Code page 437: Difference between revisions

From formulasearchengine
Jump to navigation Jump to search
en>Thewikicontributor
 
en>BattyBot
m fixed CS1 errors: dates & General fixes using AWB (9803)
Line 1: Line 1:
I woke  [http://okkyunglee.com kenney chesney] up another day and noticed - At the moment I have been solitary for a while and after much bullying from friends I today locate myself registered for online dating. They guaranteed me that there are plenty of standard, sweet and entertaining people  [http://lukebryantickets.hamedanshahr.com when is the luke bryan concert] to fulfill, so the pitch is gone by here!<br>My fam and buddies are [http://www.alexa.com/search?q=awesome&r=topsites_index&p=bigtop awesome] and spending some time together at pub gigs or dinners is obviously a necessity. I have never been into cabarets as I locate that you could never have a significant conversation with all the noise. I also got two quite cunning   [http://lukebryantickets.asiapak.net Luke bryan where is he from] and unquestionably cheeky canines that are consistently enthusiastic to meet fresh people.<br>I strive to keep as physically fit as possible being at the gym several times weekly. I appreciate my sports and attempt to play or view while many a possible. Being winter I'll often at Hawthorn suits.  [http://www.ffpjp24.org photos of luke bryan] Note: If you considered purchasing an athletics I don't brain, I've experienced the carnage of wrestling fits at stocktake sales.<br><br>
{{Probability distribution|
  name      =Wigner semicircle|
  type      =density|
  pdf_image  =[[Image:WignerS_distribution_PDF.svg|325px|Plot of the Wigner semicircle PDF]]<br /><small></small>||
  cdf_image =[[Image:WignerS_distribution_CDF.svg|325px|Plot of the Wigner semicircle CDF]]<br /><small></small>|
  parameters =<math>R>0\!</math> [[radius]] ([[real number|real]])|
  support    =<math>x \in [-R;+R]\!</math>|
  pdf        =<math>\frac2{\pi R^2}\,\sqrt{R^2-x^2}\!</math>|
  cdf        =<math>\frac12+\frac{x\sqrt{R^2-x^2}}{\pi R^2} + \frac{\arcsin\!\left(\frac{x}{R}\right)}{\pi}\!</math><br />for <math>-R\leq x \leq R</math>|
  mean      =<math>0\,</math>|
  median    =<math>0\,</math>|
  mode      =<math>0\,</math>|
  variance  =<math>\frac{R^2}{4}\!</math>|
  skewness  =<math>0\,</math>|
  kurtosis   =<math>-1\,</math>|
  entropy    =<math>\ln (\pi R) - \frac12 \,</math>|
  mgf        =<math>2\,\frac{I_1(R\,t)}{R\,t}</math>|
  char      =<math>2\,\frac{J_1(R\,t)}{R\,t}</math>|
}}
The '''Wigner semicircle distribution''', named after the physicist [[Eugene Wigner]], is the [[probability distribution]] supported on the interval [&minus;''R'', ''R''] the graph of whose [[probability density function]] ''f'' is a semicircle of radius ''R'' centered at (0, 0) and then suitably [[normalizing constant|normalized]] (so that it is really a semi-ellipse):


Check out my web-site ... luke bryan concert tickets 2014 ([http://www.netpaw.org navigate here])
:<math>f(x)={2 \over \pi R^2}\sqrt{R^2-x^2\,}\, </math>
 
for &minus;''R'' &le; ''x'' &le; ''R'', and ''f''(''x'') = 0 if ''R'' &lt; ''|x|''.
 
This distribution arises as the limiting distribution of [[eigenvalues]] of many [[random matrices|random symmetric matrices]] as the size of the matrix approaches infinity.
 
It is a scaled [[beta distribution]], more precisely, if ''Y'' is beta distributed with parameters α = β = 3/2, then ''X'' = 2''RY'' – ''R'' has the above Wigner semicircle distribution.
 
== General properties ==
The [[Chebyshev polynomials]] of the second kind are [[orthogonal polynomials]] with respect to the Wigner semicircle distribution.
 
For positive integers ''n'', the 2''n''-th [[moment (mathematics)|moment]] of this distribution is
 
:<math>E(X^{2n})=\left({R \over 2}\right)^{2n} C_n\, </math>
 
where ''X'' is any random variable with this distribution and ''C''<sub>''n''</sub> is the ''n''th [[Catalan number]]
 
:<math>C_n={1 \over n+1}{2n \choose n},\, </math>
 
so that the moments are the Catalan numbers if ''R'' = 2.  (Because of symmetry, all of the odd-order moments are zero.)
 
Making the substitution <math>x=R\cos(\theta)</math> into the defining equation for the [[moment generating function]] it can be seen that:
 
:<math>M(t)=\frac{2}{\pi}\int_0^\pi e^{Rt\cos(\theta)}\sin^2(\theta)\,d\theta</math>
 
which can be solved (see Abramowitz and Stegun [http://www.math.sfu.ca/~cbm/aands/page_376.htm §9.6.18)]
to yield:
 
:<math>M(t)=2\,\frac{I_1(Rt)}{Rt}</math>
 
where <math>I_1(z)</math> is the modified [[Bessel function]]. Similarly, the characteristic function is given by:
 
:<math>\varphi(t)=2\,\frac{J_1(Rt)}{Rt}</math>
 
where <math>J_1(z)</math> is the Bessel function. (See Abramowitz and Stegun [http://www.math.sfu.ca/~cbm/aands/page_360.htm §9.1.20)], noting that the corresponding integral involving <math>\sin(Rt\cos(\theta))</math> is zero.)
 
In the limit of <math>R</math> approaching zero, the Wigner semicircle distribution becomes a [[Dirac delta function]].
 
== Relation to free probability ==
 
In [[free probability]] theory, the role of Wigner's semicircle distribution is analogous to that of the [[normal distribution]] in classical probability theory. Namely,
in free probability theory, the role of [[cumulant]]s is occupied by "free cumulants", whose relation to ordinary cumulants is simply that the role of the set of all [[partition of a set|partitions of a finite set]] in the theory of ordinary cumulants is replaced by the set of all [[noncrossing partition]]s of a finite set.  Just the cumulants of degree more than 2 of a [[probability distribution]] are all zero [[if and only if]] the distribution is normal, so also, the ''free'' cumulants of degree more than 2 of a probability distribution are all zero if and only if the distribution is Wigner's semicircle distribution.
 
== See also ==
 
* The W.s.d. is the limit of the [[Kesten–McKay measure|Kesten–McKay distributions]], as the parameter ''d'' tends to infinity.
* In [[number theory|number-theoretic]] literature, the Wigner distribution is sometimes called the Sato–Tate distribution. See [[Sato–Tate conjecture]].
* [[Marchenko–Pastur distribution]] or [[Free Poisson distribution]]
 
==References==
 
* Milton Abramowitz and Irene A. Stegun, eds. ''[[Abramowitz and Stegun|Handbook of Mathematical Functions]] with Formulas, Graphs, and Mathematical Tables.'' New York: Dover, 1972.
 
==External links==
*[[Eric W. Weisstein]] et al., [http://mathworld.wolfram.com/WignersSemicircleLaw.html Wigner's semicircle]
 
{{ProbDistributions|continuous-bounded}}
 
[[Category:Continuous distributions]]
[[Category:Probability distributions]]

Revision as of 10:04, 22 December 2013

Template:Probability distribution The Wigner semicircle distribution, named after the physicist Eugene Wigner, is the probability distribution supported on the interval [−R, R] the graph of whose probability density function f is a semicircle of radius R centered at (0, 0) and then suitably normalized (so that it is really a semi-ellipse):

for −RxR, and f(x) = 0 if R < |x|.

This distribution arises as the limiting distribution of eigenvalues of many random symmetric matrices as the size of the matrix approaches infinity.

It is a scaled beta distribution, more precisely, if Y is beta distributed with parameters α = β = 3/2, then X = 2RYR has the above Wigner semicircle distribution.

General properties

The Chebyshev polynomials of the second kind are orthogonal polynomials with respect to the Wigner semicircle distribution.

For positive integers n, the 2n-th moment of this distribution is

where X is any random variable with this distribution and Cn is the nth Catalan number

so that the moments are the Catalan numbers if R = 2. (Because of symmetry, all of the odd-order moments are zero.)

Making the substitution into the defining equation for the moment generating function it can be seen that:

which can be solved (see Abramowitz and Stegun §9.6.18) to yield:

where is the modified Bessel function. Similarly, the characteristic function is given by:

where is the Bessel function. (See Abramowitz and Stegun §9.1.20), noting that the corresponding integral involving is zero.)

In the limit of approaching zero, the Wigner semicircle distribution becomes a Dirac delta function.

Relation to free probability

In free probability theory, the role of Wigner's semicircle distribution is analogous to that of the normal distribution in classical probability theory. Namely, in free probability theory, the role of cumulants is occupied by "free cumulants", whose relation to ordinary cumulants is simply that the role of the set of all partitions of a finite set in the theory of ordinary cumulants is replaced by the set of all noncrossing partitions of a finite set. Just the cumulants of degree more than 2 of a probability distribution are all zero if and only if the distribution is normal, so also, the free cumulants of degree more than 2 of a probability distribution are all zero if and only if the distribution is Wigner's semicircle distribution.

See also

References

External links

55 yrs old Metal Polisher Records from Gypsumville, has interests which include owning an antique car, summoners war hack and spelunkering. Gets immense motivation from life by going to places such as Villa Adriana (Tivoli).

my web site - summoners war hack no survey ios