Physics by Lamhi: Not Your Boring Physics

CLASS 12 · CHAPTER 3 · CURRENT ELECTRICITY

DETAILED NOTES

Current Electricity

The complete chapter, section by section: current and drift velocity, Ohm's law and resistivity, the electron-collision model that derives drift velocity and resistivity from first principles, resistor combinations, EMF and internal resistance, the maximum power transfer result that trips up most students, Kirchhoff's laws applied to a full two-loop circuit, cells in series and parallel, the Wheatstone bridge balance condition, and the potentiometer, explained in plain language with original worked examples.

3.1 Electric Current & Drift Velocity

Electric current is the rate of flow of charge, I=ΔQ/ΔtI = \Delta Q/\Delta t, measured in amperes. Inside a conductor, free electrons don’t travel in straight lines toward the positive terminal, they zig-zag between collisions with the lattice, but superimposed on that randomness is a slow net drift opposite to the field:

Current in terms of drift velocity
I=nqvdAI = nqv_dA

where nn is the free-charge-carrier density, qq the charge per carrier, vdv_d the drift speed, and AA the conductor’s cross-sectional area (this relation is derived properly in §3.4). Drift speeds are tiny, typically a fraction of a mm/s, which is why a circuit lights up almost instantly despite electrons barely moving: it’s the field that propagates fast, not the electrons themselves.

3.2 Ohm’s Law & Resistance

For most conductors at constant temperature, current is proportional to the potential difference applied across them:

Ohm's law
V=IRV = IR

RR, the resistance, is a property of the specific object (depends on its length, area, and material), with SI unit the ohm (Ω), 1 Ω = 1 V/A.

Worked example

Basic Ohm's law

A resistor carries a current of 0.5 A when 10 V is applied across it. Find its resistance.

R=VI=100.5=20 ΩR = \dfrac{V}{I} = \dfrac{10}{0.5} = \textcolor{#e08a1e}{20\text{ Ω}}

3.3 Resistivity & Temperature Dependence

Resistance depends on geometry; resistivity ρ\rho is the material property alone:

Resistance from resistivity
R=ρℓAR = \rho\dfrac{\ell}{A}

For most metals, resistivity rises with temperature (more lattice vibration means more electron collisions):

ρT=ρ0[1+α(T−T0)]\rho_T = \rho_0\left[1 + \alpha(T - T_0)\right]

where α\alpha is the temperature coefficient of resistivity. Semiconductors behave oppositely: resistivity falls with rising temperature, since more charge carriers get thermally freed than are lost to extra scattering.

3.4 Drift of Electrons & the Origin of Resistivity

So far, I=nqvdAI = nqv_dA in §3.1 and R=ρℓ/AR = \rho\ell/A in §3.3 have simply been stated. This section builds both from a simple picture of what the electrons inside a metal are actually doing, and in the process explains why Ohm’s law holds at all, and what the resistivity of a metal is really made of.

3.4.1 Drift velocity from the collision picture

Picture a metal as a lattice of heavy, fixed positive ions with a sea of free electrons, each of charge −e-e and mass mm, with nn of them per unit volume. Even with no field applied, these electrons are far from still: they race around at high thermal speeds, repeatedly colliding with the ions, and each collision sends an electron off in a completely random new direction. Because the directions are random, the velocities of all NN electrons average to zero, and there is no net current:

1N∑i=1Nv⃗i=0\dfrac{1}{N}\sum_{i=1}^{N}\vec{v}_i = 0

Now switch on a field E⃗\vec{E}. Every electron feels a force −eE⃗-e\vec{E}, so between collisions it accelerates at

a⃗=−eE⃗m\vec{a} = -\dfrac{e\vec{E}}{m}

Follow one electron, number ii. Suppose it left its last collision with velocity v⃗i\vec{v}_i, and a time tit_i has passed since then. Accelerating uniformly for that time, its velocity now is

V⃗i=v⃗i−eE⃗m ti\vec{V}_i = \vec{v}_i - \dfrac{e\vec{E}}{m}\,t_i

The drift velocity v⃗d\vec{v}_d is the average of V⃗i\vec{V}_i over all the electrons at one instant. Average each term separately. The first term, v⃗i\vec{v}_i, averages to zero for exactly the reason above: right after a collision the direction is random. In the second term, eE⃗/me\vec{E}/m is the same for every electron, so only tit_i needs averaging. Collisions happen at random times, so some electrons were hit a long while ago and some only just now, but the average time since the last collision is a fixed property of the metal, the relaxation time τ\tau:

v⃗d≡⟨V⃗i⟩=⟨v⃗i⟩−eE⃗m⟨ti⟩=0−eE⃗m τ\vec{v}_d \equiv \langle\vec{V}_i\rangle = \langle\vec{v}_i\rangle - \dfrac{e\vec{E}}{m}\langle t_i\rangle = 0 - \dfrac{e\vec{E}}{m}\,\tau
Drift velocity
v⃗d=−eτmE⃗⇒vd=eEτm\vec{v}_d = -\dfrac{e\tau}{m}\vec{E} \qquad\Rightarrow\qquad v_d = \dfrac{eE\tau}{m}

The minus sign says the electrons drift against the field, as negative charges should. The surprise is that the result is a constant velocity, even though every electron is being accelerated the whole time. Each one picks up a little extra velocity along −E⃗-\vec{E}, loses it to a randomising collision, picks it up again, and so on. Averaged over the whole crowd, all that is left is a steady drift. A quick unit check: eEτ/meE\tau/m has units of (N)(s)/(kg) = m/s, a velocity, as it should.

3.4.2 From drift velocity to current

Take a flat area AA inside the conductor, at right angles to the field. In a short time Δt\Delta t, every free electron within a distance vd Δtv_d\,\Delta t of that area, on the upstream side, drifts across it. Those electrons fill a cylinder of base AA and length vd Δtv_d\,\Delta t, so their number is n (A vd Δt)n\,(A\,v_d\,\Delta t), and each carries charge of magnitude ee:

ΔQ=e nAvd Δt\Delta Q = e\,n A v_d\,\Delta t

Dividing by Δt\Delta t gives the current:

Current from drift
I=ΔQΔt=neAvdI = \dfrac{\Delta Q}{\Delta t} = neAv_d

which is exactly the I=nqvdAI = nqv_dA stated in §3.1, with q=eq=e for electrons.

3.4.3 Ohm's law and resistivity from first principles

Now put the two results together. Substituting vd=eEτ/mv_d = eE\tau/m into I=neAvdI = neAv_d:

I=neA(eEτm)=(ne2τm)AEI = neA\left(\dfrac{eE\tau}{m}\right) = \left(\dfrac{ne^2\tau}{m}\right)AE

Dividing both sides by AA gives the current per unit area, the current density j=I/Aj = I/A, which points along E⃗\vec{E} (conventional current runs opposite to the electron drift):

Microscopic Ohm's law
j⃗=σE⃗,σ=ne2τm\vec{j} = \sigma\vec{E}, \qquad \sigma = \dfrac{ne^2\tau}{m}

where σ\sigma is the conductivity. To connect this with the resistance of a real wire, take a wire of length ℓ\ell and cross-section AA with a potential difference VV across it, so that the uniform field inside is E=V/ℓE = V/\ell:

I=(ne2τm)A VℓI = \left(\dfrac{ne^2\tau}{m}\right)A\,\dfrac{V}{\ell}

Rearranging for VV:

V=(mne2τ)ℓA IV = \left(\dfrac{m}{ne^2\tau}\right)\dfrac{\ell}{A}\,I

Two things fall out at once. First, VV is proportional to II, which is Ohm’s law, as long as nn and τ\tau do not themselves depend on the field. Second, comparing with V=IR=Iρℓ/AV = IR = I\rho\ell/A identifies the resistivity directly:

Resistivity from the collision model
ρ=1σ=mne2τ\rho = \dfrac{1}{\sigma} = \dfrac{m}{ne^2\tau}

As a unit check, m/(ne2τ)m/(ne^2\tau) comes out in kg/(m⁻³·C²·s) = kg m³ A⁻² s⁻³, which is exactly the unit of Ω m. This formula also explains the temperature behaviour described in §3.3. In a metal, nn barely changes with temperature, but hotter ions vibrate more and the electrons move faster, so collisions come more often and τ\tau shrinks, which makes ρ\rho rise. In a semiconductor, heating frees many more carriers, so nn climbs steeply, and that growth outweighs the fall in τ\tau, which makes ρ\rho fall.

Worked example

Relaxation time and drift speed in an aluminium wire

Aluminium has about n=1.8×1029 m−3n = 1.8\times10^{29}\text{ m}^{-3} free electrons and a resistivity of ρ=2.65×10−8 Ω m\rho = 2.65\times10^{-8}\ \Omega\text{ m} at room temperature. (a) Find the relaxation time τ\tau. (b) An aluminium wire of cross-section 2.0 mm² carries a current of 5.0 A. Find the drift speed, and check it against vd=eEτ/mv_d = eE\tau/m. (Take e=1.6×10−19 Ce = 1.6\times10^{-19}\text{ C}, m=9.11×10−31 kgm = 9.11\times10^{-31}\text{ kg}.)

(a) Rearranging ρ=m/(ne2τ)\rho = m/(ne^2\tau) for τ\tau:

τ=mne2ρ=9.11×10−31(1.8×1029)(1.6×10−19)2(2.65×10−8)≈7.46×10−15 s\tau = \dfrac{m}{ne^2\rho} = \dfrac{9.11\times10^{-31}}{(1.8\times10^{29})(1.6\times10^{-19})^2(2.65\times10^{-8})} \approx \textcolor{#e08a1e}{7.46\times10^{-15}\text{ s}}

(b) From I=neAvdI = neAv_d, with A=2.0×10−6 m2A = 2.0\times10^{-6}\text{ m}^2:

vd=IneA=5.0(1.8×1029)(1.6×10−19)(2.0×10−6)≈8.68×10−5 m/sv_d = \dfrac{I}{neA} = \dfrac{5.0}{(1.8\times10^{29})(1.6\times10^{-19})(2.0\times10^{-6})} \approx \textcolor{#e08a1e}{8.68\times10^{-5}\text{ m/s}}

For the check, the field inside the wire is E=ρj=ρI/AE = \rho j = \rho I/A:

E=(2.65×10−8)(5.0)2.0×10−6=6.63×10−2 V/mE = \dfrac{(2.65\times10^{-8})(5.0)}{2.0\times10^{-6}} = 6.63\times10^{-2}\text{ V/m}vd=eEτm=(1.6×10−19)(6.63×10−2)(7.46×10−15)9.11×10−31≈8.68×10−5 m/sv_d = \dfrac{eE\tau}{m} = \dfrac{(1.6\times10^{-19})(6.63\times10^{-2})(7.46\times10^{-15})}{9.11\times10^{-31}} \approx 8.68\times10^{-5}\text{ m/s}

The two routes agree, as they must. The electrons crawl along at under a tenth of a millimetre per second, while colliding roughly 10¹⁴ times every second.

3.5 Combinations of Resistors

3.5.1 Series

Same current flows through every resistor; voltages add:

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

always larger than the largest individual resistor.

3.5.2 Parallel

Same voltage across every resistor; currents add, so conductance (1/R) adds:

1Rparallel=1R1+1R2+⋯\dfrac{1}{R_{parallel}} = \dfrac{1}{R_1}+\dfrac{1}{R_2}+\cdots

always smaller than the smallest individual resistor, since every extra branch opens another path for charge to flow, not another obstacle.

Worked example

Two resistors, both ways

A 6 Ω and a 3 Ω resistor are combined (a) in series, (b) in parallel. Find the equivalent resistance each way.

(a) Rs=6+3=9 Ω\text{(a)}\ R_s = 6+3 = \textcolor{#e08a1e}{9\ \Omega}(b) 1Rp=16+13=12  ⇒  Rp=2 Ω\text{(b)}\ \dfrac{1}{R_p} = \dfrac{1}{6}+\dfrac{1}{3} = \dfrac{1}{2} \;\Rightarrow\; R_p = \textcolor{#e08a1e}{2\ \Omega}

3.6 EMF & Internal Resistance

A real cell isn’t a perfect voltage source: it has its own internal resistance rr, which eats into the voltage it can actually deliver once current flows:

Terminal voltage (discharging)
V=ε−IrV = \varepsilon - Ir

For a complete circuit with external resistance RR:

Circuit current
I=εR+rI = \dfrac{\varepsilon}{R+r}

When a cell is instead being charged by a stronger external source, current is forced the other way through it, and the terminal voltage is higher than the EMF, not lower:

Terminal voltage (charging)
V=ε+IrV = \varepsilon + Ir

3.7 Maximum Power Transfer

Power delivered to the external resistor is P=I2RP=I^2R. Substituting I=ε/(R+r)I=\varepsilon/(R+r):

P(R)=ε2R(R+r)2P(R) = \dfrac{\varepsilon^2 R}{(R+r)^2}

To find where this is largest, differentiate with respect to RR (treating ε\varepsilon and rr as fixed) using the quotient rule, and set the result to zero:

dPdR=ε2 (R+r)2−R⋅2(R+r)(R+r)4=ε2 r−R(R+r)3\dfrac{dP}{dR} = \varepsilon^2\,\dfrac{(R+r)^2 - R\cdot 2(R+r)}{(R+r)^4} = \varepsilon^2\,\dfrac{r-R}{(R+r)^3}

The denominator (R+r)3(R+r)^3 is always positive, so dP/dRdP/dR has the same sign as r−Rr-R: positive for R<rR<r (power still rising as RR grows) and negative for R>rR>r (power already falling), so dP/dR=0dP/dR=0 at exactly R=rR=r, a genuine maximum. Substituting back into P(R)P(R):

Maximum power transfer
Pmax⁡=ε2r(2r)2=ε24ratR=r\textcolor{#e08a1e}{P_{\max}} = \dfrac{\varepsilon^2 r}{(2r)^2} = \dfrac{\varepsilon^2}{4r}\quad\text{at}\quad R = r

Shrinking RR below rr keeps raising current, but power to RR falls, since RR itself is now the small factor in I2RI^2R. Growing RR above rr keeps current falling, so power falls too. The maximum sits exactly in between, at R=rR=r. See the interactive circuit for the live version.

3.8 Kirchhoff’s Laws

Series and parallel formulas only go so far. As soon as a circuit has two or more sources sitting in different branches, it usually cannot be reduced to a single equivalent resistor at all. Two rules, both of them conservation laws in disguise, are enough to solve any such network.

3.8.1 Junction rule

At any junction, total current in equals total current out, charge can’t pile up or vanish at a point.

3.8.2 Loop rule

Around any closed loop, the sum of EMFs equals the sum of IR drops, energy is conserved going around and coming back to the same point.

3.8.3 Putting the rules to work

Applying the loop rule is really just walking around a loop and keeping a running total of how the potential changes, which must come back to zero where you started, since potential has only one value at each point. Four sign conventions do all the work. Crossing a resistor RR in the same direction as the current II you assumed for it, the potential drops, so write −IR-IR; crossing it against that current, write +IR+IR. Crossing a cell from its negative terminal to its positive terminal, the potential rises, so write +ε+\varepsilon; crossing from positive to negative, write −ε-\varepsilon. A cell’s internal resistance is treated as just another resistor.

The procedure is then always the same. Draw an arrow for the current in each branch, guessing the direction if you have to, and use the junction rule straight away so that you introduce as few unknown currents as possible. Then apply the loop rule to as many independent loops as there are unknowns left, and solve the simultaneous equations. A guessed direction never needs to be right: if a current comes out negative, it simply flows the opposite way to its arrow, with the same magnitude.

Worked example

Solving a two-source, two-loop circuit

Two junctions, A at the top and B at the bottom, are joined by three parallel branches. Branch 1 holds a 12 V battery with its positive terminal towards A, in series with a 4 Ω resistor. Branch 2 holds a 6 V battery, also with its positive terminal towards A, in series with a 2 Ω resistor. Branch 3 is a 6 Ω resistor on its own. Treating the batteries as ideal (any internal resistance can be folded into the series resistors), find the current in each branch.

Let I1I_1 flow up through branch 1 (from B to A), I2I_2 up through branch 2, and I3I_3 down through branch 3. The junction rule at A gives

I3=I1+I2I_3 = I_1 + I_2

Loop 1, up branch 1 and down branch 3, starting from B: the battery is crossed from −- to ++, then both resistors are crossed along their currents:

12−4I1−6I3=012 - 4I_1 - 6I_3 = 0

Loop 2, up branch 2 and down branch 3:

6−2I2−6I3=06 - 2I_2 - 6I_3 = 0

Substitute I3=I1+I2I_3 = I_1 + I_2 into both loop equations:

12−4I1−6(I1+I2)=0  ⇒  5I1+3I2=612 - 4I_1 - 6(I_1+I_2) = 0 \;\Rightarrow\; 5I_1 + 3I_2 = 66−2I2−6(I1+I2)=0  ⇒  3I1+4I2=36 - 2I_2 - 6(I_1+I_2) = 0 \;\Rightarrow\; 3I_1 + 4I_2 = 3

Multiply the first by 4 and the second by 3, then subtract to eliminate I2I_2:

(20I1+12I2)−(9I1+12I2)=24−9  ⇒  11I1=15(20I_1 + 12I_2) - (9I_1 + 12I_2) = 24 - 9 \;\Rightarrow\; 11I_1 = 15I1=1511 A≈1.36 AI_1 = \dfrac{15}{11}\text{ A} \approx \textcolor{#e08a1e}{1.36\text{ A}}

Back-substituting into 3I1+4I2=33I_1 + 4I_2 = 3:

I2=3−3(15/11)4=−311 A≈−0.273 AI_2 = \dfrac{3 - 3(15/11)}{4} = -\dfrac{3}{11}\text{ A} \approx \textcolor{#e08a1e}{-0.273\text{ A}}I3=I1+I2=1211 A≈1.09 AI_3 = I_1 + I_2 = \dfrac{12}{11}\text{ A} \approx \textcolor{#e08a1e}{1.09\text{ A}}

The minus sign on I2I_2 is the interesting part: 0.273 A actually flows down through branch 2, into the 6 V battery’s positive terminal, so the stronger 12 V battery is charging the weaker one. As a check, walk the outer loop (up branch 1, down branch 2), which was never used to find the answers:

12−4(1511)+2(−311)−6=6−6011−611=6−6=012 - 4\left(\tfrac{15}{11}\right) + 2\left(-\tfrac{3}{11}\right) - 6 = 6 - \tfrac{60}{11} - \tfrac{6}{11} = 6 - 6 = 0

The third loop is automatically satisfied, which is why only two loop equations were independent.

3.9 Cells in Series & Parallel

Cells, like resistors, can be combined, and just as a network of resistors can be replaced by one equivalent resistor, a group of cells can be replaced by one equivalent cell, with some EMF εeq\varepsilon_{eq} and internal resistance reqr_{eq}. The test is always the same: the combination has to produce the same terminal voltage, V=εeq−IreqV = \varepsilon_{eq} - Ir_{eq}, as the single cell would, for every current II drawn from it.

3.9.1 Cells in series

Join nn cells, with EMFs ε1,…,εn\varepsilon_1, \ldots, \varepsilon_n and internal resistances r1,…,rnr_1, \ldots, r_n, the positive terminal of each to the negative terminal of the next, and connect the two free ends across an external resistor RR. There is only one path, so the same current II passes through every cell and through RR. Walk round the loop in the direction of the current and apply the loop rule of §3.8: each cell is crossed from −- to ++, gaining its EMF but losing IrkIr_k across its own internal resistance, and the external resistor costs IRIR:

(ε1−Ir1)+(ε2−Ir2)+⋯+(εn−Irn)−IR=0(\varepsilon_1 - Ir_1) + (\varepsilon_2 - Ir_2) + \cdots + (\varepsilon_n - Ir_n) - IR = 0(ε1+ε2+⋯+εn)−I(r1+r2+⋯+rn)=IR(\varepsilon_1 + \varepsilon_2 + \cdots + \varepsilon_n) - I(r_1 + r_2 + \cdots + r_n) = IR

The right-hand side, IRIR, is the potential difference across the external resistor, which is the terminal voltage VV of the whole combination. A single equivalent cell would give V=εeq−IreqV = \varepsilon_{eq} - Ir_{eq}. For the two expressions to agree for every value of II, the part that does not depend on II and the part proportional to II must match separately:

Cells in series
εeq=ε1+ε2+⋯+εn,req=r1+r2+⋯+rn\varepsilon_{eq} = \varepsilon_1 + \varepsilon_2 + \cdots + \varepsilon_n, \qquad r_{eq} = r_1 + r_2 + \cdots + r_n

For nn identical cells this becomes εeq=nε\varepsilon_{eq} = n\varepsilon and req=nrr_{eq} = nr, so the current through RR is I=nε/(R+nr)I = n\varepsilon/(R + nr). If one cell is connected the wrong way round, the walk crosses it from ++ to −-, so its EMF enters the sum with a minus sign, while its internal resistance still adds, because the current still has to pass through it.

3.9.2 Cells in parallel

Now join two cells (ε1,r1\varepsilon_1, r_1 and ε2,r2\varepsilon_2, r_2) positive to positive at one point and negative to negative at another, and draw a total current II from the pair. Let I1I_1 and I2I_2 be the currents leaving the two positive terminals. The junction rule at the common positive point gives

I=I1+I2I = I_1 + I_2

Both cells are connected across the same two points, so they must have the same terminal voltage VV. Writing V=ε−IrV = \varepsilon - Ir for each cell and solving for its current:

V=ε1−I1r1  ⇒  I1=ε1−Vr1,V=ε2−I2r2  ⇒  I2=ε2−Vr2V = \varepsilon_1 - I_1r_1 \;\Rightarrow\; I_1 = \dfrac{\varepsilon_1 - V}{r_1}, \qquad V = \varepsilon_2 - I_2r_2 \;\Rightarrow\; I_2 = \dfrac{\varepsilon_2 - V}{r_2}

Add the two currents:

I=ε1r1+ε2r2−V(1r1+1r2)I = \dfrac{\varepsilon_1}{r_1} + \dfrac{\varepsilon_2}{r_2} - V\left(\dfrac{1}{r_1} + \dfrac{1}{r_2}\right)

and rearrange for the terminal voltage:

V=ε1/r1+ε2/r21/r1+1/r2−I 11/r1+1/r2V = \dfrac{\varepsilon_1/r_1 + \varepsilon_2/r_2}{1/r_1 + 1/r_2} - I\,\dfrac{1}{1/r_1 + 1/r_2}

This has exactly the form V=εeq−IreqV = \varepsilon_{eq} - Ir_{eq}. Matching the term proportional to II gives the internal resistance, and the constant term then gives the EMF (multiplying top and bottom by r1r2r_1r_2 to tidy it):

1req=1r1+1r2  ⇒  req=r1r2r1+r2\dfrac{1}{r_{eq}} = \dfrac{1}{r_1} + \dfrac{1}{r_2} \;\Rightarrow\; r_{eq} = \dfrac{r_1r_2}{r_1 + r_2}
Two cells in parallel
εeq=req(ε1r1+ε2r2)=ε1r2+ε2r1r1+r2\varepsilon_{eq} = r_{eq}\left(\dfrac{\varepsilon_1}{r_1} + \dfrac{\varepsilon_2}{r_2}\right) = \dfrac{\varepsilon_1r_2 + \varepsilon_2r_1}{r_1 + r_2}

The same steps with nn cells just add more terms to each sum, since I=∑k(εk−V)/rkI = \sum_k(\varepsilon_k - V)/r_k, giving the general rule

n cells in parallel
1req=1r1+⋯+1rn,εeqreq=ε1r1+⋯+εnrn\dfrac{1}{r_{eq}} = \dfrac{1}{r_1} + \cdots + \dfrac{1}{r_n}, \qquad \dfrac{\varepsilon_{eq}}{r_{eq}} = \dfrac{\varepsilon_1}{r_1} + \cdots + \dfrac{\varepsilon_n}{r_n}

For nn identical cells, the first gives 1/req=n/r1/r_{eq} = n/r, so req=r/nr_{eq} = r/n, and the second gives εeq=(r/n)(nε/r)\varepsilon_{eq} = (r/n)(n\varepsilon/r):

n identical cells in parallel
εeq=ε,req=rn,I=εR+r/n\varepsilon_{eq} = \varepsilon, \qquad r_{eq} = \dfrac{r}{n}, \qquad I = \dfrac{\varepsilon}{R + r/n}

So the two arrangements do different jobs. Series stacking raises the EMF but piles up internal resistance, which pays off when the external resistance is large compared with nrnr. Parallel grouping leaves the EMF unchanged but divides the internal resistance, which pays off when the external resistance is small, and it also shares the current between the cells so that each one is worked less hard.

Worked example

The same two cells, in series and then in parallel

A cell of EMF 2.0 V and internal resistance 0.40 Ω and a cell of EMF 1.5 V and internal resistance 0.60 Ω drive an external resistor of 1.56 Ω. Find the current through the resistor when the cells are connected (a) in series, (b) in parallel. In (b), also find the current through each cell.

(a) In series, the EMFs and the internal resistances simply add:

I=ε1+ε2R+r1+r2=2.0+1.51.56+0.40+0.60=3.52.56≈1.37 AI = \dfrac{\varepsilon_1 + \varepsilon_2}{R + r_1 + r_2} = \dfrac{2.0 + 1.5}{1.56 + 0.40 + 0.60} = \dfrac{3.5}{2.56} \approx \textcolor{#e08a1e}{1.37\text{ A}}

(b) In parallel, first find the equivalent cell:

req=(0.40)(0.60)0.40+0.60=0.24 Ω,εeq=(2.0)(0.60)+(1.5)(0.40)0.40+0.60=1.8 Vr_{eq} = \dfrac{(0.40)(0.60)}{0.40 + 0.60} = 0.24\ \Omega, \qquad \varepsilon_{eq} = \dfrac{(2.0)(0.60) + (1.5)(0.40)}{0.40 + 0.60} = 1.8\text{ V}I=εeqR+req=1.81.56+0.24=1.00 AI = \dfrac{\varepsilon_{eq}}{R + r_{eq}} = \dfrac{1.8}{1.56 + 0.24} = \textcolor{#e08a1e}{1.00\text{ A}}

The common terminal voltage is V=IR=1.56 VV = IR = 1.56\text{ V}, so the current leaving each positive terminal is

I1=2.0−1.560.40=1.10 A,I2=1.5−1.560.60=−0.100 AI_1 = \dfrac{2.0 - 1.56}{0.40} = \textcolor{#e08a1e}{1.10\text{ A}}, \qquad I_2 = \dfrac{1.5 - 1.56}{0.60} = \textcolor{#e08a1e}{-0.100\text{ A}}

These add up to the 1.00 A through the resistor, as the junction rule demands. But I2I_2 is negative: the terminal voltage of 1.56 V is higher than the 1.5 V cell’s own EMF, so 0.100 A is pushed backwards into that cell, and the stronger cell is partly charging the weaker one. This is why cells with unequal EMFs should not be wired in parallel.

3.10 Wheatstone Bridge

Four resistors arranged in a diamond, with a galvanometer bridging the middle, let you measure an unknown resistance by finding the balance condition, zero galvanometer deflection:

Balance condition
PQ=RS\dfrac{P}{Q} = \dfrac{R}{S}

At balance, no current flows through the galvanometer branch at all, which is precisely why this method measures resistance so precisely: it doesn’t depend on the galvanometer’s own calibration, only on it reading exactly zero.

3.10.1 Deriving the balance condition from Kirchhoff's laws

Label the four corners of the diamond A, B, C and D. Resistor PP runs from A to B and QQ from B to C along one side; RR runs from A to D and SS from D to C along the other. A cell is connected across A and C (the battery arm), and a galvanometer of resistance GG across B and D (the galvanometer arm). Let a current I1I_1 flow from A into PP, a current I2I_2 from A into RR, and a current IgI_g from B to D through the galvanometer. The junction rule then fixes the other two currents: at B, QQ carries I1−IgI_1 - I_g, and at D, SS carries I2+IgI_2 + I_g.

Apply the loop rule to loop ABDA (through PP, then the galvanometer, then back through RR against its current):

−I1P−IgG+I2R=0-I_1P - I_gG + I_2R = 0

and to loop BCDB (through QQ, back through SS against its current, then back through the galvanometer against IgI_g):

−(I1−Ig)Q+(I2+Ig)S+IgG=0-(I_1 - I_g)Q + (I_2 + I_g)S + I_gG = 0

These two equations hold for any resistor values. Now impose the balance condition, Ig=0I_g = 0. The galvanometer terms vanish, and the equations reduce to

I1P=I2RandI1Q=I2SI_1P = I_2R \qquad\text{and}\qquad I_1Q = I_2S

Dividing the first equation by the second cancels both currents:

Wheatstone bridge balance condition
I1PI1Q=I2RI2S  ⇒  PQ=RS\dfrac{I_1P}{I_1Q} = \dfrac{I_2R}{I_2S} \;\Rightarrow\; \dfrac{P}{Q} = \dfrac{R}{S}

Look at what has dropped out: the cell’s EMF, its internal resistance, and the galvanometer’s resistance GG are all gone. That is the real reason the method is so precise. Physically, I1P=I2RI_1P = I_2R says the potential falls by the same amount from A to B as from A to D, so B and D sit at the same potential, and with no potential difference across it the galvanometer has no reason to carry any current. In use, PP and QQ are known ratio arms, RR is a variable known resistance adjusted until the galvanometer reads zero, and the unknown is then S=(Q/P) RS = (Q/P)\,R. (NCERT writes the same condition as R2/R1=R4/R3R_2/R_1 = R_4/R_3 with its own labels; in both cases the ratio of the two resistors on one side of the galvanometer equals the ratio of the two on the other side.)

Worked example

Finding an unknown resistance, and checking the balance

A Wheatstone bridge balances with P=150 ΩP = 150\ \Omega, Q=50 ΩQ = 50\ \Omega and R=270 ΩR = 270\ \Omega. Find the unknown SS. Then, taking the cell as an ideal 6.0 V source, confirm that B and D really are at the same potential.

S=QP R=50150×270=90 ΩS = \dfrac{Q}{P}\,R = \dfrac{50}{150}\times270 = \textcolor{#e08a1e}{90\ \Omega}

With no current in the galvanometer, each side of the diamond is just two resistors in series across 6.0 V:

I1=6.0P+Q=6.0200=0.030 A,I2=6.0R+S=6.0360=0.0167 AI_1 = \dfrac{6.0}{P + Q} = \dfrac{6.0}{200} = 0.030\text{ A}, \qquad I_2 = \dfrac{6.0}{R + S} = \dfrac{6.0}{360} = 0.0167\text{ A}VA−VB=I1P=(0.030)(150)=4.5 V,VA−VD=I2R=(6.0360)(270)=4.5 VV_A - V_B = I_1P = (0.030)(150) = 4.5\text{ V}, \qquad V_A - V_D = I_2R = \left(\tfrac{6.0}{360}\right)(270) = 4.5\text{ V}

Both points sit 4.5 V below A, so VB=VDV_B = V_D and the galvanometer, with no potential difference across it, carries no current, exactly as the balance condition promised.

3.11 The Potentiometer

A voltmeter connected across a cell always draws some current from it, so it reads the cell’s terminal voltage, ε−Ir\varepsilon - Ir, never quite the EMF itself. The potentiometer gets round this with a null method, like the Wheatstone bridge: at the moment of measurement, it draws no current at all from the cell being tested.

3.11.1 Principle: a constant potential gradient

The heart of the instrument is a long wire AB, of length LL and total resistance RwR_w, made of one material with a perfectly uniform cross-section. A driver cell (EMF εD\varepsilon_D, internal resistance rDr_D), in series with a rheostat set to RhR_h, pushes a steady current through the wire from A to B:

I=εDRw+Rh+rDI = \dfrac{\varepsilon_D}{R_w + R_h + r_D}

Because the wire is uniform, its resistance is shared out evenly along its length: a piece of length ℓ\ell has resistance (Rw/L) ℓ(R_w/L)\,\ell. With the same current II in every part of the wire, the potential drop from A to a point J a distance ℓ\ell along it is

VAJ=I(RwL)ℓV_{AJ} = I\left(\dfrac{R_w}{L}\right)\ell
Potentiometer principle
VAJ=kℓ,k=IRwL=εDRw(Rw+Rh+rD) LV_{AJ} = k\ell, \qquad k = \dfrac{IR_w}{L} = \dfrac{\varepsilon_D R_w}{(R_w + R_h + r_D)\,L}

The quantity kk, in volts per metre, is the potential gradient. As long as the current stays steady, kk is the same everywhere along the wire, so the wire turns length into a direct, linear measure of potential difference. Its units check out: (A)(Ω)/(m) = V/m.

To measure a cell of EMF ε\varepsilon and internal resistance rr, connect its positive terminal to A (the same end as the driver’s positive terminal) and its negative terminal, through a galvanometer of resistance GG, to a sliding contact (the jockey) touching the wire at J. Let IgI_g be the current flowing from J through the galvanometer and the test cell back to A. The loop rule, going from A along the wire to J, then through the galvanometer, then through the test cell from −- to ++ back to A, gives

−VAJ−IgG+(ε−Igr)=0  ⇒  Ig=ε−VAJG+r-V_{AJ} - I_gG + (\varepsilon - I_gr) = 0 \;\Rightarrow\; I_g = \dfrac{\varepsilon - V_{AJ}}{G + r}

So the galvanometer deflects one way when the jockey is too close to A (VAJ<εV_{AJ} < \varepsilon) and the other way when it is too far along (VAJ>εV_{AJ} > \varepsilon). Slide the jockey until the deflection is exactly zero. At this balance point, a distance ℓ\ell from A, Ig=0I_g = 0: the test circuit takes no current from the wire and adds none to it, so the wire current is still II, the drop to J is still exactly kℓk\ell, and no current means no IrIr loss inside the test cell. Therefore

Balance condition
ε=kℓ\varepsilon = k\ell

the full EMF, not the terminal voltage. A balance point can only exist on the wire if the drop across its whole length is larger than the EMF being measured, kL>εkL > \varepsilon, so the driver cell must be the stronger one. And the smaller kk is made (a longer wire, or less current), the longer the balance length for a given EMF, so the same reading error in the length becomes a smaller fraction of it: a lower potential gradient makes a more sensitive potentiometer.

3.11.2 Comparing the EMFs of two cells

Connect two cells, of EMFs ε1\varepsilon_1 and ε2\varepsilon_2, so that a two-way key can switch either one into the galvanometer circuit, and find the balance length for each, ℓ1\ell_1 and ℓ2\ell_2, without touching the driver circuit, so that kk stays the same. Each balance gives

ε1=kℓ1,ε2=kℓ2\varepsilon_1 = k\ell_1, \qquad \varepsilon_2 = k\ell_2

Divide one by the other, and kk cancels:

Comparing two EMFs
ε1ε2=ℓ1ℓ2\dfrac{\varepsilon_1}{\varepsilon_2} = \dfrac{\ell_1}{\ell_2}

The ratio of EMFs comes straight from a ratio of two lengths, with no need to know the current, the wire’s resistance, or the driver cell’s EMF.

3.11.3 Measuring the internal resistance of a cell

First find the balance length ℓ1\ell_1 for the cell on its own, with nothing else connected across it. No current flows through the cell, so

ε=kℓ1\varepsilon = k\ell_1

Now connect a known resistance RR directly across the cell’s terminals (through a key, closed for this step). The cell now drives a current I′I' through RR; at balance the galvanometer arm carries nothing, so all of the cell’s current goes through RR, and

I′=εR+rI' = \dfrac{\varepsilon}{R + r}

The potentiometer now balances against the cell’s terminal voltage, V=I′RV = I'R, which is smaller than ε\varepsilon, so the new balance length ℓ2\ell_2 is shorter:

V=kℓ2V = k\ell_2

Divide the two balance conditions, so kk cancels, and write both ε\varepsilon and VV in terms of I′I':

ℓ1ℓ2=εV=I′(R+r)I′R=R+rR=1+rR\dfrac{\ell_1}{\ell_2} = \dfrac{\varepsilon}{V} = \dfrac{I'(R + r)}{I'R} = \dfrac{R + r}{R} = 1 + \dfrac{r}{R}

Solving for rr:

Internal resistance by potentiometer
r=R(ℓ1ℓ2−1)=R ℓ1−ℓ2ℓ2r = R\left(\dfrac{\ell_1}{\ell_2} - 1\right) = R\,\dfrac{\ell_1 - \ell_2}{\ell_2}

Again only lengths and one known resistance appear, and the result is a resistance multiplied by a pure number, as it must be.

Worked example

Calibrating a potentiometer, then using it twice

A potentiometer wire 4.00 m long has a resistance of 10.0 Ω. It is driven by a 4.0 V cell of negligible internal resistance in series with a rheostat set to 6.0 Ω. (a) Find the potential gradient. (b) Two cells balance at 240.0 cm and 176.0 cm. Find the ratio of their EMFs, and each EMF. (c) When a 9.0 Ω resistor is connected across the first cell, its balance point moves to 216.0 cm. Find that cell’s internal resistance.

(a) The current in the wire, and the gradient it produces:

I=4.010.0+6.0=0.25 A,k=IRwL=(0.25)(10.0)4.00=0.625 V/mI = \dfrac{4.0}{10.0 + 6.0} = 0.25\text{ A}, \qquad k = \dfrac{IR_w}{L} = \dfrac{(0.25)(10.0)}{4.00} = \textcolor{#e08a1e}{0.625\text{ V/m}}

The whole wire carries a drop of kL=2.5 VkL = 2.5\text{ V}, enough for any cell up to 2.5 V to find a balance point.

(b) The ratio needs only the two lengths:

ε1ε2=ℓ1ℓ2=240.0176.0≈1.36\dfrac{\varepsilon_1}{\varepsilon_2} = \dfrac{\ell_1}{\ell_2} = \dfrac{240.0}{176.0} \approx \textcolor{#e08a1e}{1.36}ε1=kℓ1=(0.625)(2.400)=1.50 V,ε2=kℓ2=(0.625)(1.760)=1.10 V\varepsilon_1 = k\ell_1 = (0.625)(2.400) = \textcolor{#e08a1e}{1.50\text{ V}}, \qquad \varepsilon_2 = k\ell_2 = (0.625)(1.760) = \textcolor{#e08a1e}{1.10\text{ V}}

(c) With ℓ1=240.0 cm\ell_1 = 240.0\text{ cm} and ℓ2=216.0 cm\ell_2 = 216.0\text{ cm}:

r=R ℓ1−ℓ2ℓ2=9.0×240.0−216.0216.0=9.0×24.0216.0=1.0 Ωr = R\,\dfrac{\ell_1 - \ell_2}{\ell_2} = 9.0\times\dfrac{240.0 - 216.0}{216.0} = 9.0\times\dfrac{24.0}{216.0} = \textcolor{#e08a1e}{1.0\ \Omega}

As a check, the terminal voltage at the second balance is (0.625)(2.160)=1.35 V(0.625)(2.160) = 1.35\text{ V}, so the cell’s current is 1.35/9.0=0.15 A1.35/9.0 = 0.15\text{ A}, and ε−I′r=1.50−(0.15)(1.0)=1.35 V\varepsilon - I'r = 1.50 - (0.15)(1.0) = 1.35\text{ V}, which agrees.

— From the NCERT exercises

NCERT Exercise 3.8

A storage battery of EMF 8.0 V and internal resistance 0.5 Ω is being charged by a 120 V DC supply using a series resistor of 15.5 Ω. What is the terminal voltage of the battery during charging?

Solution

During charging, current is forced into the battery against its own EMF, so the supply has to overcome both the battery’s EMF and the total series resistance:

I=Vsupply−εR+r=120−815.5+0.5=11216=7 AI = \dfrac{V_{supply} - \varepsilon}{R + r} = \dfrac{120 - 8}{15.5 + 0.5} = \dfrac{112}{16} = 7\text{ A}

Since current flows into the positive terminal during charging, terminal voltage is EMF plus the Ir drop, not minus:

V=ε+Ir=8.0+(7)(0.5)=11.5 VV = \varepsilon + Ir = 8.0 + (7)(0.5) = \textcolor{#e08a1e}{11.5\text{ V}}

NCERT Exercise 3.7

Determine the current in each branch of the network shown in Fig. 3.20. (The network is a bridge ABCD with AB = 10 Ω, BC = 5 Ω, AD = 5 Ω, DC = 10 Ω, and a 5 Ω resistor across BD; a 10 V battery in series with a 10 Ω resistor is connected across A and C, driving current into A.)

Solution

This is a Wheatstone bridge that is not balanced (P/Q=10/5=2P/Q = 10/5 = 2 but R/S=5/10=1/2R/S = 5/10 = 1/2), so current flows through BD and the full Kirchhoff treatment of §3.8 is needed. Let I1I_1 flow along AB, I2I_2 along AD, and IgI_g from B to D. The junction rule gives BC a current of I1−IgI_1 - I_g, DC a current of I2+IgI_2 + I_g, and the battery branch I1+I2I_1 + I_2.

Loop ABDA:

−10I1−5Ig+5I2=0  ⇒  I2=2I1+Ig-10I_1 - 5I_g + 5I_2 = 0 \;\Rightarrow\; I_2 = 2I_1 + I_g

Loop BCDB:

−5(I1−Ig)+10(I2+Ig)+5Ig=0  ⇒  −I1+2I2+4Ig=0-5(I_1 - I_g) + 10(I_2 + I_g) + 5I_g = 0 \;\Rightarrow\; -I_1 + 2I_2 + 4I_g = 0

Outer loop A to B to C, then back through the battery and the 10 Ω resistor to A:

10−10I1−5(I1−Ig)−10(I1+I2)=0  ⇒  5I1+2I2−Ig=210 - 10I_1 - 5(I_1 - I_g) - 10(I_1 + I_2) = 0 \;\Rightarrow\; 5I_1 + 2I_2 - I_g = 2

Substitute I2=2I1+IgI_2 = 2I_1 + I_g into the BCDB equation:

−I1+2(2I1+Ig)+4Ig=0  ⇒  3I1+6Ig=0  ⇒  Ig=−I12-I_1 + 2(2I_1 + I_g) + 4I_g = 0 \;\Rightarrow\; 3I_1 + 6I_g = 0 \;\Rightarrow\; I_g = -\dfrac{I_1}{2}

so I2=2I1−I1/2=3I1/2I_2 = 2I_1 - I_1/2 = 3I_1/2. Then the outer-loop equation gives

5I1+2(32I1)+12I1=2  ⇒  172I1=2  ⇒  I1=417 A5I_1 + 2\left(\tfrac{3}{2}I_1\right) + \tfrac{1}{2}I_1 = 2 \;\Rightarrow\; \tfrac{17}{2}I_1 = 2 \;\Rightarrow\; I_1 = \dfrac{4}{17}\text{ A}

Reading off every branch:

AB: 417 A,AD: 617 A,BD: Ig=−217 A\text{AB: } \textcolor{#e08a1e}{\tfrac{4}{17}\text{ A}}, \quad \text{AD: } \textcolor{#e08a1e}{\tfrac{6}{17}\text{ A}}, \quad \text{BD: } I_g = \textcolor{#e08a1e}{-\tfrac{2}{17}\text{ A}}BC: I1−Ig=617 A,DC: I2+Ig=417 A,battery: 1017 A\text{BC: } I_1 - I_g = \textcolor{#e08a1e}{\tfrac{6}{17}\text{ A}}, \quad \text{DC: } I_2 + I_g = \textcolor{#e08a1e}{\tfrac{4}{17}\text{ A}}, \quad \text{battery: } \textcolor{#e08a1e}{\tfrac{10}{17}\text{ A}}

The negative IgI_g means 2/17 A actually flows from D to B. (NCERT’s answer lists CD as −4/17 A, which is the same 4/17 A from D to C, just labelled in the opposite direction.) As a check, the loop A to D to C and back through the battery gives 10−10(1017)−5(617)−10(417)=10−17017=010 - 10\left(\tfrac{10}{17}\right) - 5\left(\tfrac{6}{17}\right) - 10\left(\tfrac{4}{17}\right) = 10 - \tfrac{170}{17} = 0.

Want the interactive version instead? Try the circuit simulation → or take a practice paper →
Prefer Lamhi’s own class notes? The opening of this chapter is also covered in her handwritten Electrostatics notebook — download the handwritten notes (PDF) → or the cleanly typeset version →