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Radiative corrections and enhanced power corrections for the shape function in inclusive B decays. Kazuhiro Tanaka (Juntendo U). H. Kawamura (RIKEN) J. Kodaira (KEK). OPE. Light-cone expansion. ⇒factorization formula. Bigi et al. (’94), Neubert (’94) Korchemsky, Sterman (’94)
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Radiative corrections and enhanced power corrections for the shape function in inclusive B decays Kazuhiro Tanaka (Juntendo U) H. Kawamura (RIKEN) J. Kodaira (KEK)
OPE Light-cone expansion
⇒factorization formula Bigi et al. (’94), Neubert (’94) Korchemsky, Sterman (’94) Bauer, Pirjol, Sterwart (’02) perturbative nonperturbative 形状 関数 unknown
Grozin, Korchemsky (’96) Bauer,Manohar (’04), Bosch et al. (’04) Loop corrections for RG evolution
Polyakov (’80) Korchemsky (’89) Cusp divergence
Korchemsky, Sterman (’94) Bauer, Manohar (’04)
Solution of RG eq. IR renormalon ambiguity have to be compensated by the power corrections from nonperturbative effects:
Tree-level matching ● Economic way: Kawamura,Kodaira,Tanaka, Prog.Theor.Phys. 113 (’05)183 Eq. of motion constraints on nonlocal operator ⇒ nonlocal op. basis Taylor expand in the final step ⇒ independent set
0 Light-cone expansion Nachtmann corr.
4-particle correlation!!
new enhanced power corrections independent set
● to minimize complication due to alien operators● to maximize gauge invariance in Feynman rules Background field method: Fock-Schwinger gauge
Grozin, Korchemsky (’96) [coincide with Bauer, Manohar (‘04), consistent with Bosch, Lange, Neubert, Paz (‘04)]