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
Kaluza–Klein theory
(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!
== Space–time–matter theory == One particular variant of Kaluza–Klein theory is '''space–time–matter theory''' or '''induced matter theory''', chiefly promulgated by [[Paul S. Wesson|Paul Wesson]] and other members of the Space–Time–Matter Consortium.<ref>[http://5dstm.org 5Dstm.org]</ref> In this version of the theory, it is noted that solutions to the equation : <math>\widetilde{R}_{ab}=0</math> may be re-expressed so that in four dimensions, these solutions satisfy [[Einstein's equation]]s : <math>G_{\mu\nu} = 8\pi T_{\mu\nu}\,</math> with the precise form of the ''T''<sub>''μν''</sub> following from the [[Ricci-flat condition]] on the five-dimensional space. In other words, the cylinder condition of the previous development is dropped, and the stress–energy now comes from the derivatives of the 5D metric with respect to the fifth coordinate. Because the [[energy–momentum tensor]] is normally understood to be due to concentrations of matter in four-dimensional space, the above result is interpreted as saying that four-dimensional matter is induced from geometry in five-dimensional space. In particular, the [[soliton]] solutions of <math>\widetilde{R}_{ab}=0</math> can be shown to contain the [[Friedmann–Lemaître–Robertson–Walker metric]] in both radiation-dominated (early universe) and matter-dominated (later universe) forms. The general equations can be shown to be sufficiently consistent with classical [[tests of general relativity]] to be acceptable on physical principles, while still leaving considerable freedom to also provide interesting [[cosmological model]]s.
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
Kaluza–Klein theory
(section)
Add topic