Why do we need the new BNL muon g-2 experiment now?

被引:5
作者
Hertzog, David W. [1 ]
机构
[1] Univ Illinois, Dept Phys, Urbana, IL 61801 USA
关键词
D O I
10.1016/j.nuclphysbps.2007.03.032
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
New final results from the CMD-2 and SND e(+)e(-) annihilation experiments, together with radiative return measurements from BaBar, lead to recent improvements in the Standard Model prediction for the muon anomaly. The uncertainty at 0.48 ppm-a largely data-driven result-is now slightly below the experimental uncertainty of 0.54 ppm. The difference, a(mu) (expt)- a(mu) (SM) = (27.6 +/- 8.4) x 10(-10), represents a 3.3 standard deviation effect. At this level, it is one of the most compelling indicators of physics beyond the Standard Model and, at the very least, a major constraint for speculative new theories such as SUSY or extra dimensions. Others at this Workshop detailed further planned Standard Model theory improvements to a(mu). Here I outline how BNL E969 will achieve a factor of 2 or more reduction in the experimental uncertainty. The new experiment is based on a proven technique and track record. I argue that this work must be started now to have maximal impact on the interpretation of the new physics anticipated to be unearthed at the LHC.
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页码:255 / 264
页数:10
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