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
World line
(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!
==Usage in physics== A world line of an object (generally approximated as a point in space, e.g., a particle or observer) is the sequence of [[spacetime]] events corresponding to the history of the object. A world line is a special type of curve in spacetime. Below an equivalent definition will be explained: A world line is either a time-like or a null curve in spacetime. Each point of a world line is an event that can be labeled with the time and the spatial position of the object at that time. For example, the ''orbit'' of the Earth in space is approximately a circle, a three-dimensional (closed) curve in space: the Earth returns every year to the same point in space relative to the sun. However, it arrives there at a different (later) time. The ''world line'' of the Earth is therefore [[helix|helical]] in spacetime (a curve in a four-dimensional space) and does not return to the same point. Spacetime is the collection of [[event (relativity)|events]], together with a [[continuous function|continuous]] and [[smooth function|smooth]] [[coordinate system]] identifying the events. Each event can be labeled by four numbers: a time coordinate and three space coordinates; thus spacetime is a four-dimensional space. The mathematical term for spacetime is a four-dimensional [[manifold]] (a topological space that locally resembles Euclidean space near each point). The concept may be applied as well to a higher-dimensional space. For easy visualizations of four dimensions, two space coordinates are often suppressed. An event is then represented by a point in a [[Minkowski diagram]], which is a plane usually plotted with the time coordinate, say <math>t</math>, vertically, and the space coordinate, say <math>x</math>, horizontally. As expressed by F.R. Harvey :A curve M in [spacetime] is called a ''worldline of a particle'' if its tangent is future timelike at each point. The arclength parameter is called [[proper time]] and usually denoted τ. The length of M is called the ''proper time'' of the particle. If the worldline M is a line segment, then the particle is said to be in [[free fall]].<ref>{{cite book|first = F. Reese|last = Harvey|year = 1990|chapter-url = https://books.google.com/books?id=6HnNCgAAQBAJ&pg=PA62|chapter = Special Relativity" section of chapter "Euclidean / Lorentzian Vector Spaces|title = Spinors and Calibrations|pages = 62β67|publisher = [[Academic Press]]|isbn = 9780080918631}}</ref>{{rp|62β63}} A world line traces out the path of a single point in spacetime. A [[world sheet]] is the analogous two-dimensional surface traced out by a one-dimensional line (like a string) traveling through spacetime. The world sheet of an open string (with loose ends) is a strip; that of a closed string (a loop) resembles a tube. Once the object is not approximated as a mere point but has extended volume, it traces not a ''world line'' but rather a world tube.
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)