thermal voltage. This relation reflects the fundamental connection between random thermal motion (diffusion) and directed motion under a field (drift): both arise from the same scattering process, so a material that impedes one impedes the other in fixed proportion. Applying it to silicon gives an electron diffusion coefficient near 36 cm2/s and a hole diffusion coefficient near 12 cm2/s at room temperature.
Drift and diffusion together, combined with Poisson's equation relating charge density to electric field and with continuity equations that account for generation and recombination, constitute the drift-diffusion model. That system of coupled equations is what technology computer-aided design tools solve numerically, and it remains the workhorse of device simulation despite its classical approximations. Only at the smallest dimensions, where carriers cross the active region in fewer collisions than a diffusive description assumes, do engineers turn to Monte Carlo or quantum transport methods instead.
High-Field Effects
At high electric fields, carrier velocity no longer increases linearly with field. In silicon at room temperature the drift velocity saturates near 1 x 107 cm/s for electrons and around 8 x 106 cm/s for holes, because carriers gain enough energy between collisions to emit optical phonons, and additional field energy then goes into lattice heating rather than into faster motion. Saturation sets in above roughly 104 V/cm, a field reached across a 1-micrometer gap at only 1 volt, so modern nanoscale transistors operate routinely in the velocity saturation regime. This is a central reason why shrinking a transistor no longer delivers proportional gains in drive current.
At even higher fields, carriers may gain enough energy to ionize lattice atoms on impact, creating additional electron-hole pairs that are themselves accelerated, in a multiplying process called impact ionization or avalanche multiplication. Silicon enters this regime near 3 x 105 V/cm. The effect is exploited deliberately in avalanche photodiodes and IMPATT oscillators and provides the controlled clamping action of avalanche-rated power transistors, but in most devices it appears as a destructive breakdown mechanism to be designed around.
Carriers that gain high energy without ionizing anything create a subtler reliability problem. So-called hot carriers can be injected into the gate oxide of a MOSFET, where they become trapped and shift the threshold voltage over time. Limiting hot-carrier damage is one of the reasons supply voltages fell steadily as transistor dimensions shrank.
P-N Junction Physics
The p-n junction, formed at the boundary between p-type and n-type semiconductor regions, is the fundamental building block of semiconductor devices. Understanding junction physics is essential for analyzing diodes, transistors, solar cells, and LEDs.
Junction Formation and the Depletion Region
When p-type and n-type materials are brought together, electrons diffuse from the n-side (where they are plentiful) to the p-side, while holes diffuse in the opposite direction. This diffusion leaves behind ionized dopant atoms: positive donor ions on the n-side and negative acceptor ions on the p-side. These fixed charges create an electric field that opposes further diffusion.
The region depleted of mobile carriers is called the depletion region or space charge region. In equilibrium, the drift current due to the built-in field exactly balances the diffusion current, resulting in zero net current. The built-in potential follows from the doping on each side:
Vbi = (kT/q) * ln(NA * ND / ni2)
For a silicon junction with typical doping this yields roughly 0.6 to 0.8 V at room temperature. The logarithm makes the result insensitive to doping: raising either concentration by a factor of ten adds only about 60 mV. Because ni appears in the denominator, wider-bandgap materials produce larger built-in potentials, which is why a gallium arsenide diode turns on near 1.2 V and a gallium nitride LED near 3 V while a silicon diode turns on near 0.7 V.
Charge neutrality requires that the depletion region hold equal amounts of positive and negative ionized charge, so it extends farther into the more lightly doped side. A one-sided junction, in which one region is far more heavily doped than the other, therefore places almost the entire depletion region and nearly all of the voltage drop in the lightly doped side. Power devices exploit this deliberately: a thick, lightly doped drift region supports the blocking voltage, and its required thickness sets the device's on-resistance. The width of the depletion region varies as the square root of the total junction voltage, so reverse bias widens it and forward bias narrows it.
Forward and Reverse Bias
Applying a voltage across the junction changes the balance between drift and diffusion. Forward bias (positive voltage on p-side) reduces the barrier, allowing more carriers to diffuse across the junction and producing significant current. The current increases exponentially with voltage according to the ideal diode equation:
I = Is * (exp(qV/nkT) - 1)
Where Is is the saturation current (typically 10-12 to 10-15 A for small silicon diodes) and n is the ideality factor. An ideality factor near 1 indicates that diffusion of minority carriers across the junction dominates, while a value approaching 2 indicates that recombination within the depletion region dominates, as it commonly does at low current. The exponential is steep: at room temperature, each 60 mV of additional forward bias multiplies an ideal diode's current by ten, which is the basis of the logarithmic converters and bandgap voltage references built from matched junctions.
Reverse bias (negative voltage on p-side) increases the barrier, reducing current to the small saturation current caused by thermally generated minority carriers. Real silicon diodes leak considerably more than the ideal equation predicts, because carriers are also generated at defect states inside the widened depletion region. The depletion region widens under reverse bias, a property exploited in varactor diodes for voltage-controlled capacitance.
Junction Capacitance
The depletion region acts as a parallel-plate capacitor, with the ionized dopants forming the "plates" and the depleted semiconductor as the dielectric. The depletion capacitance depends on voltage:
Cj = Cj0 / (1 - V/Vbi)m
Where Cj0 is the zero-bias capacitance, Vbi is the built-in potential, and m is the grading coefficient: approximately 0.5 for an abrupt junction and about 0.33 for a linearly graded one. Hyperabrupt profiles, engineered by grading the doping, give exponents above 0.5 and a correspondingly wider tuning range, which is why they are used in voltage-controlled oscillators. Measuring capacitance against reverse bias is also a standard laboratory method for extracting a doping profile, since the slope of 1/C2 versus voltage reveals the net doping at the moving depletion edge.
Under forward bias a second and usually larger capacitance appears. Injected minority carriers stored in the neutral regions must be removed before the junction can block again, an effect modeled as diffusion capacitance and observed as the reverse recovery time of a rectifier. Fast-switching diodes shorten it by deliberately reducing carrier lifetime, and Schottky diodes avoid it almost entirely by conducting with majority carriers only.
Junction Breakdown
Under sufficient reverse bias, a junction conducts heavily. Two distinct mechanisms produce this breakdown. Zener breakdown occurs in heavily doped junctions, where the depletion region is thin enough that valence-band electrons tunnel directly into conduction-band states across the gap. Avalanche breakdown occurs in more lightly doped junctions, where the depletion region is wide enough for carriers to accelerate to ionizing energies and multiply.
In silicon, tunneling dominates below roughly 5 V and avalanche above roughly 7 V, with both contributing in between. The two mechanisms have opposite temperature coefficients: the Zener mechanism grows easier with heating, so its breakdown voltage falls, while avalanche multiplication grows harder because hotter lattices scatter carriers before they reach ionizing energy, so its breakdown voltage rises. Near 5 to 6 V the two effects cancel, which is why breakdown diodes in that range are the most temperature-stable. Precision references exploit the same cancellation deliberately, placing a breakdown junction with a positive temperature coefficient in series with forward-biased junctions whose negative coefficient offsets it, and burying the breakdown region beneath the surface where its noise and long-term drift are lower.
Avalanche breakdown is not inherently destructive; devices fail from the heat that the resulting current produces, not from the multiplication itself. Power MOSFETs are therefore rated for a specific avalanche energy, and diodes intended for clamping duty are designed to spread the breakdown current uniformly across the die rather than allow it to concentrate at an edge or corner, where the field is highest.
Quantum Mechanical Foundations
Classical physics cannot explain semiconductor behavior. Quantum mechanics provides the theoretical framework for understanding why energy bands exist, why electrons can tunnel through thin barriers, and why semiconductor properties are so sensitive to crystal structure and purity.
Wave-Particle Duality
Electrons exhibit both wave and particle properties. In a semiconductor crystal, electron waves interact with the periodic potential of the lattice, and the wavelengths that scatter coherently from the lattice planes are forbidden, leaving gaps in the allowed energy spectrum. Bands and bandgaps are thus a direct consequence of wave interference in a periodic medium, closely analogous to the stopbands of an optical or microwave filter.
The de Broglie wavelength of a thermal electron in silicon is on the order of ten nanometers, which is comparable to the dimensions of modern transistor channels and larger than the thickness of many engineered layers. When a structure becomes smaller than this scale in one or more dimensions, carriers are confined and their energy levels become discrete. Quantum wells, wires, and dots exploit that confinement deliberately, and confinement in the inversion layer of a MOSFET shifts threshold voltage measurably in advanced devices.
Quantum Tunneling
Quantum mechanics allows electrons to penetrate through potential barriers that would be insurmountable according to classical physics. This tunneling effect is important in thin oxide layers, heavily doped p-n junctions (tunnel and Zener diodes), and flash memory, where charge is deliberately driven onto and off an isolated floating gate through an oxide barrier.
Tunneling current rises exponentially as a barrier thins, and that exponential is what ended the long practice of simply making gate oxides thinner with each process generation. As silicon dioxide approached one to two nanometers, gate leakage grew to consume an unacceptable share of chip power. The industry's answer was to replace silicon dioxide with hafnium-based high-permittivity dielectrics, which provide the same electrical coupling with a physically thicker and therefore far less transparent barrier. Intel introduced such a stack at its 45-nanometer node in 2007, and high-permittivity gate dielectrics have been standard in leading-edge logic ever since.
Fermi-Dirac Statistics
Electrons are fermions and obey Fermi-Dirac statistics, which give the probability that a state at energy E is occupied as f(E) = 1 / (1 + exp((E - EF) / kT)). The Fermi level EF is the energy at which that probability is exactly one half. When the Fermi level lies more than a few kT below the conduction band edge, the exponential dominates and the expression reduces to the simpler Boltzmann form used in most device analysis. Carrier concentrations then follow directly: n = ni * exp((EF - Ei) / kT) and p = ni * exp((Ei - EF) / kT), where Ei is the intrinsic Fermi level near midgap.
Doping moves the Fermi level: toward the conduction band in n-type material and toward the valence band in p-type. When doping is heavy enough to push it into a band, the semiconductor becomes degenerate, the Boltzmann approximation fails, and the material behaves increasingly like a metal. This condition is what makes heavily doped contact regions and polysilicon gates conduct well.
The most useful property of the Fermi level is that in thermal equilibrium it is constant everywhere in a connected system. Drawing a single flat Fermi level across a junction between two differently doped regions immediately forces the bands to bend, and the amount of that bending is the built-in potential. The same construction explains metal-semiconductor contacts, predicting whether a given combination yields a rectifying Schottky barrier or an ohmic contact. Under bias or illumination the system leaves equilibrium, and electrons and holes are described by separate quasi-Fermi levels whose separation measures the departure from equilibrium; in a solar cell, that separation is what appears at the terminals as photovoltage.
Generation and Recombination
Carriers are continuously being generated (moving from valence to conduction band) and recombining (electrons falling back into holes). In thermal equilibrium, these rates are equal, maintaining constant carrier concentrations. Under non-equilibrium conditions such as illumination or current flow, generation and recombination dynamics determine device behavior.
Recombination Mechanisms
Three main recombination mechanisms occur in semiconductors:
- Radiative recombination: The electron releases energy as a photon. This is the dominant mechanism in direct bandgap materials and is exploited in LEDs and laser diodes.
- Auger recombination: The energy is transferred to another carrier rather than emitted as light. This becomes significant at high carrier concentrations.
- Shockley-Read-Hall (SRH) recombination: Recombination occurs through defect states in the bandgap. This is often the dominant mechanism in indirect bandgap materials like silicon and is why crystal quality affects device performance. Deep states near midgap are the most effective, because they capture both carrier types readily; metallic contaminants such as iron, copper, and gold create exactly such states, which is why fabrication lines guard against parts-per-billion metal contamination.
These mechanisms act in parallel, and the fastest one sets the observed lifetime. Their differing dependence on carrier density has practical consequences. Auger recombination scales with the cube of carrier concentration, so it limits the efficiency of high-brightness LEDs, is a principal suspect in the efficiency droop those devices show at high drive current, and sets the ultimate efficiency ceiling of a silicon solar cell once all defects have been eliminated. Radiative and SRH processes scale less steeply, so SRH dominates in ordinary silicon at low injection.
Deliberate lifetime control is a standard engineering tool. Introducing gold or platinum, or bombarding a wafer with electrons or protons, adds recombination centers that shorten lifetime, speeding the turn-off of rectifiers and thyristors at the cost of higher forward voltage drop. Surfaces are themselves powerful recombination sites, since the abrupt end of the crystal leaves unsatisfied bonds; passivating them with a well-formed oxide or nitride layer is essential to solar cell and image sensor performance.
Optical Generation
A photon with energy exceeding the bandgap can promote an electron across it, creating an electron-hole pair. This is the mechanism behind every photodiode, image sensor, and solar cell. Excess energy above the bandgap is lost as heat within picoseconds as the carrier relaxes to the band edge, which is the fundamental reason a single-junction solar cell cannot exceed roughly a third of the incident sunlight in efficiency, and why multi-junction cells stack materials of differing bandgaps to capture each portion of the spectrum with a better-matched absorber.
Absorption depth varies enormously with wavelength. Blue light is absorbed within a fraction of a micrometer of a silicon surface, while near-infrared light penetrates deep into the wafer. Detectors and cells are designed around this: shallow junctions and good surface passivation for short wavelengths, thick and well-passivated bulk material with light-trapping surface texture for long ones.
Carrier Lifetime and Diffusion Length
The average time a carrier survives before recombining is called the carrier lifetime, typically ranging from nanoseconds to milliseconds depending on material quality and type. The diffusion length is the average distance a carrier diffuses before recombining:
L = sqrt(D * tau)
Where D is the diffusion coefficient and tau is the lifetime. The square root makes diffusion length a forgiving measure: a hundredfold improvement in lifetime buys only a tenfold increase in the distance a carrier travels.
The consequences are direct. A solar cell only collects a carrier if the carrier reaches the junction before recombining, so a wafer must be thinner than the diffusion length or the material must be good enough that the diffusion length exceeds the wafer thickness. High-quality silicon with lifetimes in the hundreds of microseconds gives diffusion lengths from several hundred micrometers to more than a millimeter, comfortably larger than a modern cell wafer of roughly 150 micrometers, which is precisely why cell manufacturers invest so heavily in contamination control and surface passivation. Bipolar transistors depend on the same quantity from the opposite direction: their base must be much thinner than the minority-carrier diffusion length so that injected carriers cross it and reach the collector rather than recombining on the way.
Temperature Effects
Semiconductor properties vary significantly with temperature, affecting device performance across operating conditions.
- Intrinsic carrier concentration: Increases exponentially with temperature, roughly doubling for every 8 to 10 degrees Celsius of rise in silicon near room temperature.
- Mobility: Generally decreases with increasing temperature due to increased phonon scattering, though in heavily doped material at low temperature, ionized impurity scattering dominates and mobility instead rises with temperature.
- Bandgap: Decreases slightly with increasing temperature, by roughly 0.25 meV per kelvin in silicon.
- Junction characteristics: At constant current, forward voltage decreases by approximately 2 mV per degree Celsius, and reverse leakage current rises steeply, roughly doubling every 8 to 10 degrees Celsius in silicon.
- Resistance of doped regions: Increases with temperature, because the carrier count is already fixed by the fully ionized dopants while mobility falls. This positive temperature coefficient gives power MOSFETs their characteristic on-resistance rise with heating, which conveniently allows devices to share current when paralleled.
These dependencies cut both ways. The predictable 2 mV per degree slope of a forward-biased junction is the basis of the silicon bandgap temperature sensor built into nearly every microcontroller and power management chip, and the difference in base-emitter voltage between two junctions run at different current densities is proportional to absolute temperature, the principle behind the bandgap voltage reference. The same physics threatens precision analog circuits with drift and creates the risk of thermal runaway, in which rising temperature increases leakage, which increases dissipation, which raises temperature further. Bipolar power stages guard against this with emitter degeneration resistors and thermal feedback.
Wide-Bandgap and Compound Semiconductors
Silicon dominates because it is abundant, forms an excellent native oxide, and can be grown as enormous defect-free crystals. It is not, however, the best material for every purpose, and the physics explained above shows exactly where its limits lie.
A wider bandgap raises the field at which impact ionization begins. Silicon breaks down near 0.3 MV/cm, while 4H silicon carbide and gallium nitride withstand roughly ten times that field. A device made from either material can therefore support a given blocking voltage with a drift region roughly an order of magnitude thinner and far more heavily doped, which cuts on-resistance dramatically for the same voltage rating. That single relationship is why wide-bandgap transistors switch faster and dissipate less than silicon devices of equal rating, and why they have displaced silicon in electric vehicle traction inverters, solar string inverters, and compact fast chargers.
Wide-bandgap materials also tolerate heat. Because intrinsic carrier concentration depends exponentially on the ratio of bandgap to thermal energy, silicon carbide remains far from intrinsic at temperatures where silicon has lost its blocking ability. Silicon carbide's high thermal conductivity, several times that of silicon, compounds the advantage by carrying heat out of the die efficiently. Gallium nitride, whose thermal conductivity is closer to silicon's, competes instead on switching speed, dominating below about 650 V while silicon carbide leads at higher voltages.
Compound semiconductors bring other properties silicon lacks. Direct bandgaps make gallium arsenide, indium phosphide, and gallium nitride the materials of light emission and detection, and alloying them shifts the bandgap continuously, which lets designers tune an LED or laser to a chosen wavelength. Low electron effective mass gives gallium arsenide and especially indium gallium arsenide very high mobility for microwave and millimeter-wave amplifiers. Narrow-gap materials such as indium antimonide and mercury cadmium telluride detect infrared radiation that silicon cannot absorb.
These advantages come at a cost. Compound crystals are smaller, more expensive, more fragile, and more defect-prone than silicon; none has an insulating native oxide of comparable quality; and gallium nitride devices are usually grown on foreign substrates such as silicon or silicon carbide, where lattice mismatch introduces strain and defects. Material choice remains a trade-off among performance, cost, and manufacturability rather than a simple ranking.
Applications of Semiconductor Physics
Understanding semiconductor physics enables the design and optimization of countless devices:
- Transistors: MOSFETs control a surface inversion layer with a gate field, while bipolar transistors depend on minority-carrier injection across a base thinner than the diffusion length. Both trace their limits directly to mobility, velocity saturation, and carrier lifetime.
- Diodes: P-n junction physics explains rectification, the two distinct breakdown mechanisms behind Zener and avalanche devices, the voltage-dependent capacitance of varactors, and light emission in LEDs.
- Solar cells: Light generates electron-hole pairs that the junction field separates and the contacts collect. Bandgap sets the achievable voltage and the usable portion of the spectrum; diffusion length and surface passivation set the collected current.
- Photodetectors: Similar to solar cells but optimized for sensitivity and speed rather than power generation, with material chosen so that the bandgap lies below the photon energy of interest.
- Power devices: Blocking voltage, on-resistance, and switching loss follow from critical breakdown field, drift-region doping, and stored charge, which is what makes wide-bandgap materials so attractive.
- Sensors: Temperature, light, magnetic field, strain, and radiation all perturb carrier populations or transport in measurable, calibratable ways.
- Integrated circuits: Combine many transistors, diodes, resistors, and capacitors on a single semiconductor chip, where leakage, variability, and self-heating are all consequences of the same physics.
Summary
Semiconductor physics provides the foundation for understanding how electronic devices work at a fundamental level. The key concepts include the band structure of crystalline materials, the behavior of electrons and holes as charge carriers, how doping controls conductivity, carrier transport through drift and diffusion, and p-n junction behavior. These principles, grounded in quantum mechanics and solid-state physics, explain why semiconductors have such versatile and controllable electrical properties.
What makes the subject worth learning is how few ideas do so much work. A single exponential, the ratio of an energy barrier to thermal energy, governs intrinsic carrier concentration, diode current, leakage, and breakdown alike. One material parameter, the bandgap, simultaneously determines what wavelengths a device emits and absorbs, how much voltage it can block, and how hot it can run. Recognizing these recurring patterns turns a catalog of device behaviors into a small set of principles.
As devices shrink and new materials emerge, semiconductor physics continues to evolve. Quantum effects become more prominent, wide-bandgap materials such as gallium nitride and silicon carbide take over high-power and high-frequency applications, and the fundamental limits of scaling drive innovation in device architecture. A solid understanding of semiconductor physics prepares engineers to work with current technology and adapt to what follows it.
Related Topics
The physics described here underlies the materials and devices treated elsewhere on this site: