Understanding the Error Function
The error function, commonly denoted as erf(x), is a special function of sigmoid shape that occurs in probability, statistics, and partial differential equations. It is defined as the integral of the Gaussian (normal) distribution and is closely related to the cumulative distribution function of the normal distribution.
The error function is defined as: erf(x) = (2/sqrt(pi)) * integral from 0 to x of e^(-t^2) dt. The complementary error function is erfc(x) = 1 - erf(x).
Key Properties and Formulas
Taylor Series
The error function can be computed via its Maclaurin series expansion.
Complementary Error Function
erfc(x) measures the probability in the tail of the normal distribution.
Symmetry Property
The error function is an odd function, symmetric about the origin.
Limiting Values
The error function approaches +/-1 as x approaches +/-infinity.
Normal Distribution Link
The CDF of the standard normal distribution can be expressed using erf.
Derivative
The derivative of erf(x) is a Gaussian function.
Applications of the Error Function
The error function appears throughout science and engineering. In statistics, it defines confidence intervals and p-values. In physics, it describes heat diffusion and particle diffusion. In signal processing, it is used for Gaussian noise analysis. In finance, it relates to the Black-Scholes model through the cumulative normal distribution.
Common Values
- erf(0) = 0
- erf(0.5) = 0.520500 (approximately)
- erf(1.0) = 0.842701 (approximately)
- erf(1.5) = 0.966105 (approximately)
- erf(2.0) = 0.995322 (approximately)
- erf(3.0) = 0.999978 (approximately)