Commutation matrix: Difference between revisions

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commutation matrix is involution and symmetric only in special case m = n; mention this and general relation
 
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In [[mathematics]], the '''Milstein method''' is a technique for the approximate [[numerical analysis|numerical solution]] of a [[stochastic differential equation]]. It is named after [[Grigori N. Milstein]] who first published the method in 1974.<ref>{{cite journal|first=G. N.|last=Mil'shtein|title=Approximate integration of stochastic differential equations|journal=Teor. Veroyatnost. i Primenen|volume=19|issue=3|year=1974| pages=583–588| url =http://www.mathnet.ru/php/archive.phtml?wshow=paper&jrnid=tvp&paperid=2929&option_lang=eng|language=Russian}}</ref><ref>{{cite doi|10.1137/1119062}}</ref>
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==Description==
Consider the [[autonomous equation|autonomous]] [[Itō calculus|Itō]] stochastic differential equation
 
:<math>\mathrm{d} X_t = a(X_t) \, \mathrm{d} t + b(X_t) \, \mathrm{d} W_t,</math>
 
with [[initial condition]] ''X''<sub>0</sub>&nbsp;=&nbsp;''x''<sub>0</sub>, where ''W''<sub>''t''</sub> stands for the [[Wiener process]], and suppose that we wish to solve this SDE on some interval of time&nbsp;[0,&nbsp;''T'']. Then the '''Milstein approximation''' to the true solution ''X'' is the [[Markov chain]] ''Y'' defined as follows:
 
* partition the interval [0,&nbsp;''T''] into ''N'' equal subintervals of width <math>\Delta t>0</math>:
 
:<math>0 = \tau_0 < \tau_1 < \dots < \tau_N = T\text{ with }\tau_n:=n\Delta t\text{ and }\Delta t = \frac{T}{N};</math>
 
* set <math>Y_0 = x_0;</math>
 
* recursively define <math>Y_n</math> for <math>1 \leq n \leq N</math> by
 
:<math>Y_{n + 1} = Y_n + a(Y_n) \Delta t + b(Y_n) \Delta W_n + \frac{1}{2} b(Y_n) b'(Y_n) \left( (\Delta W_n)^2 - \Delta t \right),</math>
 
where <math>b'</math> denotes the [[derivative]] of <math>b(x)</math> with respect to <math>x</math> and
 
:<math>\Delta W_n = W_{\tau_{n + 1}} - W_{\tau_n}</math>
 
are [[independent and identically distributed]] [[normal distribution|normal random variables]] with [[expected value]] zero and [[variance]] <math>\Delta t</math>. Then <math>Y_n</math> will approximate <math>X_{\tau_n}</math> for <math>0 \leq n \leq N</math>, and increasing <math>N</math> will yield a better approximation.
 
The error of the Milstein method is of order <math>\Delta t</math>, which is considerably better than the [[Euler–Maruyama method]], whose error is of order <math>(\Delta t)^{1/2}</math>.<ref>V. Mackevičius, ''Introduction to Stochastic Analysis'', Wiley 2011</ref>
 
== Intuitive derivation ==
 
For this derivation, we will only look at [[geometric Brownian motion]] (GBM), the stochastic differential equation of which is given by
 
:<math>\mathrm{d} X_t = \mu X \mathrm{d} t + \sigma X d W_t</math>
 
with real constants <math>\mu</math> and <math>\sigma</math>. Using [[Itō's lemma]] we get
 
:<math>\mathrm{d}\ln X_t=\left(\mu-\frac{1}{2}\sigma^2\right)\mathrm{d}t+\sigma\mathrm{d}W_t,</math>
Thus, the solution to the GBM SDE is
 
:<math>
\begin{align}
X_{t+\Delta t}&=X_t\exp\left\{\int_t^{t+\Delta t}\left(\mu-\frac{1}{2}\sigma^2\right)\mathrm{d}t+\int_t^{t+\Delta t}\sigma\mathrm{d}W_u\right\} \\
&\approx X_t\left(1+\mu\Delta t-\frac{1}{2}\sigma^2\Delta t+\sigma\Delta W_t+\frac{1}{2}\sigma^2(\Delta W_t)^2\right) \\
&= X_t + a(X_t)\Delta t+b(X_t)\Delta W_t+\frac{1}{2}b(X_t)b'(X_t)((\Delta W_t)^2-\Delta t)
\end{align}
</math>
 
where
 
:<math> a(x) = \mu x, ~b(x) = \sigma x </math>.
 
== See also ==
* [[Euler–Maruyama method]]
 
==References==
 
{{Reflist}}
 
==Further reading==
* {{cite book | author=Kloeden, P.E., & Platen, E. | title=Numerical Solution of Stochastic Differential Equations | publisher=Springer, Berlin | year=1999 | isbn=3-540-54062-8 }}
 
[[Category:Numerical differential equations]]
[[Category:Stochastic differential equations]]

Latest revision as of 22:19, 27 June 2014

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