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
Feynman diagram
(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!
==== Spin 1: photons ==== The naive propagator for photons is infinite, since the Lagrangian for the A-field is: :<math> S = \int \tfrac14 F^{\mu\nu} F_{\mu\nu} = \int -\tfrac12\left(\partial^\mu A_\nu \partial_\mu A^\nu - \partial^\mu A_\mu \partial_\nu A^\nu \right)\,.</math> The quadratic form defining the propagator is non-invertible. The reason is the [[gauge invariance]] of the field; adding a gradient to {{mvar|A}} does not change the physics. To fix this problem, one needs to fix a gauge. The most convenient way is to demand that the divergence of {{mvar|A}} is some function {{mvar|f}}, whose value is random from point to point. It does no harm to integrate over the values of {{mvar|f}}, since it only determines the choice of gauge. This procedure inserts the following factor into the path integral for {{mvar|A}}: :<math> \int \delta\left(\partial_\mu A^\mu - f\right) e^{-\frac{f^2}{2} }\, Df\,. </math> The first factor, the delta function, fixes the gauge. The second factor sums over different values of {{mvar|f}} that are inequivalent gauge fixings. This is simply :<math> e^{- \frac{\left(\partial_\mu A_\mu\right)^2}{2}}\,.</math> The additional contribution from gauge-fixing cancels the second half of the free Lagrangian, giving the Feynman Lagrangian: :<math> S= \int \partial^\mu A^\nu \partial_\mu A_\nu </math> which is just like four independent free scalar fields, one for each component of {{mvar|A}}. The Feynman propagator is: :<math> \left\langle A_\mu(k) A_\nu(k') \right\rangle = \delta\left(k+k'\right) \frac{g_{\mu\nu}}{ k^2 }.</math> The one difference is that the sign of one propagator is wrong in the Lorentz case: the timelike component has an opposite sign propagator. This means that these particle states have negative norm—they are not physical states. In the case of photons, it is easy to show by diagram methods that these states are not physical—their contribution cancels with longitudinal photons to only leave two physical photon polarization contributions for any value of {{mvar|k}}. If the averaging over {{mvar|f}} is done with a coefficient different from {{sfrac|1|2}}, the two terms do not cancel completely. This gives a covariant Lagrangian with a coefficient <math>\lambda</math>, which does not affect anything: :<math> S= \int \tfrac12\left(\partial^\mu A^\nu \partial_\mu A_\nu - \lambda \left(\partial_\mu A^\mu\right)^2\right)</math> and the covariant propagator for QED is: :<math>\left \langle A_\mu(k) A_\nu(k') \right\rangle =\delta\left(k+k'\right)\frac{g_{\mu\nu} - \lambda\frac{k_\mu k_\nu }{ k^2} }{ k^2}.</math>
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
Feynman diagram
(section)
Add topic