RARE DECAY B-]K-STAR-GAMMA IN STANDARD AND SUPERSYMMETRIC MODELS

被引：39

作者：

ALIEV, TM

OVCHINNIKOV, AA

SLOBODENYUK, VA

机构：

[1] ACAD SCI USSR, INST NUCL RES, MOSCOW 117312, USSR

[2] PROTVINO INST HIGH ENERGY PHYS, PROTVINO 142284, USSR

来源：

PHYSICS LETTERS B | 1990年 / 237卷 / 3-4期

关键词：

D O I：

10.1016/0370-2693(90)91226-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The formfactor of the rare decay B→K*γ is calculated with the help of the QCD sum rule method for the three-point correlators. Using this formfactor we found that when the sensitivity of the measurements is raised 3-4 times, one could either obtain an upper limit on mt, or detect the decay considered. © 1990.

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页码：569 / 572

页数：4

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