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We give here as an example of a simple calculation in high energy physics the computation of the Compton scattering cross-section as given in Bjorken and Drell Eqs. (7.72) through (7.74). We wish to compute the trace of
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where ki and kf are the four-momenta of incoming and outgoing photons (with polarization vectors e and e′ and laboratory energies k and k′ respectively) and pi, pf are incident and final electron four-momenta.
Omitting therefore an overall factor 
2 we need to find one quarter of
the trace of
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A straightforward REDUCE program for this, with appropriate substitutions (using P1 for pi, PF for pf, KI for ki and KF for kf) is
on div; % this gives output in same form as Bjorken and Drell. mass ki= 0, kf= 0, p1= m, pf= m; vector e,ep; % if e is used as a vector, it loses its scalar identity % as the base of natural logarithms. mshell ki,kf,p1,pf; let p1.e= 0, p1.ep= 0, p1.pf= m^2+ki.kf, p1.ki= m*k,p1.kf= m*kp, pf.e= -kf.e, pf.ep= ki.ep, pf.ki= m*kp, pf.kf= m*k, ki.e= 0, ki.kf= m*(k-kp), kf.ep= 0, e.e= -1, ep.ep=-1; operator gp; for all p let gp(p)= g(l,p)+m; comment this is just to save us a lot of writing; gp(pf)*(g(l,ep,e,ki)/(2*ki.p1) + g(l,e,ep,kf)/(2*kf.p1)) * gp(p1)*(g(l,ki,e,ep)/(2*ki.p1) + g(l,kf,ep,e)/ (2*kf.p1))$ write "The Compton cxn is ",ws;
(We use P1 instead of PI in the above to avoid confusion with the reserved variable PI).
This program will print the following result
2 1 -1 1 -1 The Compton cxn is 2*E.EP + ---*K*KP + ---*K *KP - 1 2 2
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