Difference between revisions of "Gamma-distribution"
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− | + | A continuous probability distribution concentrated on the positive semi-axis $ 0 < x < \infty $ | |
+ | with density | ||
− | + | $$ | |
+ | g _ \alpha ( x) = \ | ||
+ | { | ||
+ | \frac{1}{\Gamma ( \alpha ) } | ||
+ | } | ||
+ | x ^ {\alpha - 1 } e ^ {- x } , | ||
+ | $$ | ||
− | + | where $ \alpha $ | |
+ | is a parameter assuming positive values, and $ \Gamma ( \alpha ) $ | ||
+ | is Euler's gamma-function: | ||
− | + | $$ | |
+ | \Gamma ( \alpha ) = \ | ||
+ | \int\limits _ { 0 } ^ \infty | ||
+ | y ^ {\alpha - 1 } | ||
+ | e ^ {- y } dy. | ||
+ | $$ | ||
− | The | + | The corresponding distribution function for $ x \leq 0 $ |
+ | is zero, and for $ x > 0 $ | ||
+ | it is expressed by the formula | ||
− | + | $$ | |
+ | G _ \alpha ( x) = \ | ||
+ | { | ||
+ | \frac{1}{\Gamma ( \alpha ) } | ||
+ | } | ||
+ | \int\limits _ { 0 } ^ { x } | ||
+ | y ^ {\alpha - 1 } | ||
+ | e ^ {- y } dy. | ||
+ | $$ | ||
− | The | + | The integral on the right-hand side is called the incomplete gamma-function. The density $ g _ \alpha ( x) $ |
+ | is unimodal and for $ \alpha > 1 $ | ||
+ | it attains the maximum $ ( \alpha - 1) ^ {\alpha - 1 } e ^ {- ( \alpha - 1 ) } / \Gamma ( \alpha ) $ | ||
+ | at the point $ x = \alpha - 1 $. | ||
+ | If $ 0 < \alpha < 1 $ | ||
+ | the density $ g _ \alpha ( x) $ | ||
+ | decreases monotonically with increasing $ x $, | ||
+ | and if $ x \downarrow 0 $, | ||
+ | $ g _ \alpha ( x) $ | ||
+ | increases without limit. The characteristic function of the gamma-distribution has the form | ||
− | + | $$ | |
+ | \phi ( t) = ( 1 - it) ^ {- \alpha } . | ||
+ | $$ | ||
− | + | The moments of the gamma-distribution are given by the formula | |
− | + | $$ | |
+ | m _ {k} = \int\limits _ { 0 } ^ \infty | ||
+ | x ^ {k} g _ \alpha ( x) dx = \ | ||
− | Gamma | + | \frac{\Gamma ( \alpha + k) }{\Gamma ( \alpha ) } |
+ | ,\ \ | ||
+ | k > - \alpha . | ||
+ | $$ | ||
− | + | In particular, the mathematical expectation and variance are equal to $ \alpha $. | |
+ | The set of gamma-distributions is closed with respect to the operation of convolution: | ||
− | + | $$ | |
+ | g _ {\alpha _ {1} } \star g _ {\alpha _ {2} } = \ | ||
+ | g _ {\alpha _ {1} + \alpha _ {2} } . | ||
+ | $$ | ||
− | = | + | Gamma-distributions play a significant, though not always an explicit, role in applications. In the particular case of $ \alpha = 1 $ |
− | + | one obtains the exponential density. In queueing theory, the gamma-distribution for an $ \alpha $ | |
+ | which assumes integer values is known as the [[Erlang distribution|Erlang distribution]]. In mathematical statistics gamma-distributions frequently occur owing to the close connection with the normal distribution, since the sum of the squares $ \chi ^ {2} = X _ {1} ^ {2} + \dots + X _ {n} ^ {2} $ | ||
+ | of independent $ ( 0, 1) $ | ||
+ | normally-distributed random variables has density $ g _ {n/2} ( x/2) /2 $ | ||
+ | and is known as the "chi-squared" distribution with $ n $ | ||
+ | degrees of freedom. For this reason the gamma-distribution is involved in many important distributions in problems of mathematical statistics dealing with quadratic forms of normally-distributed random variables (e.g. the [[Student distribution|Student distribution]], the [[Fisher-F-distribution|Fisher $ F $- | ||
+ | distribution]] and the [[Fisher z-distribution|Fisher $ z $- | ||
+ | distribution]]). If $ X _ {1} $ | ||
+ | and $ X _ {2} $ | ||
+ | are independent and are distributed with densities $ g _ {\alpha _ {1} } $ | ||
+ | and $ g _ {\alpha _ {2} } $, | ||
+ | then the random variable $ X _ {1} / ( X _ {1} + X _ {2} ) $ | ||
+ | has density | ||
+ | $$ | ||
+ | \frac{\Gamma ( \alpha _ {1} + \alpha _ {2} ) }{\Gamma ( \alpha _ {1} ) \Gamma ( \alpha _ {2} ) } | ||
− | + | x ^ {\alpha _ {1} - 1 } | |
+ | ( 1 - x) ^ {\alpha _ {2} - 1 } ,\ \ | ||
+ | 0 < x < 1, | ||
+ | $$ | ||
+ | which is known as the density of the beta-distribution. The densities of linear functions $ aX + b $ | ||
+ | of random variables $ X $ | ||
+ | obeying the gamma-distribution constitute a special class of distributions — the so-called "type III" family of Pearson distributions. The density of the gamma-distribution is the weight function of the system of orthogonal [[Laguerre polynomials|Laguerre polynomials]]. The values of the gamma-distribution may be calculated from tables of the incomplete gamma-function [[#References|[1]]], [[#References|[2]]]. | ||
====References==== | ====References==== | ||
− | <table><TR><TD valign="top">[a1]</TD> <TD valign="top"> | + | <table> |
+ | <TR><TD valign="top">[1]</TD> <TD valign="top"> V.I. Pagurova, "Tables of the incomplete gamma-function" , Moscow (1963) (In Russian) {{MR|0159040}} {{ZBL|}} </TD></TR> | ||
+ | <TR><TD valign="top">[2]</TD> <TD valign="top"> K. Pearson (ed.), ''Tables of the incomplete gamma function'' , Cambridge Univ. Press (1957)</TD></TR> | ||
+ | <TR><TD valign="top">[a1]</TD> <TD valign="top"> N.L. Johnson, S. Kotz, "Distributions in statistics" , '''1. Continuous univariate distributions''' , Wiley (1970) {{MR|0270476}} {{MR|0270475}} {{ZBL|0213.21101}} </TD></TR> | ||
+ | <TR><TD valign="top">[a2]</TD> <TD valign="top"> L.J. Comrie, "Chambers's six-figure mathematical tables" , '''II''' , Chambers (1949)</TD></TR> | ||
+ | </table> |
Latest revision as of 19:21, 10 April 2024
A continuous probability distribution concentrated on the positive semi-axis $ 0 < x < \infty $
with density
$$ g _ \alpha ( x) = \ { \frac{1}{\Gamma ( \alpha ) } } x ^ {\alpha - 1 } e ^ {- x } , $$
where $ \alpha $ is a parameter assuming positive values, and $ \Gamma ( \alpha ) $ is Euler's gamma-function:
$$ \Gamma ( \alpha ) = \ \int\limits _ { 0 } ^ \infty y ^ {\alpha - 1 } e ^ {- y } dy. $$
The corresponding distribution function for $ x \leq 0 $ is zero, and for $ x > 0 $ it is expressed by the formula
$$ G _ \alpha ( x) = \ { \frac{1}{\Gamma ( \alpha ) } } \int\limits _ { 0 } ^ { x } y ^ {\alpha - 1 } e ^ {- y } dy. $$
The integral on the right-hand side is called the incomplete gamma-function. The density $ g _ \alpha ( x) $ is unimodal and for $ \alpha > 1 $ it attains the maximum $ ( \alpha - 1) ^ {\alpha - 1 } e ^ {- ( \alpha - 1 ) } / \Gamma ( \alpha ) $ at the point $ x = \alpha - 1 $. If $ 0 < \alpha < 1 $ the density $ g _ \alpha ( x) $ decreases monotonically with increasing $ x $, and if $ x \downarrow 0 $, $ g _ \alpha ( x) $ increases without limit. The characteristic function of the gamma-distribution has the form
$$ \phi ( t) = ( 1 - it) ^ {- \alpha } . $$
The moments of the gamma-distribution are given by the formula
$$ m _ {k} = \int\limits _ { 0 } ^ \infty x ^ {k} g _ \alpha ( x) dx = \ \frac{\Gamma ( \alpha + k) }{\Gamma ( \alpha ) } ,\ \ k > - \alpha . $$
In particular, the mathematical expectation and variance are equal to $ \alpha $. The set of gamma-distributions is closed with respect to the operation of convolution:
$$ g _ {\alpha _ {1} } \star g _ {\alpha _ {2} } = \ g _ {\alpha _ {1} + \alpha _ {2} } . $$
Gamma-distributions play a significant, though not always an explicit, role in applications. In the particular case of $ \alpha = 1 $ one obtains the exponential density. In queueing theory, the gamma-distribution for an $ \alpha $ which assumes integer values is known as the Erlang distribution. In mathematical statistics gamma-distributions frequently occur owing to the close connection with the normal distribution, since the sum of the squares $ \chi ^ {2} = X _ {1} ^ {2} + \dots + X _ {n} ^ {2} $ of independent $ ( 0, 1) $ normally-distributed random variables has density $ g _ {n/2} ( x/2) /2 $ and is known as the "chi-squared" distribution with $ n $ degrees of freedom. For this reason the gamma-distribution is involved in many important distributions in problems of mathematical statistics dealing with quadratic forms of normally-distributed random variables (e.g. the Student distribution, the Fisher $ F $- distribution and the Fisher $ z $- distribution). If $ X _ {1} $ and $ X _ {2} $ are independent and are distributed with densities $ g _ {\alpha _ {1} } $ and $ g _ {\alpha _ {2} } $, then the random variable $ X _ {1} / ( X _ {1} + X _ {2} ) $ has density
$$ \frac{\Gamma ( \alpha _ {1} + \alpha _ {2} ) }{\Gamma ( \alpha _ {1} ) \Gamma ( \alpha _ {2} ) } x ^ {\alpha _ {1} - 1 } ( 1 - x) ^ {\alpha _ {2} - 1 } ,\ \ 0 < x < 1, $$
which is known as the density of the beta-distribution. The densities of linear functions $ aX + b $ of random variables $ X $ obeying the gamma-distribution constitute a special class of distributions — the so-called "type III" family of Pearson distributions. The density of the gamma-distribution is the weight function of the system of orthogonal Laguerre polynomials. The values of the gamma-distribution may be calculated from tables of the incomplete gamma-function [1], [2].
References
[1] | V.I. Pagurova, "Tables of the incomplete gamma-function" , Moscow (1963) (In Russian) MR0159040 |
[2] | K. Pearson (ed.), Tables of the incomplete gamma function , Cambridge Univ. Press (1957) |
[a1] | N.L. Johnson, S. Kotz, "Distributions in statistics" , 1. Continuous univariate distributions , Wiley (1970) MR0270476 MR0270475 Zbl 0213.21101 |
[a2] | L.J. Comrie, "Chambers's six-figure mathematical tables" , II , Chambers (1949) |
Gamma-distribution. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Gamma-distribution&oldid=18532