Feynman rules for vector bosons

Click For Summary
The discussion centers on understanding the Feynman rules for vector bosons as presented in Lewis Ryder's book, specifically equations 7.57 and 7.58. The presence of Minkowski metric terms in these rules is explained as necessary for expanding 4-vector dot products in the interacting Lagrangian, which is crucial for contracting fields. It is suggested to derive these rules starting from the LSZ reduction formula for specific scattering processes. Additionally, the role of the Minkowski metric is to determine the appropriate Clebsch-Gordon coefficients based on the polarization of vector bosons. For further clarity, Srednicki's book is recommended as a supplementary resource.
wangjiaji
Messages
3
Reaction score
0
I'm learning QFT by reading Lewis Ryder's book, so my question in short is: how he arrives at Eq 7.57 and Eq 7.58? If you don't have the book, the question is: why are there Minkowski metric terms in the Feynman rules for a gauge field coupling to itself? If the answer is complicated, simply tell me where I can find it please, I have Peskin's and Weinberg's book, too.

For me it seems impossible to proceed after Chapter 7 with this book, it doesn't have a systematic way of introducing Feynman diagrams, and the Feynman rules for vector bosons seem to be pulled out of a hat, is this a suitable book for a man learning QFT for the first time on his own?

Thank you.
 
Physics news on Phys.org
in Weinberg?

Hi wangjiaji! :smile:

I don't have Ryder's book, but I do have Weinberg's Quantum Theory of Fields Volume I …

which page number, and which equations, is it in Weinberg? :smile:
 
To derive the precise form of the Feynman rule, it would be best for you to work it out starting from the LSZ reduction formula for the scattering processes gg\rightarrow g and gg\rightarrow gg. Essentially, the Minkowski metric arises from needing to expand the 4-vector dot products between the vector fields in the interacting Lagrangian before proceeding to contract fields:
A_\mu A^\mu=g_{\mu\nu}A^\mu A^\nu​

Physically speaking, the role of the Minkowski metric in the Feynman rules for the 3- and 4- vector boson vertices is to select, depending on the polarization of the incoming and outgoing vector bosons, the appropriate Clebsch-Gordon coefficient arising from the coupling of two spin-1 systems.
 
Try Srednicki's book. A draft copy is available free at his web page.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

Similar threads

  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 8 ·
Replies
8
Views
27K