Vectors are bold ($\mathbf{F}$) or arrow-notation ($\vec{F}$). Scalar magnitudes are italic ($F$). SI units throughout. Time derivatives use dot notation ($\dot{x} = dx/dt$) or Leibniz notation as appropriate.
| Constant | Symbol | Value | MATLAB |
|---|---|---|---|
| Speed of light | $c$ | $2.998 \times 10^8$ m/s | c = 2.998e8; |
| Gravitational constant | $G$ | $6.674 \times 10^{-11}$ N·m²/kg² | G = 6.674e-11; |
| Surface gravity (Earth) | $g$ | $9.807$ m/s² | g = 9.807; |
| Boltzmann constant | $k_B$ | $1.381 \times 10^{-23}$ J/K | kB = 1.381e-23; |
| Stefan–Boltzmann | $\sigma$ | $5.670 \times 10^{-8}$ W/(m²·K⁴) | sigma = 5.670e-8; |
| Planck's constant | $h$ | $6.626 \times 10^{-34}$ J·s | h = 6.626e-34; |
| Reduced Planck | $\hbar$ | $1.055 \times 10^{-34}$ J·s | hbar = h/(2*pi); |
| Elementary charge | $e$ | $1.602 \times 10^{-19}$ C | e = 1.602e-19; |
| Coulomb constant | $k_e$ | $8.988 \times 10^9$ N·m²/C² | ke = 8.988e9; |
| Permittivity of free space | $\varepsilon_0$ | $8.854 \times 10^{-12}$ F/m | eps0 = 8.854e-12; |
| Permeability of free space | $\mu_0$ | $4\pi \times 10^{-7}$ H/m | mu0 = 4*pi*1e-7; |
| Electron mass | $m_e$ | $9.109 \times 10^{-31}$ kg | me = 9.109e-31; |
| Proton mass | $m_p$ | $1.673 \times 10^{-27}$ kg | mp = 1.673e-27; |
| Avogadro's number | $N_A$ | $6.022 \times 10^{23}$ mol⁻¹ | NA = 6.022e23; |
| Gas constant | $R$ | $8.314$ J/(mol·K) | R = 8.314; |
| Earth mass | $M_E$ | $5.972 \times 10^{24}$ kg | ME = 5.972e24; |
| Earth radius | $R_E$ | $6.371 \times 10^6$ m | RE = 6.371e6; |
LaTeX: v = v_0 + at \qquad x = x_0 + v_0 t + \tfrac{1}{2}at^2
v0 = 0; a = 9.81; t = 5; % free fall from rest
v = v0 + a*t; % 49.05 m/s
x = v0*t + 0.5*a*t^2; % 122.6 m
v0 = 30; theta = deg2rad(45); g = 9.81;
R = v0^2*sin(2*theta)/g; % 91.74 m range
h_max = v0^2*sin(theta)^2/(2*g); % 22.94 m max height
t_flight = 2*v0*sin(theta)/g; % 4.33 s total flight
r = 5; v = 10;
ac = v^2/r; % 20 m/s² centripetal
omega = v/r; % 2 rad/s
T = 2*pi/omega; % 3.14 s period
Velocity of A relative to C = velocity of A relative to B + velocity of B relative to C.
m = 10; a = 3;
F = m*a; % 30 N
m = 75; g = 9.81;
W = m*g; % 735.75 N
$f_s$ = static friction (maximum), $f_k$ = kinetic friction, $N$ = normal force, $\mu$ = coefficient.
mu_s = 0.6; mu_k = 0.4; N = 100;
f_s_max = mu_s * N; % 60 N (max before sliding)
f_k = mu_k * N; % 40 N (while sliding)
$k$ = spring constant (N/m), $x$ = displacement from equilibrium. Negative = restoring.
k = 200; x = 0.05;
F = -k*x; % -10 N (restoring)
Cd = 0.47; rho = 1.225; A = 0.01; v = 30; % sphere in air
Fd = 0.5*Cd*rho*A*v^2; % 2.59 N
m = 5; g = 9.81; theta = deg2rad(30); mu_k = 0.2;
a = g*(sin(theta) - mu_k*cos(theta)); % 3.21 m/s²
F = 50; d = 10; theta = deg2rad(30);
W = F*d*cos(theta); % 433 J
m = 2; v = 10; h = 5; g = 9.81; k = 500; x = 0.1;
KE = 0.5*m*v^2; % 100 J
PE_grav = m*g*h; % 98.1 J
PE_spring = 0.5*k*x^2; % 2.5 J
% Ball dropped from 20 m — find speed at ground
g = 9.81; h = 20; vi = 0;
vf = sqrt(vi^2 + 2*g*h); % 19.8 m/s
W = 5000; t = 10;
P = W/t; % 500 W
% or: force times velocity
F = 200; v = 2.5;
P2 = F*v; % 500 W
m = 0.145; v = 40; % baseball
p = m*v; % 5.8 kg·m/s
F = 5000; dt = p/F; % 1.16 ms contact time
| Type | Momentum | Kinetic Energy | Formula |
|---|---|---|---|
| Elastic | Conserved | Conserved | Both $p$ and $KE$ equations |
| Inelastic | Conserved | Not conserved | $p$ equation only |
| Perfectly inelastic | Conserved | Max loss | $v_f = \frac{m_1 v_1 + m_2 v_2}{m_1 + m_2}$ |
% Perfectly inelastic: 2 kg at 5 m/s hits 3 kg at rest
m1 = 2; v1 = 5; m2 = 3; v2 = 0;
vf = (m1*v1 + m2*v2)/(m1+m2); % 2 m/s
KE_lost = 0.5*m1*v1^2 - 0.5*(m1+m2)*vf^2; % 15 J lost
m1 = 2; m2 = 3; v1i = 6; v2i = 0;
v1f = ((m1-m2)*v1i + 2*m2*v2i)/(m1+m2); % -1.2 m/s (bounces back)
v2f = (2*m1*v1i + (m2-m1)*v2i)/(m1+m2); % 4.8 m/s
m = [2 5 3]; x = [1 4 7];
x_cm = sum(m.*x)/sum(m); % 4.3 m
Direct analogs of translational kinematics with $\theta \leftrightarrow x$, $\omega \leftrightarrow v$, $\alpha \leftrightarrow a$.
r = 0.5; F = 100; theta = deg2rad(90);
tau = r*F*sin(theta); % 50 N·m
| Shape | Axis | $I$ |
|---|---|---|
| Point mass | At distance $r$ | $mr^2$ |
| Solid cylinder/disk | Central axis | $\frac{1}{2}mR^2$ |
| Hollow cylinder | Central axis | $mR^2$ |
| Solid sphere | Through center | $\frac{2}{5}mR^2$ |
| Hollow sphere | Through center | $\frac{2}{3}mR^2$ |
| Thin rod (center) | Perpendicular, center | $\frac{1}{12}mL^2$ |
| Thin rod (end) | Perpendicular, end | $\frac{1}{3}mL^2$ |
Rolling without slipping: $KE_{\text{total}} = \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2$, where $v = R\omega$.
m = 5; R = 0.2; v = 4; % solid sphere rolling
I = (2/5)*m*R^2;
omega = v/R;
KE_trans = 0.5*m*v^2; % 40 J
KE_rot = 0.5*I*omega^2; % 16 J
KE_total = KE_trans + KE_rot; % 56 J
G = 6.674e-11; ME = 5.972e24; RE = 6.371e6;
g = G*ME/RE^2; % 9.82 m/s² (surface gravity)
G = 6.674e-11; ME = 5.972e24; r = 6.371e6 + 400e3; % ISS ~400 km
v_orbit = sqrt(G*ME/r); % 7,670 m/s
T = 2*pi*sqrt(r^3/(G*ME)); % 5,558 s = 92.6 min
v_esc = sqrt(2*G*ME/r); % 10,848 m/s
m = 0.5; k = 200;
T_spring = 2*pi*sqrt(m/k); % 0.314 s
L = 1; g = 9.81;
T_pend = 2*pi*sqrt(L/g); % 2.006 s
f = 440; v = 343; % A4 note in air
lambda = v/f; % 0.78 m wavelength
$T$ = tension (N), $\mu$ = linear mass density (kg/m).
v = 343; L = 0.65; % guitar string
f = (1:6)*v/(2*L); % first 6 harmonics
I = 1e-5; % W/m²
beta = 10*log10(I/1e-12); % 70 dB
Upper signs: approaching. Lower signs: receding. $v$ = speed of sound.
f = 500; v = 343; vs = 30; % source approaching
f_obs = f*(v)/(v - vs); % 548 Hz (higher pitch)
rho = 1000; g = 9.81; h = 10;
P = 101325 + rho*g*h; % 199,425 Pa at 10m depth
rho_water = 1000; V = 0.01; g = 9.81;
Fb = rho_water*V*g; % 98.1 N
% Bernoulli: find velocity from pressure drop
P1 = 200000; P2 = 150000; rho = 1000; % Pa
v2 = sqrt(2*(P1-P2)/rho); % 10.0 m/s
$Q$ = volume flow rate, $r$ = pipe radius, $\eta$ = dynamic viscosity, $L$ = pipe length.
$c$ = specific heat, $L$ = latent heat (fusion or vaporization).
m = 0.5; c = 4184; dT = 80; % heat 500g water by 80°C
Q = m*c*dT; % 167,360 J
% Phase change: melt ice
L_fus = 334000; % J/kg for water
Q_melt = m*L_fus; % 167,000 J
| Process | Constant | Work $W$ | Heat $Q$ |
|---|---|---|---|
| Isothermal | $T$ | $nRT\ln(V_f/V_i)$ | $W$ |
| Isobaric | $P$ | $P\Delta V$ | $nC_P\Delta T$ |
| Isochoric | $V$ | $0$ | $nC_V\Delta T$ |
| Adiabatic | $Q = 0$ | $-\Delta U$ | $0$ |
Monatomic: $\gamma = 5/3$. Diatomic: $\gamma = 7/5$.
TH = 600; TC = 300; % Kelvin
eta_carnot = 1 - TC/TH; % 0.50 = 50% max possible
% Radiation from a blackbody
sigma = 5.670e-8; T = 5778; % Sun surface temp
P_per_m2 = sigma * T^4; % 6.32e7 W/m² (solar luminosity/area)
ke = 8.988e9; q = 1e-6; r = 0.5;
V = ke*q/r; % 17,976 V
rho = 1.68e-8; L = 100; A = 1e-6; % copper wire
R = rho*L/A; % 1.68 Ω
mu0 = 4*pi*1e-7; I = 10; r = 0.05;
B_wire = mu0*I/(2*pi*r); % 4.0e-5 T
n1 = 1.0; theta1 = deg2rad(45); n2 = 1.5; % air → glass
theta2 = asin(n1*sin(theta1)/n2); % 28.1°
n1 = 1.5; n2 = 1.0;
theta_c = rad2deg(asin(n2/n1)); % 41.8° critical angle
Sign conventions: real image $d_i > 0$, virtual $d_i < 0$. Converging lens $f > 0$, diverging $f < 0$.
f = 0.10; do = 0.25; % 10 cm lens, object at 25 cm
di = 1/(1/f - 1/do); % 0.167 m = 16.7 cm
m = -di/do; % -0.667 (inverted, smaller)
lambda = 550e-9; d = 0.1e-3; L = 2; % green light, 0.1mm slits, 2m screen
y1 = 1*lambda*L/d; % 0.011 m = 1.1 cm spacing
c = 2.998e8; v = 0.9*c;
gamma = 1/sqrt(1 - (v/c)^2); % 2.294
$\Delta t_0$ = proper time (in rest frame). $L_0$ = proper length (in rest frame). Moving clocks run slow; moving objects are shortened.
dt0 = 1; gamma = 2.294;
dt = gamma*dt0; % 2.294 s observed
L0 = 100;
L = L0/gamma; % 43.6 m observed length
m = 9.109e-31; v = 0.9*2.998e8; c = 2.998e8;
gamma = 1/sqrt(1-(v/c)^2);
E = gamma*m*c^2; % 1.88e-13 J
E0 = m*c^2; % 8.19e-14 J (rest energy)
KE = (gamma-1)*m*c^2; % 1.06e-13 J
Replaces Galilean addition at high speeds. Ensures $u' \leq c$ always.
$\phi$ = work function (minimum energy to eject electron). $V_0$ = stopping voltage.
h = 6.626e-34; c = 2.998e8; e = 1.602e-19;
lambda = 250e-9; % UV light
phi = 4.3*e; % sodium work function (4.3 eV)
KE_max = h*c/lambda - phi; % 1.07e-19 J = 0.67 eV
LaTeX: i\hbar\frac{\partial \Psi}{\partial t} = -\frac{\hbar^2}{2m}\nabla^2\Psi + V\Psi
h = 6.626e-34; me = 9.109e-31; L = 1e-9; % 1 nm box
n = 1:5;
E = (n.^2 * h^2) / (8*me*L^2); % energy levels (J)
E_eV = E / 1.602e-19; % [0.38, 1.50, 3.38, 6.01, 9.40] eV
Compton wavelength: $\lambda_C = h/(m_e c) = 2.426 \times 10^{-12}$ m.
h = 6.626e-34; me = 9.109e-31; c = 2.998e8;
lambda_C = h/(me*c); % 2.426e-12 m
theta = deg2rad(90);
d_lambda = lambda_C*(1 - cos(theta)); % 2.426e-12 m shift
T_sun = 5778;
lambda_max = 2.898e-3 / T_sun; % 501 nm (green-yellow peak)
This reference spans the physics you'll encounter from introductory mechanics through the first courses in modern physics. The equations connect directly to your learning path diagram:
Chapters 2–9 = Physics 1 & 2 (Classical Mechanics, Waves, Fluids, Thermodynamics)
Chapter 11 = Physics 2 + E&M Theory (Electrostatics, Magnetism, Maxwell's equations)
Chapter 12 = Physics 2 (Optics)
Chapter 13 = Modern Physics (Relativity, Quantum Mechanics — prerequisites for your Kalman filter work via state-space models and for the unified physics path via QFT and General Relativity)