Next-to-next-to-leading order calculations for heavy-to-light decays

被引:33
|
作者
Blokland, I [1 ]
Czarnecki, A
Slusarczyk, M
Tkachov, F
机构
[1] Univ Alberta, Dept Phys, Edmonton, AB T6G 2J1, Canada
[2] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada
[3] Jagiellonian Univ, Inst Phys, PL-30059 Krakow, Poland
[4] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
来源
PHYSICAL REVIEW D | 2005年 / 71卷 / 05期
关键词
D O I
10.1103/PhysRevD.71.054004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present technical aspects of next-to-next-to-leading order calculations for heavy-to-light decays such as top quark decay, semileptonic b quark decay into a u quark, muon decay, and radiative decays like b -> s gamma. Algebraic reduction of integrals to a set of master integrals is described, methods of determining the master integrals are presented, and a complete list of master integrals is given. As a sample. accuracy. application, the top quark decay width is calculated to O(alpha(2)(s)) accuracy.
引用
收藏
页码:1 / 12
页数:12
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