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Newton’s second law
F = ma
Momentum
p = mv
Reduced mass of a two-body system
μ = m1m2/(m1 + m2)
Kinetic energy
K = 1/2(mv²) = p²/(2m)
Work
W = integral(F· dr)
Newton’s universal law of gravitation
F = Gm1m2/r²
Torque
τ = Iα
Angular momentum
L = r x p
Moment of Inertia (parallel axis theorem)
I = Icm + md²
Rotational Kinetic Energy
K = 1/2(Iω²)
Centripetal Acceleration
a = v²/r
Period (uniform circular motion)
T = 2πr/v
Angular velocity
ω = 2π/T = v/r
Cyclotron angular frequency of a charged particle moving in a magnetic field
ω = qB/m
Period (simple pendulum)
T = 2πsqrt(L/g)
Spring force
F = −k∆x
Potential energy of a stretched/compressed spring
U = 1/2k∆x²
Electric potential (point charge)
V(r) = q/4πε0r
Electric Field/Electric Potential relation
E(r) = −∇V(r)
Force on a charged particle in a uniform E-field
F = qE
Gauss’ Law
surface integral(E · da) = 1/ε0 volume integral(ρdV)
Force on a charged particle in a uniform magnetic field
F = qv × B
Biot-Savart Law
dB = (μ0I/4π) integral((dℓ’ x (r - r’))/|r - r’|³
Ampere’s Law (integral form)
loop integral(B · dl) = μ0 surface integral(J · da)
Faraday’s Law of induction
loop integral(E · dl) = -(d/dt) surface integral(B · da)
solenoid magnetic flux
Φ = NAB
Faraday’s Law (solenoid)
EMF = -dΦ/dt
Maxwell’s equations
∇ x H = J + ∂D/∂t
∇ x E = -∂B/∂t
∇ · D = ρ
∇ · B = 0
Poynting Vector
S = E x H
relationship between magnetic permeability, vacuum permeability, and speed of light
μ0 ε0 = 1/c²
Ohm’s Law (alternating current)
U = ZI
Impedance of an RLC circuit
Z = R + iωL + 1/iωC
Impedance (in series)
Z = Z1 + Z2 + . . .
Impedance (in parallel)
1/Z = 1/Z1 + 1/Z2 + . . .
Power (AC circuit)
P (t) = Re(I(t)) Im(V (t))
Doppler effect (sound)
f = ((c ± vr) / (c ± vs)) f0
Index of refraction
n = c/v
Snell’s law
n1sinθ1 = n2sinθ2
Focal length of a refracting telescope
l = fobjective + feyepiece
Magnification of a refracting telescope
M = fobjective/feyepiece
Work done on an ideal gas during a volume change
W = −integral from Vi to Vf (PdV)
COP (efficiency) of a refrigerator
COP ≤ Tc / (Th - Tc)
Maxwell-Boltzmann Speed Distribution Function
D(v) = (m/2πkBT)3/24πv²e-mv²/2kBT
Energy of a photon
E = hf
momentum operator
p = -ihbar∇
position-momentum commutation relation
[x,p] = ihbar
angular momentum magnitude squared-angular momentum vector commutation relation
[J², J] = 0
angular momentum x and y components commutation relation
[Jx, Jy] = ihbarJz
Pauli matrices product identity
σjσk = δjk + i ϵjkl σl
Infinite square well energy
En = n²π²hbar²/2ma²
harmonic oscillator energy
En = (n+1/2)hbarω
Characteristic energies (hydrogen-like atoms)
En = -(me(Ze²)²/2(4πε0)²hbar²)(1/n²)
Allowed quantum numbers (hydrogen-like atoms)
n = 1, 2, 3, …
l = 0, 1, … (n-1)
m = -l, … +l
β (special relativity)
β = v/c
Lorentz factor (special relativity)
γ = 1/sqrt(1-β²)
momentum of a relativistic particle
p = γm0v
Energy-momentum relation (special relativity)
E² = (pc)² + (m0c²)²
length contraction
l’ = l0/γ
time dilation
∆t′ = γ∆t0
relativistic Doppler effect
f = sqrt((1 ± β)/ (1 ∓ β)) f0
Poisson uncertainty
σ = sqrt(N)
error propagation
σ²X = sum over i[(∂X/∂zi)²σ²zi]
Lagrangian
L = T - U
Hamilton’s principle
partial L / partial x - d/dt partial L / partial xdot = 0
Hamiltonian
H = sum of piqdoti - L
Hamilton’s Equations
partial H / partial pi = qdoti
partial H / partial qdoti = -pdoti
force of friction
f = muN
Energy stored on a capacitor
E = ½ CV²
image location (mirrors)
1/image distance = 1/focal length - 1/object distance
image location (lenses)
1/ focal length = 1/object distance + 1/image distance
Rayleigh criterion
theta = 1.22 lambda/D