Physics isn't just a collection of equations—it's built on a foundation of universal constants that appear again and again across every topic you'll encounter. In AP Physics 2, you're being tested on your ability to recognize why certain constants appear in specific contexts: why Coulomb's constant shows up in electric force calculations, why Planck's constant governs photon energy, and why the elementary charge defines the smallest unit of charge in nature. These constants aren't arbitrary numbers to memorize; they're the bridge between abstract physics principles and real, measurable phenomena.
Understanding fundamental constants means understanding the deep connections between electromagnetism, quantum mechanics, and thermodynamics. When you see k=8.99×109 N\cdotpm2/C2 in a Coulomb's law problem, you should immediately think inverse-square force law and permittivity of free space. When Planck's constant appears, you should recognize energy quantization and wave-particle duality. Don't just memorize values—know what concept each constant illustrates and which equations it belongs to.
Electromagnetic Constants
These constants define how electric and magnetic fields behave in vacuum and govern all electrostatic and magnetostatic calculations. They emerge from the fundamental nature of how charges create fields and how fields exert forces.
Elementary Charge (e)
e=1.602×10−19 C—the smallest indivisible unit of free charge in nature, carried by protons (+e) and electrons (−e)
Charge quantization means all observable charges are integer multiples of e; you'll never encounter 0.5e in any problem
Directly tested in Coulomb's law problems where you calculate forces between protons, electrons, or ions
Coulomb Constant (k)
k=8.99×109 N·m²/C²—determines the strength of electrostatic force between point charges via F=kr2∣q1q2∣
Related to permittivity by k=4πε01, connecting it to how vacuum "permits" electric fields
Inverse-square dependence on distance mirrors gravitational force, making comparison questions common on exams
Permittivity of Free Space (ε₀)
ε0=8.85×10−12 F/m—quantifies how easily vacuum allows electric field lines to pass through
Appears in capacitance calculations (C=ε0dA for parallel plates) and electric field equations
Dielectric constantεr multiplies ε0 when fields pass through materials other than vacuum
Permeability of Free Space (μ₀)
μ0=4π×10−7 N/A²—measures vacuum's ability to support magnetic field lines from moving charges
Essential for inductance and magnetic field calculations in circuits and electromagnetism
Connects to speed of light through c=μ0ε01, unifying electricity, magnetism, and optics
Compare:ε0 vs. μ0—both describe vacuum's electromagnetic properties, but ε0 governs electric fields while μ0 governs magnetic fields. If an FRQ asks about electromagnetic wave propagation, remember they combine to give c.
Quantum Mechanical Constants
These constants reveal that energy, momentum, and matter behave in discrete, quantized ways at atomic scales. They replace classical continuous values with allowed "steps" that govern photons, electrons, and atomic transitions.
Planck's Constant (h)
h=6.626×10−34 J·s—the fundamental constant of quantum mechanics, relating photon energy to frequency via E=hf
Quantization signature: whenever you see h, think discrete energy levels and wave-particle duality
Appears in Bohr model (angular momentum L=n2πh), Compton scattering (Δλ=mech(1−cosθ)), and de Broglie wavelength (λ=ph)
Electron Mass (mₑ)
me=9.109×10−31 kg—determines electron behavior in atoms, fields, and quantum systems
Compton wavelengthmech sets the scale for photon-electron scattering wavelength shifts
Bohr model calculations use me to determine orbital radii and energy levels in hydrogen
Proton Mass (mₚ)
mp=1.673×10−27 kg—roughly 1836 times the electron mass, dominating atomic mass
Nuclear mass comes almost entirely from protons and neutrons; electrons contribute negligibly
Force comparisons: the same charge but vastly different mass means protons accelerate much less than electrons in electric fields
Compare:me vs. mp—both carry elementary charge e, but the proton's ~1836× greater mass means electrons dominate atomic-scale motion and energy levels. Exam questions often ask why electrons, not protons, determine chemical and optical properties.
Speed of Light and Relativity
The speed of light connects space, time, and energy, serving as the ultimate speed limit and appearing in both electromagnetic and quantum contexts.
Speed of Light in Vacuum (c)
c=3.00×108 m/s—the maximum speed for information and energy transfer in the universe
Electromagnetic connection: c=μ0ε01 shows light is an electromagnetic wave
Photon calculations use c=fλ to convert between frequency and wavelength; essential for spectral line problems
Compare:c in electromagnetism vs. quantum mechanics—in Maxwell's equations, c emerges from ε0 and μ0; in quantum physics, it appears in photon momentum (p=λh=cE) and rest energy (E=mec2). Same constant, different conceptual roles.
Thermodynamic Constants
These constants bridge the microscopic world of particles with macroscopic measurements like temperature and pressure. They translate between individual molecular behavior and bulk properties you can measure in a lab.
Boltzmann Constant (k_B)
kB=1.381×10−23 J/K—converts temperature into average molecular kinetic energy via KEˉ=23kBT
Entropy connection: Boltzmann's entropy formula S=kBlnW links microscopic states to thermodynamic entropy
Bridges scales: multiplying by Avogadro's number gives the gas constant (R=NAkB), connecting particle physics to chemistry
Avogadro's Number (N_A)
NA=6.022×1023 mol⁻¹—the number of particles in one mole, enabling atomic-to-macroscopic conversions
Molar mass connection: allows you to convert between mass in grams and number of atoms or molecules
Thermodynamics link: appears when relating per-particle constants (kB) to per-mole constants (R)
Compare:kB vs. R—both relate temperature to energy, but kB works at the single-particle level while R=NAkB works for moles of gas. Know which to use based on whether you're thinking microscopically or macroscopically.
Gravitational Constant
While less central to AP Physics 2 than electromagnetism, the gravitational constant provides crucial comparison points for understanding force laws.
Gravitational Constant (G)
G=6.674×10−11 N·m²/kg²—determines gravitational attraction strength via F=Gr2m1m2
Inverse-square parallel: same mathematical form as Coulomb's law, making force-law comparisons a common exam topic
Vastly weaker: electric forces between protons are ~1036 times stronger than gravitational forces, explaining why gravity is negligible at atomic scales
Compare: Coulomb's law vs. Newton's gravitational law—both are inverse-square, but electric forces can attract or repel while gravity only attracts. Exam questions often ask you to calculate the ratio FgFe for proton-electron pairs.
Quick Reference Table
Concept
Best Examples
Electric force and fields
e, k, ε0
Magnetic fields and circuits
μ0, e
Photon energy and quantum transitions
h, c, me
Bohr model and atomic structure
h, me, e, k
Compton scattering
h, me, c
Thermodynamics and entropy
kB, NA
Electromagnetic wave speed
c, ε0, μ0
Force law comparisons
k, G, e
Self-Check Questions
Which two constants combine to give the speed of light, and what equation relates them?
In the Bohr model, which constants appear in the quantization of angular momentum, and why does this lead to discrete energy levels?
Compare the roles of ε0 and k—how are they mathematically related, and when would you use each in a problem?
If an FRQ asks you to compare the electric and gravitational forces between a proton and electron, which constants do you need, and why is the ratio so extreme?
How does Planck's constant appear differently in photon energy (E=hf) versus Compton scattering (Δλ=mech(1−cosθ))? What physical principle does each equation illustrate?
Fundamental Constants in Physics to Know for AP Physics 2