Gaussian Distribution
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The Gaussian distribution (also called the normal distribution) is the most important probability distribution in statistics and physics.
Probability Density Function
$$ f(x) = \frac{1}{\sigma\sqrt{2\pi}} \exp\left(-\frac{(x-\mu)^2}{2\sigma^2}\right) $$where:
- $\mu$ = mean (center of the distribution)
- $\sigma$ = standard deviation (spread)
- $\sigma^2$ = variance
The standard normal distribution has $\mu = 0$ and $\sigma = 1$.
Properties
| Property | Value |
|---|---|
| Mean | $\mu$ |
| Variance | $\sigma^2$ |
| Skewness | 0 |
| Kurtosis | 3 |
68-95-99.7 Rule: Approximately 68%, 95%, and 99.7% of values lie within 1, 2, and 3 standard deviations of the mean.
Why It’s Everywhere
Central Limit Theorem
The sum of many independent random variables tends toward a Gaussian distribution, regardless of the original distributions. This explains why Gaussian distributions appear in:
- Measurement errors
- Thermal noise
- Brownian motion
Maximum Entropy
Among all distributions with a given mean and variance, the Gaussian has maximum entropy — it assumes the least additional structure.
Fourier Transform
The Gaussian is an eigenfunction of the Fourier transform:
$$ \mathcal{F}\{e^{-\pi x^2}\} = e^{-\pi f^2} $$A Gaussian transforms into another Gaussian.
Multidimensional Gaussian
In $n$ dimensions with mean $\boldsymbol{\mu}$ and covariance matrix $\boldsymbol{\Sigma}$:
$$ f(\mathbf{x}) = \frac{1}{(2\pi)^{n/2}|\boldsymbol{\Sigma}|^{1/2}} \exp\left(-\frac{1}{2}(\mathbf{x}-\boldsymbol{\mu})^T \boldsymbol{\Sigma}^{-1} (\mathbf{x}-\boldsymbol{\mu})\right) $$Applications
- Statistics and hypothesis testing
- Machine learning (Gaussian processes, GMMs)
- Physics (thermal distributions, quantum mechanics)
- Signal processing (noise models)
- Finance (Black-Scholes model)