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
Exterior algebra
(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!
=== Electromagnetic field === In [[Theory of relativity|Einstein's theories of relativity]], the [[electromagnetic field]] is generally given as a [[differential form|differential 2-form]] <math> F = dA </math> in [[4-space]] or as the equivalent [[Antisymmetric tensor|alternating tensor field]] <math> F_{ij} = A_{[i,j]} = A_{[i;j]}, </math> the [[electromagnetic tensor]]. Then <math> dF = ddA = 0 </math> or the equivalent Bianchi identity <math> F_{[ij,k]} = F_{[ij;k]} = 0. </math> None of this requires a metric. Adding the [[Lorentz metric]] and an [[Orientability#Orientability of differentiable manifolds|orientation]] provides the [[Hodge star operator]] <math> \star </math> and thus makes it possible to define <math> J = {\star}d{\star}F </math> or the equivalent tensor [[divergence]] <math> J^i = F^{ij}_{,j} = F^{ij}_{;j} </math> where <math> F^{ij} = g^{ik}g^{jl}F_{kl}. </math>
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)