Wiener process

{{Use American English|date=January 2019}}

{{Short description|Stochastic process generalizing Brownian motion}}

{{More footnotes|date=February 2010}}

{{Infobox probability distribution|name=Wiener Process|pdf_image=Wiener process with sigma.svg|mean= 0 |variance=\sigma^2 t|type=multivariate}}File:wiener process zoom.png

File:WienerProcess3D.svg

In mathematics, the Wiener process (or Brownian motion, due to its historical connection with the physical process of the same name) is a real-valued continuous-time stochastic process discovered by Norbert Wiener.{{cite book |last= Dobrow|first=Robert |author-link=Robert Dobrow |date=2016 |title=Introduction to Stochastic Processes with R |publisher=Wiley |pages=321–322 |doi=10.1002/9781118740712 |bibcode=2016ispr.book.....D |url=https://onlinelibrary.wiley.com/doi/book/10.1002/9781118740712 |isbn=9781118740651}}N.Wiener Collected Works vol.1 It is one of the best known Lévy processes (càdlàg stochastic processes with stationary independent increments). It occurs frequently in pure and applied mathematics, economics, quantitative finance, evolutionary biology, and physics.

The Wiener process plays an important role in both pure and applied mathematics. In pure mathematics, the Wiener process gave rise to the study of continuous time martingales. It is a key process in terms of which more complicated stochastic processes can be described. As such, it plays a vital role in stochastic calculus, diffusion processes and even potential theory. It is the driving process of Schramm–Loewner evolution. In applied mathematics, the Wiener process is used to represent the integral of a white noise Gaussian process, and so is useful as a model of noise in electronics engineering (see Brownian noise), instrument errors in filtering theory and disturbances in control theory.

The Wiener process has applications throughout the mathematical sciences. In physics it is used to study Brownian motion and other types of diffusion via the Fokker–Planck and Langevin equations. It also forms the basis for the rigorous path integral formulation of quantum mechanics (by the Feynman–Kac formula, a solution to the Schrödinger equation can be represented in terms of the Wiener process) and the study of eternal inflation in physical cosmology. It is also prominent in the mathematical theory of finance, in particular the Black–Scholes option pricing model.Shreve and Karatsas

Characterisations of the Wiener process

The Wiener process W_t is characterised by the following properties:{{cite book |last=Durrett |first=Rick |author-link=Rick Durrett |date=2019 |title=Probability: Theory and Examples |edition=5th |chapter=Brownian Motion |publisher=Cambridge University Press |isbn=9781108591034}}

  1. W_0= 0 almost surely
  2. W has independent increments: for every t>0, the future increments W_{t+u} - W_t, u \ge 0, are independent of the past values W_s, s< t.
  3. W has Gaussian increments: W_{t+u} - W_t is normally distributed with mean 0 and variance u, W_{t+u} - W_t\sim \mathcal N(0,u).
  4. W has almost surely continuous paths: W_t is almost surely continuous in t.

That the process has independent increments means that if {{math|0 ≤ s1 < t1s2 < t2}} then {{math|Wt1Ws1}} and {{math|Wt2Ws2}} are independent random variables, and the similar condition holds for n increments.

An alternative characterisation of the Wiener process is the so-called Lévy characterisation that says that the Wiener process is an almost surely continuous martingale with {{math|1=W0 = 0}} and quadratic variation {{math|1=[Wt, Wt] = t}} (which means that {{math|Wt2t}} is also a martingale).

A third characterisation is that the Wiener process has a spectral representation as a sine series whose coefficients are independent N(0, 1) random variables. This representation can be obtained using the Karhunen–Loève theorem.

Another characterisation of a Wiener process is the definite integral (from time zero to time t) of a zero mean, unit variance, delta correlated ("white") Gaussian process.{{Cite journal|last1=Huang|first1=Steel T.| last2=Cambanis|first2=Stamatis| date=1978|title=Stochastic and Multiple Wiener Integrals for Gaussian Processes|journal=The Annals of Probability|volume=6|issue=4|pages=585–614|doi=10.1214/aop/1176995480 |jstor=2243125 |issn=0091-1798|doi-access=free}}

The Wiener process can be constructed as the scaling limit of a random walk, or other discrete-time stochastic processes with stationary independent increments. This is known as Donsker's theorem. Like the random walk, the Wiener process is recurrent in one or two dimensions (meaning that it returns almost surely to any fixed neighborhood of the origin infinitely often) whereas it is not recurrent in dimensions three and higher (where a multidimensional Wiener process is a process such that its coordinates are independent Wiener processes).{{cite web |title= Pólya's Random Walk Constants |website= Wolfram Mathworld| url = https://mathworld.wolfram.com/PolyasRandomWalkConstants.html}} Unlike the random walk, it is scale invariant, meaning that

\alpha^{-1} W_{\alpha^2 t}

is a Wiener process for any nonzero constant {{mvar|α}}. The Wiener measure is the probability law on the space of continuous functions {{math|g}}, with {{math|1=g(0) = 0}}, induced by the Wiener process. An integral based on Wiener measure may be called a Wiener integral.

Wiener process as a limit of random walk

Let \xi_1, \xi_2, \ldots be i.i.d. random variables with mean 0 and variance 1. For each n, define a continuous time stochastic process

W_n(t)=\frac{1}{\sqrt{n}}\sum\limits_{1\leq k\leq\lfloor nt\rfloor}\xi_k, \qquad t \in [0,1].

This is a random step function. Increments of W_n are independent because the \xi_k are independent. For large n, W_n(t)-W_n(s) is close to N(0,t-s) by the central limit theorem. Donsker's theorem asserts that as n \to \infty, W_n approaches a Wiener process, which explains the ubiquity of Brownian motion.Steven Lalley, Mathematical Finance 345 Lecture 5: Brownian Motion (2001)

Properties of a one-dimensional Wiener process

= Basic properties =

The unconditional probability density function follows a normal distribution with mean = 0 and variance = t, at a fixed time {{mvar|t}}:

f_{W_t}(x) = \frac{1}{\sqrt{2 \pi t}} e^{-x^2/(2t)}.

The expectation is zero:

\operatorname E[W_t] = 0.

The variance, using the computational formula, is {{mvar|t}}:

\operatorname{Var}(W_t) = t.

These results follow immediately from the definition that increments have a normal distribution, centered at zero. Thus

W_t = W_t-W_0 \sim N(0,t).

= Covariance and correlation =

The covariance and correlation (where s \leq t):

\begin{align}

\operatorname{cov}(W_s, W_t) &= s, \\

\operatorname{corr}(W_s,W_t) &= \frac{\operatorname{cov}(W_s,W_t)}{\sigma_{W_s} \sigma_{W_t}} = \frac{s}{\sqrt{st}} = \sqrt{\frac{s}{t}}.

\end{align}

These results follow from the definition that non-overlapping increments are independent, of which only the property that they are uncorrelated is used. Suppose that t_1\leq t_2.

\operatorname{cov}(W_{t_1}, W_{t_2}) = \operatorname{E}\left[(W_{t_1}-\operatorname{E}[W_{t_1}]) \cdot (W_{t_2}-\operatorname{E}[W_{t_2}])\right] = \operatorname{E}\left[W_{t_1} \cdot W_{t_2} \right].

Substituting

W_{t_2} = ( W_{t_2} - W_{t_1} ) + W_{t_1}

we arrive at:

\begin{align}

\operatorname{E}[W_{t_1} \cdot W_{t_2}] & = \operatorname{E}\left[W_{t_1} \cdot ((W_{t_2} - W_{t_1})+ W_{t_1}) \right] \\

& = \operatorname{E}\left[W_{t_1} \cdot (W_{t_2} - W_{t_1} )\right] + \operatorname{E}\left[ W_{t_1}^2 \right].

\end{align}

Since W_{t_1}=W_{t_1} - W_{t_0} and W_{t_2} - W_{t_1} are independent,

\operatorname{E}\left [W_{t_1} \cdot (W_{t_2} - W_{t_1} ) \right ] = \operatorname{E}[W_{t_1}] \cdot \operatorname{E}[W_{t_2} - W_{t_1}] = 0.

Thus

\operatorname{cov}(W_{t_1}, W_{t_2}) = \operatorname{E} \left [W_{t_1}^2 \right ] = t_1.

A corollary useful for simulation is that we can write, for {{math|t1 < t2}}:

W_{t_2} = W_{t_1}+\sqrt{t_2-t_1}\cdot Z

where {{mvar|Z}} is an independent standard normal variable.

= Wiener representation =

Wiener (1923) also gave a representation of a Brownian path in terms of a random Fourier series. If \xi_n are independent Gaussian variables with mean zero and variance one, then

W_t = \xi_0 t+ \sqrt{2}\sum_{n=1}^\infty \xi_n\frac{\sin \pi n t}{\pi n}

and

W_t = \sqrt{2} \sum_{n=1}^\infty \xi_n \frac{\sin \left(\left(n - \frac{1}{2}\right) \pi t\right)}{ \left(n - \frac{1}{2}\right) \pi}

represent a Brownian motion on [0,1]. The scaled process

\sqrt{c}\, W\left(\frac{t}{c}\right)

is a Brownian motion on [0,c] (cf. Karhunen–Loève theorem).

= Running maximum =

The joint distribution of the running maximum

M_t = \max_{0 \leq s \leq t} W_s

and {{math|Wt}} is

f_{M_t,W_t}(m,w) = \frac{2(2m - w)}{t\sqrt{2 \pi t}} e^{-\frac{(2m-w)^2}{2t}}, \qquad m \ge 0, w \leq m.

To get the unconditional distribution of f_{M_t}, integrate over {{math|−∞ < wm}}:

\begin{align}

f_{M_t}(m) & = \int_{-\infty}^m f_{M_t,W_t}(m,w)\,dw = \int_{-\infty}^m \frac{2(2m - w)}{t\sqrt{2 \pi t}} e^{-\frac{(2m-w)^2}{2t}} \,dw \\[5pt]

& = \sqrt{\frac{2}{\pi t}}e^{-\frac{m^2}{2t}}, \qquad m \ge 0,

\end{align}

the probability density function of a Half-normal distribution. The expectation{{cite book|last=Shreve|first=Steven E| title=Stochastic Calculus for Finance II: Continuous Time Models|year=2008|publisher=Springer| isbn=978-0-387-40101-0| pages=114}} is

\operatorname{E}[M_t] = \int_0^\infty m f_{M_t}(m)\,dm = \int_0^\infty m \sqrt{\frac{2}{\pi t}}e^{-\frac{m^2}{2t}}\,dm = \sqrt{\frac{2t}{\pi}}

If at time t the Wiener process has a known value W_{t}, it is possible to calculate the conditional probability distribution of the maximum in interval [0, t] (cf. Probability distribution of extreme points of a Wiener stochastic process). The cumulative probability distribution function of the maximum value, conditioned by the known value W_t, is:

\, F_{M_{W_t}} (m) = \Pr \left( M_{W_t} = \max_{0 \leq s \leq t} W(s) \leq m \mid W(t) = W_t \right) = \ 1 -\ e^{-2\frac{m(m - W_t)}{t}}\ \, , \,\ \ m > \max(0,W_t)

= Self-similarity =

== Brownian scaling ==

For every {{math|c > 0}} the process V_t = (1 / \sqrt c) W_{ct} is another Wiener process.

== Time reversal ==

The process V_t = W_{1-t} - W_{1} for {{math|0 ≤ t ≤ 1}} is distributed like {{math|Wt}} for {{math|0 ≤ t ≤ 1}}.

== Time inversion ==

The process V_t = t W_{1/t} is another Wiener process.

== Projective invariance ==

Consider a Wiener process W(t), t\in\mathbb R, conditioned so that \lim_{t\to\pm\infty}tW(t)=0 (which holds almost surely) and as usual W(0)=0. Then the following are all Wiener processes {{harv|Takenaka|1988}}:

\begin{array}{rcl}

W_{1,s}(t) &=& W(t+s)-W(s), \quad s\in\mathbb R\\

W_{2,\sigma}(t) &=& \sigma^{-1/2}W(\sigma t),\quad \sigma > 0\\

W_3(t) &=& tW(-1/t).

\end{array}

Thus the Wiener process is invariant under the projective group PSL(2,R), being invariant under the generators of the group. The action of an element g = \begin{bmatrix}a&b\\c&d\end{bmatrix} is

W_g(t) = (ct+d)W\left(\frac{at+b}{ct+d}\right) - ctW\left(\frac{a}{c}\right) - dW\left(\frac{b}{d}\right),

which defines a group action, in the sense that (W_g)_h = W_{gh}.

== Conformal invariance in two dimensions ==

Let W(t) be a two-dimensional Wiener process, regarded as a complex-valued process with W(0)=0\in\mathbb C. Let D\subset\mathbb C be an open set containing 0, and \tau_D be associated Markov time:

\tau_D = \inf \{ t\ge 0 |W(t)\not\in D\}.

If f:D\to \mathbb C is a holomorphic function which is not constant, such that f(0)=0, then f(W_t) is a time-changed Wiener process in f(D) {{harv|Lawler|2005}}. More precisely, the process Y(t) is Wiener in D with the Markov time S(t) where

Y(t) = f(W(\sigma(t)))

S(t) = \int_0^t|f'(W(s))|^2\,ds

\sigma(t) = S^{-1}(t):\quad t = \int_0^{\sigma(t)}|f'(W(s))|^2\,ds.

= A class of Brownian martingales =

If a polynomial {{math|p(x, t)}} satisfies the partial differential equation

\left( \frac{\partial}{\partial t} + \frac{1}{2} \frac{\partial^2}{\partial x^2} \right) p(x,t) = 0

then the stochastic process

M_t = p ( W_t, t )

is a martingale.

Example: W_t^2 - t is a martingale, which shows that the quadratic variation of W on {{closed-closed|0, t}} is equal to {{mvar|t}}. It follows that the expected time of first exit of W from (−c, c) is equal to {{math|c2}}.

More generally, for every polynomial {{math|p(x, t)}} the following stochastic process is a martingale:

M_t = p ( W_t, t ) - \int_0^t a(W_s,s) \, \mathrm{d}s,

where a is the polynomial

a(x,t) = \left( \frac{\partial}{\partial t} + \frac 1 2 \frac{\partial^2}{\partial x^2} \right) p(x,t).

Example: p(x,t) = \left(x^2 - t\right)^2, a(x,t) = 4x^2; the process

\left(W_t^2 - t\right)^2 - 4 \int_0^t W_s^2 \, \mathrm{d}s

is a martingale, which shows that the quadratic variation of the martingale W_t^2 - t on [0, t] is equal to

4 \int_0^t W_s^2 \, \mathrm{d}s.

About functions {{math|p(xa, t)}} more general than polynomials, see local martingales.

= Some properties of sample paths =

The set of all functions w with these properties is of full Wiener measure. That is, a path (sample function) of the Wiener process has all these properties almost surely.

== Qualitative properties ==

  • For every ε > 0, the function w takes both (strictly) positive and (strictly) negative values on (0, ε).
  • The function w is continuous everywhere but differentiable nowhere (like the Weierstrass function).
  • For any \epsilon > 0, w(t) is almost surely not (\tfrac 1 2 + \epsilon)-Hölder continuous, and almost surely (\tfrac 1 2 - \epsilon)-Hölder continuous.{{Cite book |last1=Mörters |first1=Peter |title=Brownian motion |last2=Peres |first2=Yuval |last3=Schramm |first3=Oded |last4=Werner |first4=Wendelin |date=2010 |publisher=Cambridge University Press |isbn=978-0-521-76018-8 |series=Cambridge series in statistical and probabilistic mathematics |location=Cambridge |pages=18}}
  • Points of local maximum of the function w are a dense countable set; the maximum values are pairwise different; each local maximum is sharp in the following sense: if w has a local maximum at {{mvar|t}} then \lim_{s \to t} \frac
    w(s)-w(t)
    s-t
    \to \infty. The same holds for local minima.
  • The function w has no points of local increase, that is, no t > 0 satisfies the following for some ε in (0, t): first, w(s) ≤ w(t) for all s in (t − ε, t), and second, w(s) ≥ w(t) for all s in (t, t + ε). (Local increase is a weaker condition than that w is increasing on (tε, t + ε).) The same holds for local decrease.
  • The function w is of unbounded variation on every interval.
  • The quadratic variation of w over [0,t] is t.
  • Zeros of the function w are a nowhere dense perfect set of Lebesgue measure 0 and Hausdorff dimension 1/2 (therefore, uncountable).

== Quantitative properties ==

=== [[Law of the iterated logarithm]] ===

\limsup_{t\to+\infty} \frac{ |w(t)| }{ \sqrt{ 2t \log\log t } } = 1, \quad \text{almost surely}.

=== [[Modulus of continuity]] ===

Local modulus of continuity:

\limsup_{\varepsilon \to 0+} \frac{ |w(\varepsilon)| }{ \sqrt{ 2\varepsilon \log\log(1/\varepsilon) } } = 1, \qquad \text{almost surely}.

Global modulus of continuity (Lévy):

\limsup_{\varepsilon\to0+} \sup_{0\le s
w(s)-w(t)
{\sqrt{ 2\varepsilon \log(1/\varepsilon)}} = 1, \qquad \text{almost surely}.

=== [[Dimension doubling theorem]] ===

The dimension doubling theorems say that the Hausdorff dimension of a set under a Brownian motion doubles almost surely.

== Local time ==

The image of the Lebesgue measure on [0, t] under the map w (the pushforward measure) has a density {{math|Lt}}. Thus,

\int_0^t f(w(s)) \, \mathrm{d}s = \int_{-\infty}^{+\infty} f(x) L_t(x) \, \mathrm{d}x

for a wide class of functions f (namely: all continuous functions; all locally integrable functions; all non-negative measurable functions). The density Lt is (more exactly, can and will be chosen to be) continuous. The number Lt(x) is called the local time at x of w on [0, t]. It is strictly positive for all x of the interval (a, b) where a and b are the least and the greatest value of w on [0, t], respectively. (For x outside this interval the local time evidently vanishes.) Treated as a function of two variables x and t, the local time is still continuous. Treated as a function of t (while x is fixed), the local time is a singular function corresponding to a nonatomic measure on the set of zeros of w.

These continuity properties are fairly non-trivial. Consider that the local time can also be defined (as the density of the pushforward measure) for a smooth function. Then, however, the density is discontinuous, unless the given function is monotone. In other words, there is a conflict between good behavior of a function and good behavior of its local time. In this sense, the continuity of the local time of the Wiener process is another manifestation of non-smoothness of the trajectory.

= Information rate =

The information rate of the Wiener process with respect to the squared error distance, i.e. its quadratic rate-distortion function, is given by T. Berger, "Information rates of Wiener processes," in IEEE Transactions on Information Theory, vol. 16, no. 2, pp. 134-139, March 1970.

doi: 10.1109/TIT.1970.1054423

R(D) = \frac{2}{\pi^2 \ln 2 D} \approx 0.29D^{-1}.

Therefore, it is impossible to encode \{w_t \}_{t \in [0,T]} using a binary code of less than T R(D) bits and recover it with expected mean squared error less than D. On the other hand, for any \varepsilon>0, there exists T large enough and a binary code of no more than 2^{TR(D)} distinct elements such that the expected mean squared error in recovering \{w_t \}_{t \in [0,T]} from this code is at most D - \varepsilon.

In many cases, it is impossible to encode the Wiener process without sampling it first. When the Wiener process is sampled at intervals T_s before applying a binary code to represent these samples, the optimal trade-off between code rate R(T_s,D) and expected mean square error D (in estimating the continuous-time Wiener process) follows the parametric representation Kipnis, A., Goldsmith, A.J. and Eldar, Y.C., 2019. The distortion-rate function of sampled Wiener processes. IEEE Transactions on Information Theory, 65(1), pp.482-499.

R(T_s,D_\theta) = \frac{T_s}{2} \int_0^1 \log_2^+\left[\frac{S(\varphi)- \frac{1}{6}}{\theta}\right] d\varphi,

D_\theta = \frac{T_s}{6} + T_s\int_0^1 \min\left\{S(\varphi)-\frac{1}{6},\theta \right\} d\varphi,

where S(\varphi) = (2 \sin(\pi \varphi /2))^{-2} and \log^+[x] = \max\{0,\log(x)\}. In particular, T_s/6 is the mean squared error associated only with the sampling operation (without encoding).

Related processes

File:DriftedWienerProcess1D.svg

File:ItoWienerProcess2D.svg

File:BMonSphere.jpg. The image above is of the Brownian motion on a special manifold: the surface of a sphere.]]

The stochastic process defined by

X_t = \mu t + \sigma W_t

is called a Wiener process with drift μ and infinitesimal variance σ2. These processes exhaust continuous Lévy processes, which means that they are the only continuous Lévy processes,

as a consequence of the Lévy–Khintchine representation.

Two random processes on the time interval [0, 1] appear, roughly speaking, when conditioning the Wiener process to vanish on both ends of [0,1]. With no further conditioning, the process takes both positive and negative values on [0, 1] and is called Brownian bridge. Conditioned also to stay positive on (0, 1), the process is called Brownian excursion.{{cite journal |last=Vervaat |first=W. |year=1979 |title=A relation between Brownian bridge and Brownian excursion |journal=Annals of Probability |volume=7 |issue=1 |pages=143–149 |jstor=2242845 |doi=10.1214/aop/1176995155|doi-access=free }} In both cases a rigorous treatment involves a limiting procedure, since the formula P(A|B) = P(AB)/P(B) does not apply when P(B) = 0.

A geometric Brownian motion can be written

e^{\mu t-\frac{\sigma^2 t}{2}+\sigma W_t}.

It is a stochastic process which is used to model processes that can never take on negative values, such as the value of stocks.

The stochastic process

X_t = e^{-t} W_{e^{2t}}

is distributed like the Ornstein–Uhlenbeck process with parameters \theta = 1, \mu = 0, and \sigma^2 = 2.

The time of hitting a single point x > 0 by the Wiener process is a random variable with the Lévy distribution. The family of these random variables (indexed by all positive numbers x) is a left-continuous modification of a Lévy process. The right-continuous modification of this process is given by times of first exit from closed intervals [0, x].

The local time {{math|1=L = (Lxt)xR, t ≥ 0}} of a Brownian motion describes the time that the process spends at the point x. Formally

L^x(t) =\int_0^t \delta(x-B_t)\,ds

where δ is the Dirac delta function. The behaviour of the local time is characterised by Ray–Knight theorems.

= Brownian martingales =

Let A be an event related to the Wiener process (more formally: a set, measurable with respect to the Wiener measure, in the space of functions), and Xt the conditional probability of A given the Wiener process on the time interval [0, t] (more formally: the Wiener measure of the set of trajectories whose concatenation with the given partial trajectory on [0, t] belongs to A). Then the process Xt is a continuous martingale. Its martingale property follows immediately from the definitions, but its continuity is a very special fact – a special case of a general theorem stating that all Brownian martingales are continuous. A Brownian martingale is, by definition, a martingale adapted to the Brownian filtration; and the Brownian filtration is, by definition, the filtration generated by the Wiener process.

= Integrated Brownian motion =

The time-integral of the Wiener process

W^{(-1)}(t) := \int_0^t W(s) \, ds

is called integrated Brownian motion or integrated Wiener process. It arises in many applications and can be shown to have the distribution N(0, t3/3),{{Cite web|url=http://www.quantopia.net/interview-questions-vii-integrated-brownian-motion/|title=Interview Questions VII: Integrated Brownian Motion – Quantopia| website=www.quantopia.net| language=en-US| access-date=2017-05-14}} calculated using the fact that the covariance of the Wiener process is t \wedge s = \min(t, s).Forum, [http://wilmott.com/messageview.cfm?catid=4&threadid=39502 "Variance of integrated Wiener process"], 2009.

For the general case of the process defined by

V_f(t) = \int_0^t f'(s)W(s) \,ds=\int_0^t (f(t)-f(s))\,dW_s

Then, for a > 0,

\operatorname{Var}(V_f(t))=\int_0^t (f(t)-f(s))^2 \,ds

\operatorname{cov}(V_f(t+a),V_f(t))=\int_0^t (f(t+a)-f(s))(f(t)-f(s)) \,ds

In fact, V_f(t) is always a zero mean normal random variable. This allows for simulation of V_f(t+a) given V_f(t) by taking

V_f(t+a)=A\cdot V_f(t) +B\cdot Z

where Z is a standard normal variable and

A=\frac{\operatorname{cov}(V_f(t+a),V_f(t))}{\operatorname{Var}(V_f(t))}

B^2=\operatorname{Var}(V_f(t+a))-A^2\operatorname{Var}(V_f(t))

The case of V_f(t)=W^{(-1)}(t) corresponds to f(t)=t. All these results can be seen as direct consequences of Itô isometry.

The n-times-integrated Wiener process is a zero-mean normal variable with variance \frac{t}{2n+1}\left ( \frac{t^n}{n!} \right )^2 . This is given by the Cauchy formula for repeated integration.

= Time change =

Every continuous martingale (starting at the origin) is a time changed Wiener process.

Example: 2Wt = V(4t) where V is another Wiener process (different from W but distributed like W).

Example. W_t^2 - t = V_{A(t)} where A(t) = 4 \int_0^t W_s^2 \, \mathrm{d} s and V is another Wiener process.

In general, if M is a continuous martingale then M_t - M_0 = V_{A(t)} where A(t) is the quadratic variation of M on [0, t], and V is a Wiener process.

Corollary. (See also Doob's martingale convergence theorems) Let Mt be a continuous martingale, and

M^-_\infty = \liminf_{t\to\infty} M_t,

M^+_\infty = \limsup_{t\to\infty} M_t.

Then only the following two cases are possible:

-\infty < M^-_\infty = M^+_\infty < +\infty,

-\infty = M^-_\infty < M^+_\infty = +\infty;

other cases (such as M^-_\infty = M^+_\infty = +\infty,   M^-_\infty < M^+_\infty < +\infty etc.) are of probability 0.

Especially, a nonnegative continuous martingale has a finite limit (as t → ∞) almost surely.

All stated (in this subsection) for martingales holds also for local martingales.

= Change of measure =

A wide class of continuous semimartingales (especially, of diffusion processes) is related to the Wiener process via a combination of time change and change of measure.

Using this fact, the qualitative properties stated above for the Wiener process can be generalized to a wide class of continuous semimartingales.Revuz, D., & Yor, M. (1999). Continuous martingales and Brownian motion (Vol. 293). Springer.Doob, J. L. (1953). Stochastic processes (Vol. 101). Wiley: New York.

= Complex-valued Wiener process =

The complex-valued Wiener process may be defined as a complex-valued random process of the form Z_t = X_t + i Y_t where X_t and Y_t are independent Wiener processes (real-valued). In other words, it is the 2-dimensional Wiener process, where we identify \R^2 with \mathbb C.{{Citation|title = Estimation of Improper Complex-Valued Random Signals in Colored Noise by Using the Hilbert Space Theory| journal = IEEE Transactions on Information Theory | pages = 2859–2867 | volume = 55 | issue = 6 | doi = 10.1109/TIT.2009.2018329 | last1 = Navarro-moreno | first1 = J. | last2 = Estudillo-martinez | first2 = M.D | last3 = Fernandez-alcala | first3 = R.M. | last4 = Ruiz-molina | first4 = J.C. |year = 2009 | s2cid = 5911584 }}

== Self-similarity ==

Brownian scaling, time reversal, time inversion: the same as in the real-valued case.

Rotation invariance: for every complex number c such that |c|=1 the process c \cdot Z_t is another complex-valued Wiener process.

== Time change ==

If f is an entire function then the process f(Z_t) - f(0) is a time-changed complex-valued Wiener process.

Example: Z_t^2 = \left(X_t^2 - Y_t^2\right) + 2 X_t Y_t i = U_{A(t)} where

A(t) = 4 \int_0^t |Z_s|^2 \, \mathrm{d} s

and U is another complex-valued Wiener process.

In contrast to the real-valued case, a complex-valued martingale is generally not a time-changed complex-valued Wiener process. For example, the martingale 2 X_t + i Y_t is not (here X_t and Y_t are independent Wiener processes, as before).

= Brownian sheet =

{{main|Brownian sheet}}

The Brownian sheet is a multiparamateric generalization. The definition varies from authors, some define the Brownian sheet to have specifically a two-dimensional time parameter t while others define it for general dimensions.

See also

Notes

{{Reflist}}

References

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  • {{cite book |first1=Daniel |last1=Revuz |first2=Marc |last2=Yor |title=Continuous martingales and Brownian motion |edition=Second |publisher=Springer-Verlag |year=1994 }}
  • {{citation|title=On pathwise projective invariance of Brownian motion|first=Shigeo|last=Takenaka|journal=Proc Japan Acad|volume=64|year=1988|pages=41–44}}.