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:<math>Q(x) =\frac{1}{2}\left( \frac{2}{\sqrt{\pi}} \int_{x/\sqrt{2}}^\infty \exp\left(-t^2\right) \, dt \right) = \frac{1}{2}\operatorname{erfc} \left(\frac{x}{\sqrt{2}} \right) = \frac{1}{2} - \frac{1}{2} \operatorname{erf} \left( \frac{x}{\sqrt{2}} \right).</math>
:<math>Q(x) =\frac{1}{2}\left( \frac{2}{\sqrt{\pi}} \int_{x/\sqrt{2}}^\infty \exp\left(-t^2\right) \, dt \right) = \frac{1}{2}\operatorname{erfc} \left(\frac{x}{\sqrt{2}} \right) = \frac{1}{2} - \frac{1}{2} \operatorname{erf} \left( \frac{x}{\sqrt{2}} \right).</math>


An alternative and more useful form of the ''Q''-function known as Craig's formula, after its discoverer, is expressed as:<ref>[http://wsl.stanford.edu/~ee359/craig.pdf John W. Craig, ''A new, simple and exact result for calculating the probability of error for two-dimensional signal constellaions'', Proc. 1991 IEEE Military Commun. Conf., vol. 2, pp. 571–575.]</ref>
An alternative form of the ''Q''-function known as Craig's formula, after its discoverer, is expressed as:<ref>[http://wsl.stanford.edu/~ee359/craig.pdf John W. Craig, ''A new, simple and exact result for calculating the probability of error for two-dimensional signal constellaions'', Proc. 1991 IEEE Military Commun. Conf., vol. 2, pp. 571–575.]</ref>


:<math>Q(x) = \frac{1}{\pi} \int_0^{\frac{\pi}{2}} \exp \left( - \frac{x^2}{2 \sin^2 \theta} \right) d\theta.</math>
:<math>Q(x) = \frac{1}{\pi} \int_0^{\frac{\pi}{2}} \exp \left( - \frac{x^2}{2 \sin^2 \theta} \right) d\theta.</math>

Revision as of 16:02, 15 April 2015

A plot of the Q-function.

In statistics, the Q-function is the tail probability of the standard normal distribution .[1][2] In other words, Q(x) is the probability that a normal (Gaussian) random variable will obtain a value larger than x standard deviations above the mean.

If the underlying random variable is y, then the proper argument to the tail probability is derived as:

which expresses the number of standard deviations away from the mean.

Other definitions of the Q-function, all of which are simple transformations of the normal cumulative distribution function, are also used occasionally.[3]

Because of its relation to the cumulative distribution function of the normal distribution, the Q-function can also be expressed in terms of the error function, which is an important function in applied mathematics and physics.

Definition and basic properties

Formally, the Q-function is defined as

Thus,

where is the cumulative distribution function of the normal Gaussian distribution.

The Q-function can be expressed in terms of the error function, or the complementary error function, as[2]

An alternative form of the Q-function known as Craig's formula, after its discoverer, is expressed as:[4]

This expression is valid only for positive values of x, but it can be used in conjunction with Q(x) = 1 − Q(−x) to obtain Q(x) for negative values. This form is advantageous in that the range of integration is finite.

become increasingly tight for large x, and are often useful.
Using the substitution v =u2/2, the upper bound is derived as follows:
Similarly, using and the quotient rule,
Solving for Q(x) provides the lower bound.
  • Improved exponential bounds and a pure exponential approximation are [5]
  • A tight approximation for the whole range of arguments is given by Karagiannidis & Lioumpas (2007) [6][failed verification]

Inverse Q

The inverse Q-function can be trivially related to the inverse error function:

Values

The Q-function is well tabulated and can be computed directly in most of the mathematical software packages such as Matlab and Mathematica. Some values of the Q-function are given below for reference.

References