2 C*********************************************************************
6 C...Purpose: to calculate the running alpha_electromagnetic.
7 COMMON/LUDAT1/MSTU(200),PARU(200),MSTJ(200),PARJ(200)
10 C...Calculate real part of photon vacuum polarization.
11 C...For leptons simplify by using asymptotic (Q^2 >> m^2) expressions.
12 C...For hadrons use parametrization of H. Burkhardt et al.
13 C...See R. Kleiss et al, CERN 89-08, vol. 3, pp. 129-131.
14 AEMPI=PARU(101)/(3.*PARU(1))
15 IF(MSTU(101).LE.0.OR.Q2.LT.2E-6) THEN
17 ELSEIF(MSTU(101).EQ.2.AND.Q2.LT.PARU(104)) THEN
19 ELSEIF(MSTU(101).EQ.2) THEN
20 RPIGG=1.-PARU(101)/PARU(103)
21 ELSEIF(Q2.LT.0.09) THEN
22 RPIGG=AEMPI*(13.4916+LOG(Q2))+0.00835*LOG(1.+Q2)
24 RPIGG=AEMPI*(16.3200+2.*LOG(Q2))+0.00238*LOG(1.+3.927*Q2)
25 ELSEIF(Q2.LT.1E4) THEN
26 RPIGG=AEMPI*(13.4955+3.*LOG(Q2))+0.00165+0.00299*LOG(1.+Q2)
28 RPIGG=AEMPI*(13.4955+3.*LOG(Q2))+0.00221+0.00293*LOG(1.+Q2)
31 C...Calculate running alpha_em.
32 ULALEM=PARU(101)/(1.-RPIGG)