by Timur Dautov

Inline math#

Einstein's mass–energy equivalence: E=mc2E = mc^2.

The quadratic formula gives roots x=b±b24ac2ax = \dfrac{-b \pm \sqrt{b^2 - 4ac}}{2a}.

Display math#

The Gaussian integral:

ex2dx=π\int_{-\infty}^{\infty} e^{-x^2}\, dx = \sqrt{\pi}

Euler's identity, often called the most beautiful equation in mathematics:

eiπ+1=0e^{i\pi} + 1 = 0

Calculus#

The fundamental theorem of calculus:

abf(x)dx=f(b)f(a)\int_a^b f'(x)\, dx = f(b) - f(a)

Taylor series expansion of exe^x around x=0x = 0:

ex=n=0xnn!=1+x+x22!+x33!+e^x = \sum_{n=0}^{\infty} \frac{x^n}{n!} = 1 + x + \frac{x^2}{2!} + \frac{x^3}{3!} + \cdots

Linear algebra#

For a matrix ARn×nA \in \mathbb{R}^{n \times n}, the determinant can be computed by cofactor expansion along the first row:

det(A)=j=1n(1)1+ja1jM1j\det(A) = \sum_{j=1}^{n} (-1)^{1+j}\, a_{1j}\, M_{1j}

where M1jM_{1j} is the (1,j)(1,j) minor.