The counterterm amplitude:
The Dirac equation:
We now add the two amplitudes and demand that the complete photon propagator to order have the same pole position and residue as the bare propagator apart from gauge dependent terms (see e.g. Weinberg). Thus we demand that S'(
) have a pole at at γ
=
with residue 1, where S'(
) =
:
sigmafull to to order is
sigmafull-amp4OnShell-sigmafullOnShell
, that is, sigmafull
with substituted with
sigmafullOnShell
(since it must cancel sigmafullOnShell
).
We abbreviate sigmafull
to sigmaint[δ]
and sigmafullOnShell
to sigmaint[0]
, and this is then the residue:
This is then the value of (infinite in the limit
->4) following form the demand that the residue be 1:
Since is of the form 1-O(
), to have -
cancel sigmafullOnShell to order
,
must be simply sigmafullOnShell:
The scalar integral with the above values inserted and the limit ->4 taken. The ultraviolet (dimensional) infinities have cancelled, but infrared divergencies remain:
Converted by Mathematica (July 10, 2003)