Example:
∇ ⋅ B → = 0 {\displaystyle \nabla \cdot {\overrightarrow {B}}=0}
e i x = cos x + i sin x {\displaystyle \ e^{ix}=\cos {x}+i\sin {x}} Paul Dragulin
G μ ν + Λ g μ ν = 8 π G c 4 T μ ν {\displaystyle G_{\mu \nu }+\Lambda g_{\mu \nu }={\frac {8\pi G}{c^{4}}}T_{\mu \nu }} Scott Miller
e i π + 1 = 0 {\displaystyle \ e^{i\pi }+1=0} Kyle Serniak
i ℏ ∂ ∂ t Ψ = H ^ Ψ {\displaystyle i\hbar {\frac {\partial }{\partial t}}\Psi ={\hat {H}}\Psi } Hang Chen
p i h b a r ∗ c + 1 = P s i {\displaystyle pi^{hbar*c}+1=Psi} Robert Bebeau
Δ x Δ p ≥ ℏ 2 {\displaystyle \Delta x\Delta p\geq {\frac {\hbar }{2}}} Taylor Hynds
E 2 = p 2 c 2 + m 2 c 4 {\displaystyle E^{2}=p^{2}c^{2}+m^{2}c^{4}} Jordon Adams
V = I R {\displaystyle V=IR} Brett Israels
I = I 0 e τ {\displaystyle I=I_{0}e^{\tau }} Ben Sadler
e = lim n → ∞ ( 1 + 1 n ) n {\displaystyle e=\lim _{n\to \infty }\left(1+{\frac {1}{n}}\right)^{n}} Suhib Kiswani