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2027 exam · Equation sheet

AP® Physics C: Electricity and Magnetism equation sheet (2027), explained

The official Physics C: E&M reference sheet starts with a page of constants, unit symbols, prefixes, trig values and exam conventions. Then comes a two-column Electricity and Magnetism block, followed by the same Mechanics page and geometry, vectors and calculus page you get on the Physics C: Mechanics sheet. Below, we go through every E&M equation and every constant: what each symbol means, its unit, when to use it, the mistake students make most, and which topic teaches it. For the mechanics and math pages, we link to where they're explained on the Mechanics sheet page.

The official sheet: AP Physics C: Electricity and Magnetism Exam Reference Information (PDF, College Board) (opens in a new tab). Keep it open next to this page. We link to it instead of copying it, so you always see College Board's current version.

Checked against the 2027 version on October 5, 2026. The explanations are ours, not College Board's.

Using the sheet on exam day

  • The sheet is available for the whole exam, on paper and in the testing app. Learn where things sit before exam day: the E&M block is one page with two columns, and the left column runs from Coulomb's law down to power, while the right column runs from resistor combinations down to LC circuits.
  • Read the symbol lists next to each column. The sheet reuses letters: VV is electric potential or volume, ρ\rho is resistivity or charge density, nn is loops per unit length while NN is the total number of loops, and the same-looking ε\varepsilon means electric permittivity in the left column but emf in the right one.
  • The conventions box on the first page is worth a look: potential is zero infinitely far from an isolated point charge, current points the way positive charges would drift, resistors and bulbs are ohmic, and capacitors are air-filled with κ=1.0\kappa = 1.0 unless a problem says otherwise.
  • The sheet won't tell you when an equation applies. Gauss's law and Ampère's law only give you a field quickly when there's symmetry, Bsol=μ0nIB_{\text{sol}} = \mu_0 nI is for a long solenoid, and C=κε0AdC = \frac{\kappa\varepsilon_0 A}{d} is for parallel plates.
  • Use the prefix table before you plug in: μC, nC, pF and mH all need converting to C, F and H. The trig table also gives 37° and 53° (the 3-4-5 triangle), which turn up in flux and force problems with angles.

Constants and conversions

Coulomb constant
k=14πε0=9.0×109 (N⋅m2)/C2\displaystyle k = \frac{1}{4\pi\varepsilon_0} = 9.0\times 10^{9}\ (\text{N}\cdot\text{m}^2)/\text{C}^2
The shortcut number in Coulomb's law, point-charge fields and potentials. Writing kk or 14πε0\frac{1}{4\pi\varepsilon_0} means the same thing.
Vacuum permittivity
ε0=8.85×10−12 C2/(N⋅m2)\displaystyle \varepsilon_0 = 8.85\times 10^{-12}\ \text{C}^2/(\text{N}\cdot\text{m}^2)
Shows up in Gauss's law, C=κε0AdC = \frac{\kappa\varepsilon_0 A}{d} and κ=εε0\kappa = \frac{\varepsilon}{\varepsilon_0}. It sets how strong the field from a given charge is in empty space.
Vacuum permeability
μ0=4π×10−7 (T⋅m)/A\displaystyle \mu_0 = 4\pi\times 10^{-7}\ (\text{T}\cdot\text{m})/\text{A}
The magnetic partner of ε0\varepsilon_0: it's in the Biot–Savart law, Ampère's law and the solenoid field. Leave the π\pi in until the end, since it often cancels.
Proton mass
mp=1.67×10−27 kg\displaystyle m_p = 1.67\times 10^{-27}\ \text{kg}
For a proton speeding up through a potential difference or circling in a magnetic field.
Neutron mass
mn=1.67×10−27 kg\displaystyle m_n = 1.67\times 10^{-27}\ \text{kg}
Rare in E&M since neutrons have no charge, but it helps when you need the mass of a nucleus or an ion.
Electron mass
me=9.11×10−31 kg\displaystyle m_e = 9.11\times 10^{-31}\ \text{kg}
For an electron accelerated by a field or bent by a magnetic field. It's about 1,800 times lighter than a proton, so it speeds up far more for the same energy.
Elementary charge
e=1.60×10−19 C\displaystyle e = 1.60\times 10^{-19}\ \text{C}
The size of the charge on one proton or electron. An electron's charge is −e-e, so remember the minus sign in ΔUE=qΔV\Delta U_E = q\Delta V and F⃗B=q(v⃗×B⃗)\vec{F}_B = q(\vec{v}\times\vec{B}).
Electron volt
1 eV=1.60×10−19 J\displaystyle 1\ \text{eV} = 1.60\times 10^{-19}\ \text{J}
The energy one elementary charge gains moving through 1 V. Handy for particle energies: an electron through 200 V gains 200 eV.
Speed of light
c=3.00×108 m/s\displaystyle c = 3.00\times 10^{8}\ \text{m/s}
Use it to check that a particle's speed is reasonable. The sheet doesn't print this, but cc also links ε0\varepsilon_0 and μ0\mu_0: c=1μ0ε0c = \frac{1}{\sqrt{\mu_0\varepsilon_0}}.
Unified atomic mass unit
1 u=1.66×10−27 kg=931 MeV/c2\displaystyle 1\ \text{u} = 1.66\times 10^{-27}\ \text{kg} = 931\ \text{MeV}/c^2
Converts an ion's or nucleus's mass from u to kg before you use it in a force or energy equation.
Universal gravitational constant
G=6.67×10−11 m3/(kg⋅s2)=6.67×10−11 N⋅m2/kg2\displaystyle G = 6.67\times 10^{-11}\ \text{m}^3/(\text{kg}\cdot\text{s}^2) = 6.67\times 10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2
Comes up when you compare gravity between two particles with the electric force between them; the electric force usually wins by a huge factor.
Acceleration due to gravity at Earth's surface
g=9.8 m/s2\displaystyle g = 9.8\ \text{m/s}^2
For a charged object that also has weight, like a charged drop held still between parallel plates where qE=mgqE = mg.
Gravitational field strength at Earth's surface
g=9.8 N/kg\displaystyle g = 9.8\ \text{N/kg}
The same number as above, written as force per kilogram. It's the gravity version of an electric field, which is force per coulomb.

Electric force and field

How charges push and pull, and the field that describes that push at every point.

Coulomb's law

∣F⃗E∣=14πε0∣q1q2∣r2=k∣q1q2∣r2\displaystyle \lvert \vec{F}_E \rvert = \frac{1}{4\pi\varepsilon_0}\frac{\lvert q_1 q_2 \rvert}{r^2} = k\frac{\lvert q_1 q_2 \rvert}{r^2}

What the symbols mean

∣F⃗E∣\lvert \vec{F}_E \rvert
size of the electric force each charge puts on the other
Unit: N
q1,q2q_1, q_2
the two point charges
Unit: C
rr
distance between the charges, center to center
Unit: m
ε0\varepsilon_0
vacuum permittivity
Unit: C²/(N·m²)
kk
Coulomb constant, 14πε0\frac{1}{4\pi\varepsilon_0}
Unit: N·m²/C²

Use it when: Two point charges (or charged spheres) and their separation are given, and you want the force between them. The absolute values give you only the size; like charges repel and opposite charges attract.

Watch out: Forgetting to square rr, or forgetting to turn μC into C. With charged spheres, rr is the distance between their centers, not between their surfaces.

Try it: A 2.0 μC charge and a −3.0 μC charge are 0.30 m apart. How big is the force between them?

Answer: F=(9.0×109)(2.0×10−6)(3.0×10−6)(0.30)2=0.60F = (9.0\times 10^{9})\frac{(2.0\times 10^{-6})(3.0\times 10^{-6})}{(0.30)^2} = 0.60 N. The charges are opposite, so it's attractive.

Learn it: 8.1 Electric Charge and Electric Force

Electric field from force

E⃗=F⃗Eq\displaystyle \vec{E} = \frac{\vec{F}_E}{q}

What the symbols mean

E⃗\vec{E}
electric field at a point
Unit: N/C (same as V/m)
F⃗E\vec{F}_E
electric force on a charge placed at that point
Unit: N
qq
the charge feeling the force (the test charge)
Unit: C

Use it when: You know the force on a charge and want the field, or you know the field and want the force, F⃗E=qE⃗\vec{F}_E = q\vec{E}.

Watch out: Forgetting that a negative charge feels a force opposite to the field. The field's direction is always the direction of the force on a positive charge.

Learn it: 8.3 Electric Fields

Electric field of a continuous charge

E⃗=14πε0∫dqr2r^\displaystyle \vec{E} = \frac{1}{4\pi\varepsilon_0}\int \frac{dq}{r^2}\hat{r}

What the symbols mean

dqdq
a tiny piece of the charge
Unit: C
rr
distance from that piece to the point where you want the field
Unit: m
r^\hat{r}
unit vector pointing from the piece toward that point
Unit: none

Use it when: Charge is spread along a rod, ring or arc and you need the field at a point. Write dqdq using a charge density, like dq=λ dxdq = \lambda\,dx, then integrate.

Watch out: Integrating the field's size without splitting it into components. Use symmetry to see which components cancel, and only integrate the one that's left.

Learn it: 8.4 Electric Fields of Charge Distributions

Flux and Gauss's law

How much field passes through a surface, and how that's tied to the charge inside a closed one.

Electric flux

ΦE=∫E⃗⋅dA⃗\displaystyle \Phi_E = \int \vec{E}\cdot d\vec{A}

What the symbols mean

ΦE\Phi_E
electric flux through the surface
Unit: N·m²/C
E⃗\vec{E}
electric field at each bit of the surface
Unit: N/C
dA⃗d\vec{A}
a tiny piece of area, as a vector pointing straight out of the surface
Unit: m²

Use it when: You want how much field passes through a surface. For a uniform field and a flat surface it becomes ΦE=EAcos⁡θ\Phi_E = EA\cos\theta.

Watch out: Measuring θ\theta from the surface instead of from the area vector, which sticks straight out of the surface. Field running along a surface gives zero flux.

Learn it: 8.5 Electric Flux

Gauss's law

∮E⃗⋅dA⃗=qencε0\displaystyle \oint \vec{E}\cdot d\vec{A} = \frac{q_{\text{enc}}}{\varepsilon_0}

What the symbols mean

∮\oint
integral over a closed surface (the Gaussian surface)
Unit: none
dA⃗d\vec{A}
a tiny piece of the closed surface, pointing outward
Unit: m²
qencq_{\text{enc}}
net charge inside the closed surface
Unit: C
ε0\varepsilon_0
vacuum permittivity
Unit: C²/(N·m²)

Use it when: Charge has spherical, cylindrical or flat-sheet symmetry and you want the field. Pick a surface where EE is constant and straight through it, so the left side becomes EE times an area.

Watch out: Using all the charge instead of only the charge inside your Gaussian surface. Charges outside still change the field, but add nothing to the net flux.

Try it: A closed surface surrounds a 4.0 nC charge. What's the total electric flux through it?

Answer: ΦE=qencε0=4.0×10−98.85×10−12≈4.5×102\Phi_E = \frac{q_{\text{enc}}}{\varepsilon_0} = \frac{4.0\times 10^{-9}}{8.85\times 10^{-12}} \approx 4.5\times 10^{2} N·m²/C, whatever the surface's shape.

Learn it: 8.6 Gauss’s Law

Total charge from a charge density

Qtotal=∫ρ(r) dV\displaystyle Q_{\text{total}} = \int \rho(r)\,dV

What the symbols mean

QtotalQ_{\text{total}}
total charge in the region
Unit: C
ρ(r)\rho(r)
volume charge density, which can change with distance r from the center (here ρ is charge density, not resistivity)
Unit: C/m³
dVdV
a tiny piece of volume (here V is volume, not potential)
Unit: m³

Use it when: A sphere or cylinder's charge density changes with rr and you need the enclosed charge for Gauss's law. For a sphere, use thin shells, dV=4πr2 drdV = 4\pi r^2\,dr.

Watch out: Multiplying ρ\rho by the whole volume when ρ\rho isn't constant. If it depends on rr, you have to integrate shell by shell.

Learn it: 8.4 Electric Fields of Charge Distributions · 8.6 Gauss’s Law

Electric potential and energy

Energy stored in arrangements of charge, and potential, which is that energy per coulomb.

Potential energy of two point charges

UE=14πε0q1q2r\displaystyle U_E = \frac{1}{4\pi\varepsilon_0}\frac{q_1 q_2}{r}

What the symbols mean

UEU_E
electric potential energy of the pair
Unit: J
q1,q2q_1, q_2
the two charges, with their signs
Unit: C
rr
distance between them
Unit: m

Use it when: You want the energy stored in a pair of charges, or the work needed to bring them together from far away. For several charges, add up UEU_E for every pair.

Watch out: Dropping the signs. Unlike Coulomb's law there are no absolute values here: opposite charges give negative UEU_E. The zero is when the charges are infinitely far apart.

Learn it: 9.1 Electric Potential Energy

Electric potential of a continuous charge

V=14πε0∫dqr\displaystyle V = \frac{1}{4\pi\varepsilon_0}\int \frac{dq}{r}

What the symbols mean

VV
electric potential at a point (here V is potential, not volume)
Unit: V (J/C)
dqdq
a tiny piece of the charge, with its sign
Unit: C
rr
distance from that piece to the point
Unit: m

Use it when: Charge is spread over a rod, ring or disk and you want the potential at a point. For one point charge it's just V=14πε0qrV = \frac{1}{4\pi\varepsilon_0}\frac{q}{r}.

Watch out: Treating potential like a vector and canceling parts by symmetry. Potential is a plain number, so every piece adds; only the signs of the charges can cancel.

Learn it: 9.2 Electric Potential

Potential difference from the field

ΔV=−∫abE⃗⋅dr⃗\displaystyle \Delta V = -\int_a^b \vec{E}\cdot d\vec{r}

What the symbols mean

ΔV\Delta V
change in potential going from point a to point b, Vb−VaV_b - V_a
Unit: V
E⃗\vec{E}
electric field along the path
Unit: N/C
dr⃗d\vec{r}
a tiny step along the path from a to b
Unit: m

Use it when: You know the field (often from Gauss's law) and want the potential difference between two points, like the plates of a capacitor. In a uniform field it becomes ∣ΔV∣=Ed\lvert\Delta V\rvert = Ed.

Watch out: Losing the minus sign. Moving along the field always takes you to lower potential, so check that your sign agrees.

Learn it: 9.2 Electric Potential · 10.3 Capacitors

Field from the slope of potential

Ex=−dVdx\displaystyle E_x = -\frac{dV}{dx}

What the symbols mean

ExE_x
x-component of the electric field
Unit: V/m (same as N/C)
dVdx\frac{dV}{dx}
how fast the potential changes with position
Unit: V/m

Use it when: You have VV as a function of xx, or a graph of VV against xx, and want the field. The field is the negative slope.

Watch out: Thinking E=0E = 0 wherever V=0V = 0. The field depends on how steeply VV changes, not on the value of VV itself.

Learn it: 9.2 Electric Potential

Change in potential energy across a potential difference

ΔUE=qΔV\displaystyle \Delta U_E = q\Delta V

What the symbols mean

ΔUE\Delta U_E
change in electric potential energy
Unit: J
qq
the moving charge, with its sign
Unit: C
ΔV\Delta V
change in potential it moves through
Unit: V

Use it when: A charge moves between two points at different potentials and you want its energy change or its speed. With no other forces doing work, ΔK=−ΔUE\Delta K = -\Delta U_E.

Watch out: Dropping the sign of an electron's charge. Electrons gain kinetic energy moving toward higher potential, the opposite of positive charges.

Try it: An electron starts at rest at 0 V and moves to a point at +200 V. How does its potential energy change?

Answer: ΔUE=qΔV=(−1.60×10−19)(200)=−3.2×10−17\Delta U_E = q\Delta V = (-1.60\times 10^{-19})(200) = -3.2\times 10^{-17} J, so it gains 3.2×10−173.2\times 10^{-17} J (200 eV) of kinetic energy.

Learn it: 9.3 Conservation of Electric Energy

Capacitors and dielectrics

Devices that store charge and energy, and what filling them with an insulator does.

Capacitance

C=QΔV\displaystyle C = \frac{Q}{\Delta V}

What the symbols mean

CC
capacitance
Unit: F (C/V)
QQ
size of the charge on either plate
Unit: C
ΔV\Delta V
potential difference between the plates
Unit: V

Use it when: Any two of charge, voltage and capacitance are given and you want the third. To find CC for spherical or cylindrical capacitors, use Gauss's law for EE, integrate for ΔV\Delta V, then divide.

Watch out: Thinking CC changes when you change QQ or ΔV\Delta V. It depends only on the geometry and what's between the plates; QQ and ΔV\Delta V rise together.

Learn it: 10.3 Capacitors

Parallel-plate capacitance

C=κε0Ad\displaystyle C = \frac{\kappa\varepsilon_0 A}{d}

What the symbols mean

κ\kappa
dielectric constant of the material between the plates (1.0 for air)
Unit: none
AA
area of one plate
Unit: m²
dd
gap between the plates
Unit: m

Use it when: You're given plate area, gap and filling, and want the capacitance, or you're asked what happens when the plates move or a dielectric slides in.

Watch out: Not converting units: 1 cm² is 1×10−41\times 10^{-4} m² and 1 mm is 1×10−31\times 10^{-3} m. Small slips here throw the answer off by powers of ten.

Try it: Air-filled plates of area 0.010 m² sit 1.0 mm apart and are connected to a 12 V battery. Find the capacitance and the charge.

Answer: C=(1.0)(8.85×10−12)(0.010)1.0×10−3≈8.9×10−11C = \frac{(1.0)(8.85\times 10^{-12})(0.010)}{1.0\times 10^{-3}} \approx 8.9\times 10^{-11} F (about 89 pF), and Q=CΔV≈1.1×10−9Q = C\Delta V \approx 1.1\times 10^{-9} C.

Learn it: 10.3 Capacitors · 10.4 Dielectrics

Energy stored in a capacitor

UC=12QΔV\displaystyle U_C = \frac{1}{2}Q\Delta V

What the symbols mean

UCU_C
energy stored in the capacitor
Unit: J
QQ
charge on either plate
Unit: C
ΔV\Delta V
potential difference across it
Unit: V

Use it when: You want the energy a charged capacitor holds. Swap in Q=CΔVQ = C\Delta V to get the other forms, Q22C\frac{Q^2}{2C} and 12C(ΔV)2\frac{1}{2}C(\Delta V)^2.

Watch out: Forgetting the 12\frac{1}{2}. The battery does QΔVQ\Delta V of work, but only half ends up stored in the capacitor.

Learn it: 10.3 Capacitors

Dielectric constant

κ=εε0\displaystyle \kappa = \frac{\varepsilon}{\varepsilon_0}

What the symbols mean

κ\kappa
dielectric constant
Unit: none
ε\varepsilon
electric permittivity of the material (not emf here)
Unit: C²/(N·m²)
ε0\varepsilon_0
permittivity of empty space
Unit: C²/(N·m²)

Use it when: You're told a material's permittivity and need its dielectric constant, or the reverse. Filling the gap between a capacitor's plates with a dielectric multiplies its CC by κ\kappa.

Watch out: Mixing this ε\varepsilon up with emf. The sheet uses the same-looking letter for both: in this equation it's permittivity, a property of a material.

Learn it: 10.4 Dielectrics

Current and resistance

Charge on the move, what resists it, and the power it delivers.

Current

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

What the symbols mean

II
current
Unit: A (C/s)
dqdt\frac{dq}{dt}
rate charge flows past a point
Unit: C/s

Use it when: You know how charge changes with time and want the current, or you integrate a current to find the charge that flowed.

Watch out: Getting the direction wrong. Current points the way positive charges would drift, which is opposite to the electrons actually moving in a wire.

Learn it: 11.1 Electric Current

Current from current density

I=∫J⃗⋅dA⃗\displaystyle I = \int \vec{J}\cdot d\vec{A}

What the symbols mean

J⃗\vec{J}
current density, current per unit area
Unit: A/m²
dA⃗d\vec{A}
a tiny piece of the wire's cross section
Unit: m²

Use it when: Current isn't spread evenly across a wire, so JJ depends on rr, and you want the total current. Use rings of area dA=2πr drdA = 2\pi r\,dr.

Watch out: Multiplying JJ by πR2\pi R^2 when JJ changes across the wire. That only works when JJ is the same everywhere.

Learn it: 11.1 Electric Current

Field and current density in a material

E⃗=ρJ⃗\displaystyle \vec{E} = \rho\vec{J}

What the symbols mean

E⃗\vec{E}
electric field inside the conductor
Unit: V/m
ρ\rho
resistivity of the material (here ρ is resistivity, not charge density)
Unit: Ω·m
J⃗\vec{J}
current density
Unit: A/m²

Use it when: You want the field that drives current in a wire, or the current density a field produces. It's Ohm's law written for one point in a material.

Watch out: Reading ρ\rho as charge density. In this equation, and in R=ρℓAR = \frac{\rho\ell}{A}, it's resistivity.

Learn it: 11.3 Resistance, Resistivity, and Ohm’s Law

Resistance from resistivity

R=ρℓA\displaystyle R = \frac{\rho\ell}{A}

What the symbols mean

RR
resistance
Unit: Ω
ρ\rho
resistivity of the material
Unit: Ω·m
ℓ\ell
length of the wire
Unit: m
AA
cross-sectional area of the wire
Unit: m²

Use it when: You're given a wire's material, length and thickness and want its resistance, or asked how resistance changes if you stretch or thicken it.

Watch out: Using the diameter in A=πr2A = \pi r^2. Halve the diameter first, and convert mm to m.

Try it: A copper wire (ρ=1.7×10−8\rho = 1.7\times 10^{-8} Ω·m) is 10 m long with a cross section of 1.0×10−61.0\times 10^{-6} m². Find its resistance.

Answer: R=(1.7×10−8)(10)1.0×10−6=0.17R = \frac{(1.7\times 10^{-8})(10)}{1.0\times 10^{-6}} = 0.17 Ω.

Learn it: 11.3 Resistance, Resistivity, and Ohm’s Law

Ohm's law

I=ΔVR\displaystyle I = \frac{\Delta V}{R}

What the symbols mean

II
current through the element
Unit: A
ΔV\Delta V
potential difference across that same element
Unit: V
RR
its resistance
Unit: Ω

Use it when: Any two of current, voltage and resistance for one resistor (or a whole circuit's equivalent) are known and you want the third. The sheet assumes resistors and bulbs are ohmic.

Watch out: Using the battery's voltage across one resistor that shares the circuit with others. Use the voltage across that resistor only.

Learn it: 11.3 Resistance, Resistivity, and Ohm’s Law

Electric power

P=IΔV\displaystyle P = I\Delta V

What the symbols mean

PP
rate energy is delivered or used
Unit: W
II
current through the element
Unit: A
ΔV\Delta V
potential difference across it
Unit: V

Use it when: You want the power a resistor uses, a battery supplies, or how bright a bulb is. For a resistor, combine with Ohm's law: P=I2R=(ΔV)2RP = I^2R = \frac{(\Delta V)^2}{R}.

Watch out: Mixing the current through one element with the voltage across a different one. Both must belong to the same element.

Learn it: 11.4 Electric Power

Combining resistors and capacitors

Shrinking a circuit to one equivalent element, and how fast an RC circuit changes.

Resistors in series

Req,s=∑iRi\displaystyle R_{\text{eq},s} = \sum_i R_i

What the symbols mean

Req,sR_{\text{eq},s}
equivalent resistance of resistors in series
Unit: Ω
RiR_i
each resistor's resistance
Unit: Ω

Use it when: Resistors sit one after another on a single path, so they carry the same current. The total is always bigger than any one of them.

Watch out: Calling resistors in series just because they're drawn in a line. They're in series only if no branch splits off between them.

Learn it: 11.5 Compound Direct Current Circuits

Resistors in parallel

1Req,p=∑i1Ri\displaystyle \frac{1}{R_{\text{eq},p}} = \sum_i \frac{1}{R_i}

What the symbols mean

Req,pR_{\text{eq},p}
equivalent resistance of resistors in parallel
Unit: Ω
RiR_i
each resistor's resistance
Unit: Ω

Use it when: Resistors connect across the same two points, so they share the same potential difference. The total is always smaller than the smallest one.

Watch out: Forgetting to flip at the end. The sum gives 1Req,p\frac{1}{R_{\text{eq},p}}, so take the reciprocal before you report it.

Try it: A 6.0 Ω and a 3.0 Ω resistor are in parallel, and that pair is in series with a 4.0 Ω resistor across a 12 V battery. Find the current from the battery.

Answer: 1Req,p=16.0+13.0\frac{1}{R_{\text{eq},p}} = \frac{1}{6.0} + \frac{1}{3.0}, so Req,p=2.0R_{\text{eq},p} = 2.0 Ω. The total is 2.0+4.0=6.02.0 + 4.0 = 6.0 Ω, so I=126.0=2.0I = \frac{12}{6.0} = 2.0 A.

Learn it: 11.5 Compound Direct Current Circuits

Capacitors in series

1Ceq,s=∑i1Ci\displaystyle \frac{1}{C_{\text{eq},s}} = \sum_i \frac{1}{C_i}

What the symbols mean

Ceq,sC_{\text{eq},s}
equivalent capacitance of capacitors in series
Unit: F
CiC_i
each capacitor's capacitance
Unit: F

Use it when: Capacitors sit one after another on a single path; each holds the same charge. The total is smaller than the smallest one.

Watch out: Using the resistor rules. Capacitors combine the opposite way: series uses reciprocals, parallel just adds.

Learn it: 11.8 Resistor-Capacitor (RC) Circuits

Capacitors in parallel

Ceq,p=∑iCi\displaystyle C_{\text{eq},p} = \sum_i C_i

What the symbols mean

Ceq,pC_{\text{eq},p}
equivalent capacitance of capacitors in parallel
Unit: F
CiC_i
each capacitor's capacitance
Unit: F

Use it when: Capacitors connect across the same two points, so they share the same potential difference. Adding one is like making the plates bigger.

Watch out: Assuming parallel capacitors hold the same charge. They have the same voltage; the bigger capacitor holds more charge.

Learn it: 11.8 Resistor-Capacitor (RC) Circuits

Time constant of an RC circuit

τ=ReqCeq\displaystyle \tau = R_{\text{eq}}C_{\text{eq}}

What the symbols mean

τ\tau
time constant (not torque here)
Unit: s
ReqR_{\text{eq}}
equivalent resistance the capacitor charges or discharges through
Unit: Ω
CeqC_{\text{eq}}
equivalent capacitance
Unit: F

Use it when: You want how quickly a capacitor charges or discharges. After one τ\tau, a charging capacitor has about 63% of its final charge, and a discharging one keeps about 37%.

Watch out: Using the wrong resistance. Use only the resistance in the path the charge actually flows through, which can be different for charging and discharging.

Learn it: 11.8 Resistor-Capacitor (RC) Circuits

Magnetic fields and forces

Forces on moving charges and currents, and the fields that currents make.

Gauss's law for magnetism

∮B⃗⋅dA⃗=0\displaystyle \oint \vec{B}\cdot d\vec{A} = 0

What the symbols mean

B⃗\vec{B}
magnetic field
Unit: T
dA⃗d\vec{A}
a tiny piece of a closed surface, pointing outward
Unit: m²

Use it when: Explaining why magnetic field lines form closed loops and why there are no lone north or south poles: every line that leaves a closed surface comes back in.

Watch out: Applying the zero to an open surface. Only the net flux through a closed surface is zero; flux through a single loop of wire usually isn't.

Learn it: 12.1 Magnetic Fields

Magnetic force on a moving charge

F⃗B=q(v⃗×B⃗)\displaystyle \vec{F}_B = q\left(\vec{v}\times\vec{B}\right)

What the symbols mean

F⃗B\vec{F}_B
magnetic force on the charge
Unit: N
qq
the charge, with its sign
Unit: C
v⃗\vec{v}
velocity of the charge
Unit: m/s
B⃗\vec{B}
magnetic field
Unit: T

Use it when: A charge moves through a magnetic field and you want the force, its direction, or the radius of its circular path. The size is qvBsin⁡θqvB\sin\theta.

Watch out: Forgetting to flip the right-hand-rule answer for a negative charge like an electron.

Learn it: 12.2 Magnetism and Moving Charges

Biot–Savart law

dB⃗=μ04πI(dℓ⃗×r^)r2\displaystyle d\vec{B} = \frac{\mu_0}{4\pi}\frac{I\left(d\vec{\ell}\times\hat{r}\right)}{r^2}

What the symbols mean

dB⃗d\vec{B}
field made by one tiny piece of wire
Unit: T
μ0\mu_0
vacuum permeability
Unit: T·m/A
II
current in the wire
Unit: A
dℓ⃗d\vec{\ell}
a tiny piece of wire, pointing the way the current flows
Unit: m
r^\hat{r}
unit vector from that piece to the point where you want the field
Unit: none
rr
distance from the piece to that point
Unit: m

Use it when: You want the field from a current in a shape without enough symmetry for Ampère's law, like the center of a loop or arc, or a point near a short wire.

Watch out: Forgetting that the cross product is zero when dℓ⃗d\vec{\ell} and r^\hat{r} point the same way. Pieces of wire lined up with the point add no field there.

Learn it: 12.3 Magnetic Fields of Current-Carrying Wires and the Biot-Savart Law

Magnetic force on a current-carrying wire

F⃗B=∫I(dℓ⃗×B⃗)\displaystyle \vec{F}_B = \int I\left(d\vec{\ell}\times\vec{B}\right)

What the symbols mean

F⃗B\vec{F}_B
magnetic force on the wire
Unit: N
II
current in the wire
Unit: A
dℓ⃗d\vec{\ell}
a tiny piece of wire, pointing the way the current flows
Unit: m
B⃗\vec{B}
magnetic field at that piece
Unit: T

Use it when: A current-carrying wire sits in a magnetic field and you want the force on it. For a straight wire in a uniform field, the size is IℓBsin⁡θI\ell B\sin\theta.

Watch out: Using the whole wire's length when only part of it is in the field. Only the length inside the field feels a force.

Learn it: 12.3 Magnetic Fields of Current-Carrying Wires and the Biot-Savart Law · 13.3 Induced Currents and Magnetic Forces

Ampère's law

∮B⃗⋅dℓ⃗=μ0Ienc\displaystyle \oint \vec{B}\cdot d\vec{\ell} = \mu_0 I_{\text{enc}}

What the symbols mean

∮\oint
integral around a closed path (the Amperian loop)
Unit: none
dℓ⃗d\vec{\ell}
a tiny step along the loop
Unit: m
IencI_{\text{enc}}
net current passing through the loop
Unit: A

Use it when: Current has a lot of symmetry (a long straight wire, a thick wire, a coaxial cable, a solenoid) and you want the field. Choose a loop where BB is constant along it.

Watch out: Counting all the current instead of just the part that passes through your loop. Inside a thick wire, only the current inside radius rr counts.

Learn it: 12.4 Ampère’s Law

Field inside a long solenoid

Bsol=μ0nI\displaystyle B_{\text{sol}} = \mu_0 nI

What the symbols mean

BsolB_{\text{sol}}
field inside a long solenoid
Unit: T
nn
number of loops per unit length
Unit: 1/m
II
current in the wire
Unit: A

Use it when: You want the field inside a long coil. It's nearly uniform inside and about zero just outside.

Watch out: Plugging in the total number of loops NN. Here nn is loops per meter, n=Nℓn = \frac{N}{\ell}.

Try it: A long solenoid has 1,000 loops per meter and carries 2.0 A. What's the field inside?

Answer: B=(4π×10−7)(1000)(2.0)≈2.5×10−3B = (4\pi\times 10^{-7})(1000)(2.0) \approx 2.5\times 10^{-3} T.

Learn it: 12.4 Ampère’s Law

Induction and inductance

Changing magnetic flux makes an emf, and coils that push back against changing current.

Magnetic flux

ΦB=∫B⃗⋅dA⃗\displaystyle \Phi_B = \int \vec{B}\cdot d\vec{A}

What the symbols mean

ΦB\Phi_B
magnetic flux through the surface
Unit: T·m²
B⃗\vec{B}
magnetic field
Unit: T
dA⃗d\vec{A}
a tiny piece of area, pointing straight out of the surface
Unit: m²

Use it when: You want how much field passes through a loop, the first step of every induction problem. When the field is the same everywhere and the loop lies flat, ΦB=BAcos⁡θ\Phi_B = BA\cos\theta.

Watch out: Measuring θ\theta from the plane of the loop instead of from the line straight out of it.

Learn it: 13.1 Magnetic Flux

Faraday's law

ε=∮E⃗⋅dℓ⃗=−dΦBdt\displaystyle \varepsilon = \oint \vec{E}\cdot d\vec{\ell} = -\frac{d\Phi_B}{dt}

What the symbols mean

ε\varepsilon
induced emf around the loop (not permittivity here)
Unit: V
E⃗\vec{E}
induced electric field along the loop
Unit: V/m
dℓ⃗d\vec{\ell}
a tiny step around the loop
Unit: m
dΦBdt\frac{d\Phi_B}{dt}
rate the magnetic flux through the loop changes
Unit: T·m²/s (same as V)

Use it when: Flux through a loop changes because the field, the area, or the angle changes, and you want the emf or the induced current. The minus sign is Lenz's law: the emf opposes the change.

Watch out: Thinking a big steady flux makes an emf. Only a changing flux does; a strong field that stays put induces nothing.

Learn it: 13.2 Electromagnetic Induction

Emf in a coil of many loops

∣εsol∣=N∣dΦBdt∣\displaystyle \lvert \varepsilon_{\text{sol}} \rvert = N\left\lvert \frac{d\Phi_B}{dt} \right\rvert

What the symbols mean

εsol\varepsilon_{\text{sol}}
emf induced in the whole coil
Unit: V
NN
total number of loops
Unit: none
ΦB\Phi_B
flux through one loop
Unit: T·m²

Use it when: Flux changes through a coil with many turns and you want the size of the emf. Each loop adds its own emf, so the total is NN times one loop's.

Watch out: Forgetting the factor NN, or using flux through the whole coil and then multiplying by NN again. ΦB\Phi_B here is for one loop.

Try it: The flux through each loop of a 50-loop coil drops from 0.020 T·m² to zero in 0.10 s. What's the average emf?

Answer: ∣ε∣=NΔΦBΔt=50×0.0200.10=10\lvert\varepsilon\rvert = N\frac{\Delta\Phi_B}{\Delta t} = 50\times\frac{0.020}{0.10} = 10 V.

Learn it: 13.2 Electromagnetic Induction

Inductance of a solenoid

Lsol=μcoreN2Aℓ\displaystyle L_{\text{sol}} = \frac{\mu_{\text{core}}N^2 A}{\ell}

What the symbols mean

LsolL_{\text{sol}}
inductance of the solenoid
Unit: H
μcore\mu_{\text{core}}
magnetic permeability of the core inside the coil (μ₀ for an air or empty core)
Unit: T·m/A
NN
total number of loops
Unit: none
AA
cross-sectional area of the coil
Unit: m²
ℓ\ell
length of the coil
Unit: m

Use it when: You're given a coil's size, turns and core and want its inductance, or asked how inductance changes if you double the turns or add an iron core.

Watch out: Forgetting to square NN, or using nn (loops per meter) here. This equation uses the total number of loops.

Learn it: 13.4 Inductance

Energy stored in an inductor

UL=12LI2\displaystyle U_L = \frac{1}{2}LI^2

What the symbols mean

ULU_L
energy stored in the inductor's magnetic field
Unit: J
LL
inductance
Unit: H
II
current through it
Unit: A

Use it when: You want the energy an inductor holds, or you're tracking energy moving between an inductor and a capacitor or resistor.

Watch out: Forgetting to square the current. Doubling the current makes four times the energy.

Learn it: 13.4 Inductance · 13.6 Circuits with Capacitors and Inductors (LC Circuits)

Self-induced emf

ε=−LdIdt\displaystyle \varepsilon = -L\frac{dI}{dt}

What the symbols mean

ε\varepsilon
emf across the inductor
Unit: V
LL
inductance
Unit: H
dIdt\frac{dI}{dt}
rate the current changes
Unit: A/s

Use it when: Current through an inductor is changing and you want the voltage across it, or you're writing the loop rule for an LR or LC circuit.

Watch out: Thinking a big current means a big emf. The emf depends on how fast the current changes; a steady current gives zero.

Learn it: 13.4 Inductance · 13.5 Circuits with Resistors and Inductors (LR Circuits)

Time constant of an LR circuit

τ=LReq\displaystyle \tau = \frac{L}{R_{\text{eq}}}

What the symbols mean

τ\tau
time constant
Unit: s
LL
inductance
Unit: H
ReqR_{\text{eq}}
equivalent resistance in the inductor's path
Unit: Ω

Use it when: You want how quickly the current in an LR circuit rises or falls after a switch flips. After one τ\tau, a rising current is about 63% of its final value.

Watch out: Multiplying LL by RR the way you multiply RR by CC. For an LR circuit you divide: τ=LReq\tau = \frac{L}{R_{\text{eq}}}.

Learn it: 13.5 Circuits with Resistors and Inductors (LR Circuits)

Angular frequency of an LC circuit

ωLC=1LC\displaystyle \omega_{LC} = \frac{1}{\sqrt{LC}}

What the symbols mean

ωLC\omega_{LC}
angular frequency of the charge and current oscillation
Unit: rad/s
LL
inductance
Unit: H
CC
capacitance
Unit: F

Use it when: A charged capacitor is connected to an inductor and you want how fast energy sloshes back and forth. The period is T=2πωLCT = \frac{2\pi}{\omega_{LC}}.

Watch out: Reporting ω\omega as the frequency in Hz. Divide by 2π2\pi to get ff: for L=10L = 10 mH and C=1.0C = 1.0 μF, ω=1.0×104\omega = 1.0\times 10^{4} rad/s but f≈1.6×103f \approx 1.6\times 10^{3} Hz.

Learn it: 13.6 Circuits with Capacitors and Inductors (LC Circuits)

Pages shared with another sheet

  • Mechanics

    The E&M booklet reprints the full Mechanics page from the Physics C: Mechanics sheet. You'll use it here for forces on charges, energy conservation, circular motion of charges in magnetic fields, Newton's second law for a sliding bar in a field, and the oscillation equations that match LC circuits.

    Physics C: Mechanics equation sheet, explained →

  • Geometry, trigonometry, vectors, calculus and identities

    The last page matches the Mechanics sheet too. Its dot and cross products are what you need for flux, E⃗⋅dA⃗\vec{E}\cdot d\vec{A} and B⃗⋅dA⃗\vec{B}\cdot d\vec{A}, and for magnetic force, v⃗×B⃗\vec{v}\times\vec{B}, and its derivative and integral rules cover RC and LR circuits.

    Geometry, vectors and calculus, explained →

Not on the sheet: know these

The exam expects you to know these without being given them.

  • Kirchhoff's loop rule

    ∑ΔV=0\displaystyle \sum \Delta V = 0

    The potential differences around any closed loop add to zero. It's how you write equations for unknown currents, and for the differential equations of RC and LR circuits.

    Learn it: 11.6 Kirchhoff’s Loop Rule

  • Kirchhoff's junction rule

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

    Current into a junction equals current out, since charge can't pile up. Together with the loop rule it solves multi-loop circuits.

    Learn it: 11.7 Kirchhoff’s Junction Rule

  • Charging and discharging a capacitor

    q(t)=Qmax(1−e−t/τ),q(t)=Q0e−t/τ\displaystyle q(t) = Q_{\text{max}}\left(1 - e^{-t/\tau}\right),\quad q(t) = Q_0 e^{-t/\tau}

    The sheet gives only τ=ReqCeq\tau = R_{\text{eq}}C_{\text{eq}}. You need these exponentials (and the matching current, which decays as e−t/τe^{-t/\tau} in both cases) to find charge or current at a given time.

    Learn it: 11.8 Resistor-Capacitor (RC) Circuits

  • Current growing in an LR circuit

    I(t)=εR(1−e−t/τ)\displaystyle I(t) = \frac{\varepsilon}{R}\left(1 - e^{-t/\tau}\right)

    After a switch closes, current rises toward εR\frac{\varepsilon}{R} with τ=LR\tau = \frac{L}{R}; when the battery is removed it decays as e−t/τe^{-t/\tau}. You get it by solving the loop rule.

    Learn it: 13.5 Circuits with Resistors and Inductors (LR Circuits)

  • Capacitors and inductors right after a switch and after a long time

    An uncharged capacitor acts like a wire at first and like a break after a long time. An inductor does the opposite: a break at first (no sudden change in current), a plain wire after a long time. Many circuit questions only need these two snapshots.

    Learn it: 11.8 Resistor-Capacitor (RC) Circuits · 13.5 Circuits with Resistors and Inductors (LR Circuits)

  • Field of a long straight wire

    B=μ0I2πr\displaystyle B = \frac{\mu_0 I}{2\pi r}

    The sheet doesn't list it; you get it from Ampère's law with a circular loop. Field lines circle the wire, with direction from the right-hand rule.

    Learn it: 12.3 Magnetic Fields of Current-Carrying Wires and the Biot-Savart Law · 12.4 Ampère’s Law

  • Lenz's law

    The induced current makes a magnetic field that opposes the change in flux. The sheet shows it only as a minus sign in Faraday's law; you need it to find the direction of induced current.

    Learn it: 13.2 Electromagnetic Induction · 13.3 Induced Currents and Magnetic Forces

  • Motional emf

    ε=Bℓv\displaystyle \varepsilon = B\ell v

    A bar of length ℓ\ell sliding at speed vv through a perpendicular field has this emf. It comes from Faraday's law, and it's the start of every sliding-bar-on-rails problem.

    Learn it: 13.3 Induced Currents and Magnetic Forces

  • Conductors in electrostatic equilibrium

    Inside a conductor the field is zero, any extra charge sits on its surface, the field just outside is perpendicular to the surface, and the whole conductor is at one potential. Gauss's law problems with conducting shells depend on this.

    Learn it: 8.3 Electric Fields · 10.1 Electrostatics with Conductors · 10.2 Redistribution of Charge Between Conductors

  • Other forms of power and capacitor energy

    P=I2R=(ΔV)2R,UC=Q22C=12C(ΔV)2\displaystyle P = I^2R = \frac{(\Delta V)^2}{R},\quad U_C = \frac{Q^2}{2C} = \frac{1}{2}C(\Delta V)^2

    The sheet gives only P=IΔVP = I\Delta V and UC=12QΔVU_C = \frac{1}{2}Q\Delta V. These come from swapping in Ohm's law or Q=CΔVQ = C\Delta V, and save time when one quantity is missing.

    Learn it: 10.3 Capacitors · 11.4 Electric Power