In most books, one can find the field renormalization Z3 in Yang-Mills with fermionic matter in the fundamental. In the ¯MS scheme, tt is given by
Z3=1+g216π2ϵ[103TA−83nFTF]+O(g3)
One often writes
δ3=Z3−1.
This formula can be found in
- Eq. (73.33) of Srednicki.
- Eq. (26.83) of Matt Schwartz' book.
- Eq. (16.74) of P&S
etc.
However, I can't find any reference that lists how this result is modified if there's scalar matter present. I've already computed it and I get
Z3=1+g216π2ϵ[103TA−83nFTF−23nSTF]+O(g3)
Is this correct?
In particular, I'm really interested in computing ALL the counterterms of Yang-Mills in the presence of scalar matter. Is there any reference out there that already does that so I can match my results?
This post imported from StackExchange Physics at 2015-01-23 12:48 (UTC), posted by SE-user Prahar