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		<summary type="html">&lt;p&gt;68.193.96.140: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&#039;&#039;&#039;Differential entropy&#039;&#039;&#039; (also referred to as &#039;&#039;&#039;continuous entropy&#039;&#039;&#039;) is a concept in [[information theory]] that extends the idea of (Shannon) [[information entropy|entropy]], a measure of average [[surprisal]] of a [[random variable]], to continuous [[probability distribution]]s.&lt;br /&gt;
&lt;br /&gt;
==Definition==&lt;br /&gt;
Let &#039;&#039;X&#039;&#039; be a random variable with a [[probability density function]] &#039;&#039;f&#039;&#039; whose [[support (mathematics)|support]] is a set &amp;lt;math&amp;gt;\mathbb X&amp;lt;/math&amp;gt;. The &#039;&#039;differential entropy&#039;&#039; &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;) or &#039;&#039;h&#039;&#039;(&#039;&#039;f&#039;&#039;) is defined as&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;h(X) = -\int_\mathbb{X} f(x)\log f(x)\,dx&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
For probability distributions which don&#039;t have an explicit density function expression, but have an explicit [[quantile function]] expression, &#039;&#039;Q&#039;&#039;(&#039;&#039;p&#039;&#039;), then &#039;&#039;h&#039;&#039;(&#039;&#039;Q&#039;&#039;) can be defined in terms of the derivative of &#039;&#039;Q&#039;&#039;(&#039;&#039;p&#039;&#039;) i.e. the quantile density function &#039;&#039;Q&#039;&#039;&#039;(&#039;&#039;p&#039;&#039;) as &amp;lt;ref&amp;gt;{{Citation |last1=Vasicek  |first1=Oldrich |year=1976 |title=A Test for Normality Based on Sample Entropy |journal=Journal of the Royal Statistical Society, Series B |volume=38 |issue=1 |pages=54–59 |postscript=. }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;h(Q) = \int_0^1 \log Q&#039;(p)\,dp&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
As with its discrete analog, the units of differential entropy depend on the base of the [[logarithm]], which is usually 2 (i.e., the units are [[bit]]s). See [[logarithmic units]] for logarithms taken in different bases. Related concepts such as [[joint entropy|joint]], [[conditional entropy|conditional]] differential entropy, and [[Kullback-Leibler divergence|relative entropy]] are defined in a similar fashion. Unlike the discrete analog, the differential entropy has an offset that depends on the units used to measure &#039;&#039;X&#039;&#039;.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;Pages 183-184, {{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=[[Elementary Principles in Statistical Mechanics|Elementary Principles in Statistical Mechanics, developed with especial reference to the rational foundation of thermodynamics]] |year=1902 |publisher=[[Charles Scribner&#039;s Sons]] |location=New York}}&amp;lt;/ref&amp;gt; For example, the differential entropy of a quantity in measured millimeters will be log(1000) more than the same quantity measured in meters; a dimensionless quantity will have differential entropy of log(1000) more than the same quantity divided by 1000.&lt;br /&gt;
&lt;br /&gt;
One must take care in trying to apply properties of discrete entropy to differential entropy, since probability density functions can be greater than 1. For example, [[Uniform distribution (continuous)|Uniform]](0,1/2) has &#039;&#039;negative&#039;&#039; differential entropy &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\int_0^\frac{1}{2} -2\log(2)\,dx=-\log(2)\,&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Thus, differential entropy does not share all properties of discrete entropy.&lt;br /&gt;
&lt;br /&gt;
Note that the continuous [[mutual information]] &#039;&#039;I&#039;&#039;(&#039;&#039;X&#039;&#039;;&#039;&#039;Y&#039;&#039;) has the distinction of retaining its fundamental significance as a measure of discrete information since it is actually the limit of the discrete mutual information of &#039;&#039;partitions&#039;&#039; of &#039;&#039;X&#039;&#039; and &#039;&#039;Y&#039;&#039; as these partitions become finer and finer.  Thus it is invariant under non-linear [[homeomorphisms]] (continuous and uniquely invertible maps) &lt;br /&gt;
,&amp;lt;ref&amp;gt;{{cite journal&lt;br /&gt;
 | first = Alexander &lt;br /&gt;
 | last = Kraskov&lt;br /&gt;
 | coauthors = Stögbauer, Grassberger&lt;br /&gt;
 | year = 2004&lt;br /&gt;
 | title = Estimating mutual information&lt;br /&gt;
 | journal = Phys. Rev. E&lt;br /&gt;
 | volume = 60&lt;br /&gt;
 | pages = 066138&lt;br /&gt;
 | doi =10.1103/PhysRevE.69.066138 &lt;br /&gt;
|arxiv = cond-mat/0305641 |bibcode = 2004PhRvE..69f6138K }}&amp;lt;/ref&amp;gt; including linear &amp;lt;ref name = Reza&amp;gt;{{ cite book | title = An Introduction to Information Theory | author = Fazlollah M. Reza | publisher = Dover Publications, Inc., New York | year = 1961, 1994 | isbn = 0-486-68210-2 | url = http://books.google.com/books?id=RtzpRAiX6OgC&amp;amp;pg=PA8&amp;amp;dq=intitle:%22An+Introduction+to+Information+Theory%22++%22entropy+of+a+simple+source%22&amp;amp;as_brr=0&amp;amp;ei=zP79Ro7UBovqoQK4g_nCCw&amp;amp;sig=j3lPgyYrC3-bvn1Td42TZgTzj0Q }}&amp;lt;/ref&amp;gt; transformations of &#039;&#039;X&#039;&#039; and &#039;&#039;Y&#039;&#039;, and still represents the amount of discrete information that can be transmitted over a channel that admits a continuous space of values.&lt;br /&gt;
&lt;br /&gt;
==Properties of differential entropy==&lt;br /&gt;
* For two densities &#039;&#039;f&#039;&#039; and &#039;&#039;g&#039;&#039;, the [[Kullback-Leibler divergence]] &#039;&#039;D&#039;&#039;(&#039;&#039;f&#039;&#039;||&#039;&#039;g&#039;&#039;) is nonnegative with equality if &#039;&#039;f&#039;&#039; = &#039;&#039;g&#039;&#039; [[almost everywhere]]. Similarly, for two random variables &#039;&#039;X&#039;&#039; and &#039;&#039;Y&#039;&#039;, &#039;&#039;I&#039;&#039;(&#039;&#039;X&#039;&#039;;&#039;&#039;Y&#039;&#039;) ≥ 0 and &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;|&#039;&#039;Y&#039;&#039;) ≤ &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;) with equality [[if and only if]] &#039;&#039;X&#039;&#039; and &#039;&#039;Y&#039;&#039; are [[Statistical independence|independent]].&lt;br /&gt;
* The chain rule for differential entropy holds as in the discrete case&lt;br /&gt;
::&amp;lt;math&amp;gt;h(X_1, \ldots, X_n) = \sum_{i=1}^{n} h(X_i|X_1, \ldots, X_{i-1}) \leq \sum h(X_i)&amp;lt;/math&amp;gt;.&lt;br /&gt;
* Differential entropy is translation invariant, i.e., &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039; + &#039;&#039;c&#039;&#039;) = &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;) for a constant &#039;&#039;c&#039;&#039;.&lt;br /&gt;
* Differential entropy is in general not invariant under arbitrary invertible maps. In particular, for a constant &#039;&#039;a&#039;&#039;, &#039;&#039;h&#039;&#039;(&#039;&#039;aX&#039;&#039;) = &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;) + log|&#039;&#039;a&#039;&#039;|. For a vector valued random variable &#039;&#039;&#039;X&#039;&#039;&#039; and a matrix &#039;&#039;A&#039;&#039;, &#039;&#039;h&#039;&#039;(&#039;&#039;A&#039;&#039; &#039;&#039;&#039;X&#039;&#039;&#039;) = &#039;&#039;h&#039;&#039;(&#039;&#039;&#039;X&#039;&#039;&#039;) + log|det(&#039;&#039;A&#039;&#039;)|.&lt;br /&gt;
* In general, for a transformation from a random vector to another random vector with same dimension &#039;&#039;&#039;Y&#039;&#039;&#039; = &#039;&#039;m&#039;&#039;(&#039;&#039;&#039;X&#039;&#039;&#039;), the corresponding entropies are related via &lt;br /&gt;
::&amp;lt;math&amp;gt;h(\mathbf{Y}) \leq h(\mathbf{X}) + \int f(x) \log \left\vert \frac{\partial m}{\partial x} \right\vert dx&amp;lt;/math&amp;gt; &lt;br /&gt;
:where &amp;lt;math&amp;gt;\left\vert \frac{\partial m}{\partial x} \right\vert&amp;lt;/math&amp;gt; is the [[Jacobian matrix and determinant|Jacobian]] of the transformation &#039;&#039;m&#039;&#039;. Equality is achieved if the transform is a bijection. When &#039;&#039;m&#039;&#039; is a rigid rotation, translation, or combination thereof, the Jacobian determinant is always 1, and &#039;&#039;h&#039;&#039;(&#039;&#039;Y&#039;&#039;) = &#039;&#039;h&#039;&#039;(&#039;&#039;X&#039;&#039;).&lt;br /&gt;
* If a random vector &#039;&#039;&#039;X&#039;&#039;&#039; in &#039;&#039;&#039;R&#039;&#039;&#039;&amp;lt;sup&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sup&amp;gt; has mean zero and [[covariance]] matrix &#039;&#039;K&#039;&#039;, &amp;lt;math&amp;gt;h(\mathbf{X}) \leq \frac{1}{2} \log[(2\pi e)^n \det{K}]&amp;lt;/math&amp;gt; with equality if and only if &#039;&#039;&#039;X&#039;&#039;&#039; is [[jointly gaussian]] (see [[#Maximization in the normal distribution|below]]).&lt;br /&gt;
&lt;br /&gt;
However, differential entropy does not have other desirable properties:&lt;br /&gt;
* It is not invariant under [[change of variables]], and is therefore most useful with dimensionless variables.&lt;br /&gt;
* It can be negative.&lt;br /&gt;
A modification of differential entropy that addresses these drawbacks is the &#039;&#039;&#039;relative information entropy&#039;&#039;&#039;, also known as the [[Kullback–Leibler divergence]], which includes an [[invariant measure]] factor (see [[limiting density of discrete points]]).&lt;br /&gt;
&lt;br /&gt;
== Maximization in the normal distribution ==&lt;br /&gt;
With a [[normal distribution]], differential entropy is maximized for a given variance.  The following is a proof that a Gaussian variable has the largest entropy amongst all random variables of equal variance.  &lt;br /&gt;
&lt;br /&gt;
Let &#039;&#039;g&#039;&#039;(&#039;&#039;x&#039;&#039;) be a [[Normal distribution|Gaussian]] [[Probability density function|PDF]] with mean μ and variance σ&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and &#039;&#039;f&#039;&#039;(&#039;&#039;x&#039;&#039;) an arbitrary [[Probability density function|PDF]] with the same variance. Since differential entropy is translation invariant we can assume that &#039;&#039;f&#039;&#039;(&#039;&#039;x&#039;&#039;) has the same mean of μ as &#039;&#039;g&#039;&#039;(&#039;&#039;x&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
Consider the [[Kullback-Leibler divergence]] between the two distributions &lt;br /&gt;
:&amp;lt;math&amp;gt; 0 \leq D_{KL}(f || g) = \int_{-\infty}^\infty f(x) \log \left( \frac{f(x)}{g(x)} \right) dx = -h(f) - \int_{-\infty}^\infty f(x)\log(g(x)) dx.&amp;lt;/math&amp;gt;&lt;br /&gt;
Now note that&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \int_{-\infty}^\infty f(x)\log(g(x)) dx &amp;amp;= \int_{-\infty}^\infty f(x)\log\left( \frac{1}{\sqrt{2\pi\sigma^2}}e^{-\frac{(x-\mu)^2}{2\sigma^2}}\right) dx \\&lt;br /&gt;
 &amp;amp;= \int_{-\infty}^\infty f(x) \log\frac{1}{\sqrt{2\pi\sigma^2}} dx + \log(e)\int_{-\infty}^\infty f(x)\left( -\frac{(x-\mu)^2}{2\sigma^2}\right) dx \\&lt;br /&gt;
 &amp;amp;= -\tfrac{1}{2}\log(2\pi\sigma^2) - \log(e)\frac{\sigma^2}{2\sigma^2} \\&lt;br /&gt;
 &amp;amp;= -\tfrac{1}{2}\left(\log(2\pi\sigma^2) + \log(e)\right) \\&lt;br /&gt;
 &amp;amp;= -\tfrac{1}{2}\log(2\pi e \sigma^2)  \\&lt;br /&gt;
 &amp;amp;= -h(g)&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
because the result does not depend on &#039;&#039;f&#039;&#039;(&#039;&#039;x&#039;&#039;) other than through the variance.  Combining the two results yields&lt;br /&gt;
:&amp;lt;math&amp;gt; h(g) - h(f) \geq 0 \!&amp;lt;/math&amp;gt;&lt;br /&gt;
with equality when &#039;&#039;g&#039;&#039;(&#039;&#039;x&#039;&#039;) = &#039;&#039;f&#039;&#039;(&#039;&#039;x&#039;&#039;) following from the properties of [[Kullback-Leibler divergence]].&lt;br /&gt;
&lt;br /&gt;
This result may also be demonstrated using the [[variational calculus]]. A Lagrangian function with two Lagrangian multipliers may be defined as:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;L=\int_{-\infty}^\infty g(x)\ln(g(x))\,dx-\lambda_0\left(1-\int_{-\infty}^\infty g(x)\,dx\right)-\lambda\left(\sigma^2-\int_{-\infty}^\infty g(x)(x-\mu)^2\,dx\right)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &#039;&#039;g(x)&#039;&#039; is some function with mean μ. When the entropy of &#039;&#039;g(x)&#039;&#039; is at a maximum and the constraint equations, which consist of the normalization condition &amp;lt;math&amp;gt;\left(1=\int_{-\infty}^\infty g(x)\,dx\right)&amp;lt;/math&amp;gt; and the requirement of fixed variance &amp;lt;math&amp;gt;\left(\sigma^2=\int_{-\infty}^\infty g(x)(x-\mu)^2\,dx\right)&amp;lt;/math&amp;gt;, are both satisfied, then a small variation δ&#039;&#039;g&#039;&#039;(&#039;&#039;x&#039;&#039;) about &#039;&#039;g(x)&#039;&#039; will produce a variation δ&#039;&#039;L&#039;&#039; about &#039;&#039;L&#039;&#039; which is equal to zero:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;0=\delta L=\int_{-\infty}^\infty \delta g(x)\left (\ln(g(x))+1+\lambda_0+\lambda(x-\mu)^2\right )\,dx&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Since this must hold for any small δ&#039;&#039;g&#039;&#039;(&#039;&#039;x&#039;&#039;), the term in brackets must be zero, and solving for &#039;&#039;g(x)&#039;&#039; yields:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;g(x)=e^{-\lambda_0-1-\lambda(x-\mu)^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Using the constraint equations to solve for λ&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; and λ yields the normal distribution:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;g(x)=\frac{1}{\sqrt{2\pi\sigma^2}}e^{-\frac{(x-\mu)^2}{2\sigma^2}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Example: Exponential distribution==&lt;br /&gt;
Let &#039;&#039;X&#039;&#039; be an [[exponential distribution|exponentially distributed]] random variable with parameter λ, that is, with probability density function &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;f(x) = \lambda e^{-\lambda x} \mbox{ for } x \geq 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Its differential entropy is then&lt;br /&gt;
{|&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;h_e(X)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
| &amp;lt;math&amp;gt;=-\int_0^\infty \lambda e^{-\lambda x} \log (\lambda e^{-\lambda x})\,dx&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|&lt;br /&gt;
| &amp;lt;math&amp;gt;=  -\left(\int_0^\infty (\log \lambda)\lambda e^{-\lambda x}\,dx + \int_0^\infty (-\lambda x) \lambda e^{-\lambda x}\,dx\right) &amp;lt;/math&amp;gt; &lt;br /&gt;
|-&lt;br /&gt;
|&lt;br /&gt;
| &amp;lt;math&amp;gt;= -\log \lambda \int_0^\infty f(x)\,dx + \lambda E[X]&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|&lt;br /&gt;
| &amp;lt;math&amp;gt;= -\log\lambda + 1\,.&amp;lt;/math&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Here, &amp;lt;math&amp;gt;h_e(X)&amp;lt;/math&amp;gt; was used rather than &amp;lt;math&amp;gt;h(X)&amp;lt;/math&amp;gt; to make it explicit that the logarithm was taken to base &#039;&#039;e&#039;&#039;, to simplify the calculation.&lt;br /&gt;
&lt;br /&gt;
==Differential entropies for various distributions==&lt;br /&gt;
In the table below &amp;lt;math&amp;gt;\Gamma(x) = \int_0^{\infty} e^{-t} t^{x-1} dt&amp;lt;/math&amp;gt; is the [[gamma function]], &amp;lt;math&amp;gt;\psi(x) = \frac{d}{dx} \ln\Gamma(x)=\frac{\Gamma&#039;(x)}{\Gamma(x)}&amp;lt;/math&amp;gt; is the [[digamma function]], &amp;lt;math&amp;gt;B(p,q) = \frac{\Gamma(p)\Gamma(q)}{\Gamma(p+q)}&amp;lt;/math&amp;gt; is the [[beta function]], and γ&amp;lt;sub&amp;gt;&#039;&#039;E&#039;&#039;&amp;lt;/sub&amp;gt; is [[Euler-Mascheroni constant|Euler&#039;s constant]]. Each distribution maximizes the entropy for a particular set of functional constraints listed in the fourth column, and the constraint that x be included in the support of the probability density, which is listed in the fifth column.&amp;lt;ref&amp;gt;{{cite journal |last1=Park |first1=Sung Y. |last2=Bera |first2=Anil K. |year=2009 |title=Maximum entropy autoregressive conditional heteroskedasticity model |journal=Journal of Econometrics |volume= |issue= |pages=219–230 |publisher=Elsevier |doi= |url=http://www.wise.xmu.edu.cn/Master/Download/..%5C..%5CUploadFiles%5Cpaper-masterdownload%5C2009519932327055475115776.pdf |accessdate=2011-06-02 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;background:white&amp;quot;&lt;br /&gt;
|+ Table of differential entropies and corresponding maximum entropy constraints&lt;br /&gt;
|-&lt;br /&gt;
! Distribution Name !! Probability density function (pdf) !! Entropy in [[Nat (information)|nats]] !! Maximum Entropy Constraint || Support&lt;br /&gt;
|-&lt;br /&gt;
| [[Uniform distribution (continuous)|Uniform]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{b-a}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln(b - a) \,&amp;lt;/math&amp;gt; ||None||&amp;lt;math&amp;gt;[a,b]\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Normal distribution|Normal]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{\sqrt{2\pi\sigma^2}} \exp\left(-\frac{(x-\mu)^2}{2\sigma^2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln\left(\sigma\sqrt{2\,\pi\,e}\right) &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x)=\mu,\,E((x-\mu)^2)=\sigma^2&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Exponential distribution|Exponential]] || &amp;lt;math&amp;gt;f(x) = \lambda \exp\left(-\lambda x\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;1 - \ln \lambda \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x)=1/\lambda\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Rayleigh distribution|Rayleigh]] || &amp;lt;math&amp;gt;f(x) = \frac{x}{\sigma^2} \exp\left(-\frac{x^2}{2\sigma^2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;1 + \ln \frac{\sigma}{\sqrt{2}} + \frac{\gamma_E}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x^2)=2\sigma^2, E(\ln(x))=\frac{\ln(2\sigma^2)-\gamma_E}{2}\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Beta distribution|Beta]] || &amp;lt;math&amp;gt;f(x) = \frac{x^{\alpha-1}(1-x)^{\beta-1}}{B(\alpha,\beta)}&amp;lt;/math&amp;gt; for &amp;lt;math&amp;gt;0 \leq x \leq 1&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt; \ln B(\alpha,\beta) - (\alpha-1)[\psi(\alpha) - \psi(\alpha +\beta)]\,&amp;lt;/math&amp;gt;&amp;lt;br /&amp;gt;&amp;lt;math&amp;gt;- (\beta-1)[\psi(\beta) - \psi(\alpha + \beta)] \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\ln(x))=\psi(\alpha)-\psi(\alpha+\beta)\,&amp;lt;/math&amp;gt;&amp;lt;br /&amp;gt;&amp;lt;math&amp;gt;E(\ln(1-x))=\psi(\beta )-\psi(\alpha+\beta)\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,1]\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Cauchy distribution|Cauchy]] || &amp;lt;math&amp;gt;f(x) = \frac{\gamma}{\pi} \frac{1}{\gamma^2 + x^2}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln(4\pi\gamma) \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\ln(x^2+\gamma^2))=\ln(4\gamma^2)\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|- &lt;br /&gt;
| [[Chi distribution|Chi]] || &amp;lt;math&amp;gt;f(x) = \frac{2}{2^{k/2}  \Gamma(k/2)} x^{k-1} \exp\left(-\frac{x^2}{2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln{\frac{\Gamma(k/2)}{\sqrt{2}}} - \frac{k-1}{2} \psi\left(\frac{k}{2}\right) + \frac{k}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x^2)=k,\,E(\ln(x))=\frac{1}{2}\left[\psi\left(\frac{k}{2}\right)\!+\!\ln(2)\right]&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Chi-squared distribution|Chi-squared]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{2^{k/2} \Gamma(k/2)} x^{\frac{k}{2}\!-\!1} \exp\left(-\frac{x}{2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln 2\Gamma\left(\frac{k}{2}\right) - \left(1 - \frac{k}{2}\right)\psi\left(\frac{k}{2}\right) + \frac{k}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x)=k,\,E(\ln(x))=\psi\left(\frac{k}{2}\right)+\ln(2)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Erlang distribution|Erlang]] || &amp;lt;math&amp;gt;f(x) = \frac{\lambda^k}{(k-1)!} x^{k-1} \exp(-\lambda x)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;(1-k)\psi(k) + \ln \frac{\Gamma(k)}{\lambda} + k&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x)=k/\lambda,\,E(\ln(x))=\psi(k)-\ln(\lambda)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[F distribution|F]] || &amp;lt;math&amp;gt;f(x) = \frac{n_1^{\frac{n_1}{2}} n_2^{\frac{n_2}{2}}}{B(\frac{n_1}{2},\frac{n_2}{2})} \frac{x^{\frac{n_1}{2} - 1}}{(n_2 + n_1 x)^{\frac{n_1 + n2}{2}}}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln \frac{n_1}{n_2} B\left(\frac{n_1}{2},\frac{n_2}{2}\right) + \left(1 - \frac{n_1}{2}\right) \psi\left(\frac{n_1}{2}\right) -&amp;lt;/math&amp;gt;&amp;lt;br /&amp;gt;&amp;lt;math&amp;gt;\left(1 + \frac{n_2}{2}\right)\psi\left(\frac{n_2}{2}\right) + \frac{n_1 + n_2}{2} \psi\left(\frac{n_1\!+\!n_2}{2}\right)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Gamma distribution|Gamma]] || &amp;lt;math&amp;gt;f(x) = \frac{x^{k - 1} \exp(-\frac{x}{\theta})}{\theta^k \Gamma(k)}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln(\theta \Gamma(k)) + (1 - k)\psi(k) + k \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x)=k\theta,\,E(\ln(x))=\psi(k)+\ln(\theta)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Laplace distribution|Laplace]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{2b} \exp\left(-\frac{|x - \mu|}{b}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;1 + \ln(2b) \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(|x-\mu|)=b\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Logistic distribution|Logistic]] || &amp;lt;math&amp;gt;f(x) = \frac{e^{-x}}{(1 + e^{-x})^2}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;2 \, &amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Log-normal distribution|Lognormal]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{\sigma x \sqrt{2\pi}} \exp\left(-\frac{(\ln x - \mu)^2}{2\sigma^2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\mu + \frac{1}{2} \ln(2\pi e \sigma^2)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\ln(x))=\mu,E((\ln(x) - \mu)^2)=\sigma^2\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Maxwell-Boltzmann distribution|Maxwell-Boltzmann]] || &amp;lt;math&amp;gt;f(x) = \frac{1}{a^3}\sqrt{\frac{2}{\pi}}\,x^{2}\exp\left(-\frac{x^2}{2a^2}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\frac{1}{2}-\gamma_E-\ln(a\sqrt{2\pi})&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x^2)=3a^2,\,E(\ln(x))\!=\!1\!+\!\ln\left(\frac{a}{\sqrt{2}}\right)\!-\!\frac{\gamma_E}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Generalized Gaussian distribution|Generalized normal]] || &amp;lt;math&amp;gt;f(x) = \frac{2 \beta^{\frac{\alpha}{2}}}{\Gamma(\frac{\alpha}{2})} x^{\alpha - 1} \exp(-\beta x^2)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln{\frac{\Gamma(\alpha/2)}{2\beta^{\frac{1}{2}}}} - \frac{\alpha - 1}{2} \psi\left(\frac{\alpha}{2}\right) + \frac{\alpha}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Pareto distribution|Pareto]] || &amp;lt;math&amp;gt;f(x) = \frac{\alpha x_m^\alpha}{x^{\alpha+1}}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\ln \frac{x_m}{\alpha} + 1 + \frac{1}{\alpha}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\ln(x))=\frac{1}{\alpha}+\ln(x_m)\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[x_m,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Student&#039;s t-distribution|Student&#039;s t]] || &amp;lt;math&amp;gt;f(x) = \frac{(1 + x^2/\nu)^{-\frac{\nu+1}{2}}}{\sqrt{\nu}B(\frac{1}{2},\frac{\nu}{2})}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\frac{\nu\!+\!1}{2}\left(\psi\left(\frac{\nu\!+\!1}{2}\right)\!-\!\psi\left(\frac{\nu}{2}\right)\right)\!+\!\ln \sqrt{\nu} B\left(\frac{1}{2},\frac{\nu}{2}\right)&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\ln(x^2\!+\!\nu))=\log \left(\nu\right)\!-\!\psi \left(\frac{\nu}{2}\right)\!+\!\psi\left(\frac{\nu\!+\!1}{2} \right)\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\infty,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Triangular distribution|Triangular]] || &amp;lt;math&amp;gt; f(x) = \begin{cases} &lt;br /&gt;
\frac{2(x-a)}{(b-a)(c-a)} &amp;amp; \mathrm{for\ } a \le x \leq c, \\[4pt]&lt;br /&gt;
    \frac{2(b-x)}{(b-a)(b-c)} &amp;amp; \mathrm{for\ } c &amp;lt; x \le b, \\[4pt]&lt;br /&gt;
 \end{cases}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\frac{1}{2} + \ln \frac{b-a}{2}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,1]\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Weibull distribution|Weibull]] || &amp;lt;math&amp;gt;f(x) = \frac{k}{\lambda^k} x^{k-1} \exp\left(-\frac{x^k}{\lambda^k}\right)&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\frac{(k-1)\gamma_E}{k} + \ln \frac{\lambda}{k} + 1&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(x^k)=\lambda^k,E(\ln(x))=\ln(\lambda)-\frac{\gamma_E}{k}\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;[0,\infty)\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Multivariate normal distribution|Multivariate normal]] || &amp;lt;math&amp;gt;&lt;br /&gt;
f_X(\vec{x}) =&amp;lt;/math&amp;gt;&amp;lt;br /&amp;gt;&amp;lt;math&amp;gt; \frac{\exp \left( -\frac{1}{2} ( \vec{x} - \vec{\mu})^\top \Sigma^{-1}\cdot(\vec{x} - \vec{\mu}) \right)} {(2\pi)^{N/2} \left|\Sigma\right|^{1/2}}&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;\frac{1}{2}\ln\{(2\pi e)^{N} \det(\Sigma)\}&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;E(\vec{x})=\vec{\mu},\,E((\vec{x}-\vec{\mu})(\vec{x}-\vec{\mu})^T)=\Sigma\,&amp;lt;/math&amp;gt;||&amp;lt;math&amp;gt;(-\vec{\infty},\vec{\infty})\,&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
(Many of the differential entropies are from.&amp;lt;ref name=&amp;quot;lazorathie&amp;quot;&amp;gt;{{cite journal|author=Lazo, A. and P. Rathie|title=On the entropy of continuous probability distributions|journal=Information Theory, IEEE Transactions on|year=1978|volume=24(1)|pages=120-122|doi=10.1109/TIT.1978.1055832}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Variants==&lt;br /&gt;
As described above, differential entropy does not share all properties of discrete entropy. For example, the differential entropy can be negative; also it is not invariant under continuous coordinate transformations. [[Edwin Thompson Jaynes]] showed in fact  that the expression above is not the correct limit of the expression for a finite set of probabilities.&amp;lt;ref&amp;gt;{{cite journal |author=Jaynes, E.T. |authorlink=Edwin Thompson Jaynes |title=Information Theory And Statistical Mechanics |journal=Brandeis University Summer Institute Lectures In Theoretical Physics |volume=3 |issue=sect. 4b |pages=181–218 |year=1963 |url=http://bayes.wustl.edu/etj/articles/brandeis.pdf |format=PDF}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A modification of differential entropy adds an [[invariant measure]] factor to correct this, (see [[limiting density of discrete points]]). If &#039;&#039;m(x)&#039;&#039; is further constrained to be a probability density, the resulting notion is called [[relative entropy]] in information theory:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;D(p||m) = \int p(x)\log\frac{p(x)}{m(x)}\,dx.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The definition of differential entropy above can be obtained by partitioning the range of &#039;&#039;X&#039;&#039; into bins of length &#039;&#039;h&#039;&#039; with associated sample points &#039;&#039;ih&#039;&#039; within the bins, for &#039;&#039;X&#039;&#039; Riemann integrable. This gives a [[Quantization (signal processing)|quantized]] version of &#039;&#039;X&#039;&#039;, defined by &#039;&#039;X&amp;lt;sub&amp;gt;h&amp;lt;/sub&amp;gt;&#039;&#039; = &#039;&#039;ih&#039;&#039; if &#039;&#039;ih&#039;&#039; ≤ &#039;&#039;X&#039;&#039; ≤ (&#039;&#039;i&#039;&#039;+1)&#039;&#039;h&#039;&#039;. Then the entropy of &#039;&#039;X&amp;lt;sub&amp;gt;h&amp;lt;/sub&amp;gt;&#039;&#039; is&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;H_h=-\sum_i hf(ih)\log (f(ih)) - \sum hf(ih)\log(h).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The first term on the right approximates the differential entropy, while the second term is approximately −log(&#039;&#039;h&#039;&#039;). Note that this procedure suggests that the entropy in the discrete sense of a continuous random variable should be ∞.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[Information entropy]]&lt;br /&gt;
*[[Information theory]]&lt;br /&gt;
*[[Limiting density of discrete points]]&lt;br /&gt;
*[[Self-information]]&lt;br /&gt;
*[[Kullback-Leibler divergence]]&lt;br /&gt;
*[[Entropy estimation]]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
* Thomas M. Cover, Joy A. Thomas. &#039;&#039;Elements of Information Theory&#039;&#039; New York: Wiley, 1991. ISBN 0-471-06259-6&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
* {{springer|title=Differential entropy|id=p/d031890}}&lt;br /&gt;
* {{planetmath reference|id=1915|title=Differential entropy}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Entropy and information]]&lt;br /&gt;
[[Category:Information theory]]&lt;br /&gt;
[[Category:Statistical randomness]]&lt;br /&gt;
[[Category:Randomness]]&lt;/div&gt;</summary>
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