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Circuits

In a conductor with no applied electric field, mobile charges move randomly because of thermal motion. Their velocities point in all directions, so there is no net transport of charge.

An applied field adds a small average drift velocity v⃗d\vec v_d to that random motion. A carrier accelerates between collisions, loses its directed momentum to the lattice, and accelerates again. The individual path is irregular, but the average drift is steady when the macroscopic current is steady.

For carriers with charge qq, the drift direction depends on the sign of qq. Electrons drift opposite E⃗\vec E, but conventional current is defined in the direction positive charge would move and therefore points along E⃗\vec E in an ohmic conductor.

~E;~Ielectrondriftrandommotionwithasmallaveragedrift

Current is the rate at which charge crosses a chosen surface:

I=dQdt.I=\frac{dQ}{dt}.

Current is a scalar assigned a sign relative to a chosen direction through a wire. The current density J⃗\vec J is a vector field describing both the local direction and the amount of current per unit area. The current through an oriented surface is its flux:

I=∫SJ⃗⋅dA⃗.I=\int_S\vec J\cdot d\vec A.

For uniform current density perpendicular to a cross-section of area AA,

I=JA.I=JA.

If the mobile-carrier number density is nn, each carrier has charge qq, and their average drift velocity is v⃗d\vec v_d, then

J⃗=nqv⃗d.\vec J=nq\vec v_d.

For electrons, both qq and the component of v⃗d\vec v_d along conventional current are negative, so J⃗\vec J still points in the conventional-current direction. In magnitude form,

I=n∣q∣Avd.I=n\lvert q\rvert Av_d.

Proof (Drift-current relation). In time dtdt, carriers drift distance vd,dtv_d,dt. The cylinder of carriers that crosses an area AA has volume

dV=Avd,dt.dV=Av_d,dt.

It contains dN=nAvd,dtdN=nAv_d,dt carriers, so the charge magnitude crossing the surface is

dQ=∣q∣nAvd,dt.dQ=\lvert q\rvert nAv_d,dt.

Therefore

I=dQdt=n∣q∣Avd.I=\frac{dQ}{dt}=n\lvert q\rvert Av_d.

The vector form restores the carrier sign and direction: J⃗=nqv⃗d\vec J=nq\vec v_d.

Example. A copper wire of cross-sectional area 1.0 mm21.0\ \text{mm}^2 carries 3.0 A3.0\ \text{A}. Assume one mobile electron per atom and electron number density n=8.5×1028 m−3n=8.5\times10^{28}\ \text{m}^{-3}. Find the electron drift-speed magnitude.

Use A=1.0×10−6 m2A=1.0\times10^{-6}\ \text{m}^2 and ∣q∣=e=1.60×10−19 C\lvert q\rvert=e=1.60\times10^{-19}\ \text{C}:

vd=IneA=3.0(8.5×1028)(1.60×10−19)(1.0×10−6)≈2.2×10−4 m/s.v_d=\frac{I}{n e A} =\frac{3.0}{(8.5\times10^{28})(1.60\times10^{-19})(1.0\times10^{-6})} \approx2.2\times10^{-4}\ \text{m/s}.

The carriers drift only about 0.22 mm/s0.22\ \text{mm/s}. A circuit responds much faster than this because the electric field establishing the drift propagates through the circuit, rather than one electron traveling from the source to the device.


Charge conservation and current continuity

Section titled “Charge conservation and current continuity”

Consider a fixed volume bounded by a closed surface. Outward current removes charge from the volume, so

dQinsidedt=−∮SJ⃗⋅dA⃗.\frac{dQ_{\text{inside}}}{dt} =-\oint_S\vec J\cdot d\vec A.

Writing Qinside=∫Vρq,dVQ_{\text{inside}}=\int_V\rho_q,dV, where ρq\rho_q is charge density, and applying the divergence theorem gives the local continuity equation:

∂ρq∂t+∇⋅J⃗=0.\frac{\partial\rho_q}{\partial t}+\nabla\cdot\vec J=0.

This is charge conservation written at every point. A positive divergence means more current leaves a small region than enters it, so its charge density must decrease.

For a steady current, ∂ρq/∂t=0\partial\rho_q/\partial t=0, and therefore

∇⋅J⃗=0.\nabla\cdot\vec J=0.

Equivalently, the total current entering any junction equals the total current leaving it. If that condition failed, charge would accumulate at the junction and change the local electric field until the currents adjusted.

Example. A steady current I1=5.0 AI_1=5.0\ \text{A} enters a junction through one wire. Currents I2=1.5 AI_2=1.5\ \text{A} and I3=2.0 AI_3=2.0\ \text{A} leave through two branches. Find the current and direction in a fourth branch.

Charge does not accumulate at a steady-current junction, so

I1=I2+I3+I4.I_1=I_2+I_3+I_4.

Thus

I4=5.0−1.5−2.0=1.5 A.I_4=5.0-1.5-2.0=1.5\ \text{A}.

The positive result means the fourth current leaves the junction as assumed.


An electric field exerts force qE⃗q\vec E on each carrier. Collisions continually remove directed momentum. A simple steady-state model represents the average resistive force as proportional and opposite to drift velocity:

F⃗R=−bv⃗d.\vec F_R=-b\vec v_d.

When the average drift stops changing, the forces balance:

qE⃗−bv⃗d=0.q\vec E-b\vec v_d=0.

Therefore

v⃗d=qbE⃗,\vec v_d=\frac{q}{b}\vec E,

and the current density becomes

J⃗=nqv⃗d=nq2bE⃗=σE⃗.\vec J=nq\vec v_d =\frac{nq^2}{b}\vec E =\sigma\vec E.

This is the differential form of Ohm’s law. Conductivity and resistivity are

σ=nq2b,ρ=1σ,\sigma=\frac{nq^2}{b}, \qquad \rho=\frac1\sigma,

so the equivalent form is

E⃗=ρJ⃗.\vec E=\rho\vec J.

The proportional-drag assumption is a material model, not a fundamental law. It works for ohmic materials over an appropriate range of fields and temperatures; diodes and strongly heated filaments are important counterexamples.

For a uniform wire of length LL and area AA, assume E⃗\vec E and J⃗\vec J are uniform and parallel to the wire. Then

V=EL,I=JA.V=EL, \qquad I=JA.

Using E=ρJE=\rho J,

V=ρJL=ρLAI.V=\rho JL =\rho\frac{L}{A}I.

Comparing this with V=IRV=IR gives

R=ρLA.R=\rho\frac{L}{A}.

This familiar formula requires a uniform material and constant cross-section. For a nonuniform conductor, add differential slices in series:

R=∫ρ(r⃗)A(x),dxR=\int\frac{\rho(\vec r)}{A(x)},dx

when the current is effectively one-dimensional.

Example. A conical conductor of length LL has resistivity ρ\rho and radius increasing linearly from aa to bb. Assume current flows along its axis and each thin slice is approximately equipotential. Find its resistance.

At position xx,

r(x)=a+b−aLx,A(x)=πr(x)2.r(x)=a+\frac{b-a}{L}x, \qquad A(x)=\pi r(x)^2.

Slices of thickness dxdx are in series, so

R=∫0Lρ,dxπ(a+b−aLx)2.R=\int_0^L\frac{\rho,dx}{\pi\left(a+\frac{b-a}{L}x\right)^2}.

Let u=a+(b−a)x/Lu=a+(b-a)x/L. Then dx=L,du/(b−a)dx=L,du/(b-a), giving

R=ρLπ(b−a)∫abduu2=ρLπ(b−a)(1a−1b)=ρLπab.R=\frac{\rho L}{\pi(b-a)}\int_a^b\frac{du}{u^2} =\frac{\rho L}{\pi(b-a)}\left(\frac1a-\frac1b\right) =\frac{\rho L}{\pi ab}.

An electric field does work on charge carriers as they drift through a resistor. Collisions transfer that organized energy into random atomic motion, so electrical energy becomes thermal energy.

The power delivered to any two-terminal element is

P=IV,P=IV,

where VV is the potential drop in the direction of conventional current. For an ohmic resistor, V=IRV=IR, so

P=I2R=V2R.P=I^2R=\frac{V^2}{R}.

The local form is useful when current is spread through a material. With current density J⃗\vec J and electric field E⃗\vec E, the power per unit volume is

p=J⃗⋅E⃗.p=\vec J\cdot\vec E.

For an isotropic ohmic material, E⃗=ρJ⃗\vec E=\rho\vec J, giving

p=ρJ2=σE2,p=\rho J^2=\sigma E^2,

where ρ\rho is resistivity and σ=1/ρ\sigma=1/\rho is conductivity. Integrating over the conductor gives the total heating power:

P=∫J⃗⋅E⃗ dV.P=\int \vec J\cdot\vec E\,dV.

Proof (Joule heating for a uniform wire). Consider a wire of length LL, cross-sectional area AA, and resistivity ρ\rho carrying uniform current II. Since J=I/AJ=I/A,

P=(AL)ρJ2=ALρ(IA)2=ρLAI2.P=(AL)\rho J^2 =AL\rho\left(\frac{I}{A}\right)^2 =\frac{\rho L}{A}I^2.

Using R=ρL/AR=\rho L/A gives

P=I2R.P=I^2R.

Combining this with V=IRV=IR produces the equivalent forms P=IVP=IV and P=V2/RP=V^2/R.

Example. A heating element made from wire of resistivity 1.1×10−6 Ω⋅m1.1\times10^{-6}\ \Omega\cdot\text{m} has length 2.0 m2.0\ \text{m} and cross-sectional area 0.50 mm20.50\ \text{mm}^2. It is connected across 120 V120\ \text{V}. Find its resistance, current, and heating power.

Convert the area: 0.50 mm2=5.0×10−7 m20.50\ \text{mm}^2=5.0\times10^{-7}\ \text{m}^2. Then

R=ρLA=(1.1×10−6)2.05.0×10−7=4.4 Ω.R=\rho\frac{L}{A} =(1.1\times10^{-6})\frac{2.0}{5.0\times10^{-7}} =4.4\ \Omega.

The current and power are

I=VR=1204.4≈27 A,I=\frac{V}{R}=\frac{120}{4.4}\approx27\ \text{A}, P=V2R=(120)24.4≈3.3×103 W.P=\frac{V^2}{R}=\frac{(120)^2}{4.4}\approx3.3\times10^3\ \text{W}.

Ideal wires have negligible resistance, so every continuously connected wire region is one node at a single potential. A component works only when the surrounding connections provide a closed path for steady current.

A voltage is always a difference between two points. Saying that one point is “at 5 V5\ \text{V}” is incomplete until a reference node is chosen; circuit diagrams usually label one node as ground, V=0V=0.

An ideal voltage source maintains a fixed potential difference. Its electromotive force, or EMF, is the work done by non-electrostatic forces per unit charge:

E=Wsourceq.\mathcal E=\frac{W_{\text{source}}}{q}.

Despite its name, EMF has units of volts and is not a force. Inside a battery, chemical forces move charge from lower to higher electric potential, supplying energy to the circuit.

A real battery can be modeled as an ideal EMF E\mathcal E in series with internal resistance rr.

ErRIrealsourceload

When the battery delivers current,

Vterminal=E−Ir.V_{\text{terminal}}=\mathcal E-Ir.

Only for an open circuit, when I=0I=0, does the measured terminal voltage equal the EMF. If the terminals are shorted by negligible external resistance,

Ishort=Er,I_{\text{short}}=\frac{\mathcal E}{r},

which can be dangerously large.

If current is forced into the positive terminal while charging the battery, the sign reverses and Vterminal=E+IrV_{\text{terminal}}=\mathcal E+Ir.

Example. A battery with E=12.0 V\mathcal E=12.0\ \text{V} and internal resistance r=0.50 Ωr=0.50\ \Omega powers a 5.5 Ω5.5\ \Omega load. Find the current, terminal voltage, power delivered to the load, and efficiency.

The total series resistance is R+r=6.0 ΩR+r=6.0\ \Omega, so

I=ER+r=12.06.0=2.0 A.I=\frac{\mathcal E}{R+r}=\frac{12.0}{6.0}=2.0\ \text{A}.

The terminal voltage is

Vterminal=E−Ir=12.0−(2.0)(0.50)=11.0 V.V_{\text{terminal}}=\mathcal E-Ir =12.0-(2.0)(0.50)=11.0\ \text{V}.

Thus

Pload=I2R=(2.0)2(5.5)=22 W.P_{\text{load}}=I^2R=(2.0)^2(5.5)=22\ \text{W}.

The chemical source supplies Psource=EI=24 WP_{\text{source}}=\mathcal EI=24\ \text{W}, while I2r=2.0 WI^2r=2.0\ \text{W} is dissipated internally. The efficiency is

η=PloadPsource=2224≈92%.\eta=\frac{P_{\text{load}}}{P_{\text{source}}} =\frac{22}{24}\approx92\%.

Two components are in series only if their shared node has no other branch, so the same current must pass through both. Voltage drops add, giving

Rseries=R1+R2+⋯ .R_{\text{series}}=R_1+R_2+\cdots.

Two components are in parallel only if both ends connect to the same two nodes. They share a voltage, while their currents add:

1Rparallel=1R1+1R2+⋯ .\frac{1}{R_{\text{parallel}}} =\frac{1}{R_1}+\frac{1}{R_2}+\cdots.

Circuit layout can be deceptive. Color-coding each ideal-wire node is often the fastest way to decide which elements are actually parallel.

R1R2seriesR1R2parallel

For series resistors across total voltage VV,

Vk=VRk∑iRi.V_k=V\frac{R_k}{\sum_i R_i}.

For two parallel resistors carrying total current II,

I1=IR2R1+R2,I2=IR1R1+R2.I_1=I\frac{R_2}{R_1+R_2}, \qquad I_2=I\frac{R_1}{R_1+R_2}.

The branch with smaller resistance receives more current. In conductance form, the general current-divider rule is

Ik=IGk∑iGi,Gi=1Ri.I_k=I\frac{G_k}{\sum_iG_i}, \qquad G_i=\frac{1}{R_i}.

Example. A 24 V24\ \text{V} source drives a 4 Ω4\ \Omega resistor in series with a parallel combination of 6 Ω6\ \Omega and 3 Ω3\ \Omega. Find every branch current and resistor voltage.

The parallel pair has resistance

Rp=(16+13)−1=2 Ω,R_p=\left(\frac{1}{6}+\frac{1}{3}\right)^{-1}=2\ \Omega,

so Req=4+2=6 ΩR_{\text{eq}}=4+2=6\ \Omega and the source current is

I=246=4 A.I=\frac{24}{6}=4\ \text{A}.

The 4 Ω4\ \Omega resistor drops V4=(4)(4)=16 VV_4=(4)(4)=16\ \text{V}, leaving 8 V8\ \text{V} across each parallel branch. Therefore

I6=86=43 A,I3=83 A.I_6=\frac{8}{6}=\frac{4}{3}\ \text{A}, \qquad I_3=\frac{8}{3}\ \text{A}.

The junction check is I6+I3=4 AI_6+I_3=4\ \text{A}.

Devices intended to receive the same rated voltage are connected in parallel. Putting them in series divides the supply voltage, so neither generally operates at its rated power. A device may be modeled as a resistor near its operating point using

Rrated=Vrated2Prated,R_{\text{rated}}=\frac{V_{\text{rated}}^2}{P_{\text{rated}}},

but real lamps and other temperature-dependent devices need not remain ohmic far from that point.


An ideal voltmeter has infinite resistance and is connected in parallel. It draws no current and behaves like an open branch. An ideal ammeter has zero resistance and is connected in series. It causes no voltage drop and behaves like a wire.

AARVV

Real meters perturb the circuit. Model a voltmeter as a large but finite resistance RVR_V and an ammeter as a small nonzero resistance RAR_A, then solve the modified circuit to estimate systematic error.

Example. A voltmeter with resistance RV=1.0 MΩR_V=1.0\ \text{M}\Omega measures the voltage across a 100 kΩ100\ \text{k}\Omega resistor that is in series with another 100 kΩ100\ \text{k}\Omega resistor across a 10 V10\ \text{V} source. Find the meter reading and compare it with the unloaded voltage.

Without the meter, symmetry gives 5.0 V5.0\ \text{V}. With the meter connected, the measured resistor is in parallel with RVR_V:

Rp=(100 kΩ)(1000 kΩ)1100 kΩ≈90.9 kΩ.R_p=\frac{(100\ \text{k}\Omega)(1000\ \text{k}\Omega)}{1100\ \text{k}\Omega} \approx90.9\ \text{k}\Omega.

The voltage divider now gives

Vmeter=1090.9100+90.9≈4.76 V.V_{\text{meter}}=10\frac{90.9}{100+90.9}\approx4.76\ \text{V}.

The meter reads about 0.24 V0.24\ \text{V} low because it loads the circuit.


A Wheatstone bridge compares two voltage-divider ratios. When the bridge is balanced, the middle detector connects equal-potential points and carries zero current.

ER1R2R3R4AG

With no detector current, each horizontal path is an independent series divider. Equality of the midpoint potentials gives

R1R2=R3R4,\frac{R_1}{R_2}=\frac{R_3}{R_4},

or equivalently

R1R4=R2R3.R_1R_4=R_2R_3.

This null method can measure an unknown resistance without needing an accurately calibrated detector. It is also useful for sensors: a small change in one resistor produces a small bridge voltage centered around zero rather than a small change sitting on top of a large DC offset.

Example. A balanced Wheatstone bridge has R1=120 ΩR_1=120\ \Omega, R2=80 ΩR_2=80\ \Omega, and R3=150 ΩR_3=150\ \Omega. Find R4R_4.

Use the balance condition:

R1R4=R2R3.R_1R_4=R_2R_3.

Therefore

R4=R2R3R1=(80)(150)120=100 Ω.R_4=\frac{R_2R_3}{R_1} =\frac{(80)(150)}{120} =100\ \Omega.

Series and parallel reduction is only a shortcut. Kirchhoff’s rules work for any lumped DC network.

The junction rule expresses charge conservation in steady state:

∑Iin=∑Iout.\sum I_{\text{in}}=\sum I_{\text{out}}.

For a network with nn nodes, only n−1n-1 junction equations are independent; summing all node equations gives 0=00=0.

The loop rule expresses energy conservation:

∑loopΔV=0.\sum_{\text{loop}}\Delta V=0.

Choose current and loop directions arbitrarily, then keep the signs consistent:

  • Crossing a resistor in the assumed current direction contributes −IR-IR; crossing against it contributes +IR+IR.
  • Crossing an ideal source from negative to positive contributes +E+\mathcal E; crossing from positive to negative contributes −E-\mathcal E.
  • A negative solved current simply means the actual current is opposite the assumed arrow.
E1R1R2E2R3R4I1I2

Example. Two nodes are joined by three parallel branches. The first contains a 12 V12\ \text{V} source in series with 2 Ω2\ \Omega, the second contains a 6 Ω6\ \Omega resistor, and the third contains a 6 V6\ \text{V} source in series with 3 Ω3\ \Omega. Both sources have their positive terminals at the upper-potential node. Find the node voltage VV and each downward branch current.

Let V=Vtop−VbottomV=V_{\text{top}}-V_{\text{bottom}} and take downward current as positive. Moving downward through each source and resistor gives

I1=V−122,I2=V6,I3=V−63.I_1=\frac{V-12}{2}, \qquad I_2=\frac{V}{6}, \qquad I_3=\frac{V-6}{3}.

No external current enters the top node, so the algebraic sum of downward currents is zero:

V−122+V6+V−63=0.\frac{V-12}{2}+\frac{V}{6}+\frac{V-6}{3}=0.

Multiplying by 66 gives

3V−36+V+2V−12=0,3V-36+V+2V-12=0,

so V=8.0 VV=8.0\ \text{V}. Therefore

I1=−2.0 A,I2=43 A,I3=23 A.I_1=-2.0\ \text{A}, \qquad I_2=\frac{4}{3}\ \text{A}, \qquad I_3=\frac{2}{3}\ \text{A}.

The negative sign means 2.0 A2.0\ \text{A} actually travels upward through the first branch. The check is −2+4/3+2/3=0-2+4/3+2/3=0.


For a large linear circuit, Kirchhoff equations are most systematic in matrix form. Choose one node as ground and let the remaining node potentials form a vector V⃗\vec V. For a resistor between nodes ii and jj, the current leaving node ii is

Ii→j=Vi−VjRij=Gij(Vi−Vj),I_{i\to j}=\frac{V_i-V_j}{R_{ij}}=G_{ij}(V_i-V_j),

where Gij=1/RijG_{ij}=1/R_{ij} is conductance. Applying the junction rule at every non-ground node produces

GV⃗=I⃗,\mathbf G\vec V=\vec I,

where I⃗\vec I contains currents injected by sources. The conductance matrix is built by inspection:

  • GiiG_{ii} is the sum of all conductances connected to node ii.
  • GijG_{ij} is minus the conductance directly connecting nodes ii and jj.
  • The reduced matrix is symmetric for ordinary reciprocal resistors.

For a three-node resistive triangle before grounding,

G=(G12+G13−G12−G13−G12G12+G23−G23−G13−G23G13+G23).\mathbf G= \begin{pmatrix} G_{12}+G_{13} & -G_{12} & -G_{13}\\ -G_{12} & G_{12}+G_{23} & -G_{23}\\ -G_{13} & -G_{23} & G_{13}+G_{23} \end{pmatrix}.

Every row sums to zero because shifting all potentials by the same constant changes no current. The full matrix therefore has a zero eigenvalue with eigenvector (1,1,1)T(1,1,1)^T. Choosing ground removes that redundant mode and makes the reduced system solvable.

Example. Node AA connects to a fixed 10 V10\ \text{V} node through 2 Ω2\ \Omega, to ground through 4 Ω4\ \Omega, and to node BB through 5 Ω5\ \Omega. Node BB also connects to ground through 10 Ω10\ \Omega. Find VAV_A and VBV_B using a matrix equation.

The node equations are

VA−102+VA4+VA−VB5=0,\frac{V_A-10}{2}+\frac{V_A}{4}+\frac{V_A-V_B}{5}=0, VB−VA5+VB10=0.\frac{V_B-V_A}{5}+\frac{V_B}{10}=0.

Collecting coefficients gives

(12+14+15−15−1515+110)(VAVB)=(50).\begin{pmatrix} \frac12+\frac14+\frac15 & -\frac15\\ -\frac15 & \frac15+\frac1{10} \end{pmatrix} \begin{pmatrix} V_A\\V_B \end{pmatrix} = \begin{pmatrix} 5\\0 \end{pmatrix}.

The second equation gives VA=32VBV_A=\tfrac32V_B. Substitution into the first gives

VB=20049 V≈4.08 V,VA=30049 V≈6.12 V.V_B=\frac{200}{49}\ \text{V}\approx4.08\ \text{V}, \qquad V_A=\frac{300}{49}\ \text{V}\approx6.12\ \text{V}.

For one static circuit, Gaussian elimination is usually more direct than diagonalization. Eigenvectors become useful for a repeated or symmetric network because they identify independent voltage patterns. If

G=UΛUT,\mathbf G=\mathbf U\mathbf\Lambda\mathbf U^T,

then in modal coordinates V⃗~=UTV⃗\tilde{\vec V}=\mathbf U^T\vec V and I⃗~=UTI⃗\tilde{\vec I}=\mathbf U^T\vec I,

ΛkV~k=I~k.\Lambda_k\tilde V_k=\tilde I_k.

Each eigenmode responds independently with effective conductance Λk\Lambda_k. Symmetry often lets you guess the modes as even and odd combinations without evaluating a large determinant.

For transient circuits containing capacitors, nodal analysis produces

CV⃗˙+GV⃗=I⃗(t).\mathbf C\dot{\vec V}+\mathbf G\vec V=\vec I(t).

Natural modes have the form V⃗=a⃗e−λt\vec V=\vec a e^{-\lambda t}, so

Ga⃗=λCa⃗.\mathbf G\vec a=\lambda\mathbf C\vec a.

This is a generalized eigenvalue problem. Each positive eigenvalue gives a decay rate λk\lambda_k and time constant

τk=1λk.\tau_k=\frac{1}{\lambda_k}.

If C\mathbf C is positive definite, define the symmetric matrix

A=C−1/2GC−1/2.\mathbf A=\mathbf C^{-1/2}\mathbf G\mathbf C^{-1/2}.

Diagonalizing A\mathbf A is numerically and conceptually cleaner than treating C−1G\mathbf C^{-1}\mathbf G as if it were symmetric. Convert an eigenvector u⃗k\vec u_k of A\mathbf A back to the circuit voltage pattern using a⃗k=C−1/2u⃗k\vec a_k=\mathbf C^{-1/2}\vec u_k.

For coupled lossless LC circuits, the analogous equation is

Lq⃗¨+Kq⃗=0,\mathbf L\ddot{\vec q}+\mathbf K\vec q=0,

where K\mathbf K contains inverse-capacitance coefficients. Trying q⃗=a⃗eiωt\vec q=\vec a e^{i\omega t} gives

Ka⃗=ω2La⃗,\mathbf K\vec a=\omega^2\mathbf L\vec a,

so the eigenvalues are squared normal-mode frequencies.

Example. Two identical LC loops each have inductance LL and capacitance CC. Their inductors have mutual inductance MM, with signs chosen so the off-diagonal inductance terms are +M+M. Find the two normal modes and their frequencies.

CLLCM

The equations are

(LMML)q⃗¨+1C(1001)q⃗=0.\begin{pmatrix}L&M\\M&L\end{pmatrix}\ddot{\vec q} +\frac1C\begin{pmatrix}1&0\\0&1\end{pmatrix}\vec q=0.

Symmetry gives an in-phase eigenvector

a⃗+=12(11),\vec a_+=\frac1{\sqrt2}\begin{pmatrix}1\\1\end{pmatrix},

with effective inductance L+ML+M and frequency

ω+=1C(L+M).\omega_+=\frac1{\sqrt{C(L+M)}}.

The out-of-phase eigenvector is

a⃗−=12(1−1),\vec a_-=\frac1{\sqrt2}\begin{pmatrix}1\\-1\end{pmatrix},

with effective inductance L−ML-M and frequency

ω−=1C(L−M).\omega_-=\frac1{\sqrt{C(L-M)}}.

Any initial charge pattern is a linear combination of these two eigenvectors. Their different frequencies cause beats and energy exchange between the loops.


A delta network cannot generally be reduced by series and parallel rules. It can be replaced by an equivalent wye network that produces the same terminal behavior at its three external nodes.

ARcBRaCRbARARBBRCC

For delta sides RaR_a opposite node AA, RbR_b opposite BB, and RcR_c opposite CC, the wye arms are

RA=RbRcRa+Rb+Rc,R_A=\frac{R_bR_c}{R_a+R_b+R_c}, RB=RaRcRa+Rb+Rc,RC=RaRbRa+Rb+Rc.R_B=\frac{R_aR_c}{R_a+R_b+R_c}, \qquad R_C=\frac{R_aR_b}{R_a+R_b+R_c}.

For the reverse transformation, define

S=RARB+RBRC+RCRA.S=R_AR_B+R_BR_C+R_CR_A.

Then the delta resistor opposite a wye arm is

Ra=SRA,Rb=SRB,Rc=SRC.R_a=\frac{S}{R_A}, \qquad R_b=\frac{S}{R_B}, \qquad R_c=\frac{S}{R_C}.

For three equal delta resistors RΔR_\Delta, each equivalent wye arm is RΔ/3R_\Delta/3. For three equal wye arms RYR_Y, each delta side is 3RY3R_Y.

Example. A delta has resistances Ra=6 ΩR_a=6\ \Omega, Rb=9 ΩR_b=9\ \Omega, and Rc=3 ΩR_c=3\ \Omega. Find its equivalent wye arms.

The common denominator is 6+9+3=18 Ω6+9+3=18\ \Omega. Therefore

RA=(9)(3)18=1.5 Ω,R_A=\frac{(9)(3)}{18}=1.5\ \Omega, RB=(6)(3)18=1.0 Ω,RC=(6)(9)18=3.0 Ω.R_B=\frac{(6)(3)}{18}=1.0\ \Omega, \qquad R_C=\frac{(6)(9)}{18}=3.0\ \Omega.

Source transformations and network theorems

Section titled “Source transformations and network theorems”

An ideal voltage source maintains voltage regardless of current. An ideal current source maintains current regardless of voltage. Real sources have limits, but these idealizations make linear networks much easier to reduce.

Any linear two-terminal network of sources and resistors can be replaced by either:

  • a Thevenin equivalent: voltage source VthV_{\text{th}} in series with RthR_{\text{th}};
  • a Norton equivalent: current source INI_{\text N} in parallel with RNR_{\text N}.

They describe the same terminal relation, so

RN=Rth,IN=VthRth.R_{\text N}=R_{\text{th}}, \qquad I_{\text N}=\frac{V_{\text{th}}}{R_{\text{th}}}.
VthRthABTheveninINRNABNorton

To find a Thevenin equivalent:

  1. Remove the load and find the open-circuit terminal voltage: Vth=VocV_{\text{th}}=V_{\text{oc}}.
  2. Turn off independent sources: short ideal voltage sources and open ideal current sources.
  3. Find the resistance seen looking into the terminals: RthR_{\text{th}}.
  4. Reconnect the load.

If dependent sources are present, do not turn them off. Apply a test voltage or current at the terminals and use Rth=Vtest/ItestR_{\text{th}}=V_{\text{test}}/I_{\text{test}}.

For Norton form, the short-circuit current is IN=IscI_{\text N}=I_{\text{sc}}.

Example. A 12 V12\ \text{V} source feeds R1=4 ΩR_1=4\ \Omega in series with R2=8 ΩR_2=8\ \Omega. Output terminals are taken across R2R_2. Find the Thevenin equivalent seen by a load connected to those terminals, then find the load current for RL=6 ΩR_L=6\ \Omega.

With the load removed, the divider voltage is

Vth=1284+8=8 V.V_{\text{th}}=12\frac{8}{4+8}=8\ \text{V}.

Turn off the ideal voltage source by replacing it with a wire. Seen from the output, R1R_1 and R2R_2 are parallel:

Rth=(4)(8)4+8=83 Ω.R_{\text{th}}=\frac{(4)(8)}{4+8}=\frac83\ \Omega.

After reconnecting the load,

IL=VthRth+RL=88/3+6=1213 A≈0.923 A.I_L=\frac{V_{\text{th}}}{R_{\text{th}}+R_L} =\frac{8}{8/3+6} =\frac{12}{13}\ \text{A}\approx0.923\ \text{A}.

In a linear circuit, the current or voltage caused by several independent sources equals the algebraic sum of their separate contributions. When considering one source alone:

  • replace other ideal voltage sources with shorts;
  • replace other ideal current sources with opens.

Dependent sources remain active. Superposition applies directly to voltages and currents, not to power, because power is quadratic. Find the total current or voltage first, then calculate power.

Symmetry-equivalent nodes have equal potential. Any resistor joining such nodes carries zero current and may be removed. Mirror-image halves can sometimes be folded together, turning corresponding resistors into parallel combinations.


For capacitor geometry and dielectric behavior, see Capacitors and Dielectrics. In a DC circuit, the capacitor relation is

q=CV,q=CV,

and current is the rate at which its plate charge changes:

I=dqdt,I=\frac{dq}{dt},

with the sign determined by the chosen current and plate-charge conventions.

An initially uncharged capacitor has zero voltage and behaves like a wire at the instant switching occurs. After a long time in a constant-source circuit, its current is zero and its branch behaves like an open circuit. These are limiting statements, not claims that a physical capacitor is literally a wire or broken connection.

For a capacitor with initial charge Q0Q_0 discharging through equivalent resistance RR,

Cq=CRI

Kirchhoff’s loop rule gives

qC+Rdqdt=0,\frac{q}{C}+R\frac{dq}{dt}=0,

so

q(t)=Q0e−t/RC,q(t)=Q_0e^{-t/RC}, VC(t)=Q0Ce−t/RC,I(t)=Q0RCe−t/RCV_C(t)=\frac{Q_0}{C}e^{-t/RC}, \qquad I(t)=\frac{Q_0}{RC}e^{-t/RC}

for a current magnitude chosen in the discharge direction.

For an initially uncharged capacitor charging through RR from an ideal source E\mathcal E,

E−qC−Rdqdt=0.\mathcal E-\frac{q}{C}-R\frac{dq}{dt}=0.

The solution is

q(t)=CE(1−e−t/RC),q(t)=C\mathcal E\left(1-e^{-t/RC}\right), VC(t)=E(1−e−t/RC),I(t)=ERe−t/RC.V_C(t)=\mathcal E\left(1-e^{-t/RC}\right), \qquad I(t)=\frac{\mathcal E}{R}e^{-t/RC}.

The time constant

τ=RC\tau=RC

sets the time scale. After one time constant, a decaying quantity is e−1≈36.8%e^{-1}\approx36.8\% of its initial value, while a charging quantity has completed 1−e−1≈63.2%1-e^{-1}\approx63.2\% of its total change.

Example. A 10 μF10\ \mu\text{F} capacitor initially charged to 20 V20\ \text{V} discharges through 2.0 MΩ2.0\ \text{M}\Omega. Find the time constant, the capacitor voltage after 30 s30\ \text{s}, and the time required to reach 5.0 V5.0\ \text{V}.

The time constant is

τ=RC=(2.0×106)(10×10−6)=20 s.\tau=RC=(2.0\times10^6)(10\times10^{-6})=20\ \text{s}.

At t=30 st=30\ \text{s},

VC=20e−30/20≈4.46 V.V_C=20e^{-30/20}\approx4.46\ \text{V}.

For VC=5.0 VV_C=5.0\ \text{V},

5=20e−t/20,5=20e^{-t/20},

so

t=20ln⁡4≈27.7 s.t=20\ln4\approx27.7\ \text{s}.

The series/parallel rules are opposite those for resistors:

Cparallel=C1+C2+⋯ ,C_{\text{parallel}}=C_1+C_2+\cdots, 1Cseries=1C1+1C2+⋯ .\frac1{C_{\text{series}}}=\frac1{C_1}+\frac1{C_2}+\cdots.

There is a useful algebraic correspondence

Q⟷I,1C⟷R.Q\longleftrightarrow I, \qquad \frac1C\longleftrightarrow R.

Thus a capacitor network can be mapped to a resistor network by replacing each capacitor CC with resistance 1/C1/C. Equivalent resistance in the mapped network corresponds to 1/Ceq1/C_{\text{eq}}. This is an algebraic shortcut; the physical meanings of charge and current remain different.


An ohmic resistor has a linear II-VV relation. A diode is nonlinear and conducts much more readily in one direction than the other.

An ideal diode has two states:

  • Forward biased: a closed switch with VD=0V_D=0 and ID≥0I_D\ge0.
  • Reverse biased: an open switch with ID=0I_D=0 and VD≤0V_D\le0, using voltage measured from anode to cathode.
ERI

To analyze an ideal-diode circuit, assume each diode is on or off, solve the resulting linear circuit, then check whether the solved current and voltage satisfy the assumed state. If not, reverse the assumption.

Real diodes have a smooth nonlinear response. Two resistance-like quantities describe different questions:

RDC=VIR_{\text{DC}}=\frac{V}{I}

is the ratio at one operating point, while

rsmall=dVdIr_{\text{small}}=\frac{dV}{dI}

is the local slope used for small changes around that point. A load-line method combines the external circuit relation with the diode curve; their intersection is the operating point.

Example. A practical constant-drop model treats a silicon diode as off when reverse biased and as a fixed 0.70 V0.70\ \text{V} drop when on. A 5.0 V5.0\ \text{V} source, 430 Ω430\ \Omega resistor, and diode are connected in series in the forward direction. Find the current and verify the assumed state.

Assume the diode is on. Kirchhoff’s loop rule gives

5.0−I(430)−0.70=0,5.0-I(430)-0.70=0,

so

I=4.3430=0.010 A=10 mA.I=\frac{4.3}{430}=0.010\ \text{A}=10\ \text{mA}.

The current is positive in the forward direction, so the on-state assumption is consistent.

Intrinsic silicon has relatively few mobile carriers. Doping creates:

  • n-type material, with extra mobile electrons from donor atoms;
  • p-type material, with mobile holes from acceptor atoms.

At a p-n junction, carrier diffusion leaves behind fixed ions and creates a depletion region with an internal electric field. Forward bias narrows the barrier and allows substantial current; reverse bias widens it and suppresses current until breakdown. Some forward-biased junctions emit light, producing LEDs.