AP Physics 2 Equation & Formula Sheet 2027
Search 138 physics relationships with every variable, SI unit, model condition and physical example kept together. Use this page as a reference and equation-selection guide—not as a memorization list.
What is on the AP Physics 2 formula sheet?
This reference contains 138 equations, proportional relationships and model statements spanning all 46 topics. It also includes commonly used constants, SI unit symbols, model assumptions and a searchable unit filter so you can move from a question cue to the correct physical relationship.
Choose a model before you choose an equation
The strongest equation choice starts from the physical situation, not from matching symbols.
Name the target
What quantity or comparison is the question asking for?
Choose the model
Gas, field, circuit, magnetic force, ray, wave, photon or nucleus?
Check conditions
Read what must be true before using the relationship.
Verify the result
Check units, sign, magnitude and limiting behavior.
Equation sheet, formula sheet and reference sheet are one resource here
Those phrases usually describe the same study need. Keeping them on one canonical page prevents duplicate content and gives you one complete reference instead of three thinner pages.
Important: this is an independent study reference, not a reproduction of the official exam reference sheet. The 138 entries include derived relationships and qualitative model statements as well as equations; use the reference information provided with the actual exam when simulating exam-day conditions.
Know where the relationship lives before searching
The counts below include equations and explicit model relationships used on the 46 topic lessons.
gas models · heat transfer · thermodynamic laws · entropy
Unit 10Electric Force, Field, and Potential21charge · force · electric field · potential · capacitance · electric energy
Unit 11Electric Circuits24current · resistance · power · series/parallel networks · Kirchhoff rules · RC transients
Unit 12Magnetism and Electromagnetism12magnetic force · fields from current · flux · induction
Unit 13Geometric Optics12reflection · refraction · mirror/lens equations · magnification
Unit 14Waves, Sound, and Physical Optics27wave speed · Doppler · standing waves · diffraction · interference · thin films
Unit 15Modern Physics24photons · matter waves · spectra · blackbody radiation · photoelectric effect · Compton scattering · nuclear energy · decay
Common values worth recognizing instantly
Keep the symbol, value and unit together; convert units before substitution.
| Constant / value | Symbol | Value | Use |
|---|---|---|---|
| Avogadro constant | NA | 6.02 × 1023 mol−1 | moles ↔ particles |
| Universal gas constant | R | 8.31 J mol−1 K−1 | macroscopic ideal-gas law |
| Boltzmann constant | kB | 1.38 × 10−23 J K−1 | microscopic thermal energy |
| Atmospheric pressure | 1 atm | 1.0 × 105 Pa | gas-state conversions |
| Coulomb constant | ke | 8.99 × 109 N·m²/C² | point-charge force, field and potential |
| Proton mass | mp | 1.67 × 10−27 kg | atomic and nuclear mass |
| Neutron mass | mn | 1.67 × 10−27 kg | nuclear mass |
| Electron mass | me | 9.11 × 10−31 kg | electron dynamics and modern physics |
| Elementary charge magnitude | e | 1.60 × 10−19 C | charge quantization |
| Vacuum permittivity | ε0 | 8.85 × 10−12 C²/(N·m²) | electric-field and capacitance models |
| Vacuum permeability | μ0 | 4π × 10−7 T·m/A | magnetic-field models |
| Electron volt | 1 eV | 1.60 × 10−19 J | atomic, photon and nuclear energy |
| Planck constant | h | 6.63 × 10−34 J·s | photon and matter-wave relationships |
| Speed of light | c | 3.00 × 108 m/s | electromagnetic waves and photons |
| Wien constant | b | 2.90 × 10−3 m·K | blackbody peak wavelength |
| Stefan–Boltzmann constant | σ | 5.67 × 10−8 W·m−2·K−4 | blackbody radiated power |
| Unified atomic mass unit | 1 u | 1.66 × 10−27 kg | nuclear mass and mass defect |
| Universal gravitational constant | G | 6.67 × 10−11 N·m²/kg² | mechanics connections |
| Gravitational field near Earth | g | 9.8 N/kg = 9.8 m/s² | mechanics connections and experiments |
Small words can change the equation
Before solving, look for idealizations that make a relationship valid.
Common default assumptions
- Use an inertial reference frame unless a problem says otherwise.
- Treat wires, meters, batteries and similar components as ideal when the model calls for it.
- Use conventional current direction in circuit reasoning.
- Use Kelvin for absolute-temperature relationships.
- For an isolated point charge, define electric potential relative to zero at infinite separation.
Questions that should stop you before substitution
- Is the gas ideal and is the process specified?
- Is the resistor ohmic?
- Is the magnetic force perpendicular to velocity or current?
- Is the optical sign convention consistent?
- Does the interference condition require a phase-change check?
- Is the equation about amplitude, intensity, energy or probability?
Search all 138 relationships
Search by equation, concept, variable, topic, physical example or use condition. Filter by unit or jump from the unit map above.
Kinetic Theory of Temperature and Pressure
P = F⊥/AVariables & SI units: P pressure (Pa); F⊥ total perpendicular force on the surface (N); A surface area (m²)
Use when: macroscopic pressure from the perpendicular force exerted on a surface
A gas exerts 600 N perpendicular to a 0.020 m² wall, so P = 30 kPa.
Kinetic Theory of Temperature and Pressure
K_avg = (3/2)k_B T = (1/2)m v_rms²Variables & SI units: K_avg average translational kinetic energy per particle (J); k_B Boltzmann constant (J/K); T absolute temperature (K); m particle mass (kg); v_rms root-mean-square speed (m/s)
Use when: ideal monatomic-particle model relating temperature, average translational kinetic energy and rms speed
At the same temperature, lighter particles have a larger rms speed even though average translational kinetic energy is the same.
Kinetic Theory of Temperature and Pressure
Higher T → broader speed distribution with greater characteristic speedsInterpretation: T absolute temperature (K); graph horizontal axis molecular speed (m/s); vertical axis relative number/probability density
Use when: qualitative interpretation of a molecular-speed distribution; the exact functional form is not required
Heating a gas shifts the distribution toward higher speeds and spreads it over a wider range.
The Ideal Gas Law
PV = nRT = Nk_B TVariables & SI units: P pressure (Pa); V volume (m³); n amount (mol); R gas constant (J·mol⁻¹·K⁻¹); N particle count; k_B Boltzmann constant (J/K); T absolute temperature (K)
Use when: equilibrium states of an ideal gas
For fixed n and T, doubling V halves P.
The Ideal Gas Law
P₁V₁/T₁ = P₂V₂/T₂Variables & SI units: P₁,P₂ pressure (Pa); V₁,V₂ volume (m³); T₁,T₂ absolute temperature (K)
Use when: derived comparison for the same fixed ideal-gas sample in two equilibrium states
A sealed flexible gas sample can be compared before and after simultaneous compression and heating.
The Ideal Gas Law
At fixed amount: P ∝ T/VVariables & SI units: P pressure (Pa); T absolute temperature (K); V volume (m³); amount of gas held fixed
Use when: proportional reasoning from the ideal gas law
At fixed V, a P-versus-T(K) graph is linear and extrapolates toward zero pressure at zero kelvin in the ideal model.
Thermal Energy Transfer and Equilibrium
T_hot > T_cold → spontaneous thermal transfer hot → coldInterpretation: T_hot and T_cold are temperatures (K or °C for ordering); arrow shows net direction of spontaneous thermal transfer
Use when: two systems in thermal contact at different temperatures
A hot metal block placed in cooler water transfers energy to the water until their temperatures approach one another.
Thermal Energy Transfer and Equilibrium
Thermal equilibrium: T_A = T_B and net thermal transfer = 0Interpretation: T_A,T_B temperatures of systems in thermal contact; net transfer is energy per time summed over thermal processes
Use when: systems in thermal contact after macroscopic temperatures become equal
Two samples can still exchange microscopic energy in both directions at equilibrium, but there is no net transfer.
Thermal Energy Transfer and Equilibrium
Thermal transfer modes: conduction + convection + radiationInterpretation: No new equation is required; identify which physical mechanism carries energy and what temperature difference drives the net transfer
Use when: qualitative energy-transfer analysis
A hot cup loses energy by conduction through the cup, convection to moving air and thermal radiation to the surroundings.
The First Law of Thermodynamics
U = (3/2)nRT = (3/2)Nk_B TVariables & SI units: U internal energy of an ideal monatomic gas (J); n amount (mol); R gas constant; N particle count; k_B Boltzmann constant; T absolute temperature (K)
Use when: ideal monatomic gas whose internal energy is translational kinetic energy
For a fixed amount of ideal monatomic gas, doubling T doubles U.
The First Law of Thermodynamics
ΔU = Q + W_onVariables & SI units: ΔU internal-energy change (J); Q energy transferred into the system by heating (J, negative for cooling); W_on work done on the system (J)
Use when: closed-system energy bookkeeping with this sign convention stated explicitly
A compressed gas can gain internal energy even if no heating occurs because W_on is positive.
The First Law of Thermodynamics
W_on = −P_ext ΔV; |W| = area under a P–V pathVariables & SI units: W_on work done on gas (J); P_ext constant or average external pressure (Pa); ΔV = V_f−V_i (m³); P–V area has units Pa·m³ = J
Use when: constant/average external pressure for W_on = −P_extΔV; area reasoning for quasistatic P–V paths
Expansion has ΔV>0 so W_on<0; compression has ΔV<0 so W_on>0.
Specific Heat and Thermal Conductivity
Q = mcΔTVariables & SI units: Q energy transferred to the object by heating/cooling (J); m mass (kg); c specific heat capacity (J·kg⁻¹·K⁻¹); ΔT = T_f−T_i (K or °C difference)
Use when: temperature change with no phase change and approximately constant c
For the same Q and m, a material with larger c undergoes a smaller temperature change.
Specific Heat and Thermal Conductivity
Q/Δt = kAΔT/LVariables & SI units: Q/Δt conduction rate (W); k thermal conductivity (W·m⁻¹·K⁻¹); A cross-sectional area (m²); ΔT temperature difference (K); L conduction length/thickness (m)
Use when: steady one-dimensional conduction through a uniform slab or rod
Doubling insulation thickness halves the ideal steady conduction rate when other quantities remain fixed.
Specific Heat and Thermal Conductivity
At fixed geometry and ΔT: conduction rate ∝ kVariables & SI units: Q/Δt power (W); k conductivity; geometry A/L and temperature difference held fixed
Use when: proportional comparison of materials under the same steady-conduction conditions
A high-k metal transfers energy faster than a low-k insulating material of the same size under the same temperature difference.
Entropy and the Second Law of Thermodynamics
Isolated system: total entropy never decreasesInterpretation: No quantitative entropy calculation is required; compare initial and final entropy qualitatively for the entire isolated system
Use when: qualitative second-law reasoning for an isolated system
A hot object and a cold object inside an insulated enclosure spontaneously approach one common temperature; total entropy increases.
Entropy and the Second Law of Thermodynamics
Reversible ideal process: total entropy remains constantInterpretation: Use “reversible” as the ideal limiting case with no net entropy production; no entropy equation is required
Use when: qualitative comparison of a reversible process for the complete isolated system
An ideal reversible limit can connect equilibrium states without increasing total entropy.
Entropy and the Second Law of Thermodynamics
Irreversible spontaneous process: total entropy increases toward equilibriumInterpretation: Use qualitative evidence such as mixing, free expansion, friction or heat transfer across a finite temperature difference
Use when: real spontaneous processes in an isolated-system analysis
A gas freely expanding into an evacuated region spreads into more accessible configurations and increases total entropy.
Electric Charge and Electric Force
F_E = |q₁q₂|/(4πεr²)Variables & SI units: F_E electric-force magnitude (N); q₁,q₂ charges (C); ε permittivity of the medium (F/m); r center-to-center separation (m). In vacuum, 1/(4πε₀)=k_e≈8.99×10⁹ N·m²/C².
Use when: point charges or spherically symmetric charged objects when the point-charge model is valid
If the separation doubles while charges and medium stay fixed, the force magnitude becomes one fourth as large.
Electric Charge and Electric Force
q = neVariables & SI units: q net charge (C); n an integer counting excess or missing elementary charges; e=1.60×10⁻¹⁹ C
Use when: ordinary charge quantization
An object with 5×10⁶ excess electrons has q=−5×10⁶e.
Electric Charge and Electric Force
F_net = vector sum of F_iVariables & SI units: F_net net electrostatic force vector (N); F_i individual force vectors from the other charged objects
Use when: two to four interacting charges, or a higher-symmetry case
For three charges, determine each force direction first and add components rather than adding magnitudes.
Conservation of Electric Charge and the Process of Charging
Q_system,f = Q_system,i + Q_transferredVariables & SI units: Q_system net system charge (C); Q_transferred signed charge entering the system (C), negative if net charge leaves
Use when: charging analyzed with an explicit system boundary
If electrons enter an initially neutral isolated metal object, its final net charge is negative by exactly the transferred amount.
Conservation of Electric Charge and the Process of Charging
Q_total,isolated = constantVariables & SI units: Q_total,isolated sum of all charges inside an isolated multi-object system (C)
Use when: friction, contact or redistribution when no charge crosses the outer system boundary
Rubbing two initially neutral objects can leave equal-and-opposite net charges while the two-object total remains zero.
Conservation of Electric Charge and the Process of Charging
induction/polarization: redistribution can occur with ΔQ_system = 0Variables & SI units: ΔQ_system net-charge change (C); zero means positive and negative regions rearrange without changing the system total
Use when: a nearby charge alters the distribution inside a neutral or charged system
A charged rod brought near a neutral conductor can attract the conductor even before contact because mobile charge separates.
Electric Fields
E = F_E/q_test (vector relation)Variables & SI units: E electric field vector (N/C); F_E electric-force vector on the test charge (N); q_test positive test charge (C)
Use when: definition of electric field using a sufficiently small positive test charge
A 2.0 μC positive test charge experiencing 0.060 N to the right is in a field of 3.0×10⁴ N/C to the right.
Electric Fields
E = |Q|/(4πεr²)Variables & SI units: E field magnitude (N/C); Q source charge (C); ε medium permittivity (F/m); r distance from a point/spherical source (m)
Use when: point charge or outside a spherically symmetric isolated charge distribution
Doubling distance from an isolated point charge reduces field magnitude by a factor of four.
Electric Fields
E_net = vector sum of E_iVariables & SI units: E_net net electric-field vector (N/C); E_i individual source-field vectors
Use when: up to four source charges, or more only when high symmetry simplifies the analysis
Between equal unlike charges, the two field contributions at the midpoint point in the same direction and therefore add.
Electric Potential Energy
U_E = q₁q₂/(4πεr)Variables & SI units: U_E electric potential energy of the pair (J); q₁,q₂ charges (C); ε permittivity (F/m); r separation (m)
Use when: two point charges using zero potential energy at infinite separation
Like charges give positive U_E at finite separation; opposite charges give negative U_E with this reference.
Electric Potential Energy
U_system = Σ_pairs q_iq_j/(4πεr_ij)Variables & SI units: U_system total electric potential energy (J); each distinct charge pair is counted once
Use when: configurations of up to four point charges
For three charges, include the 1–2, 1–3 and 2–3 pair energies once each.
Electric Potential Energy
W_ext,∞→configuration = U_EVariables & SI units: W_ext work done by an external agent in assembling the configuration quasistatically from the zero reference (J); U_E resulting potential energy (J)
Use when: definition/interpretation of electric potential energy for a two-charge configuration
External work is positive when like charges are slowly brought closer from very far apart.
Electric Potential
V = U_E/q_testVariables & SI units: V electric potential (V=J/C); U_E interaction energy involving the test charge (J); q_test test charge (C)
Use when: definition of electric potential at a point
If a +2 C test charge would have 6 J of electric potential energy at a point, that point is at 3 V.
Electric Potential
V = Σ_i Q_i/(4πεr_i)Variables & SI units: V total potential (V); Q_i source charges (C); r_i distance from each source to the point (m); ε medium permittivity
Use when: up to four point charges, or more in high-symmetry cases, using zero potential at infinity
A positive and negative source can give zero potential at a point even when the electric field there is not zero.
Electric Potential
E_avg,parallel = −ΔV/ΔsVariables & SI units: E_avg component of average electric field along displacement (V/m=N/C); ΔV=V_f−V_i (V); Δs displacement along the field coordinate (m)
Use when: relating potential change to the average field along a chosen direction; in a uniform field this becomes exact along that line
Moving in the electric-field direction lowers electric potential; closely spaced equipotentials indicate a stronger field.
Capacitors
C = Q/|ΔV|Variables & SI units: C capacitance (F); Q magnitude of charge on either plate (C); |ΔV| plate potential difference (V)
Use when: definition of capacitance
For a fixed capacitor, doubling Q doubles |ΔV|; C itself does not change.
Capacitors
C = κε₀A/d; E = |ΔV|/d = Q/(κε₀A)Variables & SI units: C capacitance (F); κ dielectric constant; ε₀ vacuum permittivity; A plate area (m²); d plate separation (m); E uniform central field magnitude (N/C)
Use when: ideal parallel plates with d much smaller than plate dimensions and edge effects neglected
Increasing plate area raises C; increasing separation lowers C; inserting a dielectric raises C and reduces the field for fixed free plate charge.
Capacitors
U_C = ½Q|ΔV| = Q²/(2C) = ½C(ΔV)²Variables & SI units: U_C energy stored in capacitor/electric field (J); Q charge magnitude (C); C capacitance (F); ΔV voltage (V)
Use when: ideal capacitor energy; choose the form matching what is known and what remains fixed
At fixed C, doubling voltage quadruples stored energy; at fixed Q, increasing C lowers stored energy.
Conservation of Electric Energy
ΔU_E = qΔVVariables & SI units: ΔU_E electric potential-energy change of the object–field system (J); q moving charge (C); ΔV=V_f−V_i (V)
Use when: a charged object moves between two locations with known electric potentials
A positive charge moving to lower potential has ΔU_E<0; a negative charge has the opposite sign relation.
Conservation of Electric Energy
ΔK = −ΔU_E = −qΔVVariables & SI units: ΔK kinetic-energy change (J); ΔU_E electric potential-energy change (J)
Use when: electric force is the only force doing work and no other energy transfer crosses the chosen boundary
A released positive charge moving to lower potential gains kinetic energy equal to the electric potential-energy decrease.
Conservation of Electric Energy
K_i + U_E,i = K_f + U_E,fVariables & SI units: K kinetic energy (J); U_E electric potential energy (J)
Use when: closed conservative object–field system with no additional transfer terms
An electron accelerated through a potential difference can be analyzed by the same energy bookkeeping once the charge sign is handled correctly.
Electric Current
I = ΔQ/ΔtVariables & SI units: I current (A = C/s); ΔQ net charge crossing a cross section (C); Δt time interval (s)
Use when: average current through a chosen cross section
6 C crossing in 3 s corresponds to 2 A
Electric Current
ΔQ = IΔtVariables & SI units: ΔQ charge (C); I current (A); Δt time (s)
Use when: constant current over the interval
0.50 A for 8 s transfers 4 C
Electric Current
I = 0 ⇒ no net carrier motionVariables & SI units: I current; carrier thermal motion may still be nonzero
Use when: distinguishing zero current from zero microscopic particle speed
an open circuit can contain moving electrons microscopically while having zero net charge flow
Simple Circuits
closed loop ⇒ charge can flowInterpretation: A closed conducting path permits sustained current when a source provides potential difference
Use when: qualitative circuit-state reasoning
closing a switch completes the loop and allows current
Simple Circuits
open path ⇒ I = 0 in that branchVariables & SI units: I branch current (A)
Use when: a break interrupts the conducting path
an open switch prevents current in its branch
Simple Circuits
short path ≈ 0 ΩVariables & SI units: R path resistance (Ω), ideally near zero
Use when: a low-resistance connection joins two points directly
a wire placed across an element can bypass that element
Resistance, Resistivity, and Ohm’s Law
R = ρL/AVariables & SI units: R resistance (Ω); ρ resistivity (Ω·m); L length (m); A cross-sectional area (m²)
Use when: uniform conductor
doubling length doubles resistance; doubling area halves resistance
Resistance, Resistivity, and Ohm’s Law
ΔV = IRVariables & SI units: ΔV potential difference (V); I current (A); R resistance (Ω)
Use when: ohmic element under fixed physical conditions
a 4 Ω resistor carrying 2 A has 8 V across it
Resistance, Resistivity, and Ohm’s Law
slope depends on axesInterpretation: for ΔV vs I, slope = R; for I vs ΔV, slope = 1/R
Use when: interpreting experimental current-voltage graphs
always read axis labels before converting graph slope into resistance
Electric Power
P = IΔVVariables & SI units: P power (W = J/s); I current (A); ΔV potential difference (V)
Use when: any circuit element when current and potential difference are known
12 V across a device carrying 2 A corresponds to 24 W
Electric Power
P = I²RVariables & SI units: P power (W); I current (A); R resistance (Ω)
Use when: resistive element with current known
at fixed current, doubling R doubles power
Electric Power
P = (ΔV)²/RVariables & SI units: P power (W); ΔV potential difference (V); R resistance (Ω)
Use when: resistive element with potential difference known
at fixed voltage, doubling R halves power
Compound Direct Current (DC) Circuits
R_series = ΣR_iVariables & SI units: R_series equivalent resistance (Ω); R_i component resistances (Ω)
Use when: components carrying the same current with no branching between them
3 Ω and 5 Ω in series give 8 Ω
Compound Direct Current (DC) Circuits
1/R_parallel = Σ(1/R_i)Variables & SI units: R_parallel equivalent resistance (Ω); R_i branch resistances (Ω)
Use when: resistors connected across the same two nodes
two identical resistors in parallel have half the resistance of either one
Compound Direct Current (DC) Circuits
I_source = ΔV_source/R_eqVariables & SI units: I_source source current (A); ΔV_source source potential difference (V); R_eq equivalent resistance (Ω)
Use when: ideal source driving a reduced resistive network
reduce valid subgroups first, then determine total source current
Kirchhoff’s Loop Rule
ΣΔV_loop = 0Variables & SI units: ΔV signed potential changes (V)
Use when: any closed loop in the lumped circuit model
source rises and resistor drops sum to zero
Kirchhoff’s Loop Rule
ΔU_E = qΔVVariables & SI units: ΔU_E electric potential-energy change (J); q charge (C); ΔV potential change (V)
Use when: connecting loop potential changes to energy per charge
a positive charge gains electric potential energy when it moves through a potential rise
Kirchhoff’s Loop Rule
ideal wire: ΔV = 0Variables & SI units: ΔV potential difference (V)
Use when: points connected only by an ideal wire
all points on one ideal-wire node share the same potential
Kirchhoff’s Junction Rule
ΣI_in = ΣI_outVariables & SI units: I branch currents (A)
Use when: steady-state junction
3 A entering and 1 A leaving one branch requires 2 A to leave through the remaining branch
Kirchhoff’s Junction Rule
ΣI_signed = 0Variables & SI units: I signed branch currents (A)
Use when: algebraic node equation with a consistent sign convention
take entering currents positive and leaving currents negative, or vice versa
Kirchhoff’s Junction Rule
I_total = I_1 + I_2 + …Variables & SI units: I_total and branch currents (A)
Use when: current splitting or recombining at a junction
source current equals the sum of parallel-branch currents
Resistor-Capacitor (RC) Circuits
1/C_series = Σ(1/C_i)Variables & SI units: C_series equivalent capacitance (F); C_i capacitances (F)
Use when: capacitors connected in series
series equivalent capacitance is smaller than the smallest individual capacitance
Resistor-Capacitor (RC) Circuits
C_parallel = ΣC_iVariables & SI units: C_parallel equivalent capacitance (F); C_i capacitances (F)
Use when: capacitors connected across the same two nodes
parallel capacitances add directly
Resistor-Capacitor (RC) Circuits
τ = RCVariables & SI units: τ time constant (s); R effective resistance (Ω); C capacitance (F)
Use when: ideal first-order RC timescale; use qualitatively for charging/discharging speed
after one time constant charging reaches about 63% of final charge while discharging retains about 37% of its initial charge
Magnetic Fields
magnetic field lines form closed loopsInterpretation: B magnetic-field vector (T); no isolated magnetic monopole is used in this course model
Use when: representing magnetic-field direction around magnets and magnetic materials
outside a bar magnet the field points away from the north pole and toward the south pole, then continues through the magnet
Magnetic Fields
dipole alignment → magnetic responseInterpretation: magnetic-domain/dipole alignment; qualitative relationship
Use when: comparing permanent, induced, paramagnetic, and diamagnetic behavior
a ferromagnetic sample can retain substantial alignment after an external field is removed, whereas a paramagnetic sample does not
Magnetic Fields
μ₀ = 4π × 10⁻⁷ T·m/AInterpretation: μ₀ vacuum permeability; T tesla; m meter; A ampere
Use when: recognizing the free-space permeability constant used in later magnetic-field equations
the long-straight-wire field model in Topic 12.3 uses μ₀
Magnetism and Moving Charges
F_B = |q|vB sinθVariables & SI units: F_B magnetic-force magnitude (N); q charge magnitude (C); v speed (m/s); B magnetic field (T); θ angle between v and B
Use when: moving charge in a magnetic field; numerical angle treatment here is limited to 0°, 90°, and 180°
for v perpendicular to B, F_B=|q|vB; for v parallel or antiparallel to B, F_B=0
Magnetism and Moving Charges
r = mv/(|q|B)Variables & SI units: r circular-path radius (m); m particle mass (kg); v speed (m/s); q charge magnitude (C); B field (T)
Use when: derived for motion perpendicular to a uniform magnetic field when magnetic force supplies centripetal force
doubling speed doubles the radius while doubling B halves the radius
Magnetism and Moving Charges
qE and qvB act independentlyInterpretation: E electric field (N/C); B magnetic field (T); q charge (C); v velocity; vector directions matter
Use when: regions containing both electric and magnetic fields; balance can be analyzed by superposition
in perpendicular crossed fields, equal and opposite electric and magnetic forces can transmit a selected particle speed
Magnetism and Current-Carrying Wires
B = μ₀I/(2πr)Variables & SI units: B magnetic field (T); μ₀ vacuum permeability (T·m/A); I current (A); r perpendicular distance from wire axis (m)
Use when: long straight current-carrying wire in free space
doubling I doubles B; doubling r halves B
Magnetism and Current-Carrying Wires
F_B = IℓB sinθVariables & SI units: F_B magnetic-force magnitude (N); I current (A); ℓ wire length inside the field (m); B external field (T); θ angle between current direction and B
Use when: straight current segment in a magnetic field
a wire perpendicular to B experiences maximum force; a parallel wire experiences zero force
Magnetism and Current-Carrying Wires
B_net = vector sum of source fieldsVariables & SI units: B_net and source fields measured in tesla; directions determined before adding
Use when: two or more current-carrying wires contribute magnetic field at one location
fields in opposite directions subtract in magnitude, while fields in the same direction add
Electromagnetic Induction and Faraday’s Law
Φ_B = BA cosθVariables & SI units: Φ_B magnetic flux (Wb = T·m²); B field (T); A area (m²); θ angle between B and area vector
Use when: uniform magnetic field through a flat area
flux is maximum in magnitude when B is parallel to the area vector and zero when B lies in the surface plane
Electromagnetic Induction and Faraday’s Law
|ε| = N|ΔΦ_B/Δt|Variables & SI units: ε induced emf (V); N number of turns; ΔΦ_B change in flux per turn (Wb); Δt time interval (s)
Use when: average induced emf in an N-turn coil
doubling the flux change in the same time doubles the emf magnitude
Electromagnetic Induction and Faraday’s Law
ε = BℓvVariables & SI units: ε motional emf (V); B field (T); ℓ conducting-rod length in the field (m); v rod speed (m/s)
Use when: conducting rod moving on rails in a uniform magnetic field with perpendicular geometry
doubling rod speed doubles the motional emf
Reflection
θ_i = θ_rVariables & SI units: θ_i angle of incidence; θ_r angle of reflection; both measured from the local normal
Use when: reflection of a light ray from a surface
a ray arriving 35° from the normal leaves 35° from the normal on the other side
Reflection
ray direction ⟂ wavefrontInterpretation: ray direction and wavefront orientation; geometric relationship
Use when: geometric-optics situations where the wave nature of light can be neglected
parallel planar wavefronts correspond to parallel light rays normal to those wavefronts
Reflection
local normal variation → diffuse or specular reflectionInterpretation: local surface normal direction; qualitative model
Use when: comparing rough and smooth reflecting surfaces
paper can look bright from many viewing directions because different microscopic patches have different normals
Images Formed by Mirrors
1/f = 1/s_o + 1/s_iVariables & SI units: f focal length (m); s_o object distance (m); s_i image distance (m)
Use when: plane or spherical-mirror image calculations with a consistent sign convention
a concave mirror with an object beyond its focal point can produce a positive real-image distance
Images Formed by Mirrors
M = h_i/h_o = −s_i/s_oVariables & SI units: M magnification (dimensionless); h_i image height; h_o object height; s_i image distance; s_o object distance
Use when: mirror image size and orientation
negative M represents an inverted image under the stated sign convention
Images Formed by Mirrors
f = R/2 for a spherical mirrorVariables & SI units: f focal length (m); R signed radius of curvature (m)
Use when: concave or convex spherical mirrors in the geometric/paraxial model
a concave spherical mirror with R=40 cm has |f|=20 cm
Refraction
n = c/vVariables & SI units: n refractive index; c vacuum light speed (m/s); v light speed in the medium (m/s)
Use when: relating propagation speed and refractive index in a transparent medium
larger n corresponds to smaller light speed v
Refraction
n₁ sinθ₁ = n₂ sinθ₂Variables & SI units: n₁,n₂ refractive indices; θ₁ incidence angle; θ₂ refraction angle; angles measured from the normal
Use when: light crossing a boundary between two transparent media
air-to-glass transmission bends toward the normal because n increases
Refraction
sinθ_c = n₂/n₁Variables & SI units: θ_c critical angle; n₁ higher refractive index; n₂ lower refractive index
Use when: critical-angle calculation only when n₁>n₂
for glass-to-air, incidence greater than θ_c produces total internal reflection
Images Formed by Lenses
1/f = 1/s_o + 1/s_iVariables & SI units: f focal length (m); s_o object distance (m); s_i image distance (m)
Use when: thin-lens image calculations with a consistent sign convention
a converging lens with an object beyond f can form a real image on the transmitted side
Images Formed by Lenses
M = h_i/h_o = −s_i/s_oVariables & SI units: M magnification (dimensionless); h_i image height; h_o object height; s_i image distance; s_o object distance
Use when: thin-lens image size and orientation
negative magnification corresponds to an inverted real image under the stated convention
Images Formed by Lenses
principal rays locate the imageInterpretation: parallel ray ↔ focal point; central ray passes straight through the thin-lens center; focal ray ↔ parallel ray
Use when: constructing ray diagrams for thin converging or diverging lenses
two correctly drawn principal rays are sufficient to locate an image, while a third provides a consistency check
Properties of Wave Pulses and Waves
v_string = √(F_T/μ)Variables & SI units: v_string wave speed on an ideal string (m/s); F_T tension (N); μ linear mass density (kg/m)
Use when: a transverse wave on a stretched uniform string
increasing tension raises wave speed; increasing linear density lowers it
Properties of Wave Pulses and Waves
μ = m/ℓVariables & SI units: μ linear mass density (kg/m); m string mass (kg); ℓ string length (m)
Use when: converting a uniform string mass and length into the property that controls string-wave speed
a 0.020 kg string 2.0 m long has μ=0.010 kg/m
Properties of Wave Pulses and Waves
greater amplitude → greater transported energyInterpretation: qualitative model statement; compare otherwise similar waves in the same medium
Use when: comparing how much energy similar wave disturbances carry
a larger-amplitude sound wave is associated with greater intensity/loudness than an otherwise similar smaller-amplitude wave
Periodic Waves
v = fλVariables & SI units: v wave speed (m/s); f frequency (Hz); λ wavelength (m)
Use when: any periodic wave when speed, frequency, and wavelength refer to the same wave in the same medium
at v=12 m/s and f=4 Hz, λ=3 m
Periodic Waves
T = 1/fVariables & SI units: T period (s); f frequency (Hz)
Use when: converting between temporal repeat time and cycles per second
a 50 Hz wave has T=0.020 s
Periodic Waves
sinusoidal wave: y(x)=A sin(2πx/λ+φ)Variables & SI units: y displacement (m); A amplitude (m); x position (m); λ wavelength (m); φ phase constant (rad)
Use when: reading or constructing a sinusoidal displacement-versus-position representation at a fixed instant
successive crests are separated by one wavelength
Boundary Behavior of Waves and Polarization
f_reflected = f_transmitted = f_incidentVariables & SI units: all frequencies in Hz; the boundary is stationary and the source frequency is unchanged
Use when: reflection and transmission at a stationary boundary
the transmitted wavelength can change when speed changes even though frequency does not
Boundary Behavior of Waves and Polarization
I = P_avg/AVariables & SI units: I intensity (W/m²); P_avg average power (W); A area normal to energy flow (m²)
Use when: average wave power spread over an area
6 W distributed across 2 m² corresponds to 3 W/m²
Boundary Behavior of Waves and Polarization
transmitted speed decreases → reflected pulse invertedInterpretation: qualitative boundary model; compare wave speed before and after the boundary
Use when: predicting reflected-pulse orientation for the boundary model
a pulse reflecting where the transmitted-wave speed is lower returns inverted; if transmitted speed is higher, it returns without inversion
Electromagnetic Waves
c = fλVariables & SI units: c vacuum light speed (m/s); f frequency (Hz); λ vacuum wavelength (m)
Use when: electromagnetic radiation propagating in vacuum
higher-frequency electromagnetic radiation has shorter wavelength
Electromagnetic Waves
E ⟂ B ⟂ propagationInterpretation: E electric-field direction; B magnetic-field direction; qualitative vector geometry
Use when: plane electromagnetic-wave representation
if the wave travels in +x and E oscillates along y, B is perpendicular to both
Electromagnetic Waves
radio → microwave → infrared → visible → ultraviolet → X-ray → gammaInterpretation: qualitative ordering from longer wavelength/lower frequency toward shorter wavelength/higher frequency
Use when: classifying electromagnetic radiation without memorizing exact wavelength cutoffs
visible light lies between infrared and ultraviolet in the spectrum
The Doppler Effect
approaching → f_observed > f_restInterpretation: qualitative comparison of observed and rest frequency
Use when: source and observer move toward one another
an approaching siren is heard at a higher frequency than when there is no relative motion
The Doppler Effect
receding → f_observed < f_restInterpretation: qualitative comparison of observed and rest frequency
Use when: source and observer move away from one another
after the siren passes and moves away, the observed frequency is lower
The Doppler Effect
greater relative speed → greater |frequency shift|Interpretation: qualitative model statement; no numerical Doppler equation is required
Use when: comparing two approach or recession scenarios
a faster approach produces a larger upward frequency shift than a slower approach
Wave Interference and Standing Waves
y_total = Σy_iVariables & SI units: y_total resultant displacement (m); y_i individual wave displacements (m)
Use when: linear superposition when waves overlap
equal and opposite pulses can momentarily cancel before continuing through each other
Wave Interference and Standing Waves
f_beat = |f₁−f₂|Variables & SI units: f_beat beat frequency (Hz); f₁,f₂ component frequencies (Hz)
Use when: two nearby frequencies producing audible or measurable beats
440 Hz and 444 Hz produce 4 beats per second
Wave Interference and Standing Waves
L=nλ/2 (same-end type); L=(2n−1)λ/4 (node-antinode)Variables & SI units: L resonant length (m); λ wavelength (m); n positive integer
Use when: ideal standing-wave modes for two like boundary conditions or one node/one antinode
a closed-open air column supports odd quarter-wavelength modes
Diffraction
a sinθ_m = mλVariables & SI units: a slit width (m); θ_m dark-minimum angle; m=1,2,…; λ wavelength (m)
Use when: single-slit diffraction minima
a narrower slit makes the first minimum occur at a larger angle
Diffraction
y_m ≈ mλL/aVariables & SI units: y_m dark-minimum position from center (m); λ wavelength (m); L screen distance (m); a slit width (m)
Use when: single-slit small-angle geometry
increasing screen distance spreads the observed pattern
Diffraction
central maximum width ≈ 2λL/aVariables & SI units: central width (m); λ wavelength (m); L screen distance (m); a slit width (m)
Use when: estimating the distance between the first minima on opposite sides at small angle
doubling λ approximately doubles the central-maximum width
Double-Slit Interference and Diffraction Gratings
d sinθ_m = mλVariables & SI units: d slit/grating spacing (m); θ_m constructive angle; m integer order; λ wavelength (m)
Use when: double-slit or diffraction-grating constructive maxima
longer wavelength produces a larger angle at the same order and spacing
Double-Slit Interference and Diffraction Gratings
y_m ≈ mλL/dVariables & SI units: y_m bright-fringe position (m); m order; λ wavelength (m); L screen distance (m); d slit spacing (m)
Use when: small-angle double-slit screen geometry
larger slit separation moves neighboring fringes closer together
Double-Slit Interference and Diffraction Gratings
d = 1/NVariables & SI units: d grating spacing (m); N line density (lines/m)
Use when: converting grating line density to opening spacing
600 lines/mm corresponds to d≈1.67×10⁻⁶ m
Thin-Film Interference
optical path difference = 2ntVariables & SI units: n film refractive index; t film thickness (m); 2nt optical round-trip path at normal incidence
Use when: thin-film reflected-light comparison at normal incidence before including reflection phase changes
changing thickness changes which wavelengths reinforce or cancel
Thin-Film Interference
one net phase reversal: constructive 2nt=(m+1/2)λ₀; destructive 2nt=mλ₀Variables & SI units: n index; t thickness (m); m integer; λ₀ vacuum wavelength (m)
Use when: reflected-light interference at normal incidence with exactly one 180° reflection phase reversal
an oil film can enhance different colors as its thickness varies
Thin-Film Interference
quarter-wave AR: t=λ₀/(4n)Variables & SI units: t coating thickness (m); λ₀ target vacuum wavelength (m); n coating index
Use when: simplest normal-incidence antireflection coating when the reflection phase conditions support cancellation
a coating can suppress reflection of a chosen wavelength by making the two reflected rays arrive out of phase
Quantum Theory and Wave-Particle Duality
E = hfVariables & SI units: E photon energy (J); h Planck constant (J·s); f photon frequency (Hz)
Use when: photon energy or an energy transfer involving one photon
a higher-frequency photon carries more energy
Quantum Theory and Wave-Particle Duality
pγ = h/λVariables & SI units: pγ photon momentum (kg·m/s); h Planck constant; λ photon wavelength (m)
Use when: photon momentum and momentum-transfer reasoning
a shorter-wavelength photon carries greater momentum
Quantum Theory and Wave-Particle Duality
λdB = h/pVariables & SI units: λdB de Broglie wavelength (m); h Planck constant; p particle momentum (kg·m/s)
Use when: matter-wave behavior of a particle
increasing a particle’s momentum decreases its de Broglie wavelength
The Bohr Model of Atomic Structure
A = Z + NnVariables & SI units: A nucleon (mass) number; Z proton (atomic) number; Nn neutron number
Use when: nuclear notation and isotope bookkeeping
carbon-14 has Z=6 and therefore Nn=8 neutrons
The Bohr Model of Atomic Structure
ke²/r² = mv²/rVariables & SI units: k Coulomb constant; e elementary charge; r electron–nucleus separation (m); m electron mass (kg); v model speed (m/s)
Use when: historical single-electron Bohr circular-motion model where electric attraction supplies radial force
changing allowed radius changes the electric force and model orbital speed
The Bohr Model of Atomic Structure
2πr = nλdB = nh/(mv)Variables & SI units: r model orbit radius (m); n positive integer; λdB de Broglie wavelength (m); h Planck constant; m electron mass; v model speed
Use when: standing-wave condition in the historical Bohr/de Broglie picture
only circumferences containing an integer number of de Broglie wavelengths satisfy the standing-wave condition
Emission and Absorption Spectra
|ΔE| = hfVariables & SI units: |ΔE| magnitude of the atomic energy-level difference (J); h Planck constant; f photon frequency (Hz)
Use when: one-photon absorption or emission between two allowed levels
a larger level gap corresponds to a higher-frequency photon
Emission and Absorption Spectra
|ΔE| = hc/λVariables & SI units: |ΔE| transition energy (J); h Planck constant; c speed of light; λ photon wavelength (m)
Use when: converting an allowed transition energy to a spectral wavelength
larger energy gaps produce shorter wavelengths
Emission and Absorption Spectra
absorption: Ef = Ei + hf; emission: hf = Ei − EfVariables & SI units: Ei and Ef atomic-system energies (J or eV used consistently); hf photon energy
Use when: direction of a one-photon transition on an energy-level diagram
an upward arrow requires photon absorption; a downward arrow corresponds to photon emission
Blackbody Radiation
λmax T = bVariables & SI units: λmax peak wavelength (m); T absolute temperature (K); b Wien displacement constant (m·K)
Use when: peak wavelength of an ideal blackbody spectrum
a hotter blackbody peaks at a shorter wavelength
Blackbody Radiation
P = σAT⁴Variables & SI units: P total emitted power (W); σ Stefan–Boltzmann constant (W·m⁻²·K⁻⁴); A surface area (m²); T absolute temperature (K)
Use when: total emitted power of an ideal blackbody
doubling T at fixed A increases P by a factor of 16
Blackbody Radiation
P₂/P₁ = (A₂/A₁)(T₂/T₁)⁴Variables & SI units: P power; A surface area; T absolute temperature; both situations use the ideal-blackbody model
Use when: comparing two blackbodies without separately calculating σ
at equal area, a 20% temperature increase raises power by (1.2)⁴
The Photoelectric Effect
Kmax = hf − φVariables & SI units: Kmax maximum emitted-electron kinetic energy (J); h Planck constant; f incident-light frequency (Hz); φ work function (J)
Use when: photoelectric emission when hf≥φ
at fixed material, increasing frequency raises Kmax linearly
The Photoelectric Effect
eVs = KmaxVariables & SI units: e elementary-charge magnitude (C); Vs stopping-potential magnitude (V); Kmax maximum kinetic energy (J)
Use when: ideal stopping-potential measurement
a 2.0 eV maximum kinetic energy corresponds to a 2.0 V stopping-potential magnitude
The Photoelectric Effect
f0 = φ/hVariables & SI units: f0 threshold frequency (Hz); φ work function (J); h Planck constant
Use when: onset of photoelectric emission
below f0, raising intensity does not cause emission in the one-photon model
Compton Scattering
Δλ = (h/mec)(1 − cosθ)Variables & SI units: Δλ=λf−λi wavelength increase (m); h Planck constant; me electron mass; c light speed; θ photon scattering angle
Use when: Compton scattering of a photon from an approximately free electron
θ=0 gives no Compton wavelength shift; backscatter gives the maximum shift
Compton Scattering
pγ = h/λVariables & SI units: pγ photon momentum (kg·m/s); h Planck constant; λ photon wavelength (m)
Use when: incident or scattered photon momentum
because λf>λi after an energy-transferring scatter, the photon momentum decreases
Compton Scattering
Eγ = hc/λVariables & SI units: Eγ photon energy (J); h Planck constant; c light speed; λ wavelength (m)
Use when: photon energy before and after scattering
a longer scattered wavelength means lower photon energy, with the difference transferred to the electron/system
Fission, Fusion, and Nuclear Decay
ΔE = Δmc²Variables & SI units: ΔE change in rest-mass energy (J); Δm mass difference (kg); c speed of light (m/s)
Use when: nuclear reactions/processes where rest mass and other energy forms are exchanged
a small decrease in total rest mass can appear as kinetic energy of products and/or photon energy
Fission, Fusion, and Nuclear Decay
λ = ln(2)/t1/2Variables & SI units: λ decay constant (s⁻¹); t1/2 half-life (s)
Use when: connecting the exponential decay rate to half-life
a shorter half-life corresponds to a larger decay constant
Fission, Fusion, and Nuclear Decay
N = N0e^(−λt) = N0(1/2)^(t/t1/2)Variables & SI units: N remaining radioactive nuclei; N0 initial nuclei; λ decay constant (s⁻¹); t time; t1/2 half-life
Use when: statistical population decay or age/remaining-fraction calculations
after three half-lives the expected remaining population is N0/8
Types of Radioactive Decay
alpha: A→A−4, Z→Z−2 + ⁴₂HeInterpretation: A parent nucleon number; Z parent proton number; emitted alpha has A=4 and Z=2
Use when: alpha-decay nuclear bookkeeping
the daughter has four fewer nucleons and two fewer protons than the parent
Types of Radioactive Decay
β−: n→p + e− + anti-ν; β+: p→n + e+ + νInterpretation: n neutron; p proton; e− electron; e+ positron; ν neutrino; anti-ν antineutrino
Use when: beta-minus or beta-plus decay with charge, nucleon and lepton bookkeeping
β− raises daughter Z by 1 at fixed A; β+ lowers daughter Z by 1 at fixed A
Types of Radioactive Decay
gamma: excited nucleus → lower-energy same nucleus + γInterpretation: γ photon; parent and daughter retain the same A and Z
Use when: gamma de-excitation after an excited nuclear state
gamma emission changes nuclear energy but not the element or isotope identity
No relationships match that search. Try the quantity name, topic name, unit number or a related concept.
Match the wording of the problem to the physical quantity
These cues are not shortcuts around reasoning; they help you identify the model that deserves a closer look.
| If the question emphasizes… | Think about… | Check before solving |
|---|---|---|
| pressure, volume, temperature, molecules | ideal-gas and kinetic-theory relationships | absolute temperature, particle count vs moles, process conditions |
| charge arrangement, force, field, potential | Coulomb/field/potential/energy models | vector vs scalar quantity, sign of charge, reference point |
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| moving charge/current in a magnetic field | Lorentz force and magnetic-field relationships | angle, direction rule, whether magnetic force does work |
| changing magnetic flux | induction and Faraday/Lenz reasoning | what changes flux: field, area, angle or loop motion? |
| image location, size, focus, refraction | ray geometry, Snell, mirror/lens and magnification | sign convention and whether image is real or virtual |
| fringe spacing, resonance, diffraction, phase | wave speed, standing-wave and interference models | boundary condition, path difference, phase shifts, small-angle use |
| photon energy, wavelength, emission, ejected electrons | quantum/photon and photoelectric relationships | frequency vs intensity, threshold/work function, energy units |
| nuclear mass change, half-life, activity | mass-energy and decay relationships | mass defect, exponential/half-life model, conserved quantities |
Errors that look mathematical but are actually model errors
Use these checks before blaming algebra.
Short answers to the most common reference-sheet searches
The interactive library above is the main tool; these answers clarify how to use it.
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For most students, yes: both phrases mean the equation/reference material used while studying. This page intentionally owns both search intents and adds explanations, conditions and examples around the equations.
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The complete learning library contains 138 equations and model relationships across 46 topics. It is broader than a compact exam reference because it also includes course relationships that are useful for learning and derivation.
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No. Memorize what the quantities mean and learn how the relationships behave. You should be able to recognize the right model, interpret its variables and predict how changing one quantity affects another.
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Search the physical quantity or concept—such as capacitance, induced emf, Doppler, focal length or photoelectric effect—then filter by unit if needed.
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