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000321045 0881_ $$ahep-ph/0102005; NYU-TH-00-09-09; CERN-TH-2001-002; DESY-01-008
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000321045 1001_ $$0P:(DE-HGF)0$$aGrassi, P. A.$$b0
000321045 245__ $$aThe Algebraic method
000321045 260__ $$aAmsterdam$$bNorth-Holland Publ. Co.$$c2001
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000321045 500__ $$aTheorie
000321045 520__ $$aCombining the effect of an intermediate renormalization prescription (zero momentum subtraction) and the background field method (BFM), we show that the algebraic renormalization procedure needed for the computation of radiative corrections within non-invariant regularization schemes is drastically simplified. The present technique is suitable for gauge models and, here, is applied to the Standard Model. The use of the BFM allows a powerful organization of the counterterms and avoids complicated Slavnov–Taylor identities. Furthermore, the Becchi–Rouet–Stora–Tyutin (BRST) variation of background fields plays a special role in disentangling Ward–Takahashi identities (WTI) and Slavnov–Taylor identities (STI). Finally, the strategy to be applied to physical processes is exemplified for the process b → sγ .
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000321045 7001_ $$0P:(DE-HGF)0$$aHurth, T.$$b1
000321045 7001_ $$0P:(DE-HGF)0$$aSteinhauser, M.$$b2
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