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Probability density function The purple curve is the standard Cauchy distribution 

Cumulative distribution function 

Parameters  location (real) scale (real) 

Support  
CDF  
Mean  undefined 
Median  
Mode  
Variance  undefined 
Skewness  undefined 
Ex. kurtosis  undefined 
Entropy  
MGF  does not exist 
CF 
The Cauchy distribution, named after Augustin Cauchy, is a continuous probability distribution. It is also known, especially among physicists, as the Lorentz distribution (after Hendrik Lorentz), Cauchy–Lorentz distribution, Lorentz(ian) function, or Breit–Wigner distribution.
The Cauchy distribution is often used in statistics as the canonical example of a "pathological" distribution. Its mean does not exist and its variance is infinite. The Cauchy distribution does not have finite moments of order greater than or equal to one; only fractional absolute moments exist.^{[1]} The Cauchy distribution has no moment generating function.
Its importance in physics is the result of its being the solution to the differential equation describing forced resonance.^{[2]} In mathematics, it is closely related to the Poisson kernel, which is the fundamental solution for the Laplace equation in the upper halfplane. In spectroscopy, it is the description of the shape of spectral lines which are subject to homogeneous broadening in which all atoms interact in the same way with the frequency range contained in the line shape. Many mechanisms cause homogeneous broadening, most notably collision broadening, and Chantler–Alda radiation.^{[3]} In its standard form, it is the maximum entropy probability distribution for a random variate X for which .^{[4]}
Contents 
The Cauchy distribution has the probability density function
where x_{0} is the location parameter, specifying the location of the peak of the distribution, and γ is the scale parameter which specifies the halfwidth at halfmaximum (HWHM). γ is also equal to half the interquartile range and is sometimes called the probable error. AugustinLouis Cauchy exploited such a density function in 1827 with an infinitesimal scale parameter, defining what would now be called a Dirac delta function.
The amplitude of the above Lorentzian function is given by
The special case when x_{0} = 0 and γ = 1 is called the standard Cauchy distribution with the probability density function
In physics, a threeparameter Lorentzian function is often used:
where is the height of the peak.
The cumulative distribution function is:
and the quantile function (inverse cdf) of the Cauchy distribution is
It follows that the first and third quartiles are , and hence the interquartile range is 2γ.
The derivative of the quantile function, the quantile density function, for the Cauchy distribution is:
The differential entropy of a distribution can be defined in terms of its quantile density,^{[5]} specifically
The Cauchy distribution is an example of a distribution which has no mean, variance or higher moments defined. Its mode and median are well defined and are both equal to x_{0}.
When U and V are two independent normally distributed random variables with expected value 0 and variance 1, then the ratio U/V has the standard Cauchy distribution.
If are independent and identically distributed random variables, each with a standard Cauchy distribution, then the sample mean has the same standard Cauchy distribution (the sample median, which is not affected by extreme values, can be used as a measure of central tendency). To see that this is true, compute the characteristic function of the sample mean:
where is the sample mean. This example serves to show that the hypothesis of finite variance in the central limit theorem cannot be dropped. It is also an example of a more generalized version of the central limit theorem that is characteristic of all stable distributions, of which the Cauchy distribution is a special case.
The Cauchy distribution is an infinitely divisible probability distribution. It is also a strictly stable distribution.^{[6]}
The standard Cauchy distribution coincides with the Student's tdistribution with one degree of freedom.
Like all stable distributions, the locationscale family to which the Cauchy distribution belongs is closed under linear transformations with real coefficients. In addition, the Cauchy distribution is the only univariate distribution which is closed under linear fractional transformations with real coefficients.^{[7]} In this connection, see also McCullagh's parametrization of the Cauchy distributions.
Let X denote a Cauchy distributed random variable. The characteristic function of the Cauchy distribution is given by
which is just the Fourier transform of the probability density. The original probability density may be expressed in terms of the characteristic function, essentially by using the inverse Fourier transform:
Observe that the characteristic function is not differentiable at the origin: this corresponds to the fact that the Cauchy distribution does not have an expected value.
If a probability distribution has a density function f(x), then the mean is
The question is now whether this is the same thing as
If at most one of the two terms in (2) is infinite, then (1) is the same as (2). But in the case of the Cauchy distribution, both the positive and negative terms of (2) are infinite. This means (2) is undefined. Moreover, if (1) is construed as a Lebesgue integral, then (1) is also undefined, because (1) is then defined simply as the difference (2) between positive and negative parts.
However, if (1) is construed as an improper integral rather than a Lebesgue integral, then (2) is undefined, and (1) is not necessarily welldefined. We may take (1) to mean
and this is its Cauchy principal value, which is zero, but we could also take (1) to mean, for example,
which is not zero, as can be seen easily by computing the integral.
Because the integrand is bounded and is not Lebesgue integrable, it is not even Henstock–Kurzweil integrable. Various results in probability theory about expected values, such as the strong law of large numbers, will not work in such cases.
The Cauchy distribution does not have finite moments of any order. Some of the higher raw moments do exist and have a value of infinity, for example the raw second moment:
Higher evenpowered raw moments will also evaluate to infinity. Oddpowered raw moments, however, do not exist at all (i.e. are undefined), which is distinctly different from existing with the value of infinity. (Consider 1/0, which is defined with the value of infinity, vs. 0/0, which is undefined.) The oddpowered raw moments are undefined because their values are essentially equivalent to since the two halves of the integral both diverge and have opposite signs. The first raw moment is the mean, which, being odd, does not exist. (See also the discussion above about this.) This in turn means that all of the central moments and standardized moments do not exist (are undefined), since they are all based on the mean. The variance — which is the second central moment — is likewise nonexistent (despite the fact that the raw second moment exists with the value infinity).
The results for higher moments follow from Hölder's inequality, which implies that higher moments (or halves of moments) diverge if lower ones do.
Because the mean and variance of the Cauchy distribution are not defined, attempts to estimate these parameters will not be successful. For example, if n samples are taken from a Cauchy distribution, one may calculate the sample mean as:
Although the sample values x_{i} will be concentrated about the central value x_{0}, the sample mean will become increasingly variable as more samples are taken, because of the increased likelihood of encountering sample points with a large absolute value. In fact, the distribution of the sample mean will be equal to the distribution of the samples themselves; i.e., the sample mean of a large sample is no better (or worse) an estimator of x_{0} than any single observation from the sample. Similarly, calculating the sample variance will result in values that grow larger as more samples are taken.
Therefore, more robust means of estimating the central value x_{0} and the scaling parameter γ are needed. One simple method is to take the median value of the sample as an estimator of x_{0} and half the sample interquartile range as an estimator of γ. Other, more precise and robust methods have been developed ^{[8]}^{[9]} For example, the truncated mean of the middle 24% of the sample order statistics produces an estimate for x_{0} that is more efficient than using either the sample median or the full sample mean.^{[10]}^{[11]} However, because of the fat tails of the Cauchy distribution, the efficiency of the estimator decreases if more than 24% of the sample is used.^{[10]}^{[11]}
Maximum likelihood can also be used to estimate the parameters x_{0} and γ. However, this tends to be complicated by the fact that this requires finding the roots of a high degree polynomial, and there can be multiple roots that represent local maxima.^{[12]} Also, while the maximum likelihood estimator is asymptotically efficient, it is relatively inefficient for small samples.^{[13]} The loglikelihood function for the Cauchy distribution for sample size n is:
Maximizing the log likelihood function with respect to x_{0} and γ produces the following system of equations:
Note that is a monotone function in γ and that the solution γ must satisfy . Solving just for x_{0} requires solving a polynomial of degree 2n − 1,^{[12]} and solving just for γ requires solving a polynomial of degree n (first for , then x_{0}). Therefore, whether solving for one parameter or for both paramters simultaneously, a numerical solution on a computer is typically required. The benefit of maximum likelihood estimation is asymptotic efficiency; estimating x_{0} using the sample median is only about 81% as asymptotically efficient as estimating x_{0} by maximum likelihood.^{[11]}^{[14]} The truncated sample mean using the middle 24% order statistics is about 88% as asymptotically efficient an estimator of x_{0} as the maximum likelihood estimate.^{[11]} When Newton's method is used to find the solution for the maximum likelihood estimate, the middle 24% order statistics can be used as an initial solution for x_{0}.
If X is Cauchy distributed with median μ and scale parameter γ, then the complex variable
has unit modulus and is distributed on the unit circle with density:
with respect to the angular variable ,^{[citation needed]} where
and expresses the two parameters of the associated linear Cauchy distribution for x as a complex number:
The distribution is called the circular Cauchy distribution ^{[15]}^{[16]} (also the complex Cauchy distribution)^{[citation needed]} with parameter . The circular Cauchy distribution is related to the wrapped Cauchy distribution. If is a wrapped Cauchy distribution with the parameter representing the parameters of the corresponding "unwrapped" Cauchy distribution in the variable y where , then
See also McCullagh's parametrization of the Cauchy distributions and Poisson kernel for related concepts.
The circular Cauchy distribution expressed in complex form has finite moments of all orders
for integer . For , the transformation
is holomorphic on the unit disk, and the transformed variable is distributed as complex Cauchy with parameter .
Given a sample of size n > 2, the maximumlikelihood equation
can be solved by a simple fixedpoint iteration:
starting with The sequence of likelihood values is nondecreasing, and the solution is unique for samples containing at least three distinct values. ^{[17]}
The maximumlikelihood estimate for the median () and scale parameter () of a real Cauchy sample is obtained by the inverse transformation:
For n ≤ 4, closedform expressions are known for .^{[12]} The density of the maximumlikelihood estimator at t in the unit disk is necessarily of the form:
where
Formulae for and are available.^{[18]}
A random vector X = (X_{1}, ..., X_{k})′ is said to have the multivariate Cauchy distribution if every linear combination of its components Y = a_{1}X_{1} + ... + a_{k}X_{k} has a Cauchy distribution. That is, for any constant vector a ∈ R^{k}, the random variable Y = a′X should have a univariate Cauchy distribution.^{[19]} The characteristic function of a multivariate Cauchy distribution is given by:
where x_{0}(t) and γ(t) are real functions with x_{0}(t) a homogeneous function of degree one and γ(t) a positive homogeneous function of degree one.^{[19]} More formally:^{[19]}
An example of a bivariate Cauchy distribution can be given by:^{[20]}
Note that in this example, even though there is no analogue to a covariance matrix, x and y are not statistically independent.^{[20]}
Analogously to the univariate density, the multidimensional Cauchy density also relates to the multivariate Student distribution. They are equivalent when the degrees of freedom parameter is equal to one. The density of a k dimension Student distribution with one degree of freedom becomes:
Properties and details for this density can be obtained by taking it as a particular case of the multivariate Student density.
In nuclear and particle physics, the energy profile of a resonance is described by the relativistic Breit–Wigner distribution, while the Cauchy distribution is the (nonrelativistic) Breit–Wigner distribution.^{[citation needed]}


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