Probing Supergravity Grand Unification in the Brookhaven g-2 Experiment
arXiv:hep-ph/9507386 · doi:10.1103/PhysRevD.53.1648
Abstract
A quantitative analysis of $\amu\equiv{1\over 2}(g-2)_μ$ within the framework of Supergravity Grand Unification and radiative breaking of the electro-weak symmetry is given. It is found that is dominated by the chiral interference term from the light chargino exchange, and that this term carries a signature which correlates strongly with the sign of . Thus as a rule for and for with very few exceptions when tan. At the quantitative level it is shown that if the E821 BNL experiment can reach the expected sensitivity of and there is a reduction in the hadronic error by a factor of four or more, then the experiment will explore a majority of the parameter space in plane in the region $m_0\lsim 400$ GeV, $m_{\tilde g}\lsim 700$ GeV for $\tanbeta \gsim 10$ assuming the experiment will not discard the Standard Model result within its uncertainty limit. For smaller $\tanbeta$, the SUSY reach of E821 will still be considerable. Further, if no effect within limit of the Standard Model value is seen, then large $\tanbeta$ scenarios will be severely constrained within the current naturalness criterion, ie., $m_0, m_{\tilde g}\lsim 1$ TeV.
27 pages, Latex, uuencoded figure file to be obtained and processed separately for two figures. Figures may also be sent on request by mail
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