b→sγ and supersymmetry with large tan β

被引:309
作者
Carena, M
Garcia, D
Nierste, U
Wagner, CEM
机构
[1] Fermi Natl Accelerator Lab, Batavia, IL 60510 USA
[2] CERN, Div Theory, CH-1211 Geneva 23, Switzerland
[3] Argonne Natl Lab, Theoret HEP Div, Argonne, IL 60439 USA
[4] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[5] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
关键词
D O I
10.1016/S0370-2693(01)00009-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the constraints on the supersymmetric parameter space from the decay mode b --> s gamma for large values of tan beta. We improve the theoretical prediction Tol the decay rate by summing very large radiative corrections to all orders in perturbation theory. This extends the validity of the perturbative calculation to the large tan beta regime. This resummation of terms of order alpha (n)(s) tan(n+1) beta is based on a recently proposed effective Lagrangian for the Yukawa interaction of bottom quarks. Moreover, we identify an additional source of tan beta -enhanced terms, which are of order alpha (s) tan beta and involve the charged Higgs boson, and analyse their behaviour in higher orders of perturbation theory. After correcting the current expressions for this rare decay branching ratio at next-to-leading order, we obtain that, contrary to recent claims, the measured branching ratio of b --> s gamma constrains the supersymmetric parameter space in a relevant way, even if tan beta is large. (C) 2001 Published by Elsevier Science B.V.
引用
收藏
页码:141 / 146
页数:6
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