F-distribution

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In probability theory and statistics, the F-distribution or F-ratio, also known as Snedecor's F distribution or the Fisher–Snedecor distribution (after Ronald Fisher and George W. Snedecor), is a continuous probability distribution that arises frequently as the null distribution of a test statistic, most notably in the analysis of variance (ANOVA) and other F-tests.[1][2][3][4]

Definitions

The F-distribution with d1 and d2 degrees of freedom is the distribution of

X=U1/d1U2/d2

where U1 and U2 are independent random variables with chi-square distributions with respective degrees of freedom d1 and d2.

It can be shown to follow that the probability density function (pdf) for X is given by

f(x;d1,d2)=(d1x)d1d2d2(d1x+d2)d1+d2xB(d12,d22)=1B(d12,d22)(d1d2)d12xd121(1+d1d2x)d1+d22

for real x > 0. Here B is the beta function. In many applications, the parameters d1 and d2 are positive integers, but the distribution is well-defined for positive real values of these parameters.

The cumulative distribution function is

F(x;d1,d2)=Id1x/(d1x+d2)(d12,d22),

where I is the regularized incomplete beta function.

Properties

The expectation, variance, and other details about the F(d1, d2) are given in the sidebox; for d2 > 8, the excess kurtosis is

γ2=12d1(5d222)(d1+d22)+(d24)(d22)2d1(d26)(d28)(d1+d22).

The k-th moment of an F(d1, d2) distribution exists and is finite only when 2k < d2 and it is equal to

μX(k)=(d2d1)kΓ(d12+k)Γ(d12)Γ(d22k)Γ(d22).[5]

The F-distribution is a particular parametrization of the beta prime distribution, which is also called the beta distribution of the second kind.

The characteristic function is listed incorrectly in many standard references (e.g.,[2]). The correct expression [6] is

φd1,d2F(s)=Γ(d1+d22)Γ(d22)U(d12,1d22,d2d1ıs)

where U(a, b, z) is the confluent hypergeometric function of the second kind.

Relation to the chi-squared distribution

In instances where the F-distribution is used, for example in the analysis of variance, independence of U1 and U2 (defined above) might be demonstrated by applying Cochran's theorem.

Equivalently, since the chi-squared distribution is the sum of squares of independent standard normal random variables, the random variable of the F-distribution may also be written

X=s12σ12÷s22σ22,

where s12=S12d1 and s22=S22d2, S12 is the sum of squares of d1 random variables from normal distribution N(0,σ12) and S22 is the sum of squares of d2 random variables from normal distribution N(0,σ22).

In a frequentist context, a scaled F-distribution therefore gives the probability p(s12/s22σ12,σ22), with the F-distribution itself, without any scaling, applying where σ12 is being taken equal to σ22. This is the context in which the F-distribution most generally appears in F-tests: where the null hypothesis is that two independent normal variances are equal, and the observed sums of some appropriately selected squares are then examined to see whether their ratio is significantly incompatible with this null hypothesis.

The quantity X has the same distribution in Bayesian statistics, if an uninformative rescaling-invariant Jeffreys prior is taken for the prior probabilities of σ12 and σ22.[7] In this context, a scaled F-distribution thus gives the posterior probability p(σ22/σ12s12,s22), where the observed sums s12 and s22 are now taken as known.

In general

See also

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References

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