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Equation sheet · formula sheet · reference sheet

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.

PV thermodynamics +q −q electric field circuit geometric optics waves & interference B magnetism AP Physics 2 connects fields, energy and waves. Translate between models, graphs and evidence.

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.

138relationships
46topic connections
7unit filters
100%meaning + units + conditions
How to use the sheet

Choose a model before you choose an equation

The strongest equation choice starts from the physical situation, not from matching symbols.

01

Name the target

What quantity or comparison is the question asking for?

02

Choose the model

Gas, field, circuit, magnetic force, ray, wave, photon or nucleus?

03

Check conditions

Read what must be true before using the relationship.

04

Verify the result

Check units, sign, magnitude and limiting behavior.

Search intent note

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.

Formula map by unit

Know where the relationship lives before searching

The counts below include equations and explicit model relationships used on the 46 topic lessons.

Constants & reference values

Common values worth recognizing instantly

Keep the symbol, value and unit together; convert units before substitution.

Constant / valueSymbolValueUse
Avogadro constantNA6.02 × 1023 mol−1moles ↔ particles
Universal gas constantR8.31 J mol−1 K−1macroscopic ideal-gas law
Boltzmann constantkB1.38 × 10−23 J K−1microscopic thermal energy
Atmospheric pressure1 atm1.0 × 105 Pagas-state conversions
Coulomb constantke8.99 × 109 N·m²/C²point-charge force, field and potential
Proton massmp1.67 × 10−27 kgatomic and nuclear mass
Neutron massmn1.67 × 10−27 kgnuclear mass
Electron massme9.11 × 10−31 kgelectron dynamics and modern physics
Elementary charge magnitudee1.60 × 10−19 Ccharge quantization
Vacuum permittivityε08.85 × 10−12 C²/(N·m²)electric-field and capacitance models
Vacuum permeabilityμ04π × 10−7 T·m/Amagnetic-field models
Electron volt1 eV1.60 × 10−19 Jatomic, photon and nuclear energy
Planck constanth6.63 × 10−34 J·sphoton and matter-wave relationships
Speed of lightc3.00 × 108 m/selectromagnetic waves and photons
Wien constantb2.90 × 10−3 m·Kblackbody peak wavelength
Stefan–Boltzmann constantσ5.67 × 10−8 W·m−2·K−4blackbody radiated power
Unified atomic mass unit1 u1.66 × 10−27 kgnuclear mass and mass defect
Universal gravitational constantG6.67 × 10−11 N·m²/kg²mechanics connections
Gravitational field near Earthg9.8 N/kg = 9.8 m/s²mechanics connections and experiments
Model assumptions

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?
Interactive formula library

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.

138matching relationships
Topic 9.1Unit 9

Kinetic Theory of Temperature and Pressure

P = F⊥/A

Variables & 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

Physical example

A gas exerts 600 N perpendicular to a 0.020 m² wall, so P = 30 kPa.

Topic 9.1Unit 9

Kinetic Theory of Temperature and Pressure

K_avg = (3/2)k_B T = (1/2)m v_rms²

Variables & 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

Physical example

At the same temperature, lighter particles have a larger rms speed even though average translational kinetic energy is the same.

Topic 9.1 · ModelUnit 9

Kinetic Theory of Temperature and Pressure

Higher T → broader speed distribution with greater characteristic speeds

Interpretation: 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

Physical example

Heating a gas shifts the distribution toward higher speeds and spreads it over a wider range.

Topic 9.2Unit 9

The Ideal Gas Law

PV = nRT = Nk_B T

Variables & 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

Physical example

For fixed n and T, doubling V halves P.

Topic 9.2Unit 9

The Ideal Gas Law

P₁V₁/T₁ = P₂V₂/T₂

Variables & 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

Physical example

A sealed flexible gas sample can be compared before and after simultaneous compression and heating.

Topic 9.2Unit 9

The Ideal Gas Law

At fixed amount: P ∝ T/V

Variables & 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

Physical example

At fixed V, a P-versus-T(K) graph is linear and extrapolates toward zero pressure at zero kelvin in the ideal model.

Topic 9.3 · ModelUnit 9

Thermal Energy Transfer and Equilibrium

T_hot > T_cold → spontaneous thermal transfer hot → cold

Interpretation: 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

Physical example

A hot metal block placed in cooler water transfers energy to the water until their temperatures approach one another.

Topic 9.3 · ModelUnit 9

Thermal Energy Transfer and Equilibrium

Thermal equilibrium: T_A = T_B and net thermal transfer = 0

Interpretation: 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

Physical example

Two samples can still exchange microscopic energy in both directions at equilibrium, but there is no net transfer.

Topic 9.3 · ModelUnit 9

Thermal Energy Transfer and Equilibrium

Thermal transfer modes: conduction + convection + radiation

Interpretation: 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

Physical example

A hot cup loses energy by conduction through the cup, convection to moving air and thermal radiation to the surroundings.

Topic 9.4Unit 9

The First Law of Thermodynamics

U = (3/2)nRT = (3/2)Nk_B T

Variables & 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

Physical example

For a fixed amount of ideal monatomic gas, doubling T doubles U.

Topic 9.4Unit 9

The First Law of Thermodynamics

ΔU = Q + W_on

Variables & 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

Physical example

A compressed gas can gain internal energy even if no heating occurs because W_on is positive.

Topic 9.4Unit 9

The First Law of Thermodynamics

W_on = −P_ext ΔV; |W| = area under a P–V path

Variables & 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

Physical example

Expansion has ΔV>0 so W_on<0; compression has ΔV<0 so W_on>0.

Topic 9.5Unit 9

Specific Heat and Thermal Conductivity

Q = mcΔT

Variables & 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

Physical example

For the same Q and m, a material with larger c undergoes a smaller temperature change.

Topic 9.5Unit 9

Specific Heat and Thermal Conductivity

Q/Δt = kAΔT/L

Variables & 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

Physical example

Doubling insulation thickness halves the ideal steady conduction rate when other quantities remain fixed.

Topic 9.5Unit 9

Specific Heat and Thermal Conductivity

At fixed geometry and ΔT: conduction rate ∝ k

Variables & 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

Physical example

A high-k metal transfers energy faster than a low-k insulating material of the same size under the same temperature difference.

Topic 9.6 · ModelUnit 9

Entropy and the Second Law of Thermodynamics

Isolated system: total entropy never decreases

Interpretation: 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

Physical example

A hot object and a cold object inside an insulated enclosure spontaneously approach one common temperature; total entropy increases.

Topic 9.6 · ModelUnit 9

Entropy and the Second Law of Thermodynamics

Reversible ideal process: total entropy remains constant

Interpretation: 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

Physical example

An ideal reversible limit can connect equilibrium states without increasing total entropy.

Topic 9.6 · ModelUnit 9

Entropy and the Second Law of Thermodynamics

Irreversible spontaneous process: total entropy increases toward equilibrium

Interpretation: 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

Physical example

A gas freely expanding into an evacuated region spreads into more accessible configurations and increases total entropy.

Topic 10.1Unit 10

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

Physical example

If the separation doubles while charges and medium stay fixed, the force magnitude becomes one fourth as large.

Topic 10.1Unit 10

Electric Charge and Electric Force

q = ne

Variables & 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

Physical example

An object with 5×10⁶ excess electrons has q=−5×10⁶e.

Topic 10.1Unit 10

Electric Charge and Electric Force

F_net = vector sum of F_i

Variables & 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

Physical example

For three charges, determine each force direction first and add components rather than adding magnitudes.

Topic 10.2Unit 10

Conservation of Electric Charge and the Process of Charging

Q_system,f = Q_system,i + Q_transferred

Variables & 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

Physical example

If electrons enter an initially neutral isolated metal object, its final net charge is negative by exactly the transferred amount.

Topic 10.2Unit 10

Conservation of Electric Charge and the Process of Charging

Q_total,isolated = constant

Variables & 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

Physical example

Rubbing two initially neutral objects can leave equal-and-opposite net charges while the two-object total remains zero.

Topic 10.2Unit 10

Conservation of Electric Charge and the Process of Charging

induction/polarization: redistribution can occur with ΔQ_system = 0

Variables & 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

Physical example

A charged rod brought near a neutral conductor can attract the conductor even before contact because mobile charge separates.

Topic 10.3Unit 10

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

Physical example

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.

Topic 10.3Unit 10

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

Physical example

Doubling distance from an isolated point charge reduces field magnitude by a factor of four.

Topic 10.3Unit 10

Electric Fields

E_net = vector sum of E_i

Variables & 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

Physical example

Between equal unlike charges, the two field contributions at the midpoint point in the same direction and therefore add.

Topic 10.4Unit 10

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

Physical example

Like charges give positive U_E at finite separation; opposite charges give negative U_E with this reference.

Topic 10.4Unit 10

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

Physical example

For three charges, include the 1–2, 1–3 and 2–3 pair energies once each.

Topic 10.4Unit 10

Electric Potential Energy

W_ext,∞→configuration = U_E

Variables & 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

Physical example

External work is positive when like charges are slowly brought closer from very far apart.

Topic 10.5Unit 10

Electric Potential

V = U_E/q_test

Variables & 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

Physical example

If a +2 C test charge would have 6 J of electric potential energy at a point, that point is at 3 V.

Topic 10.5Unit 10

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

Physical example

A positive and negative source can give zero potential at a point even when the electric field there is not zero.

Topic 10.5Unit 10

Electric Potential

E_avg,parallel = −ΔV/Δs

Variables & 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

Physical example

Moving in the electric-field direction lowers electric potential; closely spaced equipotentials indicate a stronger field.

Topic 10.6Unit 10

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

Physical example

For a fixed capacitor, doubling Q doubles |ΔV|; C itself does not change.

Topic 10.6Unit 10

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

Physical example

Increasing plate area raises C; increasing separation lowers C; inserting a dielectric raises C and reduces the field for fixed free plate charge.

Topic 10.6Unit 10

Capacitors

U_C = ½Q|ΔV| = Q²/(2C) = ½C(ΔV)²

Variables & 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

Physical example

At fixed C, doubling voltage quadruples stored energy; at fixed Q, increasing C lowers stored energy.

Topic 10.7Unit 10

Conservation of Electric Energy

ΔU_E = qΔV

Variables & 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

Physical example

A positive charge moving to lower potential has ΔU_E<0; a negative charge has the opposite sign relation.

Topic 10.7Unit 10

Conservation of Electric Energy

ΔK = −ΔU_E = −qΔV

Variables & 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

Physical example

A released positive charge moving to lower potential gains kinetic energy equal to the electric potential-energy decrease.

Topic 10.7Unit 10

Conservation of Electric Energy

K_i + U_E,i = K_f + U_E,f

Variables & SI units: K kinetic energy (J); U_E electric potential energy (J)

Use when: closed conservative object–field system with no additional transfer terms

Physical example

An electron accelerated through a potential difference can be analyzed by the same energy bookkeeping once the charge sign is handled correctly.

Topic 11.1Unit 11

Electric Current

I = ΔQ/Δt

Variables & 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

Physical example

6 C crossing in 3 s corresponds to 2 A

Topic 11.1Unit 11

Electric Current

ΔQ = IΔt

Variables & SI units: ΔQ charge (C); I current (A); Δt time (s)

Use when: constant current over the interval

Physical example

0.50 A for 8 s transfers 4 C

Topic 11.1Unit 11

Electric Current

I = 0 ⇒ no net carrier motion

Variables & SI units: I current; carrier thermal motion may still be nonzero

Use when: distinguishing zero current from zero microscopic particle speed

Physical example

an open circuit can contain moving electrons microscopically while having zero net charge flow

Topic 11.2 · ModelUnit 11

Simple Circuits

closed loop ⇒ charge can flow

Interpretation: A closed conducting path permits sustained current when a source provides potential difference

Use when: qualitative circuit-state reasoning

Physical example

closing a switch completes the loop and allows current

Topic 11.2Unit 11

Simple Circuits

open path ⇒ I = 0 in that branch

Variables & SI units: I branch current (A)

Use when: a break interrupts the conducting path

Physical example

an open switch prevents current in its branch

Topic 11.2Unit 11

Simple Circuits

short path ≈ 0 Ω

Variables & SI units: R path resistance (Ω), ideally near zero

Use when: a low-resistance connection joins two points directly

Physical example

a wire placed across an element can bypass that element

Topic 11.3Unit 11

Resistance, Resistivity, and Ohm’s Law

R = ρL/A

Variables & SI units: R resistance (Ω); ρ resistivity (Ω·m); L length (m); A cross-sectional area (m²)

Use when: uniform conductor

Physical example

doubling length doubles resistance; doubling area halves resistance

Topic 11.3Unit 11

Resistance, Resistivity, and Ohm’s Law

ΔV = IR

Variables & SI units: ΔV potential difference (V); I current (A); R resistance (Ω)

Use when: ohmic element under fixed physical conditions

Physical example

a 4 Ω resistor carrying 2 A has 8 V across it

Topic 11.3 · ModelUnit 11

Resistance, Resistivity, and Ohm’s Law

slope depends on axes

Interpretation: for ΔV vs I, slope = R; for I vs ΔV, slope = 1/R

Use when: interpreting experimental current-voltage graphs

Physical example

always read axis labels before converting graph slope into resistance

Topic 11.4Unit 11

Electric Power

P = IΔV

Variables & 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

Physical example

12 V across a device carrying 2 A corresponds to 24 W

Topic 11.4Unit 11

Electric Power

P = I²R

Variables & SI units: P power (W); I current (A); R resistance (Ω)

Use when: resistive element with current known

Physical example

at fixed current, doubling R doubles power

Topic 11.4Unit 11

Electric Power

P = (ΔV)²/R

Variables & SI units: P power (W); ΔV potential difference (V); R resistance (Ω)

Use when: resistive element with potential difference known

Physical example

at fixed voltage, doubling R halves power

Topic 11.5Unit 11

Compound Direct Current (DC) Circuits

R_series = ΣR_i

Variables & SI units: R_series equivalent resistance (Ω); R_i component resistances (Ω)

Use when: components carrying the same current with no branching between them

Physical example

3 Ω and 5 Ω in series give 8 Ω

Topic 11.5Unit 11

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

Physical example

two identical resistors in parallel have half the resistance of either one

Topic 11.5Unit 11

Compound Direct Current (DC) Circuits

I_source = ΔV_source/R_eq

Variables & 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

Physical example

reduce valid subgroups first, then determine total source current

Topic 11.6Unit 11

Kirchhoff’s Loop Rule

ΣΔV_loop = 0

Variables & SI units: ΔV signed potential changes (V)

Use when: any closed loop in the lumped circuit model

Physical example

source rises and resistor drops sum to zero

Topic 11.6Unit 11

Kirchhoff’s Loop Rule

ΔU_E = qΔV

Variables & 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

Physical example

a positive charge gains electric potential energy when it moves through a potential rise

Topic 11.6Unit 11

Kirchhoff’s Loop Rule

ideal wire: ΔV = 0

Variables & SI units: ΔV potential difference (V)

Use when: points connected only by an ideal wire

Physical example

all points on one ideal-wire node share the same potential

Topic 11.7Unit 11

Kirchhoff’s Junction Rule

ΣI_in = ΣI_out

Variables & SI units: I branch currents (A)

Use when: steady-state junction

Physical example

3 A entering and 1 A leaving one branch requires 2 A to leave through the remaining branch

Topic 11.7Unit 11

Kirchhoff’s Junction Rule

ΣI_signed = 0

Variables & SI units: I signed branch currents (A)

Use when: algebraic node equation with a consistent sign convention

Physical example

take entering currents positive and leaving currents negative, or vice versa

Topic 11.7Unit 11

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

Physical example

source current equals the sum of parallel-branch currents

Topic 11.8Unit 11

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

Physical example

series equivalent capacitance is smaller than the smallest individual capacitance

Topic 11.8Unit 11

Resistor-Capacitor (RC) Circuits

C_parallel = ΣC_i

Variables & SI units: C_parallel equivalent capacitance (F); C_i capacitances (F)

Use when: capacitors connected across the same two nodes

Physical example

parallel capacitances add directly

Topic 11.8Unit 11

Resistor-Capacitor (RC) Circuits

τ = RC

Variables & 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

Physical example

after one time constant charging reaches about 63% of final charge while discharging retains about 37% of its initial charge

Topic 12.1 · ModelUnit 12

Magnetic Fields

magnetic field lines form closed loops

Interpretation: 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

Physical example

outside a bar magnet the field points away from the north pole and toward the south pole, then continues through the magnet

Topic 12.1 · ModelUnit 12

Magnetic Fields

dipole alignment → magnetic response

Interpretation: magnetic-domain/dipole alignment; qualitative relationship

Use when: comparing permanent, induced, paramagnetic, and diamagnetic behavior

Physical example

a ferromagnetic sample can retain substantial alignment after an external field is removed, whereas a paramagnetic sample does not

Topic 12.1 · ModelUnit 12

Magnetic Fields

μ₀ = 4π × 10⁻⁷ T·m/A

Interpretation: μ₀ vacuum permeability; T tesla; m meter; A ampere

Use when: recognizing the free-space permeability constant used in later magnetic-field equations

Physical example

the long-straight-wire field model in Topic 12.3 uses μ₀

Topic 12.2Unit 12

Magnetism and Moving Charges

F_B = |q|vB sinθ

Variables & 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°

Physical example

for v perpendicular to B, F_B=|q|vB; for v parallel or antiparallel to B, F_B=0

Topic 12.2Unit 12

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

Physical example

doubling speed doubles the radius while doubling B halves the radius

Topic 12.2 · ModelUnit 12

Magnetism and Moving Charges

qE and qvB act independently

Interpretation: 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

Physical example

in perpendicular crossed fields, equal and opposite electric and magnetic forces can transmit a selected particle speed

Topic 12.3Unit 12

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

Physical example

doubling I doubles B; doubling r halves B

Topic 12.3Unit 12

Magnetism and Current-Carrying Wires

F_B = IℓB sinθ

Variables & 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

Physical example

a wire perpendicular to B experiences maximum force; a parallel wire experiences zero force

Topic 12.3Unit 12

Magnetism and Current-Carrying Wires

B_net = vector sum of source fields

Variables & 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

Physical example

fields in opposite directions subtract in magnitude, while fields in the same direction add

Topic 12.4Unit 12

Electromagnetic Induction and Faraday’s Law

Φ_B = BA cosθ

Variables & 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

Physical example

flux is maximum in magnitude when B is parallel to the area vector and zero when B lies in the surface plane

Topic 12.4Unit 12

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

Physical example

doubling the flux change in the same time doubles the emf magnitude

Topic 12.4Unit 12

Electromagnetic Induction and Faraday’s Law

ε = Bℓv

Variables & 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

Physical example

doubling rod speed doubles the motional emf

Topic 13.1Unit 13

Reflection

θ_i = θ_r

Variables & 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

Physical example

a ray arriving 35° from the normal leaves 35° from the normal on the other side

Topic 13.1 · ModelUnit 13

Reflection

ray direction ⟂ wavefront

Interpretation: ray direction and wavefront orientation; geometric relationship

Use when: geometric-optics situations where the wave nature of light can be neglected

Physical example

parallel planar wavefronts correspond to parallel light rays normal to those wavefronts

Topic 13.1 · ModelUnit 13

Reflection

local normal variation → diffuse or specular reflection

Interpretation: local surface normal direction; qualitative model

Use when: comparing rough and smooth reflecting surfaces

Physical example

paper can look bright from many viewing directions because different microscopic patches have different normals

Topic 13.2Unit 13

Images Formed by Mirrors

1/f = 1/s_o + 1/s_i

Variables & 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

Physical example

a concave mirror with an object beyond its focal point can produce a positive real-image distance

Topic 13.2Unit 13

Images Formed by Mirrors

M = h_i/h_o = −s_i/s_o

Variables & 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

Physical example

negative M represents an inverted image under the stated sign convention

Topic 13.2Unit 13

Images Formed by Mirrors

f = R/2 for a spherical mirror

Variables & SI units: f focal length (m); R signed radius of curvature (m)

Use when: concave or convex spherical mirrors in the geometric/paraxial model

Physical example

a concave spherical mirror with R=40 cm has |f|=20 cm

Topic 13.3Unit 13

Refraction

n = c/v

Variables & 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

Physical example

larger n corresponds to smaller light speed v

Topic 13.3Unit 13

Refraction

n₁ sinθ₁ = n₂ sinθ₂

Variables & 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

Physical example

air-to-glass transmission bends toward the normal because n increases

Topic 13.3Unit 13

Refraction

sinθ_c = n₂/n₁

Variables & SI units: θ_c critical angle; n₁ higher refractive index; n₂ lower refractive index

Use when: critical-angle calculation only when n₁>n₂

Physical example

for glass-to-air, incidence greater than θ_c produces total internal reflection

Topic 13.4Unit 13

Images Formed by Lenses

1/f = 1/s_o + 1/s_i

Variables & 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

Physical example

a converging lens with an object beyond f can form a real image on the transmitted side

Topic 13.4Unit 13

Images Formed by Lenses

M = h_i/h_o = −s_i/s_o

Variables & 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

Physical example

negative magnification corresponds to an inverted real image under the stated convention

Topic 13.4 · ModelUnit 13

Images Formed by Lenses

principal rays locate the image

Interpretation: 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

Physical example

two correctly drawn principal rays are sufficient to locate an image, while a third provides a consistency check

Topic 14.1Unit 14

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

Physical example

increasing tension raises wave speed; increasing linear density lowers it

Topic 14.1Unit 14

Properties of Wave Pulses and Waves

μ = m/ℓ

Variables & 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

Physical example

a 0.020 kg string 2.0 m long has μ=0.010 kg/m

Topic 14.1 · ModelUnit 14

Properties of Wave Pulses and Waves

greater amplitude → greater transported energy

Interpretation: qualitative model statement; compare otherwise similar waves in the same medium

Use when: comparing how much energy similar wave disturbances carry

Physical example

a larger-amplitude sound wave is associated with greater intensity/loudness than an otherwise similar smaller-amplitude wave

Topic 14.2Unit 14

Periodic Waves

v = fλ

Variables & 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

Physical example

at v=12 m/s and f=4 Hz, λ=3 m

Topic 14.2Unit 14

Periodic Waves

T = 1/f

Variables & SI units: T period (s); f frequency (Hz)

Use when: converting between temporal repeat time and cycles per second

Physical example

a 50 Hz wave has T=0.020 s

Topic 14.2Unit 14

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

Physical example

successive crests are separated by one wavelength

Topic 14.3Unit 14

Boundary Behavior of Waves and Polarization

f_reflected = f_transmitted = f_incident

Variables & 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

Physical example

the transmitted wavelength can change when speed changes even though frequency does not

Topic 14.3Unit 14

Boundary Behavior of Waves and Polarization

I = P_avg/A

Variables & 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

Physical example

6 W distributed across 2 m² corresponds to 3 W/m²

Topic 14.3 · ModelUnit 14

Boundary Behavior of Waves and Polarization

transmitted speed decreases → reflected pulse inverted

Interpretation: qualitative boundary model; compare wave speed before and after the boundary

Use when: predicting reflected-pulse orientation for the boundary model

Physical example

a pulse reflecting where the transmitted-wave speed is lower returns inverted; if transmitted speed is higher, it returns without inversion

Topic 14.4Unit 14

Electromagnetic Waves

c = fλ

Variables & SI units: c vacuum light speed (m/s); f frequency (Hz); λ vacuum wavelength (m)

Use when: electromagnetic radiation propagating in vacuum

Physical example

higher-frequency electromagnetic radiation has shorter wavelength

Topic 14.4 · ModelUnit 14

Electromagnetic Waves

E ⟂ B ⟂ propagation

Interpretation: E electric-field direction; B magnetic-field direction; qualitative vector geometry

Use when: plane electromagnetic-wave representation

Physical example

if the wave travels in +x and E oscillates along y, B is perpendicular to both

Topic 14.4 · ModelUnit 14

Electromagnetic Waves

radio → microwave → infrared → visible → ultraviolet → X-ray → gamma

Interpretation: qualitative ordering from longer wavelength/lower frequency toward shorter wavelength/higher frequency

Use when: classifying electromagnetic radiation without memorizing exact wavelength cutoffs

Physical example

visible light lies between infrared and ultraviolet in the spectrum

Topic 14.5 · ModelUnit 14

The Doppler Effect

approaching → f_observed > f_rest

Interpretation: qualitative comparison of observed and rest frequency

Use when: source and observer move toward one another

Physical example

an approaching siren is heard at a higher frequency than when there is no relative motion

Topic 14.5 · ModelUnit 14

The Doppler Effect

receding → f_observed < f_rest

Interpretation: qualitative comparison of observed and rest frequency

Use when: source and observer move away from one another

Physical example

after the siren passes and moves away, the observed frequency is lower

Topic 14.5 · ModelUnit 14

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

Physical example

a faster approach produces a larger upward frequency shift than a slower approach

Topic 14.6Unit 14

Wave Interference and Standing Waves

y_total = Σy_i

Variables & SI units: y_total resultant displacement (m); y_i individual wave displacements (m)

Use when: linear superposition when waves overlap

Physical example

equal and opposite pulses can momentarily cancel before continuing through each other

Topic 14.6Unit 14

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

Physical example

440 Hz and 444 Hz produce 4 beats per second

Topic 14.6Unit 14

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

Physical example

a closed-open air column supports odd quarter-wavelength modes

Topic 14.7Unit 14

Diffraction

a sinθ_m = mλ

Variables & SI units: a slit width (m); θ_m dark-minimum angle; m=1,2,…; λ wavelength (m)

Use when: single-slit diffraction minima

Physical example

a narrower slit makes the first minimum occur at a larger angle

Topic 14.7Unit 14

Diffraction

y_m ≈ mλL/a

Variables & 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

Physical example

increasing screen distance spreads the observed pattern

Topic 14.7Unit 14

Diffraction

central maximum width ≈ 2λL/a

Variables & 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

Physical example

doubling λ approximately doubles the central-maximum width

Topic 14.8Unit 14

Double-Slit Interference and Diffraction Gratings

d sinθ_m = mλ

Variables & 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

Physical example

longer wavelength produces a larger angle at the same order and spacing

Topic 14.8Unit 14

Double-Slit Interference and Diffraction Gratings

y_m ≈ mλL/d

Variables & 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

Physical example

larger slit separation moves neighboring fringes closer together

Topic 14.8Unit 14

Double-Slit Interference and Diffraction Gratings

d = 1/N

Variables & SI units: d grating spacing (m); N line density (lines/m)

Use when: converting grating line density to opening spacing

Physical example

600 lines/mm corresponds to d≈1.67×10⁻⁶ m

Topic 14.9Unit 14

Thin-Film Interference

optical path difference = 2nt

Variables & 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

Physical example

changing thickness changes which wavelengths reinforce or cancel

Topic 14.9Unit 14

Thin-Film Interference

one net phase reversal: constructive 2nt=(m+1/2)λ₀; destructive 2nt=mλ₀

Variables & 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

Physical example

an oil film can enhance different colors as its thickness varies

Topic 14.9Unit 14

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

Physical example

a coating can suppress reflection of a chosen wavelength by making the two reflected rays arrive out of phase

Topic 15.1Unit 15

Quantum Theory and Wave-Particle Duality

E = hf

Variables & 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

Physical example

a higher-frequency photon carries more energy

Topic 15.1Unit 15

Quantum Theory and Wave-Particle Duality

pγ = h/λ

Variables & SI units: pγ photon momentum (kg·m/s); h Planck constant; λ photon wavelength (m)

Use when: photon momentum and momentum-transfer reasoning

Physical example

a shorter-wavelength photon carries greater momentum

Topic 15.1Unit 15

Quantum Theory and Wave-Particle Duality

λdB = h/p

Variables & SI units: λdB de Broglie wavelength (m); h Planck constant; p particle momentum (kg·m/s)

Use when: matter-wave behavior of a particle

Physical example

increasing a particle’s momentum decreases its de Broglie wavelength

Topic 15.2Unit 15

The Bohr Model of Atomic Structure

A = Z + Nn

Variables & SI units: A nucleon (mass) number; Z proton (atomic) number; Nn neutron number

Use when: nuclear notation and isotope bookkeeping

Physical example

carbon-14 has Z=6 and therefore Nn=8 neutrons

Topic 15.2Unit 15

The Bohr Model of Atomic Structure

ke²/r² = mv²/r

Variables & 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

Physical example

changing allowed radius changes the electric force and model orbital speed

Topic 15.2Unit 15

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

Physical example

only circumferences containing an integer number of de Broglie wavelengths satisfy the standing-wave condition

Topic 15.3Unit 15

Emission and Absorption Spectra

|ΔE| = hf

Variables & 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

Physical example

a larger level gap corresponds to a higher-frequency photon

Topic 15.3Unit 15

Emission and Absorption Spectra

|ΔE| = hc/λ

Variables & 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

Physical example

larger energy gaps produce shorter wavelengths

Topic 15.3Unit 15

Emission and Absorption Spectra

absorption: Ef = Ei + hf; emission: hf = Ei − Ef

Variables & 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

Physical example

an upward arrow requires photon absorption; a downward arrow corresponds to photon emission

Topic 15.4Unit 15

Blackbody Radiation

λmax T = b

Variables & 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

Physical example

a hotter blackbody peaks at a shorter wavelength

Topic 15.4Unit 15

Blackbody Radiation

P = σAT⁴

Variables & 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

Physical example

doubling T at fixed A increases P by a factor of 16

Topic 15.4Unit 15

Blackbody Radiation

P₂/P₁ = (A₂/A₁)(T₂/T₁)⁴

Variables & 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

Physical example

at equal area, a 20% temperature increase raises power by (1.2)⁴

Topic 15.5Unit 15

The Photoelectric Effect

Kmax = hf − φ

Variables & 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

Physical example

at fixed material, increasing frequency raises Kmax linearly

Topic 15.5Unit 15

The Photoelectric Effect

eVs = Kmax

Variables & SI units: e elementary-charge magnitude (C); Vs stopping-potential magnitude (V); Kmax maximum kinetic energy (J)

Use when: ideal stopping-potential measurement

Physical example

a 2.0 eV maximum kinetic energy corresponds to a 2.0 V stopping-potential magnitude

Topic 15.5Unit 15

The Photoelectric Effect

f0 = φ/h

Variables & SI units: f0 threshold frequency (Hz); φ work function (J); h Planck constant

Use when: onset of photoelectric emission

Physical example

below f0, raising intensity does not cause emission in the one-photon model

Topic 15.6Unit 15

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

Physical example

θ=0 gives no Compton wavelength shift; backscatter gives the maximum shift

Topic 15.6Unit 15

Compton Scattering

pγ = h/λ

Variables & SI units: pγ photon momentum (kg·m/s); h Planck constant; λ photon wavelength (m)

Use when: incident or scattered photon momentum

Physical example

because λf>λi after an energy-transferring scatter, the photon momentum decreases

Topic 15.6Unit 15

Compton Scattering

Eγ = hc/λ

Variables & SI units: Eγ photon energy (J); h Planck constant; c light speed; λ wavelength (m)

Use when: photon energy before and after scattering

Physical example

a longer scattered wavelength means lower photon energy, with the difference transferred to the electron/system

Topic 15.7Unit 15

Fission, Fusion, and Nuclear Decay

ΔE = Δmc²

Variables & 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

Physical example

a small decrease in total rest mass can appear as kinetic energy of products and/or photon energy

Topic 15.7Unit 15

Fission, Fusion, and Nuclear Decay

λ = ln(2)/t1/2

Variables & SI units: λ decay constant (s⁻¹); t1/2 half-life (s)

Use when: connecting the exponential decay rate to half-life

Physical example

a shorter half-life corresponds to a larger decay constant

Topic 15.7Unit 15

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

Physical example

after three half-lives the expected remaining population is N0/8

Topic 15.8 · ModelUnit 15

Types of Radioactive Decay

alpha: A→A−4, Z→Z−2 + ⁴₂He

Interpretation: A parent nucleon number; Z parent proton number; emitted alpha has A=4 and Z=2

Use when: alpha-decay nuclear bookkeeping

Physical example

the daughter has four fewer nucleons and two fewer protons than the parent

Topic 15.8 · ModelUnit 15

Types of Radioactive Decay

β−: n→p + e− + anti-ν; β+: p→n + e+ + ν

Interpretation: 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

Physical example

β− raises daughter Z by 1 at fixed A; β+ lowers daughter Z by 1 at fixed A

Topic 15.8 · ModelUnit 15

Types of Radioactive Decay

gamma: excited nucleus → lower-energy same nucleus + γ

Interpretation: γ photon; parent and daughter retain the same A and Z

Use when: gamma de-excitation after an excited nuclear state

Physical example

gamma emission changes nuclear energy but not the element or isotope identity

Equation-selection guide

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, moleculesideal-gas and kinetic-theory relationshipsabsolute temperature, particle count vs moles, process conditions
charge arrangement, force, field, potentialCoulomb/field/potential/energy modelsvector vs scalar quantity, sign of charge, reference point
current, voltage, resistance, brightness, chargingcircuit conservation, power and RC modelsseries/parallel structure, junction/loop rules, time dependence
moving charge/current in a magnetic fieldLorentz force and magnetic-field relationshipsangle, direction rule, whether magnetic force does work
changing magnetic fluxinduction and Faraday/Lenz reasoningwhat changes flux: field, area, angle or loop motion?
image location, size, focus, refractionray geometry, Snell, mirror/lens and magnificationsign convention and whether image is real or virtual
fringe spacing, resonance, diffraction, phasewave speed, standing-wave and interference modelsboundary condition, path difference, phase shifts, small-angle use
photon energy, wavelength, emission, ejected electronsquantum/photon and photoelectric relationshipsfrequency vs intensity, threshold/work function, energy units
nuclear mass change, half-life, activitymass-energy and decay relationshipsmass defect, exponential/half-life model, conserved quantities
Common formula mistakes

Errors that look mathematical but are actually model errors

Use these checks before blaming algebra.

Using Celsius in an absolute-temperature relationshipConvert to kelvin when the physics depends on absolute temperature.
Treating electric field and electric potential as the same kind of quantityField is a vector; potential is a scalar.
Assuming current is “used up” in a resistorCharge flow is constrained by circuit conservation; energy transfer is the relevant loss.
Using magnetic force as if it changes kinetic energyA magnetic force perpendicular to velocity changes direction, not speed.
Ignoring optical or interference sign/phase conventionsWrite the convention before applying the equation.
Substituting before checking unitsCarry units through the setup so dimensional errors appear before the final line.
Formula-sheet questions

Short answers to the most common reference-sheet searches

The interactive library above is the main tool; these answers clarify how to use it.

Is the AP Physics 2 equation sheet the same as the formula sheet?

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.

How many relationships are on this page?

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.

Should I memorize every equation?

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.

What is the fastest way to find a formula?

Search the physical quantity or concept—such as capacitance, induced emf, Doppler, focal length or photoelectric effect—then filter by unit if needed.

Why are conditions shown on every formula card?

Because many wrong answers come from using a mathematically correct relationship outside the model where it applies.

Can I print this page?

Yes. Use the “Print / Save PDF” button in the formula finder. Print styling hides navigation and preserves the reference content.