Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Brownian motion
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Riemannian manifolds=== [[File:BMonSphere.jpg|thumb|upright=1.8|Brownian motion on a sphere]] Brownian motion is usually considered to take place in [[Euclidean space]]. It is natural to consider how such motion generalizes to more complex shapes, such as [[surface]]s or higher dimensional [[manifold]]s. The formalization requires the space to possess some form of a [[derivative]], as well as a [[metric space|metric]], so that a [[Laplacian]] can be defined. Both of these are available on [[Riemannian manifold]]s. Riemannian manifolds have the property that [[geodesic]]s can be described in [[polar coordinates]]; that is, displacements are always in a radial direction, at some given angle. Uniform random motion is then described by Gaussians along the radial direction, independent of the angle, the same as in Euclidean space. The [[Infinitesimal generator (stochastic processes)|infinitesimal generator]] (and hence [[characteristic operator]]) of Brownian motion on Euclidean {{math|'''R'''<sup>''n''</sup>}} is {{math|{{sfrac|1|2}}Δ}}, where {{math|Δ}} denotes the [[Laplace operator]]. Brownian motion on an {{mvar|m}}-dimensional [[Riemannian manifold]] {{math|(''M'', ''g'')}} can be defined as diffusion on {{mvar|M}} with the characteristic operator given by {{math|{{sfrac|1|2}}Δ<sub>LB</sub>}}, half the [[Laplace–Beltrami operator]] {{math|Δ<sub>LB</sub>}}. One of the topics of study is a characterization of the [[Poincaré recurrence theorem|Poincaré recurrence time]] for such systems.<ref name=Grigoryan-1999/>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Brownian motion
(section)
Add topic