Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Hamiltonian system
(section)
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!
=== Origins === The concept of chaos in Hamiltonian systems has its roots in the works of [[Henri Poincaré]], who in the late 19th century made pioneering contributions to the understanding of the [[three-body problem]] in [[celestial mechanics]]. Poincaré showed that even a simple [[Newton's law of universal gravitation|gravitational system]] of three bodies could exhibit complex behavior that could not be predicted over the long term. His work is considered to be one of the earliest explorations of chaotic behavior in [[Physics|physical systems]].<ref name="Poincare2">Poincaré, Henri. "New Methods of Celestial Mechanics." (1892)</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)